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An introduction to inflation after Planck: from theory to observations,
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How many new particles do we need after the Higgs boson?,
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CosPA2013: Outlook,
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Galaxy formation,
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Towards the Chalonge 17th Paris Cosmology Colloquium 2013: highlights and conclusions of the Chalonge 16th Paris Cosmology Colloquium 2012,
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What do we really know about Dark Energy?,
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Cosmological Tests of General Relativity. [Durrer:2011gq]
Proceedings of the 2009 CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 March 2009,
C. Grojean, M. Spiropulu,
arXiv:1010.5976, 2010.CERN Yellow Report. [Grojean:2010zza]
Particle cosmology,
A. Riotto,
arXiv:1010.2642, 2010.5th CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 Mar 2009. [Riotto:2010jd]
The violent Universe: the Big Bang,
Keith A. Olive,
arXiv:1005.3955, 2010.2009 European School of High-Energy Physics, Bautzen, Germany, June 2009. [Olive:2010mh]
The connection between cosmology and neutrino physics,
Steen Hannestad,
arXiv:1003.4119, 2010.Workshop 'European Strategy for Future Neutrino Physics', CERN, oct.2009. [Hannestad:2010qz]
Dark Energy and Dark Matter,
Keith A. Olive,
Conf. Proc. C0908171 (2009) 257-270,arXiv:1001.5014.
XXIV International Symposium on Lepton Photon Interactions at High Energies, Hamburg Germany, August 2009. [Olive:2010qw]
Fundamental Symmetries of the Early Universe and the Precision Frontier,
Michael J. Ramsey-Musolf,
AIP Conf. Proc. 1182 (2009) 635-643,arXiv:0907.3916.
CIPANP 2009. [RamseyMusolf:2009ga]
Dark Matter Astrophysics,
Guido D'Amico, Marc Kamionkowski, Kris Sigurdson,
arXiv:0907.1912, 2009.Villa Olmo School on 'The Dark Side of the Universe,' 14-18 May 2007 and XIX Heidelberg Physics Graduate Days, 8-12 October 2007. [DAmico:2009tep]
Great Surveys of the Universe,
Steven T. Myers,
arXiv:0904.2593, 2009.Great Surveys of Astronomy Workshop, 20-22 November 2008, Santa Fe, NM. [Myers:2009ve]
Cosmologists in the dark,
Vicent J. Martinez, Virginia Trimble,
ASP Conf.Ser. 409 (2009) 47,arXiv:0904.1126.
Cosmology across Cultures, Granada, Spain, 2008. [Martinez:2009nq]
Baryogenesis and cosmological antimatter,
A.D. Dolgov,
AIP Conf. Proc. 1116 (2009) 155-170,arXiv:0901.2100.
XIII Mexican School of Particles and Fields, San Carlos, October, 2008. [Dolgov:2009py]
Dark matter and dark energy proposals: maintaining cosmology as a true science?,
George F. R. Ellis,
EAS Publ.Ser. 36 (2009) 325-336,arXiv:0811.3529.
CRAL-IPNL conference 'Dark Energy and Dark Matter', Lyon 2008. [Ellis:2008up]
Neutrinos as cosmic messengers,
J. W. F. Valle,
AIP Conf. Proc. 1115 (2009) 13-26,arXiv:0811.0707.
4th International Workshop on the Dark Side of the Universe (DSU08) Conference, Cairo. [Valle:2008rg]
Neutrinos and Future Concordance Cosmologies,
Peter Adshead, Richard Easther,
J. Phys. Conf. Ser. 136 (2008) 022044,arXiv:0810.2591.
Neutrino 2008. [Adshead:2008ky]
Cosmology for Particle Physicists,
U. A. Yajnik,
arXiv:0808.2236, 2008.SERC School on Theoretical High Energy Physics, PRL Ahmedabad, February 2006. [Yajnik:2006kn]
Neutrinos and BBN (and the CMB),
Gary Steigman,
arXiv:0807.3004, 2008.NO-VE IV International Workshop on: Neutrino Oscillations in Venice. [Steigman:2008eb]
The ART of Cosmological Simulations,
Stefan Gottloeber, Anatoly Klypin,
arXiv:0803.4343, 2008.High Performance Computing in Science and Engineering Garching/Munich 2007. [Gottloeber:2008ac]
Recent Developments in Gravitational Microlensing,
Andrew Gould,
ASP Conf.Ser. 403 (2009) 86,arXiv:0803.4324.
The Variable Universe: A Celebration of Bohdan Paczynski, 29 Sept 2007. [Gould:2008zu]
Cosmology and Neutrino Properties,
A. D. Dolgov,
Phys. Atom. Nucl. 71 (2008) 2152-2164,arXiv:0803.3887.
Meeting of Nuclear Physics Division of Russian Academy of Sci., November, 2007, Moscow. [Dolgov:2008hz]
Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination,
Wayne Hu,
arXiv:0802.3688, 2008.XIX Canary Island Winter School of Astrophysics. [Hu:2008hd]
The evidence for unusual gravity from the large-scale structure of the Universe,
A. Diaferio,
arXiv:0802.2532, 2008.1st AFI symposium. [Diaferio:2008jy]
RICAP-07: Summary comments,
Thomas K. Gaisser,
Nucl. Instrum. Meth. A588 (2008) 276-280,arXiv:0801.4546.
Roma International Conference on Astroparticle Physics, June 2007. [Gaisser:2008cr]
Cosmological model: from initial conditions to structure formation,
V. Lukash,
Nuovo Cim. 122B (2007) 1411-1422,arXiv:0712.3356.
A Century of Cosmology : Past, Present and Future, August 27-31 2007, Venezia, Italy. [Lukash:2007ns]
The Future of Cosmology,
George Efstathiou,
Nuovo Cim. 122B (2007) 1423-1435,arXiv:0712.1513.
A Century of Cosmology, S. Servolo, August 2007. [Efstathiou:2007gz]
Observational approaches to understanding dark energy,
Yun Wang,
arXiv:0712.0041, 2007.23rd International Symposium on Lepton and Photon Interactions at High Energy (LP07). [Wang:2007sq]
CPT violations in Astrophysics and Cosmology,
G. Auriemma,
Chin.J.Astron.Astrophys.Suppl. 8 (2008) 33,arXiv:0711.0504.
Frascati Workshop 2007 Vulcano (Italy), May 28 - June 2, 2007. [Auriemma:2007bm]
Cosmology and the Unexpected,
Edward W. Kolb,
Subnucl.Ser. 45 (2009) 337-363,arXiv:0709.3102.
International School of Subnuclear Physics, Searching for the 'totally unexpected' in the LHC era, Erice, Italy 2007. [Kolb:2007gb]
WMAPping the Inflationary Universe,
Raghavan Rangarajan,
arXiv:0706.4166, 2007.17th DAE-BRNS High Energy Physics Symposium at the Indian Institute of Technology, Kharagpur, December 11-15, 2006. [Rangarajan:2007ff]
TASI Lectures on Astrophysical Aspects of Neutrinos,
John F. Beacom,
arXiv:0706.1824, 2007.Exploring New Frontiers Using Colliders and Neutrinos (TASI 2006), Boulder, Colorado, 4-30 Jun 2006. [Beacom:2007av]
Physics Beyond the Standard Model and Cosmological Connections: A Summary from LCWS 06,
K. Sridhar,
Pramana 69 (2007) 719-726,arXiv:hep-ph/0702109.
International Linear Collider Workshop in Bangalore, India in March 2006. [Sridhar:2007vv]
Gamow Legacy and the Primordial Abundance of Light Elements,
E. Terlevich, R. Terlevich, V. Luridiana,
arXiv:astro-ph/0701744, 2007.Astrophysics and Cosmology after Gamow - Theory and Observations, Odessa, August 8-14, 2004. [Terlevich:2007ym]
BBN And The CBR Probe The Early Universe,
Gary Steigman,
AIP Conf. Proc. 903 (2007) 40-47,arXiv:hep-ph/0611209.
SUSY06, 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006'. [Steigman:2006yn]
Varying 'constants' in astrophysics and cosmology,
Thomas Dent,
AIP Conf. Proc. 903 (2007) 665-668,arXiv:hep-ph/0610376.
SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006. [Dent:2006mn]
Cosmic Microwave Background anisotropies: the power spectrum and beyond,
Enrique Martinez-Gonzalez,
Lect.Notes Phys. 665 (2009) 79,arXiv:astro-ph/0610162.
Valencia Summer School 'Data Analysis in Cosmology, September 2004. [MartinezGonzalez:2006na]
Dark Energy and Some Alternatives: a Brief Overview,
J.S. Alcaniz,
Braz. J. Phys. 36 (2006) 1109,arXiv:astro-ph/0608631.
XXVI Brazilian National Meeting on Particles and Fields, Sao Lourenco, Brazil. [Alcaniz:2006ay]
Probing dark energy with future surveys,
Roberto Trotta,
arXiv:astro-ph/0607496, 2006.'Cosmology, galaxy formation and astroparticle physics on the pathway to the SKA', Oxford, April 10-12 2006. [Trotta:2006pw]
Integrated Sachs-Wolfe effect in the era of precision cosmology,
Levon Pogosian,
New Astron. Rev. 50 (2006) 932-937,arXiv:astro-ph/0606626.
Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006. [Pogosian:2006ay]
Future state of the Universe,
Mariusz P. Dabrowski,
Annalen Phys. 15 (2006) 352-363,arXiv:astro-ph/0606574.
Pomeranian Workshop in Fundamental Cosmology (COSMOFUN'05), Pobierowo, Poland, 1-6 September 2005. [Dabrowski:2006iv]
Cosmological quests in the CMB sky,
Tarun Souradeep,
Int. J. Mod. Phys. D15 (2006) 1725-1743,arXiv:astro-ph/0606512.
International Conference on Einstein's Legacy in the New Millennium, December 15 - 22, 2005, Puri, India. [Souradeep:2006vm]
Cosmology and New Physics,
A.D. Dolgov,
Phys. Atom. Nucl. 71 (2008) 651-670,arXiv:hep-ph/0606230.
9th International Moscow School of Physics (34th ITEP Winter School). [Dolgov:2006xi]
Constraints on cosmological parameters,
A. Balbi,
PoS CMB2006 (2006) 009,arXiv:astro-ph/0606183.
'CMB and Physics of the Early Universe' - International Conference - Ischia, Italy, 20-22 April 2006. [Balbi:2006mg]
Sub-eV upper limits on neutrino masses from cosmology,
Oystein Elgaroy, Ofer Lahav,
Phys. Scripta T127 (2006) 105-106,arXiv:hep-ph/0606007.
SNOW 2006, Stockholm, May 2-6, 2006. [Elgaroy:2006ii]
Cosmology with clusters of galaxies,
Stefano Borgani,
Lect.Notes Phys. (2006),arXiv:astro-ph/0605575.
2005 Guillermo Haro Summer School on Clusters. [Borgani:2006ba]
What is the Role of Neutrinos in Shaping the Universe?,
Lawrence M. Krauss,
arXiv:astro-ph/0605378, 2006.International Workshop on NO-VE, Venice, 2006. [Krauss:2006eb]
The Cosmology - Particle Physics Connection,
Mark Trodden,
AIP Conf. Proc. 842 (2006) 945-953,arXiv:hep-ph/0605284.
Particles and Nuclei International Conference (PANIC05) and CMB and Physics of the Early Universe International Conference (2006). [Trodden:2006ed]
Understanding Galaxy Formation and Evolution,
V. Avila-Reese,
arXiv:astro-ph/0605212, 2006.IV Mexican School of Astrophysics, July 18-25, 2005. [AvilaReese:2006rg]
Non Thermal Features in the Cosmic Neutrino Background,
G. Mangano,
arXiv:astro-ph/0603603, 2006.'Neutrino Oscillations in Venice' Conference, Venice, February 7-10 2006. [Mangano:2006xs]
Dark Energy: Mystery of the Millennium,
T. Padmanabhan,
AIP Conf. Proc. 861 (2006) 179-196,arXiv:astro-ph/0603114.
Albert Einstein Century International Conference at Palais de l'Unesco, Paris, France, 18-23 July, 2005. [Padmanabhan:2006ag]
Probing the Fundamental Symmetries of the Early Universe: The Low Energy Frontier,
M. J. Ramsey-Musolf,
AIP Conf. Proc. 842 (2006) 661-671,arXiv:hep-ph/0603023.
PANIC05 (Sante Fe, NM). [RamseyMusolf:2006ur]
The present and the future of cosmology with Gamma Ray Bursts,
G. Ghirlanda, G. Ghisellini,
arXiv:astro-ph/0602498, 2006.Science with the New Generation of High-Energy Gamma-Ray Experiments, Cividale del Friuli (Italy), 30 May - 1 June 2005. [Ghirlanda:2006bj]
Advanced Topics in Cosmology: A Pedagogical Introduction,
T. Padmanabhan,
AIP Conf. Proc. 843 (2006) 111-166,arXiv:astro-ph/0602117.
X Special Courses at Observatorio Nacional, Rio de Janeiro, Brazil during 26-30 Sept, 2005. [Padmanabhan:2006kz]
Cosmological constraints from galaxy clustering,
Will J. Percival,
Lect. Notes Phys. 720 (2007) 157-186,arXiv:astro-ph/0601538.
Third Aegean Summer School, The invisible universe: Dark matter and Dark energy. [Percival:2006kh]
Accelerating Universe: Observational Status and Theoretical Implications,
L. Perivolaropoulos,
AIP Conf. Proc. 848 (2006) 698-712,arXiv:astro-ph/0601014.
Third Aegean Summer School: `The Invisible Universe Dark Matter and Dark Energy'. [Perivolaropoulos:2006ce]
The Ups and Downs of the Hubble Constant,
G.A. Tammann,
Rev. Mod. Astron. 19 (2006) 1,arXiv:astro-ph/0512584.
79th Annual Scientific Meeting of the Astronomische Gesellschaft 2005. [Tammann:2005nx]
Primordial Black Holes: Do They Exist and Are They Useful?,
B. J. Carr,
arXiv:astro-ph/0511743, 2005.'Inflating Horizon of Particle Astrophysics and Cosmology', Universal Academy Press Inc and Yamada Science Foundation (2005). [Carr:2005zd]
First Light and Reionization: A Conference Summary,
E. J. Barton, J. S. Bullock, A. Cooray, M. Kaplinghat,
New Astron. Rev. 50 (2006) 1,arXiv:astro-ph/0511637.
UC Irvine Workshop on 'First Light and Reionization: Theoretical Study and Experimental Detection of the First Luminous Sources'. [Barton:2005kg]
Varying Constants,
John D. Barrow,
Phil. Trans. Roy. Soc. Lond. A363 (2005) 2139,arXiv:astro-ph/0511440.
Royal Society Discussion Meeting on 'The Fundamental Constants of Physics, Precision Measurements and the Base Units of SI', London, Feb. 14-15 (2005). [Barrow:2005hw]
Absolute Neutrino Masses,
Carlo Giunti,
Acta Phys. Polon. B36 (2005) 3215,arXiv:hep-ph/0511131.
XXIX International Conference of Theoretical Physics 'Matter To The Deepest: Recent Developments In Physics Of Fundamental Interactions', 8-14 September 2005, Ustron, Poland. [Giunti:2005qd]
The Standard Cosmological Model,
Douglas Scott,
Can. J. Phys. 84 (2006) 419-435,arXiv:astro-ph/0510731.
'Theory Canada 1', June 2005, Vancouver. [Scott:2005uf]
Darker Side of the Universe,
T. Padmanabhan,
arXiv:astro-ph/0510492, 2005.29th International Cosmic Ray Conference, Aug 3-10, 2005, Pune, India. [Padmanabhan:2005ur]
Dark energy - dark matter - and black holes: The music of the universe,
Peter L. Biermann,
arXiv:astro-ph/0510024, 2005.Carpathian Summer School in Physics 2005 (CSSP2005). [Biermann:2005qh]
The Cosmic Microwave Background anisotropies: open problems,
E. Martinez-Gonzalez, P. Vielva,
arXiv:astro-ph/0510003, 2005.The Many Scales of the Universe - JENAM 2004 Astrophysics Reviews. [MartinezGonzalez:2005pk]
Formation of the First Stars,
Volker Bromm,
IAU Symp. (2005),arXiv:astro-ph/0509354.
'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution', IAU Symposium 228. [Bromm:2005gs]
Dark energy and dark matter from cosmological observations,
Steen Hannestad,
Int. J. Mod. Phys. A21 (2006) 1938-1949,arXiv:astro-ph/0509320.
22nd International Symposium on Lepton-Photon Interactions at High Energy (LP 2005), Uppsala, Sweden, 30 June - 5 Jul 2005. [Hannestad:2005fg]
ILC Cosmology,
Jonathan L. Feng,
eConf C050318 (2005) 0013,arXiv:hep-ph/0509309.
2005 International Linear Collider Workshop, Stanford, California, USA, 18-22 March 2005. [Feng:2005nz]
The Dark Side of the Universe,
Katherine Freese,
Nucl. Instrum. Meth. A559 (2006) 337,arXiv:astro-ph/0508279.
LTD-11 WOrkshop in Tokyo, August 2005. [Freese:2005hy]
Neutrinos and Cosmology: an update,
Ofelia Pisanti, P.D. Serpico,
Aip Conf. Proc. 794 (2005) 232,arXiv:astro-ph/0507346.
IFAE, Catania 2005. [Pisanti:2005yz]
Neutrino mass and mixing parameters: A short review,
G.L. Fogli et al.,
arXiv:hep-ph/0506307, 2005.40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005. [Fogli:2005gs]
Theory Summary of the Electroweak Session for Moriond 2005,
R. D. Peccei,
arXiv:hep-ph/0506016, 2005.Electroweak Session of the 2005 Moriond Meeting. [Peccei:2005pc]
Massive neutrinos and cosmology,
Sergio Pastor,
arXiv:hep-ph/0505148, 2005.XXXXth Moriond session on Electroweak Interactions and Unified Theories (La Thuile, 5-12 March 2005), and the XIth Int. Workshop on Neutrino Telescopes (Venice, 22-25 Feb 2005). [Pastor:2005qd]
From Little Bangs to the Big Bang,
John Ellis,
J. Phys. Conf. Ser. 50 (2006) 8-21,arXiv:astro-ph/0504501.
International Conference on the Physics and Astrophysics of the Quark-Gluon Plasma, Kolkata, Feb. 2005. [Ellis:2005xq]
Cosmology with Gamma Ray Bursts,
G. Ghisellini et al.,
Nuovo Cim. 28C (2005) 639,arXiv:astro-ph/0504306.
4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004. [Ghisellini:2005vk]
Relic Gravitational Waves and Cosmology,
L. P. Grishchuk,
Phys. Usp. 48 (2005) 1235-1247,arXiv:gr-qc/0504018.
`Zeldovich-90', Moscow, December 2004. [Grishchuk:2005qe]
Extracting New Physics from the CMB,
B. Greene, K. Schalm, G. Shiu, J.P. van der Schaar,
eConf C041213 (2004) 0001,arXiv:astro-ph/0503458.
XXII Texas Symposium on Relativistic Astrophysics, Stanford University, 13-17 December 2004. [Greene:2005aj]
Measuring the cosmological density perturbation,
Subir Sarkar,
Nucl. Phys. Proc. Suppl. 148 (2005) 1,arXiv:hep-ph/0503271.
Workshop on 'The Density Perturbation in the Universe', Athens, June 2004. [Sarkar:2005fq]
Cosmological neutrino bounds for non-cosmologists,
Max Tegmark,
Phys. Scripta T121 (2005) 153,arXiv:hep-ph/0503257.
'Neutrino Physics', Proceedings of Nobel Symposium 129. [Tegmark:2005cy]
Primordial Gravitational Waves and Inflation: CMB and Direct Detection With Space-Based Laser Interferometers,
Asantha Cooray,
Mod. Phys. Lett. (2005) (2005),arXiv:astro-ph/0503118.
Daniel Chalonge International School of Astrophysics: WMAP and the Early Universe, Observatoire de Paris, December 2004. [Cooray:2005xr]
Cosmology and Astrophysics,
Juan Garcia-Bellido,
arXiv:astro-ph/0502139, 2005.CERN-JINR European School of High Energy Physics, San Feliu (Spain), 30 May - 12 June 2004. [Capozziello:2013kla]
The Shape of Space after WMAP data,
Jean-Pierre Luminet,
Braz. J. Phys. 36 (2006) 107,arXiv:astro-ph/0501189.
25th Brazilian Meeting of Particle Physics and Fields, Caxambu, Minas Gerais, Brazil, 24-27 Aug 2004. [Luminet:2005tn]
Neutrinos And Big Bang Nucleosynthesis,
Gary Steigman,
Phys. Scripta T121 (2005) 142,arXiv:hep-ph/0501100.
Nobel Symposium 129, Neutrino Physics. [Steigman:2005ys]
Dealing with dark energy,
Eric V. Linder,
arXiv:astro-ph/0501057, 2005.DARK 2004: 5th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, College Station, Texas, 3-9 Oct 2004. [Linder:2005qz]
Massive Neutrinos in Astrophysics and Cosmology,
F. Villante, 2005.ISAPP 2005, International School on AstroParticle Physics (European Doctorate School): High Energy Cosmic Rays, 30 June - 9 July 2005, Belgirate, Lago Maggiore, Italy.http://www.isapp2005.to.infn.it/Lessons/Villante.pdf.
[Villante-ISAPP05]
From COBE to WMAP: A Decade of Data Under Scrutiny,
Louise M. Ord,
arXiv:astro-ph/0412354, 2004.5th Rencontres du Vietnam 'New Views on the Universe', Aug 5-11, 2004. [Ord:2004eb]
Dark Matter and Galaxy Formation: Challenges for the Next Decade,
Joseph Silk,
Aip Conf. Proc. 743 (2005) 33,arXiv:astro-ph/0412297.
Mitchell Symposium on Observational Cosmology and Strings and Cosmology Conference, College Station, April 2004, and C. Pope, AIP, New York, and PASCOS04/NathFest, Boston, August 2004. [Silk:2004uj]
What are the Building Blocks of Our Universe?,
Kameshwar C. Wali,
arXiv:astro-ph/0411321, 2004.International Conference on Cosmology, Facts and Problems (College de France, Paris, June 8-11, 2004). [Wali:2004zk]
Big Bang and Heavy Particles,
A.D. Dolgov,
arXiv:hep-ph/0411283, 2004.INFN Eloisatron Project, 44th Workshop, QCD at Cosmic Energies, August 29 - September 5, 2004, Erice, Italy. [Dolgov:2004gn]
The current status of observational cosmology,
Jeremiah P. Ostriker, Tarun Souradeep,
Pramana 63 (2004) 817,arXiv:astro-ph/0409131.
ICGC-04. [Ostriker:2004ht]
Lectures on astroparticle physics,
Guenter Sigl,
Aip Conf. Proc. 782 (2005) 1,arXiv:hep-ph/0408165.
XIth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 26 - August 4, 2004. [Sigl:2004cq]
Modern Cosmology,
Juan Garcia-Bellido,
arXiv:hep-ph/0407111, 2004.XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004. [GarciaBellido:2004ri]
The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous,
Lawrence M. Krauss,
arXiv:astro-ph/0406673, 2004.XIV Canary Islands Winter School in Astrophysics, 2002. [Krauss:2004iq]
The Cosmic Microwave Background and Its Polarization,
Angelica de Oliveira-Costa,
ASP Conf.Ser. 343 (2005) 485,arXiv:astro-ph/0406358.
'Astronomical Polarimetry - Current Status and Future Directions', Hawaii, USA, March 15-19, 2004. [deOliveiraCosta:2004zs]
Summary of the XXXIX Rencontres de Moriond,
Matts Roos,
arXiv:astro-ph/0405625, 2004.XXXIX Rencontres de Moriond 'Exploring the Universe'. [Roos:2004nd]
Astroparticle Physics,
I. I. Tkachev,
arXiv:hep-ph/0405168, 2004.2003 European School of High-Energy Physics, Tsakhkadzor, Armenia, 24 August - 6 September 2003. [Tkachev:2004ee]
Problems of vacuum energy and dark energy,
A.D. Dolgov,
Frascati Phys.Ser. 34 (2004) 75-94,arXiv:hep-ph/0405089.
18th Rencontre de Physique de la Vallee d'Aosta on Results and Perspectives in Particle Physics, 29/02 - 06/03, 2004. [Dolgov:2004xu]
Anisotropies in the Cosmic Microwave Background,
Anthony Challinor,
arXiv:astro-ph/0403344, 2004.2nd Aegean Summer School on the Early Universe (Springer LNP), 22-30 September 2003. [Challinor:2004bd]
Dark Matter and Dark Energy,
Varun Sahni,
Lect. Notes Phys. 653 (2004) 141,arXiv:astro-ph/0403324.
Second Aegean Summer School on the Early Universe, Syros, Greece, September 2003. [Sahni:2004ai]
Cosmic Topology: a Brief Overview,
M.J. Reboucas, G.I. Gomero,
Braz. J. Phys. 34 (2004) 1358,arXiv:astro-ph/0402324.
'XIV National Meeting of the Brazilian Physical Society, section Particles and Fields, Caxambu - MG, Brazil, from September 30 to October 04, 2003. [Reboucas:2004dv]
Observational Cosmology,
R.H. Sanders,
Lect. Notes Phys. 653 (2004) 105,arXiv:astro-ph/0402065.
Second Aegean Summer School on the Early Universe. [Sanders:2004xi]
TASI Lectures: Introduction to Cosmology,
Mark Trodden, Sean M. Carroll,
arXiv:astro-ph/0401547, 2004.TASI-02 and TASI-03 summer schools. [Trodden:2004st]
What we know and what we don't know about the universe,
Marcelo Gleiser,
Int. J. Mod. Phys. D13 (2004) 1381,arXiv:astro-ph/0401213.
1st International Workshop on Astronomy and Relativistic Astrophysics, Olinda, Brazil, 12-17 Oct 2003. [Gleiser:2004ny]
Precision Cosmology,
A. Primack, 2004.Sixth UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, February 18-20, 2004, Marina del Rey, California, US.http://www.physics.ucla.edu/hep/dm04/talks/primack.pdf.
[Primack:DM2004]
Neutrinos and astrophysics,
S. Hannestad, 2004.SEESAW25,International Conference on the Seesaw Mechanism, 10-11 June 2004, Paris, France.http://seesaw25.in2p3.fr/trans/hannestad.pdf.
[Hannestad:SEESAW2004]
Inflation and Precision Cosmology,
Jerome Martin,
Braz. J. Phys. 34 (2004) 1307,arXiv:astro-ph/0312492.
XXIV Brazilian National Meeting on Particles and Fields (Caxambu, Brazil, 30 Sep - 4 Oct 2003). [Martin:2003bt]
Neutrino cosmology - an update,
Steen Hannestad,
arXiv:hep-ph/0312122, 2003.Thinking, observing, and mining the universe, Sorrento, Italy (22-27 September 2003). [Hannestad:2003px]
Open Problems in Cosmology,
P. J. E. Peebles,
Nucl. Phys. Proc. Suppl. 138 (2005) 5,arXiv:astro-ph/0311435.
TAUP 2003, Seattle, September, 2003. [Peebles:2003pk]
Status of observational cosmology and inflation,
L. Covi,
eConf C030626 (2003) THBT01,arXiv:hep-ph/0309238.
XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003. [Covi:2003ku]
Gravitational lensing as a probe of structure,
Peter Schneider,
arXiv:astro-ph/0306465, 2003.XIV Canary Islands Winter School of Astrophysics 'Dark Matter and Dark Energy in the Universe' Tenerife. [Schneider:2003yb]
Magnetic fields in cosmology,
A. D. Dolgov,
arXiv:astro-ph/0306443, 2003.17th Rencontre de Physique de la Vallee d'Aoste on Results and Perspectives in Particle Physics, March 9-15, 2003. [Dolgov:2003xd]
Relic neutrinos: neutrino properties from cosmology,
S. Pastor,
arXiv:hep-ph/0306233, 2003.X Int. Workshop on Neutrino Telescopes, Venice, March 11-14, 2003. [Pastor:2003jx]
Cosmology at the Turn of Centuries,
A.D. Dolgov,
arXiv:hep-ph/0306200, 2003.International Conference I.Ya. Pomeranchuk and Physics at the Turn of Centuries, January 24-28, 2003, Moscow, Russia. [Dolgov:2003zg]
Cosmological Constraints on Neutrino Masses and Mixings,
A.D. Dolgov,
arXiv:hep-ph/0306154, 2003.NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan. [Dolgov:2003hi]
Theoretical Overview of Cosmic Microwave Background Anisotropy,
E. L. Wright,
arXiv:astro-ph/0305591, 2003.Carnegie Observatories Centennial Symposium II. [Wright:2003ig]
The Polarization of the Cosmic Microwave Background,
Matias Zaldarriaga,
arXiv:astro-ph/0305272, 2003.Carnegie Observatories Centenial Symposium II. [Zaldarriaga:2003bb]
Gravitational Lensing by Large Scale Structures: A Review,
L. Van Waerbeke, Y. Mellier,
arXiv:astro-ph/0305089, 2003.Aussois winter school, january 2003. [VanWaerbeke:2003uq]
Introductory Overview of Modern Cosmology,
Burin Gumjudpai,
arXiv:astro-ph/0305063, 2003.The Second Tah Poe School on Cosmology 'Modern Cosmology' (TPCosmo II), 17-25 April 2003, Naresuan University, Phitsanulok, Thailand. [Gumjudpai:2003nd]
Particle Physics and Cosmology,
John Ellis,
arXiv:astro-ph/0305038, 2003.Australian National University Summer School on the New Cosmology, January 2003. [Ellis:2003ch]
Physics of Structure Formation in the Universe,
T. Roy Choudhury,
Bull. Astron. Soc. India 31 (2003) 281,arXiv:astro-ph/0305033.
22nd meeting of Astronomical Society of India (2003). [Choudhury:2003cc]
Quasar Lensing: the Observer's Point of View,
F. Courbin,
arXiv:astro-ph/0304497, 2003.'Gravitational Lensing: a unique tool for cosmology', Aussois, France, January 2003. [Courbin:2003ip]
Ten major challenges in cosmology,
Reuven Opher,
arXiv:astro-ph/0304369, 2003.Xth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 29 - Aug. 9, 2002. [Opher:2003gv]
Inflation, Large Scale Structure and Particle Physics,
S. F. King,
Pramana 62 (2004) 307,arXiv:hep-ph/0304264.
9th International Symposium on Particles, Strings and Cosmology (PASCOS 03), Mumbai (Bombay) India, 3-8 Jan 2003. [King:2003jw]
Dark Matter and Dark Energy: Summary and Future Directions,
John Ellis,
Phil. Trans. Roy. Soc. Lond. A361 (2003) 2607,arXiv:astro-ph/0304183.
Royal Society Discussion Meeting on Dark Matter and Dark Energy, January 2003. [Ellis:2003ug]
Clusters of galaxies: a fundamental pillar of cosmology,
Africa Castillo-Morales, Sabine Schindler,
arXiv:astro-ph/0303609, 2003.Vulcano Workshop 2002 'Frontier Objects in Astrophysics and Particle Physics'. [CastilloMorales:2003ns]
Cosmology from Topological Defects,
Alejandro Gangui,
Aip Conf. Proc. 668 (2003) 226,arXiv:astro-ph/0303504.
Xth Brazilian School on Cosmology and Gravitation, Mangaratiba, Rio de Janeiro, July 29 - August 9, 2002. [Gangui:2003uu]
The evolution of the universe,
Juan Garcia-Bellido,
arXiv:hep-ph/0303153, 2003.International Colloquium on TIME AND MATTER, Venice, Italy, August 11 - 17, 2002. [GarciaBellido:2003ih]
Cosmology, inflation, and the physics of nothing,
William H. Kinney,
NATO Adv.Study Inst.Ser.II.Math.Phys.Chem. 123 (2003) 189-243,arXiv:astro-ph/0301448.
NATO Advanced Study Institute on Techniques and Concepts of High Energy Physics, St. Croix, USVI (2002). [Kinney:2003xf]
Cosmological Parameters: Fashion and Facts,
A. Blanchard,
arXiv:astro-ph/0301137, 2003.th Workshop on 'New Worlds in Astroparticle Physics' in Faro, Portugal, September 2003. [Blanchard:2003wf]
Could Dark Energy be Measured from Redshift Surveys ?,
Ofer Lahav,
arXiv:astro-ph/0212358, 2002.XVIIIth IAP meeting `On the Nature of Dark Energy', Paris 2002. [Lahav:2002rp]
The New Cosmology: Mid-term Report Card for Inflation,
Michael S. Turner,
Annales Henri Poincare 4 (2003) S333,arXiv:astro-ph/0212281.
Th2002 Congress (Paris, France, July 2002). [Turner:2002ts]
Particle Physics and Cosmology,
Juan Garcia-Bellido,
Frascati Phys. Ser. 31 (2003) 321,arXiv:hep-ph/0211316.
First International Workshop on Frontier Science, October 6-11, 2002, Frascati (Italy). [GarciaBellido:2002vv]
Neutrinos in cosmology, with some significant digressions,
R. R. Volkas,
Aip Conf. Proc. 655 (2003) 220,arXiv:hep-ph/0211309.
3rd Tropical Workshop on Particle Physics and Cosmology, San Juan, Puerto Rico, Aug 19-24 2002. [Volkas:2002vn]
High-Energy Astrophysics and Cosmology,
John Ellis,
arXiv:astro-ph/0210580, 2002.XIIth International Symposium on Very-High-Energy Cosmic-Ray Interactions, CERN, July 2002. [Ellis:2003aa]
Can We See the Shape of the Universe?,
G. I. Gomero,
Int. J. Mod. Phys. A17 (2002) 4281-4286,arXiv:astro-ph/0210279.
5th Alexander Friedmann Seminar on Gravitation and Cosmology. [Gomero:2002ki]
Inflation and the Theory of Cosmological Perturbations,
Antonio Riotto,
ICTP Lect.Notes Ser. 14 (2003) 317-413,arXiv:hep-ph/0210162.
'ICTP Summer School on Astroparticle Physics and Cosmology', Trieste, 17 June - 5 July 2002. [Riotto:2002yw]
Cosmological Implications of Neutrino Mass,
S. F. King,
arXiv:hep-ph/0210089, 2002.4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002. [King:2002js]
Phenomenological and Cosmological Implications of Neutrino Oscillations,
S. F. King,
J. Phys. G29 (2003) 1551,arXiv:hep-ph/0210081.
4th Workshop on Neutrino Factories based on Muon Storage Rings (NuFact'02), Imperial College, London, July 1-6, 2002. [King:2002jq]
Cosmic Distances: Current Odds and Future Perspectives,
G. Bono,
ASP Conf.Ser. (2002),arXiv:astro-ph/0210068.
To appear in 'Hubble's Science Legacy: Future Optical-Ultraviolet Astronomy from Space'. [Bono:2002ze]
Cosmological implications of neutrinos,
A. D. Dolgov,
Surveys High Energ. Phys. 17 (2002) 91,arXiv:hep-ph/0208222.
5th Moscow International School of Physics and 30th ITEP Winter School of Physics, Moscow, Russia, 20-28 Feb 2002. [Dolgov:2002ad]
From Precision Cosmology to Accurate Cosmology,
P. J. E. Peebles,
arXiv:astro-ph/0208037, 2002.Moriond Conference on the Cosmological Model, Les Arcs, March 2002. [Peebles:2002iq]
Astrophysical and Cosmological Neutrinos,
G. G. Raffelt,
Proc.Int.Sch.Phys.Fermi 152 (2003) 161-181,arXiv:hep-ph/0208024.
International School of Physics 'Enrico Fermi,' CLII Course 'Neutrino Physics,' 23 July-2 August 2002, Varenna, Lake Como, Italy. [Raffelt:2002nz]
A review of self-tuning solutions of cosmological constant,
Jihn E. Kim,
arXiv:hep-ph/0207360, 2002.'5th Int. UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe', Marina del Rey, CA, 20-22 Feb. 2002. [Kim:2002ps]
Neutrino masses in astroparticle physics,
G. G. Raffelt,
New Astron. Rev. 46 (2002) 699-708,arXiv:astro-ph/0207220.
Dennis Sciama Memorial Volume of NAR. [Raffelt:2002ed]
Stars and Fundamental Physics,
G. G. Raffelt,
arXiv:hep-ph/0207144, 2002.ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics (4-7 March 2002, Garching, Germany). [Raffelt:2002vg]
Cosmology Rounding the Cape,
Alessandro Melchiorri,
arXiv:astro-ph/0204262, 2002.4th Heidelberg International Conference on Dark Matter in Astro- and Particle Physics, Cape Town, South Africa (February 2002. Eds. H. Klapdor-Kleingrothaus and R. Viollier). [Melchiorri:2002yya]
CMB and Cosmological Parameters: Current Status and Prospects,
Alessandro Melchiorri,
PoS AHEP2003 (2003) AHEP2003/067,arXiv:astro-ph/0204017.
XIII Rencontres de Blois - Frontiers of the Universe, June 17-23, 2001. [Melchiorri:2002ne]
The Cosmological Constant,
U. Ellwanger,
arXiv:hep-ph/0203252, 2002.XIV Workshop 'Beyond the Standard Model', Bad Honnef, 11-14 March 2002. [Ellwanger:2002cd]
Big bang nucleosynthesis, implications of recent CMB data and supersymmetric dark matter,
K. A. Olive,
arXiv:astro-ph/0202486, 2002.1st NCTS Workshop on Astroparticle Physics, Taiwan, China, 6-9 Dec 2001. [Olive:2002qg]
Neutrino Masses in Astrophysics and Cosmology,
G. Raffelt, 2002.Lecture at the International School on Astroparticle and Neutrino Physics, 10-15 June 2002, Villa Cipressi, Varenna, Italy.http://wwwth.mppmu.mpg.de/members/raffelt/mytalks/varenna.pdf.
[Raffelt:Varenna02]
Cosmological parameters from CMB and LSS,
J. Peacock, 2002.4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002.http://www.shef.ac.uk/~phys/idm2002/talks/pdfs/peacock.pdf.
[Peacock-talk:2002a]
big bang nucleosynthesis and cosmological constraints on neutrino oscillation parameters,
Daniela Kirilova, Mihail Chizhov,
arXiv:astro-ph/0108341, 2001.BLTP Research Workshop on Hot Points in Astrophysics, Dubna, Russia, 22-26 Aug 2000. [Kirilova:2001rs]
Massive neutrinos in astrophysics,
G. G. Raffelt, W. Rodejohann,
arXiv:hep-ph/9912397, 1999.4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998. [Raffelt:1998qp]
Introduction to Microwave Background Polarization,
A. Kosowsky,
New Astron. Rev. 43 (1999) 157,arXiv:astro-ph/9904102.
International School of Space and Science: 1998 Course on 3K Cosmology from Space, L'Aquila, Italy, 2-12 Sep 1998. [Kosowsky:1998mb]
Big bang nucleosynthesis: Reprise,
Subir Sarkar,
arXiv:astro-ph/9903183, 1999.2nd International Conference on Dark Matter in Astro and Particle Physics (DARK98), Heidelberg, Germany, 20-25 Jul 1998. [Sarkar:1998gx]
Particle physics in the early universe,
Edward W. Kolb,
NATO Adv.Study Inst.Ser.C.Math.Phys.Sci. 534 (1999) 239-262,arXiv:hep-ph/9810362.
10th NATO ASI on Techniques and Concepts of High-Energy Physics, St. Croix, U.S. Virgin Islands, 18-29 June 1998. [Kolb:1998kj]
Possible relics from new physics in the early universe: Inflation, the cosmic microwave background, and particle dark matter,
Marc Kamionkowski,
arXiv:astro-ph/9809214, 1998.Workshop on The Early and Future Universe, Beijing, China, 22-27 June 1998. [Kamionkowski:1998is]
Calculations of cosmic background radiation anisotropies and implications,
Emory F. Bunn,
arXiv:astro-ph/9607088, 1996.1996 NATO Advanced Study Institute on 'The Cosmic Background Radiation'. [Bunn:1996qg]
Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background,
Girish Kumar Chakravarty, Gaetano Lambiase, Subhendra Mohanty,
Int.J.Mod.Phys. D26 (2017) 1730023,arXiv:1607.06325.
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A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND,
Stacy S. McGaugh,
Can.J. Phys. 93 (2015) 250-259,arXiv:1404.7525.
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The modified Newtonian dynamics-MOND-and its implications for new physics,
Jacob D. Bekenstein,
Contemp.Phys. (2007),arXiv:astro-ph/0701848.
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Observational Cosmology: caveats and open questions in the standard model,
M. Lopez-Corredoira,
Astron.Astrophys. (2003),arXiv:astro-ph/0310214.
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The MOND paradigm,
Mordehai Milgrom,
arXiv:0801.3133, 2008.XIX Rencontres de Blois 'Matter and energy in the Universe: from nucleosynthesis to cosmology', May 2007. [Milgrom:2008rv]
Introduction to Modified Gravity and Gravitational Alternative for Dark Energy,
S. Nojiri, S.D. Odintsov,
Int. J. Geom. Meth. Mod. Phys. 4 (2006) 115-146,arXiv:hep-th/0601213.
42 Karpacz Winter School on Theor Physics. [Nojiri:2006ri]
A systematic approach to generalisations of General Relativity and their cosmological implications,
Lavinia Heisenberg,
arXiv:1807.01725, 2018. [Heisenberg:2018vsk]
Euclidean wormholes, baby universes, and their impact on particle physics and cosmology,
Arthur Hebecker, Thomas Mikhail, Pablo Soler,
arXiv:1807.00824, 2018. [Hebecker:2018ofv]
Dynamical systems applied to cosmology: dark energy and modified gravity,
Sebastian Bahamonde et al.,
Phys.Rept. 775-777 (2018) 1-122,arXiv:1712.03107.
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Interactions relevant to the decoupling of the neutrini/antineutrini in the early Universe,
Evangelos Matsinos,
arXiv:1702.02872, 2017. [Matsinos:2017gqr]
Inhomogeneous cosmology and backreaction: current status and future prospects,
Krzysztof Bolejko, Mikolaj Korzynski,
Int.J.Mod.Phys. D26 (2017) 1730011,arXiv:1612.08222.
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Bouncing cosmologies with dark matter and dark energy,
Yi-Fu Cai, Antonino Marciano, Dong-Gang Wang, Edward Wilson-Ewing,
Universe 3 (2017) 1,arXiv:1610.00938.
[Cai:2016hea]
Topological Structure of the Vacuum, Cosmological Constant and Dark Energy,
B.G. Sidharth, A. Das, C.R. Das, L.V. Laperashvili, H.B. Nielsen,
Int.J.Mod.Phys. A31 (2016) 1630051,arXiv:1605.01169.
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Quantum cosmology from group field theory condensates: a review,
Steffen Gielen, Lorenzo Sindoni,
SIGMA 12 (2016) 082,arXiv:1602.08104.
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Dark Energy vs. Modified Gravity,
Austin Joyce, Lucas Lombriser, Fabian Schmidt,
Ann.Rev.Nucl.Part.Sci. 66 (2016) 95-122,arXiv:1601.06133.
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A Concise Introduction to Perturbation Theory in Cosmology,
Karim A. Malik, David R. Matravers,
Class. Quant. Grav. 25 (2008) 193001,arXiv:0804.3276.
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On the cosmological mass function theory,
A. Del Popolo,
Astron. Rep. 51 (2007) 709-734,arXiv:astro-ph/0609166.
Astronomy Reports, in print. [DelPopolo:2006gn]
Dynamics of dark energy,
Edmund J. Copeland, M. Sami, Shinji Tsujikawa,
Int. J. Mod. Phys. D15 (2006) 1753-1936,arXiv:hep-th/0603057.
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Phase transitions in the early and the present Universe,
D. Boyanovsky, H. J. de Vega, D. J. Schwarz,
Ann. Rev. Nucl. Part. Sci. 56 (2006) 441-500,arXiv:hep-ph/0602002.
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Insights into Dark Energy: Interplay Between Theory and Observation,
Rachel Bean, Sean Carroll, Mark Trodden,
arXiv:astro-ph/0510059, 2005. [Bean:2005ru]
Inflation Dynamics and Reheating,
Bruce A. Bassett, Shinji Tsujikawa, David Wands,
Rev. Mod. Phys. 78 (2006) 537-589,arXiv:astro-ph/0507632.
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Braneworld black holes in cosmology and astrophysics,
A. S. Majumdar, N. Mukherjee,
Int. J. Mod. Phys. D14 (2005) 1095,arXiv:astro-ph/0503473.
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Theoretical tools for the physics of CMB anisotropies,
Massimo Giovannini,
Int. J. Mod. Phys. D14 (2005) 363,arXiv:astro-ph/0412601.
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A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism,
Yen-Ting Lin, Benjamin D. Wandelt,
Astropart. Phys. 25 (2006) 151,arXiv:astro-ph/0409734.
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Expanding Confusion: common misconceptions of cosmological horizons and the superluminal expansion of the Universe,
T. M. Davis, C. H. Lineweaver,
Proc.Astron.Soc.Austral. (2003),arXiv:astro-ph/0310808.
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WMAPing the Universe: Supersymmetry, Dark Matter, Dark Energy, Proton Decay and Collider Physics,
A. B. Lahanas, N. E. Mavromatos, D. V. Nanopoulos,
Int. J. Mod. Phys. D12 (2003) 1529,arXiv:hep-ph/0308251.
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Standard Cosmology and Alternatives: A Critical Appraisal,
J. V. Narlikar, T. Padmanabhan,
Annual Review of Astronomy and Astrophysics 39 (2001) 211-248. [Narlikar-Padmanabhan-2001ARA&A-39-211N]
Particle physics models of inflation and the cosmological density perturbation,
David H. Lyth, Antonio Riotto,
Phys. Rep. 314 (1999) 1-146,arXiv:hep-ph/9807278.
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Electroweak baryon number non-conservation in the early universe and in high-energy collisions,
V. A. Rubakov, M. E. Shaposhnikov,
Usp. Fiz. Nauk 166 (1996) 493-537,arXiv:hep-ph/9603208.
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The Theory of Inflation,
Jerome Martin,
arXiv:1807.11075, 2018.International School of Physics Enrico Fermi, Villa Monastero, Varenna, Lake of Como (Italy), July 2017. [Martin:2018ycu]
On the problem of initial conditions for inflation,
Andrei Linde,
Found.Phys. 48 (2018) 1246-1260,arXiv:1710.04278.
Black Holes, Gravitational Waves and Spacetime Singularities, Specola Vaticana 9-12 May 2017. [Linde:2017pwt]
No-Scale Inflation,
John Ellis, Marcos A. G. Garcia, Dimitri V. Nanopoulos, Keith A. Olive,
Class.Quant.Grav. 33 (2016) 094001,arXiv:1507.02308.
[Ellis:2015xna]
Nonequilibrium Quantum Fields: From Cold Atoms to Cosmology,
J. Berges,
arXiv:1503.02907, 2015.Les Houches Summer School on 'Strongly interacting quantum systems out of equilibrium'. [Berges:2015kfa]
Cosmological constant and vacuum energy: old and new ideas,
Joan Sola,
J. Phys. Conf. Ser. 453 (2013) 012015,arXiv:1306.1527.
15th Conference on Recent Developments in Gravity (NEB 15): Chania, Crete, Greece, June 20-23, 2012. [Sola:2013gha]
From Quark-Gluon Universe to Neutrino Decoupling: $200 < T < 2$ MeV,
Michael J. Fromerth, Inga Kuznetsova, Lance Labun, Jean Letessier, Jan Rafelski,
Acta Phys. Polon. B43 (2012) 2261,arXiv:1211.4297.
52 Krakow School of Theoretical Physics: Astroparticle Physics in the LHC Era, Zakopane, May 19-27, 2012. [Fromerth:2012fe]
Early Universe: inflation and cosmological perturbations,
David Langlois,
arXiv:0811.4329, 2008.Geometry, Topology, QFT and Cosmology, Paris (28-30 May 2008). [Langlois:2008ng]
Quintessence: a mini-review,
Jerome Martin,
Mod. Phys. Lett. A23 (2008) 1252-1265,arXiv:0803.4076.
2007 International Symposium on Cosmology and Particle Astrophysics, November 13-15, Taipei, Taiwan. [Martin:2008qp]
Cosmological Inflation: A Personal Perspective,
Demosthenes Kazanas,
arXiv:0803.2080, 2008.Symposium 'Chaos in Astronomy 2007', Athens, Greece, September 2007. [Kazanas:2008jz]
Physics Beyond the Standard Model and Dark Matter,
Hitoshi Murayama,
arXiv:0704.2276, 2007.Les Houches Summer School, Session 86, Particle Physics and Cosmology: the Fabric of Spacetime, July 31- August 25, 2006. [Murayama:2007ek]
Introduction to leptogenesis,
Yosef Nir,
arXiv:hep-ph/0702199, 2007.6th Recontres du Vietnam, `Challenges in Particle Astrophysics,' Hanoi, Vietnam, August 6-12, 2006. [Nir:2007zq]
Dilaton cosmology and phenomenology,
M. Gasperini,
Lect. Notes Phys. 737 (2008) 787-844,arXiv:hep-th/0702166.
String theory and fundamental interactions: celebrating Gabriele Veneziano on his 65th birthday. [Gasperini:2007ar]
String Gas Cosmology and Structure Formation - A Brief Review,
Robert Brandenberger,
Mod. Phys. Lett. A22 (2007) 1875-1885,arXiv:hep-th/0702001.
CosPA 2006, Nov. 15 - 17, 2006, National Taiwan University, Taipei. [Brandenberger:2007zza]
Baryogenesis,
James M. Cline,
arXiv:hep-ph/0609145, 2006.Les Houches Summer School, Session 86: Particle Physics and Cosmology: the Fabric of Spacetime, 7-11 Aug. 2006. [Cline:2006ts]
Matter-Antimatter Asymmetry in the Universe and an Arrow for Time,
R. D. Peccei,
arXiv:hep-ph/0608226, 2006.World Summit on Physics Beyond the Standard Model, Galapagos Islands, Ecuador, June 22-25, 2006. [Peccei:2006hh]
Basics of inflationary cosmology,
George Lazarides,
J. Phys. Conf. Ser. 53 (2006) 528-550,arXiv:hep-ph/0607032.
Corfu Summer Institute on Elementary Particle Physics (CORFU2005), Corfu, Greece, 4-26 September 2005. [Lazarides:2006ep]
Particle Physics Approach to Dark Matter,
George Lazarides,
Lect. Notes PHys. 720 (2007) 3-34,arXiv:hep-ph/0601016.
Third Aegean Summer School 'The Invisible Universe: Dark Matter and Dark Energy', 26 September-1 October 2005, Karfas, Island of Chios, Greece. [Lazarides:2006jw]
CP violation in cosmology,
A.D. Dolgov,
arXiv:hep-ph/0511213, 2005.Varenna School 'CP Violation: From Quarks to Leptons', Varenna, Italy, July, 2005. [Dolgov:2005wf]
The Influence of Evolving Dark Energy on Cosmology,
Luke Barnes, Matthew J. Francis, Geraint F. Lewis, Eric V. Linder,
Publ.Astron.Soc.Austral. 22 (2005) 315,arXiv:astro-ph/0510791.
[Barnes:2005bn]
Cosmic strings: progress and problems,
Alexander Vilenkin,
arXiv:hep-th/0508135, 2005.'Inflating Horizons of Particle Astrophysics and Cosmology', honoring Katsuhiko Sato on his 60th birthday. [Vilenkin:2005jg]
Introduction to Dark Energy and Dark Matter,
Paul H. Frampton,
arXiv:astro-ph/0506676, 2005.40th Rencontre de Moriond, La Thuile, Italy. March 5-12, 2005. [Frampton:2005za]
From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation,
Norbert Straumann,
Annalen Phys. 15 (2006) 701-847,arXiv:hep-ph/0505249.
Physik-Combo, in Halle, Leipzig and Jena, winter semester 2004/5. [Straumann:2005mz]
A brief introduction to cosmic topology,
M.J. Reboucas,
Aip Conf. Proc. 782 (2005) 188,arXiv:astro-ph/0504365.
XIth Brazilian School of Cosmology and Gravitation. [Reboucas:2005ix]
Inflation and string cosmology,
Andrei Linde,
eConf C040802 (1990) L024,arXiv:hep-th/0503195.
SLAC Summer School 'Nature's Greatest Puzzles', Cosmo04 in Toronto, VI Mexican School on Gravitation, XXII Texas Symposium on Relativistic Astrophysics in 2004. [Linde:2005ht]
Dark Energy in the Universe, the Irreversibility of Time and Neutrinos,
N. E. Mavromatos,
Braz. J. Phys. 35 (2005) 284,arXiv:gr-qc/0411067.
DICE2004 international conference, Piombino (Italy), September 1-4 2004. [Mavromatos:2004gh]
Dark energy: A pedagogic review,
Paul H. Frampton,
arXiv:astro-ph/0409166, 2004.5th Rencontres du Vietnam on Particle Physics and Astrophysics: New Views in Particle Physics (Vietnam 2004), Hanoi, Vietnam, 5-11 Aug 2004. [Frampton:2004nh]
Modern Cosmology,
Juan Garcia-Bellido,
arXiv:hep-ph/0407111, 2004.XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004. [GarciaBellido:2004ri]
Supersymmetry and Cosmology,
Jonathan L. Feng,
eConf C0307282 (2003) L11,arXiv:hep-ph/0405215.
2003 SLAC Summer Institute: Cosmic Connections to Particle Physics. [Feng:2003zu]
Theory of Cosmic Microwave Background Polarization,
Paolo Cabella, Marc Kamionkowski,
arXiv:astro-ph/0403392, 2004.2003 Villa Mondragone School of Gravitation and Cosmology: 'The Polarization of the Cosmic Microwave Background,' Rome, Italy, September 6-11, 2003. [Cabella:2004mk]
Cosmological perturbation theory,
Ruth Durrer,
Lect. Notes Phys. 653 (2004) 31,arXiv:astro-ph/0402129.
Second Aegean Summerschool on the Early Universe. [Durrer:2004fx]
Alternative Dark Energy Models: An Overview,
J. A. S. Lima,
Braz. J. Phys. 34 (2004) 194,arXiv:astro-ph/0402109.
XXIII Brazilian National Meeting on Particles and Fields, Aguas de Lindoia, Sao Paulo, Brazil. [Lima:2004cq]
Prospects of Inflation,
Andrei Linde,
Phys. Scripta T117 (2005) 40,arXiv:hep-th/0402051.
Nobel Symposium 'Cosmology and String Theory,' August 2003. [Linde:2004kg]
A Briefing on the Ekpyrotic/Cyclic Universe,
Justin Khoury,
arXiv:astro-ph/0401579, 2004.Sixth RESCEU Symposium, Nov. 2003, Tokyo, Japan. [Khoury:2004xi]
Cosmological constant problem,
J. W. Moffat,
arXiv:gr-qc/0312115, 2003.Sixth Workshop on Quantum Field Theory under the Influence of External Conditions (QFEXT03), Norman, Oklahoma, 15-19 Sep 2003. [Moffat:2003az]
Early Cosmology and Fundamental Physics,
Hector De Vega,
arXiv:astro-ph/0307477, 2003.9th Chalonge School in Astrofundamental Physics, Palermo, September 2002. [DeVega:2003qm]
Inflation and Cosmological Perturbations,
A. H. Guth,
arXiv:astro-ph/0306275, 2003.Conference on the Future of Theoretical Physics and Cosmology in Honor of Steven Hawking's 60th Birthday, Cambridge, England, 7-10 Jan 2002. [Guth:2003rn]
Lectures on the Theory of Cosmological Perturbations,
Robert H. Brandenberger,
Lect. Notes Phys. 646 (2004) 127,arXiv:hep-th/0306071.
Vth Mexican School, November 2002, Playa del Carmen, Mexico. [Brandenberger:2003vk]
Baryogenesis and the New Cosmology,
Mark Trodden,
Pramana 62 (2004) 451,arXiv:hep-ph/0302151.
PASCOS-03, Mumbai, India; COSMO-02, Chicago; Aspen Winter 2003 Conference on Particle Physics: At the Frontiers of Particle Physics, Aspen Center for Physics. [Trodden:2003yn]
Time Since the Beginning,
Alan H. Guth,
ASP Conf.Ser. (2003),arXiv:astro-ph/0301199.
'Astrophysical Ages and Time Scales,' Hilo, Hawaii, 5-9 February 2001. [Guth:2003ev]
Inflationary cosmology: Theory and phenomenology,
Andrew R Liddle,
Class. Quant. Grav. 19 (2002) 3391-3402,arXiv:astro-ph/0109439.
Meeting on the Early Universe and Cosmological Observations: A Critical Review, Cape Town, South Africa, 23-25 Jul 2001. [Liddle:2001bk]
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Astron.Astrophys. 594 (2016) A9,arXiv:1502.05956.
[Adam:2015tpy]
Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold Clumps,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A28,arXiv:1502.01599.
[Ade:2015oya]
Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A27,arXiv:1502.01598.
[Ade:2015gva]
Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A24,arXiv:1502.01597.
[Ade:2015fva]
Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect,
N. Aghanim et al.(Planck),
Astron.Astrophys. 594 (2016) A22,arXiv:1502.01596.
[Aghanim:2015eva]
Planck 2015 results. XXI. The integrated Sachs-Wolfe effect,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A21,arXiv:1502.01595.
[Ade:2015dva]
Planck 2015 results. XIX. Constraints on primordial magnetic fields,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A19,arXiv:1502.01594.
[Ade:2015cva]
Planck 2015 results. XVIII. Background geometry & topology,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A18,arXiv:1502.01593.
[Ade:2015bva]
Planck 2015 results. XVII. Constraints on primordial non-Gaussianity,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A17,arXiv:1502.01592.
[Ade:2015ava]
Planck 2015 results. XIV. Dark energy and modified gravity,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A14,arXiv:1502.01590.
[Ade:2015rim]
Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps,
R. Adam et al.(Planck),
Astron.Astrophys. 594 (2016) A8,arXiv:1502.01587.
[Adam:2015vua]
Planck 2015 results. IV. Low Frequency Instrument beams and window functions,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A4,arXiv:1502.01584.
[Ade:2015tua]
Planck 2015 results. II. Low Frequency Instrument data processing,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 594 (2016) A2,arXiv:1502.01583.
[Ade:2015sua]
Planck 2015 results. I. Overview of products and scientific results,
R. Adam et al.(Planck),
Astron.Astrophys. 594 (2016) A1,arXiv:1502.01582.
[Adam:2015rua]
Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum,
P. A. R. Ade et al.(Planck),
Astron. Astrophys. 581 (2015) A14,arXiv:1502.00543.
[Ade:2015mva]
Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes,
R. Adam et al.(Planck),
Astron. Astrophys. 586 (2016) A133,arXiv:1409.5738.
[Adam:2014bub]
CFHTLenS: Cosmological constraints from a combination of cosmic shear two-point and three-point correlations,
Liping Fu, Martin Kilbinger, Thomas Erben, Catherine Heymans, Hendrik Hildebrandt et al.,
Mon.Not.Roy.Astron.Soc. 441 (2014) 2725-2743,arXiv:1404.5469.
[Fu:2014loa]
Detection of B-Mode Polarization at Degree Angular Scales by BICEP2,
P.A.R. Ade et al.(BICEP2),
Phys. Rev. Lett. 112 (2014) 241101,arXiv:1403.3985.
[Ade:2014xna]
Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?,
Vinicius C. Busti, Chris Clarkson, Marina Seikel,
Mon.Not.Roy.Astron.Soc. 441 (2014) 11,arXiv:1402.5429.
[Busti:2014dua]
The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$,
Holger Israel et al.,
Astron.Astrophys. 564 (2014) A129,arXiv:1402.3267.
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3D Cosmic Shear: Cosmology from CFHTLenS,
T.D. Kitching et al.(CFHTLenS),
Mon.Not.Roy.Astron.Soc. 442 (2014) 1326-1349,arXiv:1401.6842.
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Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-correlation with the Cosmic Infrared Background,
P.A.R. Ade et al.(POLARBEAR),
Phys. Rev. Lett. 112 (2014) 131302,arXiv:1312.6645.
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The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring growth rate and geometry with anisotropic clustering,
Lado Samushia et al.,
Mon.Not.Roy.Astron.Soc. 439 (2014) 3504-3519,arXiv:1312.4899.
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS and LOWZ anisotropic galaxy clustering,
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples,
Lauren Anderson et al.(BOSS),
Mon.Not.Roy.Astron.Soc. 441 (2014) 24-62,arXiv:1312.4877.
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples,
Ariel G. Sanchez et al.,
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The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors,
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles,
Florian Beutler et al.(BOSS),
Mon.Not.Roy.Astron.Soc. 443 (2014) 1065,arXiv:1312.4611.
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Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data,
D. Barkats et al.(BICEP1),
Astrophys.J. 783 (2014) 67,arXiv:1310.1422.
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Precision measures of the primordial abundance of deuterium,
Ryan Cooke, Max Pettini, Regina A. Jorgenson, Michael T. Murphy, Charles C. Steidel,
Astrophys. J. 781 (2014) 31,arXiv:1308.3240.
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Planck intermediate results. XIII. Constraints on peculiar velocities,
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Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. (2013),arXiv:1303.5089.
[Ade:2013skr]
Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A28,arXiv:1303.5088.
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Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove,
N. Aghanim et al.(Planck),
Astron.Astrophys. 571 (2014) A27,arXiv:1303.5087.
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Planck 2013 results. XXVI. Background geometry and topology of the Universe,
P. A. R. Ade et al.(Planck),
Grav.Cosmol. 20 (2014) 15-20,arXiv:1303.5086.
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Planck 2013 results. XXV. Searches for cosmic strings and other topological defects,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A25,arXiv:1303.5085.
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Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A24,arXiv:1303.5084.
[Ade:2013ydc]
Planck 2013 results. XXIII. Isotropy and Statistics of the CMB,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A23,arXiv:1303.5083.
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Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A20,arXiv:1303.5080.
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Planck 2013 results. XIX. The integrated Sachs-Wolfe effect,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A19,arXiv:1303.5079.
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Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A18,arXiv:1303.5078.
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Planck 2013 results. XVII. Gravitational lensing by large-scale structure,
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Astron.Astrophys. 571 (2014) A17,arXiv:1303.5077.
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Planck 2013 results X. Energetic particle effects: characterization, removal, and simulation,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A10,arXiv:1303.5071.
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Planck 2013 results. VIII. HFI photometric calibration and mapmaking,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A8,arXiv:1303.5069.
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Planck 2013 results. VI. High Frequency Instrument data processing,
P. A. R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A6,arXiv:1303.5067.
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Planck 2013 results. IV. Low Frequency Instrument beams and window functions,
N. Aghanim et al.(Planck),
Astron.Astrophys. 571 (2014) A4,arXiv:1303.5065.
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Planck 2013 results. II. The Low Frequency Instrument data processing,
N. Aghanim et al.(Planck),
Astron.Astrophys. 571 (2014) A2,arXiv:1303.5063.
[Aghanim:2013ysa]
Planck 2013 results. I. Overview of products and scientific results,
P.A.R. Ade et al.(Planck),
Astron.Astrophys. 571 (2014) A1,arXiv:1303.5062.
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The Atacama Cosmology Telescope: temperature and gravitational lensing power spectrum measurements from three seasons of data,
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The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data,
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JCAP 1310 (2013) 060,arXiv:1301.0824.
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The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data,
Matthew Hasselfield et al.,
JCAP 1307 (2013) 008,arXiv:1301.0816.
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The Atacama Cosmology Telescope: likelihood for small-scale CMB data,
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JCAP 1307 (2013) 025,arXiv:1301.0776.
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Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500-square degree SPT-SZ Survey,
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CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing,
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Monthly Notices of the Royal Astronomical Society 430 (2013) 2200-2220,arXiv:1212.3338.
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample,
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A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey,
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The WiggleZ Dark Energy Survey: Final data release and cosmological results,
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CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey,
Catherine Heymans, Ludovic Van Waerbeke, Lance Miller, Thomas Erben, Hendrik Hildebrandt et al.,
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Two accurate time-delay distances from strong lensing: Implications for cosmology,
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The luminosity of supernovae of type Ia from TRGB distances and the value of $H_0$,
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Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant,
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The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789,
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The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey,
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The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey,
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Competitive Crossing Check for a 3% Determination of the Hubble Constant,
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A new, precise measurement of the primordial abundance of Deuterium,
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Mon.Not.Roy.Astron.Soc. 425 (2012) 2477-2486,arXiv:1205.3785.
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering,
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function,
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample,
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies,
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Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies,
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A measurement of gravitational lensing of the microwave background using South Pole Telescope data,
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Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications,
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The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies,
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Cepheid Period-Luminosity Relations in the Near-Infrared and the Distance to M31 from the Hubble Space Telescope Wide Field Camera 3,
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The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations,
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The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant,
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The Atacama Cosmology Telescope: a measurement of the primordial power spectrum,
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A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3,
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Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy,
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The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey,
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A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey,
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Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey,
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Are There Cosmic Microwave Background Anomalies?,
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The primordial abundance of 4He: evidence for non-standard big bang nucleosynthesis,
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Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample,
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Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies,
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Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant,
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A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder,
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The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures,
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The Seventh Data Release of the Sloan Digital Sky Survey,
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Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?,
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results,
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation,
E. Komatsu et al.(WMAP),
Astrophys. J. Suppl. 180 (2009) 330-376,arXiv:0803.0547. From the abstract:The WMAP 5-year data provide stringent limits on deviations from the minimal, 6-parameter $\Lambda\text{CDM}$ model.... We detect no convincing deviations from the minimal model.... $\Omega_\Lambda = 0.721\pm 0.015$,..., $H_0 = 70.1\pm 1.3 \, \text{km} \, \text{s}^{-1} \, \text{Mpc}^{-1}$, $\Omega_b = 0.0462\pm 0.0015$, $\Omega_c = 0.233\pm 0.013$,... We obtain tight, simultaneous limits on the (constant) equation of state of dark energy and the spatial curvature of the universe: $-0.11<1+w<0.14\, \text{(95\% CL)}$ and $-0.0175<\Omega_k<0.0085\, \text{(95\% CL)}$.... We find the limit on the total mass of massive neutrinos of $\sum m_\nu < 0.61 \, \text{eV}\, \text{(95\% CL)}$, which is free from the uncertainty in the normalization of the large-scale structure data. The number of relativistic degrees of freedom, expressed in units of the effective number of neutrino species, is constrained as $N_{\rm eff} = 4.4\pm 1.5$ (68\%), consistent with the standard value of 3.04. [Komatsu:2008hk]
High resolution CMB power spectrum from the complete ACBAR data set,
C.L. Reichardt, P.A.R. Ade, J.J. Bock, J. Richard Bond, J.A. Brevik et al.,
Astrophys.J. 694 (2009) 1200-1219,arXiv:0801.1491.
[Reichardt:2008ay]
The Sixth Data Release of the Sloan Digital Sky Survey,
Jennifer K. Adelman-McCarthy et al.(SDSS),
Astrophys.J.Suppl. 175 (2008) 297-313,arXiv:0707.3413.
[AdelmanMcCarthy:2007aa]
The Fifth Data Release of the Sloan Digital Sky Survey,
Jennifer K. Adelman-McCarthy(SDSS),
Astrophys. J. Suppl. 172 (2007) 634-644,arXiv:0707.3380.
[AdelmanMcCarthy:2007wh]
COSMOS: 3D weak lensing and the growth of structure,
Richard Massey et al.,
Astrophys. J. Suppl. 172 (2007) 239-253,arXiv:astro-ph/0701480.
[Massey:2007gh]
The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1,
Alison L. Coil et al.,
Astrophys. J. 654 (2006) 115-124,arXiv:astro-ph/0607454.
[Coil:2006ji]
The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33,
Alceste Z. Bonanos et al.,
Astrophys. J. 652 (2006) 313,arXiv:astro-ph/0606279. From the article:... our LMC distance would imply a 15\% decrease in the Hubble constant to $ H_{0} = 61\; \rm km\;s^{-1}\; Mpc^{-1} $. [Bonanos:2006jd]
A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo,
Kim Nilsson et al.,
Astron. Astrophys. 452 (2006) L23-L26,arXiv:astro-ph/0512396.
[Nilsson:2005rk]
First cosmic shear results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey,
H. Hoekstra et al.,
Astrophys. J. 647 (2006) 116-127,arXiv:astro-ph/0511089. From the abstract:Assuming a Cold Dark Matter model and marginalising over the Hubble parameter $h\in[0.6,0.8]$, the source redshift distribution and systematics, we constrain $\sigma_8$, the amplitude of the matter power spectrum. At a fiducial matter density $\Omega_m=0.3$ we find $\sigma_8=0.85\pm0.06$. This estimate is in excellent agreement with previous studies. Combination of our results with those from the Deep component of the CFHTLS enables us to place a constraint on a constant equation of state for the dark energy, based on cosmic shear data alone. We find that $w_0<-0.8$ at 68\% confidence. [Hoekstra:2005cs]
The DEEP2 Galaxy Redshift Survey: Discovery of Luminous, Metal-poor, Sta r-forming Galaxies at Redshifts z~0.7,
Carlos Hoyos et al.,
Astrophys. J. 635 (2005) L21,arXiv:astro-ph/0510843.
[Hoyos:2005hc]
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set,
P. Astier et al.(SNLS),
Astron. Astrophys. 447 (2006) 31,arXiv:astro-ph/0510447. From the abstract:With this data set, we have built a Hubble diagram extending to $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$ model; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations. [Astier:2005qq]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications,
A. Clocchiatti et al.(High Z SN Search),
Astrophys. J. 642 (2006) 1-21,arXiv:astro-ph/0510155.
[Clocchiatti:2005vy]
GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang,
G. Tagliaferri et al.,
Astron. Astrophys. 443 (2005) L1-L5,arXiv:astro-ph/0509766.
[Tagliaferri:2005cw]
The Fourth Data Release of the Sloan Digital Sky Survey,
J.K. Adelman-McCarthy et al.(SDSS),
Astrophys. J. Suppl. 162 (2006) 38,arXiv:astro-ph/0507711.
[AdelmanMcCarthy:2005se]
A Measurement of the CMB < EE > Spectrum from the 2003 Flight of BOOMERANG,
T.E. Montroy et al.,
Astrophys. J. 647 (2006) 813,arXiv:astro-ph/0507514.
[Montroy:2005yx]
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG,
S Masi et al.,
Astron.Astrophys. 458 (2006) 687,arXiv:astro-ph/0507509.
[Masi:2005ys]
A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave Background from the 2003 flight of BOOMERANG,
F Piacentini et al.,
Astrophys. J. 647 (2006) 833,arXiv:astro-ph/0507507.
[Piacentini:2005yq]
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of Boomerang,
W. C. Jones et al.,
Astrophys. J. 647 (2006) 823,arXiv:astro-ph/0507494.
[Jones:2005yb]
Keck Deep Fields. I. Observations, Reductions, and the Selection of Faint Star-Forming Galaxies at Redshifts z~4, 3, and 2,
Marcin Sawicki, David Thompson,
Astrophys. J. 635 (2005) 100,arXiv:astro-ph/0507424.
[Sawicki:2005qk]
First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization,
Chris J. Willott et al.,
Astrophys. J. 633 (2005) 630,arXiv:astro-ph/0507183.
[Willott:2005zr]
Second Data Release of the 6dF Galaxy Survey,
D. Heath Jones, Will Saunders, Mike Read, Matthew Colless,
Publ.Astron.Soc.Austral. (2005),arXiv:astro-ph/0505068.
[Jones:2005ya]
Detection of Cosmic Magnification with the Sloan Digital Sky Survey,
Ryan Scranton et al.(SDSS),
Astrophys. J. 633 (2005) 589,arXiv:astro-ph/0504510.
SDSS News Release. [Scranton:2005ci]
The 2dF QSO Redshift Survey - XV. Correlation analysis of redshift-Space distortions,
J. da Angela et al.,
Mon. Not. Roy. Astron. Soc. 360 (2005) 1040-1054,arXiv:astro-ph/0504438. From the abstract:$ \Omega_{\text{M}} = 0.35 {}^{+0.19}_{-0.13} $. [daAngela:2005id]
The H I opacity of the intergalactic medium at redshifts 1.6 < z < 3.2,
David Kirkman et al.,
Mon. Not. Roy. Astron. Soc. 360 (2005) 1373,arXiv:astro-ph/0504391.
[Kirkman:2005jz]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$,
Serena Nobili et al.(Supernova Cosmology Project),
Astron.Astrophys. (2005),arXiv:astro-ph/0504139.
[Nobili:2005tr]
The Sloan Digital Sky Survey Quasar Catalog III. Third Data Release,
D. P. Schneider et al.(The SDSS),
Astron. J. 130 (2005) 367-380,arXiv:astro-ph/0503679.
[Schneider:2005vy]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant,
Adam G. Riess et al.,
Astrophys. J. 627 (2005) 579,arXiv:astro-ph/0503159. From the abstract:$H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$. [Riess:2005zi]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey,
Louis-Gregory Strolger, Adam G. Riess,
Astron. J. 131 (2006) 1629-1638,arXiv:astro-ph/0503093.
[Strolger:2005uk]
The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications,
S. Cole et al.(The 2dFGRS),
Mon. Not. Roy. Astron. Soc. 362 (2005) 505,arXiv:astro-ph/0501174. From the abstract:Fitting to a CDM model, assuming a primordial $n_{\text{s}}=1$ spectrum, $h=0.72$ and negligible neutrino mass, the preferred parameters are $\Omega_{\text{m}} h = 0.168 \pm 0.016$ and a baryon fraction $\Omega_{\text{b}} /\Omega_{\text{m}} = 0.185\pm0.046$ (1$\sigma$ errors).... This analysis therefore implies a density significantly below the standard $\Omega_{\text{m}} =0.3$: in combination with CMB data from WMAP, we infer $\Omega_{\text{m}} =0.231\pm 0.021$. From the article:$\Omega_{\text{m}} = 0.231 \pm 0.021$, $\Omega_{\text{b}} = 0.042 \pm 0.002$, $h = 0.766 \pm 0.032$, $n_{\text{s}} = 1.027 \pm 0.050$. [Cole:2005sx]
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies,
Daniel J. Eisenstein et al.(SDSS),
Astrophys. J. 633 (2005) 560,arXiv:astro-ph/0501171. From the abstract:We find a well-detected peak in the correlation function at $100 \, h^{-1} \, \text{Mpc} $ separation that is an excellent match to the predicted shape and location of the imprint of the recombination-epoch acoustic oscillations on the low-redshift clustering of matter. This detection demonstrates the linear growth of structure by gravitational instability between $z\approx 1000$ and the present and confirms a firm prediction of the standard cosmological theory. The acoustic peak provides a standard ruler by which we can measure the ratio of the distances to $z=0.35$ and $z=1089$ to 4\% fractional accuracy and the absolute distance to $z=0.35$ to 5\% accuracy. From the overall shape of the correlation function, we measure the matter density $\Omega_mh^2$ to 8\% and find agreement with the value from cosmic microwave background (CMB) anisotropies. Independent of the constraints provided by the CMB acoustic scale, we find $\Omega_m=0.273\pm0.025+0.123(1+w_0)+0.137\Omega_K$. Including the CMB acoustic scale, we find that the spatial curvature is $\Omega_K=-0.010\pm0.009$ if the dark energy is a cosmological constant. [Eisenstein:2005su]
Weak lensing measurements of dark matter halos of galaxies from COMBO-17,
M. Kleinheinrich et al.,
Astron.Astrophys. (2004),arXiv:astro-ph/0412615.
[Kleinheinrich:2004vs]
The CMB temperature power spectrum from an improved analysis of the Archeops data,
Matthieu Tristram et al.,
Astron. Astrophys. 436 (2005) 785-797,arXiv:astro-ph/0411633.
[Tristram:2004ke]
The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2,
Lih-Wai Lin et al.,
Astrophys. J. 617 (2004) L9-L12,arXiv:astro-ph/0411104.
[Lin:2004kb]
The DEEP2 Galaxy Redshift Survey: First results on galaxy groups,
Brian F. Gerke et al.,
Astrophys. J. 625 (2005) 6,arXiv:astro-ph/0410721.
[Gerke:2004ra]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT,
C. Lidman et al.(Supernova Cosmology Project),
Astron.Astrophys. (2004),arXiv:astro-ph/0410506.
[Lidman:2004en]
The Third Data Release of the Sloan Digital Sky Survey,
K. Abazajian et al.(SDSS),
Astron. J. 129 (2005) 1755,arXiv:astro-ph/0410239.
[Abazajian:2004it]
The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z~1,
Charlie Conroy et al.,
Astrophys. J. 635 (2005) 982,arXiv:astro-ph/0409305.
[Conroy:2004tz]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models,
L. G. Strolger et al.,
Astrophys. J. 613 (2004) 200-223,arXiv:astro-ph/0406546.
[Strolger:2004kk]
The 2dF Galaxy Redshift Survey: Spherical Harmonics analysis of fluctuations in the final catalogue,
Will J. Percival et al.(The 2dFGRS),
Mon. Not. Roy. Astron. Soc. 353 (2004) 1201,arXiv:astro-ph/0406513.
[Percival:2004fs]
The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey,
Patrick McDonald et al.(SDSS),
Astrophys. J. Suppl. 163 (2006) 80,arXiv:astro-ph/0405013.
[McDonald:2004eu]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa,
Gabriele Garavini et al.(The Supernova Cosmology Project),
Mon. Not. Roy. Astron. Soc. 356 (2004) 456,arXiv:astro-ph/0404393.
[Garavini:2004fa]
The Second Data Release of the Sloan Digital Sky Survey,
K. Abazajian et al.(SDSS),
Astron. J. 128 (2004) 502,arXiv:astro-ph/0403325.
[Abazajian:2004aja]
Design and Calibration of a Cryogenic Blackbody Calibrator at Centimeter Wavelengths,
A. Kogut et al.(ARCADE),
Rev. Sci. Instrum. 75 (2004) 5079,arXiv:astro-ph/0402580.
[Kogut:2004hq]
An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths,
A. Kogut et al.(ARCADE),
Astrophys.J. (2004),arXiv:astro-ph/0402578.
[Kogut:2004hn]
Type Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 607 (2004) 665,arXiv:astro-ph/0402512. From the abstract:We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. ... A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99\% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at $z=0.46 \pm 0.13$. The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat Universe with a cosmological constant, we measure $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$. ... Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy. [Ivanov:2004qa]
High sensitivity measurements of the CMB power spectrum with the extended Very Small Array,
Clive Dickinson et al.,
Mon. Not. Roy. Astron. Soc. 353 (2004) 732,arXiv:astro-ph/0402498.
[Dickinson:2004yr]
Extended Mosaic Observations with the Cosmic Background Imager,
A. C. S. Readhead et al.,
Astrophys. J. 609 (2004) 498-512,arXiv:astro-ph/0402359.
[Readhead:2004gy]
The 2dF Galaxy Redshift Survey: Higher order galaxy correlation functions,
D. J. Croton et al.(2dFGRS Team),
Mon. Not. Roy. Astron. Soc. 352 (2004) 1232,arXiv:astro-ph/0401434.
[Croton:2004hy]
The Millennium Galaxy Catalogue: The photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR and DR1 datasets,
N. J. G. Cross et al.,
Mon. Not. Roy. Astron. Soc. 349 (2004) 576,arXiv:astro-ph/0312317.
[Cross:2003es]
The 2dF QSO Redshift Survey - XIII. A Measurement of Lambda from the QSO Power Spectrum,
P.J. Outram et al.,
Mon. Not. Roy. Astron. Soc. 348 (2004) 745,arXiv:astro-ph/0310873. From the abstract:Assuming a flat ($\Omega_{\rm m}+\Omega_{\Lambda}=1$) cosmology and a $\Lambda$ cosmology $r(z)$ function to convert from redshift into comoving distance, we find best fit values of $\Omega_{\Lambda}=0.71^{+0.09}_{-0.17}$ and $\beta_q(z\sim1.4)=0.45^{+0.09}_{-0.11}$. [Outram:2003ew]
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$,
Brian J. Barris et al.,
Astrophys. J. 602 (2004) 571,arXiv:astro-ph/0310843. From the abstract:This sample of 23 high-redshift supernovae includes 15 at $z\geq0.7$, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB [27-239]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation. [Barris:2003dq]
Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies,
Y. I. Izotov, T. X. Thuan,
Astrophys. J. 602 (2004) 200-230,arXiv:astro-ph/0310421.
[Izotov:2003xn]
New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST,
Robert A. Knop et al.(The Supernova Cosmology Project),
Astrophys. J. 598 (2003) 102,arXiv:astro-ph/0309368. From the abstract:We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$. [Knop:2003iy]
An update on Archeops: flights and data products,
J. Delabrouille, Ph. Filliatre(Archeops),
Astrophys. Space Sci. 290 (2004) 119,arXiv:astro-ph/0307550.
[Delabrouille:2003mr]
Measuring CMB Polarization with BOOMERANG,
T. Montroy et al.,
New Astron. Rev. 47 (2003) 1057-1065,arXiv:astro-ph/0305593.
'The Cosmic Microwave Background and its Polarization', New Astronomy Reviews. [Montroy:2003ii]
The DEEP2 Redshift Survey: Spectral classification of galaxies at z~1,
D. S Madgwick et al.(The DEEP2 Survey),
Astrophys. J. 599 (2003) 997-1005,arXiv:astro-ph/0305587.
[Madgwick:2003cg]
The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data,
Alison L. Coil et al.(The DEEP2 Survey),
Astrophys. J. 609 (2004) 525,arXiv:astro-ph/0305586.
[Coil:2003cf]
First Results from the Arcminute Cosmology Bolometer Array Receiver,
M. C. Runyan et al.,
New Astron.Rev. (2003),arXiv:astro-ph/0305553.
[Runyan:2003aw]
The First Data Release of the Sloan Digital Sky Survey,
Kevork Abazajian et al.(SDSS),
Astron. J. 126 (2003) 2081,arXiv:astro-ph/0305492.
[Abazajian:2003jy]
The XMM-LSS Survey II. First high redshift galaxy clusters: relaxed and collapsing systems,
I. Valtchanov et al.,
Astron. Astrophys. 423 (2004) 75,arXiv:astro-ph/0305192.
[Valtchanov:2003it]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources,
M. R. Nolta et al.(WMAP),
Astrophys. J. 608 (2004) 10,arXiv:astro-ph/0305097.
[Nolta:2003uy]
Cosmological Results from High-z Supernovae,
John L. Tonry et al.(Supernova Search Team),
Astrophys. J. 594 (2003) 1,arXiv:astro-ph/0305008. From the abstract:The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence. [Tonry:2003zg]
The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type,
D. S. Madgwick et al.,
Mon. Not. Roy. Astron. Soc. 344 (2003) 847,arXiv:astro-ph/0303668.
[Madgwick:2003bd]
The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation,
Andrea Grazian et al.,
Astron. J. 127 (2004) 592,arXiv:astro-ph/0303382.
[Grazian:2003cx]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation,
H. V. Peiris et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 213,arXiv:astro-ph/0302225.
[Peiris:2003ff]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization,
N. Jarosik et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 29,arXiv:astro-ph/0302224.
[Jarosik:2003fe]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity,
E. Komatsu et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 119,arXiv:astro-ph/0302223.
[Komatsu:2003fd]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits,
G. Hinshaw et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 63,arXiv:astro-ph/0302222.
[Hinshaw:2003fc]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks,
L. Page et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 233,arXiv:astro-ph/0302220.
[Page:2003fa]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology,
L. Verde et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 195,arXiv:astro-ph/0302218.
[Verde:2003ey]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum,
G. Hinshaw et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 135,arXiv:astro-ph/0302217.
[Hinshaw:2003ex]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup,
C. Barnes et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 51,arXiv:astro-ph/0302215.
[Barnes:2003ev]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions,
L. Page et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 39,arXiv:astro-ph/0302214.
[Page:2003eu]
Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization,
A. Kogut et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 161,arXiv:astro-ph/0302213.
[Kogut:2003et]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission,
C. Bennett et al.(WMAP),
Astrophys. J. Suppl. 148 (2003) 97,arXiv:astro-ph/0302208.
[Bennett:2003ca]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results,
C. L. Bennett et al.(WMAP),
Astrophys. J. Supp. Ser. 148 (2003) 1-27,arXiv:astro-ph/0302207. From the abstract:A best-fit cosmological model to the CMB and other measures of large scale structure works remarkably well with only a few parameters. The age of the best-fit universe is $t_0 = 13.7 \pm 0.2 \text{ Gyr}$ old. Decoupling was $t_{dec} = 379^{+ 8}_{- 7} \text{ kyr}$ after the Big Bang at a redshift of $z_{dec} = 1089 \pm 1$. The thickness of the decoupling surface was $\Delta z_{dec} = 195 \pm 2$. The matter density of the universe is $\Omega_mh^2 = 0.135^{+ 0.008}_{- 0.009}$, the baryon density is $\Omega_bh^2 = 0.0224 \pm 0.0009$, and the total mass-energy of the universe is $\Omega_{tot} = 1.02 \pm 0.02$.... This flat universe model is composed of 4.4% baryons, 22% dark matter and 73% dark energy.... Inflation theory is supported with $n_s\approx 1$, $\Omega_{tot}\approx 1$, Gaussian random phases of the CMB anisotropy, and superhorizon fluctuations implied by the TE anticorrelations at decoupling. [Bennett:2003bz]
The size distribution of galaxies in the Sloan Digital Sky Survey,
Shiyin Shen et al.,
Mon. Not. Roy. Astron. Soc. 343 (2003) 978,arXiv:astro-ph/0301527.
[Shen:2003sda]
The CMB power spectrum out to l=1400 measured by the VSA,
Keith Grainge et al.,
Mon. Not. Roy. Astron. Soc. 341 (2003) L23,arXiv:astro-ph/0212495.
[Grainge:2002da]
High Resolution Observations of the CMB Power Spectrum with ACBAR,
C.L. Kuo et al.(ACBAR),
Astrophys. J. 600 (2004) 32,arXiv:astro-ph/0212289.
[Kuo:2002ua]
Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations,
J. E. Ruhl et al.,
Astrophys. J. 599 (2003) 786,arXiv:astro-ph/0212229.
[Ruhl:2002cz]
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops,
A. Benoit et al.(Archeops),
Astron. Astrophys. 399 (2003) L19-L23,arXiv:astro-ph/0210305.
[Benoit:2002mk]
Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey Radio-Selected Gravitational Lens Statistics,
K. H. Chae et al.(CLASS),
Phys. Rev. Lett. 89 (2002) 151301,arXiv:astro-ph/0209602.
[Chae:2002mb]
Detection of Polarization in the Cosmic Microwave Background using DASI,
J. Kovac, E. M. Leitch, C. Pryke J. E. Carlstrom, N. W. Halverson W. L. Holzapfel,
Nature 420 (2002) 772,arXiv:astro-ph/0209478.
[Kovac:2002fg]
The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager,
T. J. Pearson et al.(CBI),
Astrophys. J. 591 (2003) 556,arXiv:astro-ph/0205388.
[Pearson:2002tr]
Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA,
J. L. Sievers et al.(CBI),
Astrophys. J. 591 (2003) 599,arXiv:astro-ph/0205387.
[Sievers:2002tq]
The Sunyaev-Zeldovich effect in CMB-calibrated theories applied to the Cosmic Background Imager anisotropy power at l > 2000,
J. R. Bond et al.(CBI),
Astrophys. J. 626 (2005) 12,arXiv:astro-ph/0205386.
[Bond:2002tp]
A Fast Gridded Method for the Estimation of the Power Spectrum of the CMB from Interferometer Data with Application to the Cosmic Background Imager,
S. T. Myers et al.(CBI),
Astrophys. J. 591 (2003) 575,arXiv:astro-ph/0205385.
[Myers:2002tn]
The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager,
B. S. Mason et al.(CBI),
Astrophys. J. 591 (2003) 540,arXiv:astro-ph/0205384.
[Mason:2002tm]
First results from the Very Small Array - II. Observations of the CMB,
Angela C. Taylor et al.,
Mon. Not. Roy. Astron. Soc. 341 (2003) 1066,arXiv:astro-ph/0205381.
[Taylor:2002ti]
The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe,
Licia Verde et al.(2dF team),
Mon. Not. Roy. Astron. Soc. 335 (2002) 432,arXiv:astro-ph/0112161.
[Verde:2001sf]
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data,
Scott Dodelson et al.(SDSS),
Astrophys. J. 572 (2001) 140-156,arXiv:astro-ph/0107421.
[Dodelson:2001ux]
Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology,
P. de Bernardis et al.(BOOMERANG),
Astrophys. J. 564 (2002) 559-566,arXiv:astro-ph/0105296.
[deBernardis:2001xk]
The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,
Will J. Percival et al.(The 2dFGRS),
Mon. Not. Roy. Astron. Soc. 327 (2001) 1297,arXiv:astro-ph/0105252.
[Percival:2001hw]
Cosmological Parameter Extraction from the First Season of Observations with DASI,
C. Pryke et al.,
Astrophys. J. 568 (2002) 46-51,arXiv:astro-ph/0104490.
[Pryke:2001yz]
DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum,
N. W. Halverson et al.,
Astrophys. J. 568 (2002) 38-45,arXiv:astro-ph/0104489.
[Halverson:2001yy]
A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data,
A. T. Lee et al.,
Astrophys. J. 561 (2001) L1-L6,arXiv:astro-ph/0104459.
[Lee:2001yp]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 560 (2001) 49-71,arXiv:astro-ph/0104455.
[Riess:2001gk]
A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey,
J. A. Peacock et al.,
Nature 410 (2001) 169-173,arXiv:astro-ph/0103143.
[Peacock:2001gs]
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant,
W. L. Freedman et al.(HST),
Astrophys. J. 553 (2001) 47-72,arXiv:astro-ph/0012376.
[Freedman:2000cf]
Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4,
Rupert A. C. Croft et al.,
Astrophys. J. 581 (2002) 20-52,arXiv:astro-ph/0012324.
[Croft:2000hs]
A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method,
Patrick McDonald et al.,
Astrophys. J. 562 (2001) 52-75,arXiv:astro-ph/0005553.
[McDonald:2000nn]
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation,
P. de Bernardis et al.(Boomerang),
Nature 404 (2000) 955-959,arXiv:astro-ph/0004404.
[deBernardis:2000gy]
The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest,
Patrick McDonald et al.,
Astrophys. J. 543 (2000) 1-23,arXiv:astro-ph/9911196.
[McDonald:1999dt]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter et al.(Supernova Cosmology Project),
Astrophys. J. 517 (1999) 565-586,arXiv:astro-ph/9812133. From the abstract:The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology. [Perlmutter:1998np]
Calibrator Design for the COBE Far Infrared Absolute Spectrophotometer (FIRAS),
J. C. Mather, D. J. Fixsen, R. A. Shafer, C. Mosier, D. T. Wilkinson,
Astrophys. J. 512 (1999) 511-520,