SDSS

(Sloan Digital Sky Survey)

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References

1 - Reviews

[1-1]
Clusters of Galaxies in the SDSS, Robert C. Nichol, arXiv:astro-ph/0305041, 2003.
[Nichol:2003ih]
[1-2]
The Sloan Digital Sky Survey, Jon Loveday (SDSS), Contemp. Phys. 43 (2002) 437-449, arXiv:astro-ph/0207189.
[Loveday:2002ax]

2 - Articles

[2-1]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Shadab Alam et al., Mon.Not.Roy.Astron.Soc. 470 (2017) 2617-2652, arXiv:1607.03155.
[Alam:2016hwk]
[2-2]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space, Yuting Wang et al., arXiv:1607.03154, 2016.
[Wang:2016wjr]
[2-3]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space, Gong-Bo Zhao et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 762-779, arXiv:1607.03153.
[Zhao:2016das]
[2-4]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: double-probe measurements from BOSS galaxy clustering \& Planck data - towards an analysis without informative priors, Marcos Pellejero-Ibanez et al., Mon.Not.Roy.Astron.Soc. 468 (2017) 4116-4133, arXiv:1607.03152.
[Pellejero-Ibanez:2016ypj]
[2-5]
The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model, Chia-Hsun Chuang et al., arXiv:1607.03151, 2016.
[Chuang:2016uuz]
[2-6]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space, Florian Beutler et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 2242-2260, arXiv:1607.03150.
[Beutler:2016arn]
[2-7]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space, Florian Beutler et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 3409-3430-3430, arXiv:1607.03149.
[Beutler:2016ixs]
[2-8]
BOSS DR12 combined galaxy sample: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions, Siddharth Satpathy et al., arXiv:1607.03148, 2016.
[Satpathy:2016tct]
[2-9]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges, Ariel G. Sanchez et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1640-1658, arXiv:1607.03147.
[Sanchez:2016sas]
[2-10]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions, Ariel G. Sanchez et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1493-1501, arXiv:1607.03146.
[Sanchez:2016gky]
[2-11]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function, Ashley J. Ross et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1168-1191, arXiv:1607.03145.
[Ross:2016gvb]
[2-12]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications, Salvador Salazar-Albornoz et al., arXiv:1607.03144, 2016.
[Salazar-Albornoz:2016psd]
[2-13]
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample, Jan Niklas Grieb et al., Mon.Not.Roy.Astron.Soc. 467 (2017) 2085, arXiv:1607.03143. 24 pages, 16 figures in the main text, appendix of 6 pages and 5 figures; submitted to MNRAS. The data used in this analysis will be made publicly available (final URL to appear in the revised version of this paper).
[Grieb:2016uuo]
[2-14]
SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues, Beth Reid et al., Mon. Not. Roy. Astron. Soc. 455 (2016) 1553, arXiv:1509.06529.
[Reid:2015gra]
[2-15]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release, Sergio A. Rodriguez-Torres et al., Mon.Not.Roy.Astron.Soc. 460 (2016) 1173-1187, arXiv:1509.06404.
[Rodriguez-Torres:2015vqa]
[2-16]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the final BOSS Data Release, Francisco-Shu Kitaura et al., Mon. Not. Roy. Astron. Soc. 456 (2016) 4156, arXiv:1509.06400.
[Kitaura:2015uqa]
[2-17]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies, Hector Gil-Marin et al., Mon.Not.Roy.Astron.Soc. 460 (2016) 4188-4209, arXiv:1509.06386.
[Gil-Marin:2015sqa]
[2-18]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Effect of smoothing of density field on reconstruction and anisotropic BAO analysis, M. Vargas-Magana, S.Ho, S. Fromenteau, A. J.Cuesta, arXiv:1509.06384, 2015.
[Vargas-Magana:2015rqa]
[2-19]
Detecting Effects of Filaments on Galaxy Properties in the Sloan Digital Sky Survey III, Yen-Chi Chen et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 1880, arXiv:1509.06376.
[Chen:2015oqa]
[2-20]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies, Hector Gil-Marin et al., Mon.Not.Roy.Astron.Soc. 460 (2016) 4210-4219, arXiv:1509.06373.
[Gil-Marin:2015nqa]
[2-21]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12, Antonio J. Cuesta et al., Mon. Not. Roy. Astron. Soc. 457 (2016) 1770, arXiv:1509.06371.
[Cuesta:2015mqa]
[2-22]
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.
[Samushia:2013yga]
[2-23]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS and LOWZ anisotropic galaxy clustering, Chia-Hsun Chuang et al., Mon.Not.Roy.Astron.Soc. 461 (2016) 3781-3793, arXiv:1312.4889.
[Chuang:2013wga]
[2-24]
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.
[Anderson:2013zyy]
[2-25]
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., Mon.Not.Roy.Astron.Soc. 433 (2013) 1202-1222, arXiv:1312.4854.
[Sanchez:2013tga]
[2-26]
The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors, Will J. Percival et al., Mon.Not.Roy.Astron.Soc. 439 (2014) 2531, arXiv:1312.4841.
[Percival:2013sga]
[2-27]
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.
[Beutler:2013yhm]
[2-28]
The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey, Christopher P. Ahn et al. (SDSS), Astrophys.J.Suppl. 203 (2012) 21, arXiv:1207.7137.
[Smee:2012wd]
[2-29]
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, Beth A. Reid, Lado Samushia, Martin White, Will J. Percival, Marc Manera et al., Mon.Not.Roy.Astron.Soc. 426 (2012) 2719, arXiv:1203.6641.
[Reid:2012sw]
[2-30]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function, Ariel G. Sanchez, C.G. Scoccola, A.J. Ross, W. Percival, M. Manera et al., Mon.Not.Roy.Astron.Soc. 425 (2012) 415, arXiv:1203.6616.
[Sanchez:2012sg]
[2-31]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample, Lauren Anderson, Eric Aubourg, Stephen Bailey, Dmitry Bizyaev, Michael Blanton et al., Mon.Not.Roy.Astron.Soc. 428 (2013) 1036-1054, arXiv:1203.6594.
[Anderson:2012sa]
[2-32]
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies, Rita Tojeiro, W.J. Percival, J. Brinkmann, J.R. Brownstein, D. Eisenstein et al., Mon.Not.Roy.Astron.Soc. 424 (2012) 2339, arXiv:1203.6565.
[Tojeiro:2012rp]
[2-33]
A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey, Benjamin Dilday et al. (SDSS), Astrophys.J. 715 (2010) 1021-1035, arXiv:1003.1521.
[Dilday:2010xe]
[2-34]
Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey, Benjamin Dilday et al. (SDSS), Astrophys.J. 713 (2010) 1026-1036, arXiv:1001.4995.
[Dilday:2010qk]
[2-35]
First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters, Richard Kessler, Andrew Becker, David Cinabro, Jake Vanderplas, Joshua A. Frieman et al., Astrophys.J.Suppl. 185 (2009) 32-84, arXiv:0908.4274.
[Kessler:2009ys]
[2-36]
Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample, Will J. Percival et al. (SDSS), Mon.Not.Roy.Astron.Soc. 401 (2010) 2148-2168, arXiv:0907.1660.
[Percival:2009xn]
[2-37]
Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies, Beth A. Reid, Will J. Percival, Daniel J. Eisenstein, Licia Verde, David N. Spergel et al., Mon.Not.Roy.Astron.Soc. 404 (2010) 60-85, arXiv:0907.1659.
[Reid:2009xm]
[2-38]
The Seventh Data Release of the Sloan Digital Sky Survey, Kevork N. Abazajian et al. (SDSS), Astrophys.J.Suppl. 182 (2009) 543-558, arXiv:0812.0649.
[Abazajian:2008wr]
[2-39]
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]
[2-40]
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]
[2-41]
Cosmological Constraints from the SDSS Luminous Red Galaxies, M Tegmark et al. (SDSS), Phys. Rev. D74 (2006) 123507, arXiv:astro-ph/0608632.
[Tegmark:2006az]
[2-42]
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]
[2-43]
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]
[2-44]
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]
[2-45]
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]
[2-46]
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]
[2-47]
Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy, Uros Seljak et al. (SDSS), Phys. Rev. D71 (2005) 103515, arXiv:astro-ph/0407372.
From the abstract: We find no evidence of neutrino mass: for the case of 3 massive neutrino families with an inflationary prior, $\sum m_{\nu}<0.42$eV and the mass of lightest neutrino is $m_1<0.13$eV at 95\% c.l. For the 3 massless + 1 massive neutrino case we find $m_{\nu}<0.79$eV for the massive neutrino, excluding at 95\% c.l. all neutrino mass solutions compatible with the LSND results.
[Seljak:2004xh]
[2-48]
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]
[2-49]
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]
[2-50]
Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts, Adrian C. Pope et al. (SDSS), Astrophys. J. 607 (2004) 655, arXiv:astro-ph/0401249.
[Pope:2004cc]
[2-51]
Sloan Digital Sky Survey Spectroscopic Lens Search: I. Discovery of Intermediate-Redshift Star-Forming Galaxies Behind Foreground Luminous Red Galaxies, A. S. Bolton et al. (SDSS), Astron. J. 127 (2004) 1860, arXiv:astro-ph/0311055.
[Bolton:2003cw]
[2-52]
The 3D power spectrum of galaxies from the SDSS, M. Tegmark et al. (SDSS), Astrophys. J. 606 (2004) 702, arXiv:astro-ph/0310725.
[Tegmark:2003uf]
[2-53]
Cosmological parameters from SDSS and WMAP, M. Tegmark et al. (SDSS), Phys. Rev. D69 (2004) 103501, arXiv:astro-ph/0310723.
From the abstract: We measure cosmological parameters using the three-dimensional power spectrum $P(k)$ from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our results are consistent with a 'vanilla' flat adiabatic $\Lambda\text{CDM}$ model without tilt ($n_s=1$), running tilt, tensor modes or massive neutrinos. Adding SDSS information more than halves the WMAP-only error bars on some parameters, tightening $1\sigma$ constraints on the Hubble parameter from $h\approx 0.74^{+0.18}_{-0.07}$ to $h\approx 0.70^{+0.04}_{-0.03}$, on the matter density from $\Omega_m\approx 0.25\pm 0.10$ to $\Omega_m\approx 0.30\pm 0.04$ $(1\sigma)$ and on neutrino masses from $<11\,\text{eV}$ to $<0.6\,\text{eV}$ (95\%).
From the article: The most favored value is $\sum_k m_{\nu_k}=0$, and obtain a 95\% upper limit $\sum_k m_{\nu_k}<1.7\,\text{eV}$.
...
The WMAP team obtains the constraint $\sum_k m_{\nu_k}<0.7\,\text{eV}$ [astro-ph/0302209] by combining WMAP with the 2dFGRS. This limit is a factor of three lower than ours because of their stronger priors, most importantly that on galaxy bias $b$ determined using a bispectrum analysis of the 2dF galaxy clustering data [astro-ph/0112161].... Since the bias is marginalized over, our SDSS neutrino constraints come not from the amplitude of the power spectrum, only from its shape.

[Tegmark:2003ud]
[2-54]
SDSS J0903+5028: A New Gravitational Lens, D. E. Johnston et al. (SDSS), Astron. J. 126 (2003) 2281, arXiv:astro-ph/0307371.
[Johnston:2003vs]
[2-55]
Physical Evidence for Dark Energy, R. Scranton et al. (SDSS), arXiv:astro-ph/0307335, 2003.
[Scranton:2003in]
[2-56]
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]
[2-57]
The size distribution of galaxies in the Sloan Digital Sky Survey, S. Shen et al. (SDSS), Mon. Not. Roy. Astron. Soc. 343 (2003) 978, arXiv:astro-ph/0301527.
[Shen:2003sda]
[2-58]
SDSS Catalog of Stars in the Draco Dwarf Spheroidal Galaxy, H. A. Rave et al. (SDSS), Astrophys. J. Suppl. 145 (2003) 245, arXiv:astro-ph/0301185. To appear in ApJS 14 pages, 6 figures.
[Rave:2003ef]
[2-59]
A Survey of $z > 5.7$ Quasars in the Sloan Digital Sky Survey II: Discovery of Three Additional Quasars at $z > 6$, X. Fan et al. (SDSS), Astron. J. 125 (2003) 1649, arXiv:astro-ph/0301135.
[Fan:2003wd]
[2-60]
Astrometric Calibration of the Sloan Digital Sky Survey, J. R. Pier et al., Astron. J. 125 (2003) 1559, arXiv:astro-ph/0211375.
[Pier:2002iq]
[2-61]
The Sloan Digital Sky Survey, J. Loveday (SDSS), Contemp. Phys. 43 (2002) 437-449, arXiv:astro-ph/0207189.
[Loveday:2002ax]
[2-62]
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data, S. Dodelson et al. (SDSS), Astrophys. J. 572 (2001) 140-156, arXiv:astro-ph/0107421.
[Dodelson:2001ux]

3 - Type Ia Supernovae - Conference Proceedings

[3-1]
The Fall 2004 SDSS Supernova Survey, Masao Sako et al. (The SDSS), eConf C041213 (2004) 1424, arXiv:astro-ph/0504455. 22nd Texas Symposium on Relativistic Astrophysics.
[Sako:2005ps]

4 - Detector

[4-1]
The 2.5 m Telescope of the Sloan Digital Sky Survey, James E. Gunn, Walter A. Siegmund, Edward J. Mannery et al. (SDSS), Astron. J. 131 (2006) 2332, arXiv:astro-ph/0602326.
[Gunn:2006tw]

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Authors:
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Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Wed 20 Sep 2017, 09:48:59 UTC