(ANtarctic
Impulsive
Transient
Antenna)
Other Web pages:
INSPIRE
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[1-1]
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Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA),
R. Prechelt et al.
(ANITA),
Phys.Rev.D 105 (2022) 042001,
arXiv:2112.07069.
[ANITA:2021xxh]
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[1-2]
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A search for ultrahigh-energy neutrinos associated with astrophysical sources using the third flight of ANITA,
C. Deaconu et al.
(ANITA),
JCAP 2104 (2021) 017,
arXiv:2010.02869.
[ANITA:2020sds]
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[1-3]
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icemc: A Monte Carlo Simulation for Cosmogenic Neutrinos interacting in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA),
L. Cremonesi et al.,
JINST 14 (2019) P08011,
arXiv:1903.11043.
[ANITA:2019xbi]
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[1-4]
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Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA,
P. W. Gorham et al.
(ANITA),
Phys.Rev. D99 (2019) 122001,
arXiv:1902.04005.
[ANITA:2019wyx]
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[1-5]
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Observation of an Unusual Upward-going Cosmic-ray-like Event in the Third Flight of ANITA,
P. W. Gorham et al.
(ANITA),
Phys.Rev.Lett. 121 (2018) 161102,
arXiv:1803.05088.
[ANITA:2018sgj]
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[1-6]
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Constraints on the diffuse high-energy neutrino flux from the third flight of ANITA,
P. Allison et al.
(ANITA),
Phys.Rev. D98 (2018) 022001,
arXiv:1803.02719.
[ANITA:2018vwl]
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[1-7]
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Antarctic Surface Reflectivity Measurements from the ANITA-3 and HiCal-1 Experiments,
P. W. Gorham et al.
(ANITA),
J.Astron.Inst. 06 (2017) 1740002,
arXiv:1703.00415.
[Gorham:2017xbo]
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[1-8]
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Antarctic Radio Frequency Albedo and Implications for Cosmic Ray Reconstruction,
D. Z. Besson et al.
(ANITA),
arXiv:1301.4423, 2013.
[Besson:2013jm]
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[1-9]
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Erratum: Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment,
P. W. Gorham et al.
(ANITA),
Phys. Rev. D85 (2012) 049901,
arXiv:1011.5004.
[ANITA:2010hzc]
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[1-10]
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Constraints on cosmic neutrino fluxes from the anita experiment,
S. W. Barwick et al.
(ANITA),
Phys. Rev. Lett. 96 (2006) 171101,
arXiv:astro-ph/0512265.
[ANITA:2005gdw]
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[2-1]
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Dynamic tunable notch filters for the Antarctic Impulsive Transient Antenna (ANITA),
P.Allison et al.,
Nucl.Instrum.Meth. A894 (2018) 47-56,
arXiv:1709.04536.
[Allison:2017vtk]
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[2-2]
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An Interferometric Analysis Method for Radio Impulses from Ultra-high Energy Particle Showers,
A. Romero-Wolf, S. Hoover, A. Vieregg, P. Gorham
(ANITA),
arXiv:1304.5663, 2013.
[Romero-Wolf:2013mla]
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[2-3]
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The Antarctic Impulsive Transient Antenna Ultra-high Energy Neutrino Detector Design, Performance, and Sensitivity for 2006-2007 Balloon Flight,
ANITA
(ANITA),
Astropart. Phys. 32 (2009) 10-41,
arXiv:0812.1920.
[ANITA:2008mzi]
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[2-4]
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Observations of the Askaryan Effect in Ice,
ANITA
(ANITA),
Phys. Rev. Lett. 99 (2007) 171101,
arXiv:hep-ex/0611008.
[ANITA:2006nif]
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[3-1]
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Searches for Ultra-High Energy Neutrinos with ANITA,
Cosmin Deaconu
(ANITA),
PoS ICRC2019 (2019) 867,
arXiv:1908.00923.
ICRC19.
[Deaconu:2019rdx]
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[3-2]
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Recent Results from ANITA,
Cosmin Deaconu
(ANITA),
arXiv:1810.00820, 2018.
CIPANP2018.
[Deaconu:2018twx]
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[3-3]
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Upward-Pointing Cosmic-Ray-like Events Observed with ANITA,
Andres Romero-Wolf et al.
(ANITA),
PoS ICRC2017 (2018) 935,
arXiv:1810.00439.
International Cosmic Ray Conference 2017, Busan, South Korea.
[ANITA:2017qmn]
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[3-4]
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Towards Determining the energy of the UHECRs observed by the ANITA detector,
Konstantin Belov
(ANITA),
AIP Conf. Proc. 1535 (2013) 209,
arXiv:1303.2172.
accepted to AIP conference proceedings.
[Belov:2013gsb]
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[3-5]
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Tuning into UHE Neutrinos in Antarctica - The ANITA Experiment,
P. Miocinovic et al.
(ANITA),
eConf C041213 (2004) 2516,
arXiv:astro-ph/0503304.
22nd Texas Symposium on Relativistic Astrophysics at Stanford, Palo Alto, 13-17 December 2004.
[ANITA:2004sje]
Last Update: Thu 15 Oct 2026, 12:29:31 CET
