ANITA

(Antarctic Impulsive Transient Antenna)

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References

1 - Articles

[1-1]
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]
[1-2]
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]
[1-3]
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]
[1-4]
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]
[1-5]
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]
[1-6]
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]
[1-7]
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]
[1-8]
Antarctic Radio Frequency Albedo and Implications for Cosmic Ray Reconstruction, D. Z. Besson et al. (ANITA), arXiv:1301.4423, 2013.
[Besson:2013jm]
[1-9]
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]
[1-10]
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]

2 - Detector

[2-1]
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]
[2-2]
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]
[2-3]
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]
[2-4]
Observations of the Askaryan Effect in Ice, ANITA (ANITA), Phys. Rev. Lett. 99 (2007) 171101, arXiv:hep-ex/0611008.
[ANITA:2006nif]

3 - Talks

[3-1]
Searches for Ultra-High Energy Neutrinos with ANITA, Cosmin Deaconu (ANITA), PoS ICRC2019 (2019) 867, arXiv:1908.00923. ICRC19.
[Deaconu:2019rdx]
[3-2]
Recent Results from ANITA, Cosmin Deaconu (ANITA), arXiv:1810.00820, 2018. CIPANP2018.
[Deaconu:2018twx]
[3-3]
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]
[3-4]
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]
[3-5]
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]

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Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Fri 29 Mar 2024, 11:15:41 CET