ADAPT (the Antarctic Demonstrator for the Advanced
Particle-astrophysics Telescope) is a NASA suborbital mission planned for a
high-altitude flight from Antarctic in 2025.
ADAPT is a 0.5mx0.5m cross-section instrument consisting of a
scintillating fiber-tracker, and imaging (CsI)
calorimeter and silicon strip detector for gamma-ray and cosmic-ray
measurements. The ADAPT instrument will
demonstrate the major detector components for the larger space-based APT
mission and will provide sensitivity to gamma-ray transients and a sky map in the MeV-GeV range
during the ~30 day flight. ADAPT will
also make cosmic-ray measurements during its flight, demonstrating the
potential for a longer duration space experiment (APT) measure the elemental
abundance of rare ultra-heavy cosmic-rays.
Even during the brief flight, ADAPT is expected to provide prompt degree-scale
localizations and polarization constraints on a few gamma-ray bursts, and
provide better instantaneous sensitivity than existing instruments at energies
below 100 MeV. The ADAPT instrument is
being constructed by the APT collaboration including participants from
Washington University (the PI institution), the Erlangen
Centre for Astroparticle Physics, the NASA Goddard Space Flight Center, Louisiana State University, the INFN Bari, the INFN Pisa, the Naval Research
Lab, University of Hawaii, and the University of Minnesota.
APT Collaboration
S.
Alnussirat1, C. Altomare2, R. G. Bose3, D. Braun3, J. H.
Buckley3*,
J. D. Buhler4,
E. Burns1,
R. D. Chamberlain4,
W. Chen5,
M. L. Cherry1,
L. Di Venere6,2,
J. Dumonthier7, M. Errando3, S. Funk8, F. Giordano6,2, J.
Hoffman3,
Z. Hughes3,
D. J. Huth3, P. L. Kelly5, J. F. Krizmanic9,10,11, M. Kuwahara12, F. Licciulli2, G. Liu13, M. N. Mazziotta 2, J. G. Mitchell14,15, J. W. Mitchell9, G. A. de Nolfo15, R. Paoletti16, R. Pillera17,2, B. F.
Rauch3,
D. Serini2, G. Simburger3, M. Sudvarg4, G. Suarez7, T. Tatoli15,18, G. S.
Varner12,
E. Wulf19,
A. Zink8,
W. V. Zober3
1Department
of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803,
USA, 2Istituto Nazionale di Fisica Nucleare, Sezione di Bari,
I-70126 Bari, Italy, 3Department of Physics and McDonnell Center for the Space
Sciences, Washington University, St. Louis, MO 63130, USA, 4Department of
Computer Science & Engineering, Washington University, St. Louis, MO 63130,
USA, 5Department
of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA, 6Dipartimento di Fisica “M.
Merlin” dell’Università e del Politecnico
di Bari, I-70126 Bari, Italy, 7NASA Goddard Space Flight Center, Greenbelt, MD
20771, USA, 8Friedrich-Alexander-Universität Erlangen-Nürnberg,
Erlangen Centre for Astroparticle Physics, D-91058
Erlangen, Germany, 9Center for Space Sciences and Technology, University of Maryland
Baltimore County, Baltimore, Maryland 21250, USA, 10Astroparticle
Physics Laboratory, NASA/GSFC, Greenbelt, Maryland 20771, USA, 11Center for
Research and Exploration in Space Sciences and Technology, NASA/GSFC,
Greenbelt, Maryland 20771, USA, 12Department of Engineering, University of Hawai‘i
at Ma ̄noa, Honolulu, HI 96822, USA, 13Department of Physics and Astronomy, University
of Hawai‘i at Ma ̄noa, Honolulu, HI 96822, USA, 14Department of Physics, The George
Washington University, Washington, DC 20052, USA, 15Heliospheric
Physics Laboratory, NASA/GSFC, Greenbelt, MD 20771, USA, 16Università di Siena and INFN Pisa, I-53100 Siena, Italy, 17Politecnico di Bari, Department of Mechanics, Mathematics
and Management, via Orabona, 4, I-70125 Bari, Italy, 18Department
of Physics, Catholic University of America, Washington, DC 20064, USA, 19Naval
Research Laboratory, Washington, DC 20375, USA .
*ADAPT,
Principal Investigator
Publications
1. [2] J. Buckley, The Advanced Particle-astrophysics
Telescope (APT) Project Status, in Proceedings of 37th International
Cosmic Ray Conference — PoS(ICRC2021), vol. 395,
p. 655, 2021, DOI.
2.
Z.
Hughes and J. Buckley, Characterization of a prototype imaging calorimeter
for the Advanced Particle-astrophysics Telescope from an Antarctic balloon
flight and CERN beam test, in Proceedings of 37th International Cosmic
Ray Conference — PoS(ICRC2021),
vol. 395, p. 137, 2021, DOI.
3.
[2] APT collaboration, The advanced
particle-astrophysics telescope: Simulation of the instrument performance for
gamma-ray detection, in Proceedings of 37th International Cosmic Ray
Conference — PoS(ICRC2021), vol. 395, p. 590,
2021, DOI.
4.
[3] M. Sudvarg, J. Buhler, J.
Buckley, W. Chen, Z. Hughes, E. Ramey et al., A Fast GRB Source Localization
Pipeline for the Advanced Particle-astrophysics Telescope, in Proceedings
of 37th International Cosmic Ray Conference — PoS(ICRC2021),
vol. 395, p. 588, 2021, DOI.