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| 001 | 600606 | ||
| 005 | 20250112114445.0 | ||
| 024 | 7 | _ | |a arXiv:2304.14482 |2 arXiv |
| 024 | 7 | _ | |a 2655389 |2 inspire |
| 024 | 7 | _ | |a 10.3204/PUBDB-2023-08030 |2 datacite_doi |
| 037 | _ | _ | |a PUBDB-2023-08030 |
| 041 | _ | _ | |a English |
| 088 | _ | _ | |a arXiv:2304.14482 |2 arXiv |
| 100 | 1 | _ | |a Shvartzvald, Y. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a ULTRASAT: A wide-field time-domain UV space telescope |
| 260 | _ | _ | |c 2023 |
| 336 | 7 | _ | |a Preprint |b preprint |m preprint |0 PUB:(DE-HGF)25 |s 1704799454_313856 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a WORKING_PAPER |2 ORCID |
| 336 | 7 | _ | |a Electronic Article |0 28 |2 EndNote |
| 336 | 7 | _ | |a preprint |2 DRIVER |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a Output Types/Working Paper |2 DataCite |
| 500 | _ | _ | |a 40 pages, 16 figures, 3 tables. Submitted to the AAS journals |
| 520 | _ | _ | |a The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is scheduled to be launched to geostationary orbit in 2026. It will carry a telescope with an unprecedentedly large field of view (204 deg$^2$) and NUV (230-290nm) sensitivity (22.5 mag, 5$\sigma$, at 900s). ULTRASAT will conduct the first wide-field survey of transient and variable NUV sources and will revolutionize our ability to study the hot transient universe: It will explore a new parameter space in energy and time-scale (months long light-curves with minutes cadence), with an extra-Galactic volume accessible for the discovery of transient sources that is $>$300 times larger than that of GALEX and comparable to that of LSST. ULTRASAT data will be transmitted to the ground in real-time, and transient alerts will be distributed to the community in $<$15 min, enabling a vigorous ground-based follow-up of ULTRASAT sources. ULTRASAT will also provide an all-sky NUV image to $>$23.5 AB mag, over 10 times deeper than the GALEX map. Two key science goals of ULTRASAT are the study of mergers of binaries involving neutron stars, and supernovae: With a large fraction ($>$50%) of the sky instantaneously accessible, fast (minutes) slewing capability and a field-of-view that covers the error ellipses expected from GW detectors beyond 2025, ULTRASAT will rapidly detect the electromagnetic emission following BNS/NS-BH mergers identified by GW detectors, and will provide continuous NUV light-curves of the events; ULTRASAT will provide early (hour) detection and continuous high (minutes) cadence NUV light curves for hundreds of core-collapse supernovae, including for rarer supernova progenitor types. |
| 536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF4-613) |0 G:(DE-HGF)POF4-613 |c POF4-613 |f POF IV |x 0 |
| 588 | _ | _ | |a Dataset connected to arXivarXiv |
| 693 | _ | _ | |0 EXP:(DE-H253)ULTRASAT-20211201 |5 EXP:(DE-H253)ULTRASAT-20211201 |e Ultraviolet Transient Astronomy Satellite |x 0 |
| 700 | 1 | _ | |a Waxman, E. |b 1 |
| 700 | 1 | _ | |a Gal-Yam, A. |b 2 |
| 700 | 1 | _ | |a Ofek, E. O. |b 3 |
| 700 | 1 | _ | |a Ben-Ami, S. |b 4 |
| 700 | 1 | _ | |a Berge, D. |0 P:(DE-H253)PIP1080570 |b 5 |u desy |
| 700 | 1 | _ | |a Kowalski, Marek |0 P:(DE-H253)PIP1006050 |b 6 |u desy |
| 700 | 1 | _ | |a Bühler, Rolf |0 P:(DE-H253)PIP1018733 |b 7 |u desy |
| 700 | 1 | _ | |a Worm, S. |0 P:(DE-H253)PIP1089976 |b 8 |u desy |
| 700 | 1 | _ | |a Rhoads, J. E. |b 9 |
| 700 | 1 | _ | |a Arcavi, I. |b 10 |
| 700 | 1 | _ | |a Maoz, D. |b 11 |
| 700 | 1 | _ | |a Polishook, D. |b 12 |
| 700 | 1 | _ | |a Stone, N. |b 13 |
| 700 | 1 | _ | |a Trakhtenbrot, B. |b 14 |
| 700 | 1 | _ | |a Ackermann, Markus |0 P:(DE-H253)PIP1014130 |b 15 |u desy |
| 700 | 1 | _ | |a Aharonson, O. |b 16 |
| 700 | 1 | _ | |a Birnholtz, O. |b 17 |
| 700 | 1 | _ | |a Chelouche, D. |b 18 |
| 700 | 1 | _ | |a Guetta, D. |b 19 |
| 700 | 1 | _ | |a Hallakoun, N. |b 20 |
| 700 | 1 | _ | |a Horesh, A. |b 21 |
| 700 | 1 | _ | |a Kushnir, D. |b 22 |
| 700 | 1 | _ | |a Mazeh, T. |b 23 |
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| 700 | 1 | _ | |a Pe'er, A. |b 28 |
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| 700 | 1 | _ | |a Soumagnac, M. |b 35 |
| 700 | 1 | _ | |a Tal-Or, L. |b 36 |
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| 700 | 1 | _ | |a Zackay, B. |b 38 |
| 700 | 1 | _ | |a Guttman, O. |b 39 |
| 700 | 1 | _ | |a Rekhi, P. |b 40 |
| 700 | 1 | _ | |a Townsend, A. |0 P:(DE-H253)PIP1101637 |b 41 |
| 700 | 1 | _ | |a Weinstein, A. |b 42 |
| 700 | 1 | _ | |a Wold, I. |b 43 |
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