The 157 Month <i>Swift</i>/BAT All-sky Hard X-Ray Survey
Abstract The Burst Alert Telescope (BAT) on board the Neil Gehrels Swift Observatory has been serving as a survey instrument for the hard X-ray sky, and has detected thousands of X-ray sources (e.g., active galactic nuclei, X-ray binaries, etc). BAT monitors these X-ray sources and follows their light curves on timescales from minutes to years. In addition, BAT has discovered hundreds of new X-ray sources in survey images stacked throughout the mission lifetime. We present an updated BAT survey catalog since the last published BAT 105 month survey catalog with additional 4.5 yr of data until 2017 December. Data since 2007 are reprocessed to include updated instrumental calibrations. Analysis in this study shows that additional systematic noise can be seen in the 157 month mosaic images, resulting in decreases in the expected improvement in sensitivity and the number of new detections. The BAT 157 month survey reaches a sensitivity of 8.83 × 10 −12 erg s −1 cm −2 for 90% of the sky and 6.44 × 10 −12 erg s −1 cm −2 for 10% of the sky. This catalog includes spectra, and monthly and snapshot light curves in eight energy bands (14–20, 20–24, 24–35, 35–50, 50–75, 75–100, 100–150, and 150–195 keV) for 1888 sources, including 256 new detections above a detection threshold of 4.8 σ . The light curves, spectra, and tables that summarize the information of the detected-sources are available in the online journal and on the catalog web page: https://swift.gsfc.nasa.gov/results/bs157mon/ .
Authors
- D. M. Palmer (ORCID: https://orcid.org/0000-0001-7128-0802)
- S. D. Barthelmy
- Kyuseok Oh (ORCID: https://orcid.org/0000-0002-5037-951X)
- H. A. Krimm (ORCID: https://orcid.org/0000-0003-4348-6058)
- Michael Koss (ORCID: https://orcid.org/0000-0002-7998-9581)
- Nicholas R. Collins (ORCID: https://orcid.org/0000-0002-8837-8803)
- W. H. Baumgartner (ORCID: https://orcid.org/0000-0002-5106-0463)
- L. Marcotulli (ORCID: https://orcid.org/0000-0002-8472-3649)
- Tyler Parsotan (ORCID: https://orcid.org/0000-0002-4299-2517)
- Sibasish Laha (ORCID: https://orcid.org/0000-0003-2714-0487)
- A. Y. Lien (ORCID: https://orcid.org/0000-0002-7851-9756)
- T. Sakamoto (ORCID: https://orcid.org/0000-0001-6276-6616)
- R. F. Mushotzky (ORCID: https://orcid.org/0000-0002-7962-5446)
- S. B. Cenko (ORCID: https://orcid.org/0000-0003-1673-970X)
- C. B. Markwardt (ORCID: https://orcid.org/0000-0001-9803-3879)
Institutions
- Marshall Space Flight Center (US)
- Goddard Space Flight Center (US)
- U.S. National Science Foundation (US)
- Aoyama Gakuin University (JP)
- Los Alamos National Laboratory (US)
- Korea Astronomy and Space Science Institute (KR)
- Yale University (US)
- New Mexico Consortium (US)
- Joint Space Science Institute (US)
- Eureka Scientific (US)
- Deleted Institution
- University of Maryland, College Park (US)
- University of Maryland, Baltimore County (US)
- University of Tampa (US)
Publication Details
- Journal
- The Astrophysical Journal
- Published
- 2025-08-12
- DOI
- https://doi.org/10.3847/1538-4357/ade676
- Citations
- 9
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 10.39
Funders
- National Aeronautics and Space Administration
- National Research Foundation of Korea