The 157-month Swift-BAT All-Sky Hard X-Ray Survey

Files

2506.04109v1.pdf (7.63 MB)

Links to Files

http://arxiv.org/abs/2506.04109

Permanent Link

https://doi.org/10.48550/arXiv.2506.04109
 http://hdl.handle.net/11603/39346

Collections

UMBC Faculty Collection
UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
UMBC Physics Department

Author/Creator

Author/Creator ORCID

https://orcid.org/0000-0002-7851-9756
 https://orcid.org/0000-0003-2714-0487

Date

2025-06-04

Type of Work

journal articles
postprints
Text

Department

Program

Citation of Original Publication

Rights

This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
Public Domain

Subjects

Astrophysics - High Energy Astrophysical Phenomena

Abstract

The Burst Alert Telescope (BAT) onboard 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., AGNs, X-ray binaries, etc). BAT monitors these X-ray sources and follows their light curves on time scales from minutes to years. In addition, BAT discovers hundreds of new X-ray sources in survey images stacked throughout the mission lifetime. We present the updated BAT survey catalog since the last published BAT 105 month survey catalog (Oh et al. 2018) with additional of 4.5 years of data until December 2017. Data since 2007 are reprocessed to include updated instrumental calibration. 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, 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 the detection threshold of 4.8σ. The light curves, spectra, and tables that summarize the information of the detected-sources are available in the online journal and in the catalog web page https://swift.gsfc.nasa.gov/results/bs157mon/.