3 February 2004 Swift/BAT calibration and the estimated BAT hard x-ray survey sensitivity
Author Affiliations +
Abstract
In addition to providing the initial gamma-ray burst trigger and location, the Swift Burst Alert Telescope (BAT) will also perform an all-sky hard x-ray survey based on serendipitous pointings resulting from the study of gamma-ray bursts. BAT was designed with a very wide field-of-view (FOV) so that it can observe roughly 1/7 of the sky at any time. Since gamma-ray bursts are uniformly distributed over the sky, the final BAT survey coverage is expected to be nearly uniform. BAT's large effective area and long sky exposures will produce a 15 - 150 keV survey with up to 30 times better sensitivity than any previous hard x-ray survey (e.g. HEAO A4). Since the sensitivity of deep exposures in this energy range is systematics limited, the ultimate survey sensitivity depends on the relative sizes of the statistical and systematic errors in the data. Many careful calibration experiments were performed at NASA/Goddard Space Flight Center to better understand the BAT instrument's response to 15-150 keV gamma-rays incident from any direction within the FOV. Using radioactive sources of gamma-rays with known locations and energies, the Swift team can identify potential systematic errors in the telescope's performance and estimate the actual Swift hard x-ray survey sensitivity in flight. These calibration results will be discussed and a preliminary parameterization of the BAT instrument response will be presented. While the details of the individual BAT CZT detector response will be presented elsewhere in these proceedings, this talk will focus on the translation of the calibration experimental data into overall hard x-ray survey sensitivity.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ann M. Parsons, Ann M. Parsons, Jack Tueller, Jack Tueller, Hans Krimm, Hans Krimm, Scott D. Barthelmy, Scott D. Barthelmy, James Cummings, James Cummings, Craig Markwardt, Craig Markwardt, Derek Hullinger, Derek Hullinger, Neil Gehrels, Neil Gehrels, Ed Fenimore, Ed Fenimore, David Palmer, David Palmer, Goro Sato, Goro Sato, Kazuhiro Nakazawa, Kazuhiro Nakazawa, Tadayuki Takahashi, Tadayuki Takahashi, Shin Watanabe, Shin Watanabe, Yuu Okada, Yuu Okada, Hiromitsu Takahashi, Hiromitsu Takahashi, Masaya Suzuki, Masaya Suzuki, Makoto Tashiro, Makoto Tashiro, } "Swift/BAT calibration and the estimated BAT hard x-ray survey sensitivity", Proc. SPIE 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII, (3 February 2004); doi: 10.1117/12.506309; https://doi.org/10.1117/12.506309
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

The Canadian Astro-H Metrology System
Proceedings of SPIE (July 23 2014)
Burst locations with an arc second telescope (BLAST)
Proceedings of SPIE (October 17 1996)
In orbit performance of wide field x ray monitor on...
Proceedings of SPIE (March 10 2003)
EXIST: mission design concept and technology program
Proceedings of SPIE (March 10 2003)

Back to Top