X-ray transient search using XRISM/Xtend
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Tsuboi, Yohko, Koichiro Akasu, Noboru Nemoto, et al. “X-Ray Transient Search Using XRISM/Xtend.” Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray 13093 (August 2024): 1763–68. https://doi.org/10.1117/12.3019733.
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©2024 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
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Abstract
The X-ray Imaging Spectroscopy Mission (XRISM) was launched on 2023-09-06 (UT). The onboard Xtend camera is now performing spectral imaging in the 0.4–13 keV band. Utilizing the wide field of view of Xtend of 38′ ×38′, we have been conducting searches for transient sources once a day, under the name of “XRISM/Xtend Transient Search (XTS)”. We report an Astronomer’s Telegram (ATel) within ~1 day after downlinking the data from the satellite. Since the beginning of March 2024, when the XTS began full-scale operations, through early July, we issued nine ATel reports. The sensitivity limit of XTS is about 10⁻¹⁴ erg s⁻¹cm⁻² for a one-day observation, i.e. for an exposure time of ~40 ks with the typical XRISM observing efficiency of about 50%. This sensitivity limit is orders of magnitude fainter than those obtained with all-sky survey missions such as MAXI and Einstein probe. It is comparable to those of Swift/XRT and eROSITA/SRG. XRISM observations are 4 days long on average, allowing for searches of sources that vary on time scales of more than one day, and down to the 10⁻¹⁴ erg s⁻¹ cm⁻² flux range. Consequently, XRISM now plays a key role in time-domain astronomy.