The 7-year MAXI/GSC X-ray Source Catalog in the High Galactic-Latitude Sky (3MAXI)
Taiki Kawamuro, Yoshihiro Ueda, Megumi Shidatsu, Takafumi Hori, Morii, Mikio, Satoshi Nakahira, Naoki Isobe, Nobuyuki Kawai, Tatehiro Mihara, Masaru, Matsuoka, Takashi Morita, Motoki Nakajima, Hitoshi Negoro, Saeko Oda,, Takanori Sakamoto, Motoko Serino, Mutsumi Sugizaki

TL;DR
This paper presents a comprehensive 7-year high-latitude X-ray source catalog from MAXI/GSC, detecting 682 sources, analyzing their properties, variability, and counterparts, significantly expanding previous surveys in this sky region.
Contribution
The study provides the third MAXI/GSC high-latitude catalog with improved sensitivity, detailed spectral and variability analysis, and cross-identification with multiple X-ray surveys, enhancing the understanding of X-ray sources.
Findings
Detected 682 sources with high significance in 4--10 keV band.
Achieved sensitivity of approximately 0.48 mCrab over half the survey area.
Identified counterparts and characterized source variability over one year.
Abstract
We present the third MAXI/GSC catalog in the high Galactic-latitude sky () based on the 7-year data from 2009 August 13 to 2016 July 31, complementary to that in the low Galactic-latitude sky (; Hori et al. 2018). We compile 682 sources detected at significances of in the 4--10 keV band. A two-dimensional image fit based on the Poisson likelihood algorithm (-statistics) is adopted for the detections and constraints on their fluxes and positions. The 4--10 keV sensitivity reaches mCrab, or erg cm s, over the half of the survey area. Compared with the 37-month catalog (Hiroi et al. 2013), which adopted a threshold of , the source number increases by a factor of 1.4. The fluxes in the 3--4 keV and 10--20 keV bands are further…
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