X-ray counterpart detection and γ-ray analysis of the supernova remnant G279.0+01.1 with eROSITA and Fermi-LAT

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Table 1

eROSITA, XMM-Newton (MOS1, MOS2, and PN), and ROSAT observations analyzed in this work.

Instrument	ObsID	Year	Mode	Exposure (ks)	Pointing
eROSITA	eRASS:4 (150144, 145144,150141,145141)	2019–2021	survey	25.9 ^(a)	–

MOS1, MOS2, PN	0823031001	2018	Full frame (×3)	17.7/17.7/15.8	South West
MOS1, MOS2, PN	0823030401	2018	Full frame (×3)	16.7/16.7/14.8	South West
MOSl, MOS2, PN	0823030301	2018	Full frame (×3)	9.0/9.0/7.1	North

ROSAT	RASS (932618, 932619,932716,932717)	1990	Survey	14.0 ^(b)	–

Notes. The pointing column describes the position of the XMM-Newton observations with respect to the remnant’s center. ^(a)Total on-source exposure time. ^(b) Livetime, on time.

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