Continuation of the X-ray monitoring of Sgr A*: the increase in bright flaring rate confirmed

E. Mossoux; B. Finociety; J.-M. Beckers; F. H. Vincent

doi:10.1051/0004-6361/201937136

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Volume 636 (April 2020)

A&A, 636 (2020) A25

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Table A.1.

Observation log of public XMM-Newton observations in 2016–2018.

Observations							Flares

											Mean
ObsID	PI	Start ^(a)	End ^(a)	Exposure ^(b)	Instrument	Nonflaring level	Number	Start	Stop	Duration	Count rate	Flux
		(UT)	(UT)	(ks)		(count s⁻¹)		(UT)	(UT)	(s)	(count s⁻¹)	(10⁻¹² erg s⁻¹ cm⁻²)
0790180401	Schartel	2016-02-26 16:20:13	2016-02-27 02:36:53	37.0	EPIC/pn ^(c)	3.5 ± 0.02	...	.........	.........	......	............	............

Notes.

^(a)

First and last good time intervals (GTI) start and stop in universal time (UT) reference.

^(b)

The sum of the GTI.

^(c)

The EPIC camera was in timing mode.

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