Overview of an extensive multi-wavelength study of GX 339−4 during the 2010 outburst

M. Cadolle Bel; J. Rodriguez; P. D’Avanzo; D. M. Russell; J. Tomsick; S. Corbel; F. W. Lewis; F. Rahoui; M. Buxton; P. Goldoni; E. Kuulkers

doi:10.1051/0004-6361/201117684

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Volume 534 (October 2011)

A&A, 534 (2011) A119

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201117684e]

Table 1

Log of the GX 339 − 4 observations analysed in this paper.

Observatory	Instrument	Bandpass	Period	Observation Type
			(MJD−55000)


INTEGRAL^a	IBIS/ISGRI	18–200 keV	237.5–303.3	ToO (5 × 5^b, Hex^c)
	JEM-X	5–25 keV	237.5–303.3	ToO
RXTE^a	PCA	3–25 keV	208.5–345.4	Public
Swift^d	XRT	0.3–10 keV	217.7–352.3	Public
	BAT	20–100 keV	217.7–352.3	Public
	UVOT	180–600 nm	217.7–352.3	Public
REM^d	ROSS, REMIR	550–2159 nm	260.2–261.4 and 303	ToO
FTS^d	Merope	460–883 nm	237.7–337.8	Public
ATCA^d	–	5.5–9 GHz	261–263	ToO

Notes.

^(a)

Interrupted observations: almost all Rev. (~3 days) between # 895–916 for INTEGRAL; Galactic Bulge monitoring for RXTE.

^(b)

5 × 5 dither pattern around the nominal target location.

^(c)

Hexagonal pattern around the nominal target location.

^(d)

Snap-shot observations with the specified instruments or receivers.

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