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

Home

All issues

Volume 534 (October 2011)

A&A, 534 (2011) A119

Full HTML

Press Release

Free Access

This article has an erratum: [erratum]

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.