Near-infrared survey of high mass X-ray binary candidates

J. M. Torrejón; I. Negueruela; D. M. Smith; T. E. Harrison

doi:10.1051/0004-6361/200912619

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Volume 510 (February 2010)

A&A, 510 (2010) A61

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Table 1:

$JHK^{\prime }$ infrared photometry for the sources included in our survey.
Source	2MASS	RA	Dec	Ref.	J ( $1.27~\mu$ m)	H ( $1.63~\mu$ m)	$K^{\prime }$ ( $2.12~\mu$ m)
IGR J18027-2016	2MASS J18024194-2017172	18 02 41.94	-20 17 17.3	C	$12.79\pm 0.06$	$11.96\pm 0.08$	$11.48\pm 0.05$
SAX J18186-1703	2MASS J18183790-1702479	18 18 37.90	-17 02 47.9	Z1	$10.08\pm 0.06$	$8.94\pm 0.08$	$7.79\pm 0.05$
IGR J18483-0311^a	2MASS J18481720-0310168	18 48 17.20	-03 10 16.8	C	$10.84\pm 0.03$	$9.38\pm 0.02$	$8.47\pm 0.02$
IGR J19140+0951	2MASS J19140422+0952577	19 14 04.23	+09 52 57.7	Z2	$11.33\pm 0.06$	$9.71\pm 0.08$	$8.83\pm 0.05$

Notes. ^(a) Photometry from Rahoui & Chaty (2008). For this source, the filters are centered on 1.25, 1.65 and $2.20~\mu$ m respectively.
References. C: Chaty et al. (2008); Z1: in't Zand et al. (2006a); Z2: in't Zand et al. (2006b).

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