Possible IR counterpart of the newly discovered X-ray MSP SWIFT J1756.9-2508

Details Possible IR counterpart of the newly discovered X-ray MSP SWIFT J1756.9-2508 Possible IR counterpart of the newly discovered X-ray MSP SWIFT J1756.9-2508

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1132....1b&link_type=abstract

The Astronomer's Telegram, #1132

Physics

Optics

4

Infra-Red, Optical, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

We have observed the region of the sky including the X-ray position of the accreting millisecond pulsar SWIFT J1756.9-2508 (ATEL #1105, 1108) with the ESO-VLT Yepun equipped with the adaptive optics near-IR camera NAOS-CONICA (NACO) in two different epochs (June 19, 2007 and July 1, 2007) within the ESO-DDT program 279.D-5032 in the Ks band. About 70 objects have been detected within the 3.5 arcsec error circle reported by Swift/XRT (ATEL #1111).

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