Candidate Near-IR Counterpart to the X-ray Transient Pulsar GRO J1744-28

Details Candidate Near-IR Counterpart to the X-ray Transient Pulsar GRO J1744-28 Candidate Near-IR Counterpart to the X-ray Transient Pulsar GRO J1744-28

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1014....1w&link_type=abstract

The Astronomer's Telegram, #1014

Astronomy and Astrophysics

Astronomy

2

Infra-Red, Binaries, Neutron Stars, Transients

Scientific paper

We previously obtained near-IR multiband images of the field containing the quiescent X-ray transient pulsar GRO J1744-28 (the "Bursting Pulsar") on 2004 Feb 11 using the PANIC camera on the 6.5-meter Magellan/Baade telescope at Las Campanas Observatory in Chile. The exposure times were 5 min in J-band and 2.5 min in each of H- and K-bands. We find a candidate counterpart within the error circle (0.6" radius; this includes the uncertainty from our astrometric calibration) of the reported X-ray position (Muno et al.

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