Correlated X-ray and IR decaying flux from the Anomalous X-ray Pulsar XTE J1810-197

Details Correlated X-ray and IR decaying flux from the Anomalous X-ray Pulsar XTE J1810-197 Correlated X-ray and IR decaying flux from the Anomalous X-ray Pulsar XTE J1810-197

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..284....1r&link_type=abstract

The Astronomer's Telegram, #284

Physics

Optics

5

Infra-Red, X-Ray, Neutron Stars, Pulsars, Transients

Scientific paper

The field of XTE J1810-197 was imaged by VLT-UT4 Yepun with the Nasmith Adaptive Optics System and the High Resolution Near IR Camera (NAOS-CONICA) on 2004 March 12, 13, and 14, as part of a monitoring program for this source. Observations were obtained with sub-arcsecond seeing and good sky conditions, resulting in a point-like source PSF between 0.09" and 0.12". J, H and Ks band images were obtained for a total exposure time of 48, 36 and 52 minutes, respectively.

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