Optical decline of HETE J1900.1-2455

Details Optical decline of HETE J1900.1-2455 Optical decline of HETE J1900.1-2455

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1090....1t&link_type=abstract

The Astronomer's Telegram, #1090

Astronomy and Astrophysics

Astronomy

3

Optical, X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

Following the recently reported decline of the X-ray flux from the millisecond pulsar HETE J1900.1-2455 (Galloway et al. 2007, ATel #1086), we acquired images of its optical counterpart using the Wide Field Camera mounted on the 2.5m Isaac Newton Telescope at La Palma. The images were obtained on 2007 May 29 4:10-4:33 UT and May 30 3:42-4:17 UT and photometrically calibrated using the standard stars SA 113-260 and BD+33 2642.

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