UV Detection of Accreting Millisecond Pulsar IGR J00291+5934 with Swift/UVOT

Details UV Detection of Accreting Millisecond Pulsar IGR J00291+5934 with Swift/UVOT UV Detection of Accreting Millisecond Pulsar IGR J00291+5934 with Swift/UVOT

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1668....1m&link_type=abstract

The Astronomer's Telegram, #1668

Astronomy and Astrophysics

Astronomy

3

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

Scientific paper

For the millisecond X-ray pulsar IGR J00291+5934 (ATEL #1660, #1664, #1665, #1666, #1667), we report on UVOT analysis of the Swift observation taken 2008-08-15 at 14:50 UT (Markwardt & Swank, ATEL #1664). IGR J00291+5934 was detected in the UVW2 filter of UVOT. The UVW2 filter has a central wavelength of 1928 Angstroms. The observed magnitude was 19.6 +/- 0.2 in the UVOT photometric system (Poole et al, 2008, MNRAS 383,627), uncorrected for the expected reddening.

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