XTE J1814-338 is likely the EXOSAT slew source EXMS B1810-337

Details XTE J1814-338 is likely the EXOSAT slew source EXMS B1810-337 XTE J1814-338 is likely the EXOSAT slew source EXMS B1810-337

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..166....1w&link_type=abstract

The Astronomer's Telegram, #166

Astronomy and Astrophysics

Astronomy

5

X-Ray, A Comment, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

We report that the new X-ray transient and accretion-driven millisecond X-ray pulsar XTE J1814-338 (IAUC 8144, ATEL #164 and #165) is at a position consistent with the source EXMS B1810-337 listed in the EXOSAT medium-energy slew survey catalogue (Reynolds et al. 1999, A&AS 134, 287, Table 5). The error box of EXMS B1810-337 fully encompasses the error circle quoted for XTE J1814-338 in IAUC 8144 and ATEL #164, indicating that EXMS B1810-337 is most likely the same source as XTE J1814-338.

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