Swift/BAT detects renewed hard X-ray activity from the neutron star transient XTE J1701-462

Details Swift/BAT detects renewed hard X-ray activity from the neutron star transient XTE J1701-462 Swift/BAT detects renewed hard X-ray activity from the neutron star transient XTE J1701-462

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3028....1k&link_type=abstract

The Astronomer's Telegram, #3028

Astronomy and Astrophysics

Astronomy

X-Ray, Request For Observations, Binary, Neutron Star, Transient

Scientific paper

The Swift/BAT hard X-ray transient monitor reports renewed activity in the 15-50 keV band for the transient neutron star Z source and low mass X-ray binary system XTE J1701-262. Starting on 2010-Nov-08 (MJD 55508), the source has increased in intensity from an undetectable level (one-sigma upper limit for a daily average of 0.0016 cts/cm2/sec or 8 mcrab) up to a current level of 0.010 ± 0.003 cts/cm2/sec (45 mcrab) averaged over the data from 2010-Nov-09 through Nov-11.

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