Swift and VLT monitoring of AXP 1E1048.1-5937

Details Swift and VLT monitoring of AXP 1E1048.1-5937 Swift and VLT monitoring of AXP 1E1048.1-5937

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1077....1i&link_type=abstract

The Astronomer's Telegram, #1077

Astronomy and Astrophysics

Astronomy

3

Infra-Red, X-Ray, Neutron Stars, Pulsars, Soft Gamma-Ray Repeaters, Transients

Scientific paper

X-ray and near-IR monitoring observations have been carried out during the latest weeks by means of the Swift XRT (0.3-10keV) and VLT-UT4 (equipped with the NAOS-CONICA camera). The observations cover the time interval 4th April - 17th May (for Swift) and 6th April - 10th May (for the VLT). The 1-10keV source flux remained at a relatively high level of 3.5x10^-11 ergs/cm^2/s (absorbed) until approximately the end of April 2007.

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