Refined Orbital Timing Solution for IGR J17498-2921

Details Refined Orbital Timing Solution for IGR J17498-2921 Refined Orbital Timing Solution for IGR J17498-2921

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3601....1m&link_type=abstract

The Astronomer's Telegram, #3601

Astronomy and Astrophysics

Astronomy

X-Ray, Neutron Star, Transient, Pulsar

Scientific paper

We report a refined solution for the accreting millisecond X-ray pulsar IGR J17498-2921 (ATels #3551, #3555, #3556, #3558, #3559, #3560, #3561, #3562, #3563, #3568). Analysis is based on RXTE PCA data in the energy band 2-30 keV between 2011-08-13 and 2011-08-23, for total exposure of 121 ksec. A coherent orbit solution was found using the Z^2 technique (Bucheri et al 1983). We caution that this solution is preliminary in the sense that definitive RXTE orbit and fine clock correction data are not yet used.

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