Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3542....1g&link_type=abstract
The Astronomer's Telegram, #3542
Astronomy and Astrophysics
Astronomy
1
X-Ray, Neutron Star, Soft Gamma-Ray Repeater, Pulsar
Scientific paper
RXTE/PCA observed the new source, Swift J1834.9-0846 (D'Elia et al. GCN Circ. 12253, Guiriec et al. 12255) on 2011 August 9-10, for a net exposure time of 9.7 ks. We performed a timing analysis using the barycentered photon arrival times in the 2-10 keV band and detected a coherent pulsation at 0.402853(2) Hz which corresponds to a spin period of 2.482295 s. Note that an earlier PCA observation on 2011 August 9 of the same field with a 3.4 ks exposure did not reveal the pulsed signal clearly but it does confirm the signal at a consistent frequency.
Gogus Ersin
Kouveliotou Chryssa
No associations
LandOfFree
RXTE Discovery of the Spin Period of Swift J1834.9-0846 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with RXTE Discovery of the Spin Period of Swift J1834.9-0846, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RXTE Discovery of the Spin Period of Swift J1834.9-0846 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1021873