Improved Swift-XRT position of the transient source in Terzan 5

Details Improved Swift-XRT position of the transient source in Terzan 5 Improved Swift-XRT position of the transient source in Terzan 5

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3723....1e&link_type=abstract

The Astronomer's Telegram, #3723

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Globular Cluster, Neutron Star, Transient

Scientific paper

We have analysed the Swift-XRT observations of the transient object in Terzan 5 reported in ATEL #3720 (obsID 00032148001), using the online Swift "User Object" tools (http://www.swift.ac.uk/user_objects). These tools account for pile-up in the source localisation process by using PSF profiles appropriate for piled-up sources: details are given in Evans et al.

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