Follow-up of PTF10bzf with Swift

Details Follow-up of PTF10bzf with Swift Follow-up of PTF10bzf with Swift

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2471....1k&link_type=abstract

The Astronomer's Telegram, #2471

Astronomy and Astrophysics

Astronomy

1

Optical, Ultra-Violet, X-Ray, Novae, Supernovae, Transients

Scientific paper

We triggered our Swift Target Of Opportunity program ("Unveiling New Classes of Transients with Palomar Transient Factory", PI S. R. Kulkarni) for PTF10bzf (see ATEL#2470). Thus far, we have obtained two epochs. Our first 5ks epoch was on UT 2010 Mar 4.029 and second 2.5ks epoch was on Mar 8.303. We do not detect PTF10bzf with Swift/XRT down to a 3-sigma limiting count rate (assuming an 18" radius) of 3.7e-4 cps and 7.7e-4 cps respectively in the two epochs.

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