The Palomar Transient Factory (PTF) is a fully-automated, wide-field survey aimed at a systematic exploration of the optical transient sky.


News

October 2009: Mysterious transients unmasked as the bright blue death throes of massive stars submitted to Nature (embargoed for discussion in the press).

August 2009: PTF in the news: 1,2,3,4

29 June 2009: Two new papers: a detailed description of the PTF project and the commissioning results (astro-ph/0906.5350) and a study of the science planned for PTF (astro-ph/0906.5355).

23 May 2009: Discovery, Photometric and Spectroscopic Follow Up Of Another Fifteen Optical Transients (ATel #2055)

28 Apr 2009: The Palomar Transient Factory Discovers a Possible super-Chandrasekhar Type Ia Supernova (ATel #2037)

2 Apr 2009: Another 25 transient detections and followups from PTF (ATel #2005)

22 March 2009: Eleven more transient detections from PTF (ATel #1983)

11 March 2009: The first PTF transient detections! (ATel #1964)


The PTF Project

The program is centered on a 12Kx8K, 7.8 square degree CCD array (CFH12K) re-engineered for the 1.2-m Oschin Telescope at Palomar Observatory by COO (Rahmer et al. 2008). Photometric followup is undertaken by the automated Palomar 1.5-m telescope (Cenko et al. 2006) and other facilities provided by consortium members.

PTF uses eighty percent of the 1.2-m and fifty percent of the 1.5-m telescope time. With an exposure of 60-s the survey reaches an approximate depth of m_R=20.5 and m_g'=21.

Two major transient detection experiments are planned for the five-year project:

1) a 5-day cadence supernova search

2) an exotic transient search with cadences between 90 seconds and 1 day.

PTF provides automatic, realtime transient classification and followup, as well as a database including every source detected in each frame.

PTF is a collaboration of Caltech, LBNL, IPAC, Berkeley, LCOGT, Oxford, Columbia and the Weizmann Institute.

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