Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
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note
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The Fermi LAT Collaboration is supported by NASA and the U.S. Department of Energy; the Commissariat à l'Energie Atomique and CNRS/Institut National de Physique Nucléaire et de Physique des Particules (France); the Agenzia Spaziale Italiana, Istituto Nazionale di Fisica Nucleare, and Istituto Nazionale di Astrofisica (Italy); the Ministry of Education, Culture, Sports, Science and Technology, High Energy Accelerator Research Organization (KEK), and Japan Aerospace Exploration Agency (Japan); and the K. A. Wallenberg Foundation, Swedish Research Council, and National Space Board (Sweden). Much of this work was carried out on the Pleiades supercomputer at the Department of Astronomy, University of California, Santa Cruz. This work made extensive use of the ATNF pulsar database. We thank N. Gehrels for granting Swift/XRT time to explore the LAT error circles, the Swift MOC staff for performing the observations, F. Camilo and S. Ransom for contributions, and M. Roberts for useful discussions.
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