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Title: FIVE NEW MILLISECOND PULSARS FROM A RADIO SURVEY OF 14 UNIDENTIFIED FERMI-LAT GAMMA-RAY SOURCES

Journal Article · · Astrophysical Journal Letters
 [1];  [2];  [3]; ;  [4]; ;  [5];  [6]; ; ;  [7];  [8]; ;  [9];  [10]
  1. W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305 (United States)
  2. Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 (United States)
  3. National Academy of Sciences, Washington, DC 20001 (United States)
  4. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  5. Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, 53121 Bonn (Germany)
  6. Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo (Netherlands)
  7. CSIRO Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710 (Australia)
  8. National Radio Astronomy Observatory (NRAO), Charlottesville, VA 22903 (United States)
  9. Space Science Division, Naval Research Laboratory, Washington, DC 20375-5352 (United States)
  10. CSIRO Parkes Observatory, Parkes, NSW 2870 (Australia)

We have discovered five millisecond pulsars (MSPs) in a survey of 14 unidentified Fermi Large Area Telescope sources in the southern sky using the Parkes radio telescope. PSRs J0101-6422, J1514-4946, and J1902-5105 reside in binaries, while PSRs J1658-5324 and J1747-4036 are isolated. Using an ephemeris derived from timing observations of PSR J0101-6422 (P = 2.57 ms, DM = 12 pc cm{sup -3}), we have detected {gamma}-ray pulsations and measured its proper motion. Its {gamma}-ray spectrum (a power law of {Gamma} = 0.9 with a cutoff at 1.6 GeV) and efficiency are typical of other MSPs, but its radio and {gamma}-ray light curves challenge simple geometric models of emission. The high success rate of this survey-enabled by selecting {gamma}-ray sources based on their detailed spectral characteristics-and other similarly successful searches indicate that a substantial fraction of the local population of MSPs may soon be known.

OSTI ID:
22047975
Journal Information:
Astrophysical Journal Letters, Vol. 748, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
Country of Publication:
United States
Language:
English

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X-ray follow-ups of XSS J12270-4859: a low-mass X-ray binary with gamma-ray Fermi -LAT association journal January 2013
DISCOVERY OF THE OPTICAL COUNTERPARTS TO FOUR ENERGETIC FERMI MILLISECOND PULSARS journal May 2013
SEARCH FOR GAMMA-RAY EMISSION FROM FOUR ACCRETING MILLISECOND PULSARS WITH FERMI /LAT journal May 2013
SEARCH FOR GAMMA-RAY-EMITTING ACTIVE GALACTIC NUCLEI IN THE FERMI -LAT UNASSOCIATED SAMPLE USING MACHINE LEARNING journal January 2014
PARKES RADIO SEARCHES OF FERMI GAMMA-RAY SOURCES AND MILLISECOND PULSAR DISCOVERIES journal September 2015
THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS journal September 2013
Unidentified sources in the Fermi-LAT second source catalog: the case for DM subhalos journal November 2012
Understanding the Evolution of Close Binary Systems with Radio Pulsars journal April 2014
High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array journal March 2016
The International Pulsar Timing Array: second data release journal October 2019
Pulsar Searching and Timing journal January 2013
SIX NEW MILLISECOND PULSARS FROM ARECIBO SEARCHES OF FERMI GAMMA-RAY SOURCES journal February 2016
The Einstein@Home Gamma-ray Pulsar Survey. II. Source Selection, Spectral Analysis, and Multiwavelength Follow-up journal February 2018
The Second Fermi Large area Telescope Catalog of Gamma-Ray Pulsars text January 2013
Unidentified sources in the Fermi-LAT second source catalog: the case for DM subhalos text January 2012
Discovery of the Optical Counterparts to Four Energetic Fermi Millisecond Pulsars text January 2013
Understanding the evolution of close binary systems with radio pulsars text January 2014
Parkes radio searches of Fermi gamma-ray sources and millisecond pulsar discoveries text January 2015
Six New Millisecond Pulsars from Arecibo Searches of Fermi Gamma-Ray Sources text January 2016
High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array text January 2016
The Einstein@Home Gamma-Ray Pulsar Survey II. Source Selection, Spectral Analysis and Multi-wavelength Follow-up text January 2017