Discovery Of Nine Gamma-Ray Pulsars In Fermi Large Area Telescope Data Using A New Blind Search Method
- Max Planck Inst. fur Gravitationsphysik, Hannover (Germany); Leibniz Univ., Hannover (Germany)
- Max Planck Inst. for Radioastronomy, Bonn (Germany)
- Max Planck Inst. fur Gravitationsphysik, Hannover (Germany); Leibniz Univ., Hannover (Germany); Univ. of Wisconsin, Milwaukee, WI (United States)
- Max Planck Inst. for Radioastronomy, Bonn (Germany); Univ. of Manchester (United Kingdom)
- Naval Research Lab. (NRL), Washington, DC (United States)
- Univ. of California, Santa Cruz, CA (United States); Univ. degli Studi di Pavia (Italy); Istituto Nazionale di Astrofisica (INAF), Milano (Italy)
- Columbia Univ., New York, NY (United States). Columbia Astrophysics Lab.
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland Baltimore County (UMBC), Baltimore, MD (United States)
- Univ. of California, Santa Cruz, CA (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. of Amsterdam (Netherlands); Netherlands Inst. for Radio Astronomy, Postbus (Netherlands)
- Australia Telescope National Facility, Epping, NSW (Australia)
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Istituto Universitario di Studi Superiori (IUSS), Pavia (Italy)
- Univ. of Manchester (United Kingdom)
- West Virginia Univ., Morgantown, WV (United States)
- Naval Research Lab. (NRL), Washington, DC (United States); George Mason Univ., Fairfax, VA (United States)
- National Radio Astronomy Observatory (NRAO), Charlottesville, VA (United States)
- Univ. of California, Santa Cruz, CA (United States); Istituto Nazionale di Fisica Nucleare (INFN), Pisa (Italy)
We report the discovery of nine previously unknown gamma-ray pulsars in a blind search of data from the Fermi Large Area Telescope (LAT). The pulsars were found with a novel hierarchical search method originally developed for detecting continuous gravitational waves from rapidly rotating neutron stars. Designed to find isolated pulsars spinning at up to kHz frequencies, the new method is computationally efficient, and incorporates several advances, including a metric-based gridding of the search parameter space (frequency, frequency derivative and sky location) and the use of photon probability weights. The nine pulsars have spin frequencies between 3 and 12 Hz, and characteristic ages ranging from 17 kyr to 3 Myr. Two of them, PSRs J1803–2149 and J2111+4606, are young and energetic Galactic-plane pulsars (spin-down power above 6X1035 erg s-1 and ages below 100 kyr). The seven remaining pulsars, PSRs J0106+4855, J0622+3749, J1620–4927, J1746–3239, J2028+3332, J2030+4415, J2139+4716, are older and less energetic; two of them are located at higher Galactic latitudes (jbj > 10°). PSR J0106+4855 has the largest characteristic age (3 Myr) and the smallest surface magnetic field (2X1011G) of all LAT blind-search pulsars. PSR J2139+4716 has the lowest spin-down power (3X1033 erg s-1) among all non-recycled gamma-ray pulsars ever found. Despite extensive multi-frequency observations, only PSR J0106+4855 has detectable pulsations in the radio band. The other eight pulsars belong to the increasing population of radio-quiet gamma-ray pulsars.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1356767
- Journal Information:
- The Astrophysical Journal, Vol. 744, Issue 2; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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