Pulsar timing for the Fermi gamma-ray space telescope
Abstract
Here, we describe a comprehensive pulsar monitoring campaign for the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope (formerly GLAST). The detection and study of pulsars in gamma rays give insights into the populations of neutron stars and supernova rates in the Galaxy, into particle acceleration mechanisms in neutron star magnetospheres, and into the “engines” driving pulsar wind nebulae. LAT's unprecedented sensitivity between 20 MeV and 300 GeV together with its 2.4 sr field-of-view makes detection of many gamma-ray pulsars likely, justifying the monitoring of over two hundred pulsars with large spin-down powers. To search for gamma-ray pulsations from most of these pulsars requires a set of phase-connected timing solutions spanning a year or more to properly align the sparse photon arrival times. We describe the choice of pulsars and the instruments involved in the campaign. Attention is paid to verifications of the LAT pulsar software, using for example giant radio pulses from the Crab and from PSR B1937+21 recorded at Nançay, and using X-ray data on PSR J0218+4232 from XMM-Newton. We demonstrate accuracy of the pulsar phase calculations at the microsecond level.
- Authors:
-
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- Univ. of Bordeaux, Gradignan (France). Centre d'etudes nucleaires de Bordeaux Gradignan, Centre National de la Recherche Scientifique, Inst. National de Physique Nucleaire et de Physique des Particules (CNRS/IN2P3)
- Columbia Univ., New York, NY (United States). Columbia Astrophysics Lab.
- Univ. of Orleans (France). Lab. of Physics and Chemistry of Environment and Space; Paris Observatory (France). Nancay radio telescope
- Univ. of Manchester, Macclesfield (United Kingdom). Jodrell Bank Observatory
- Arecibo Observatory (Puerto Rico)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Commonwealth Scientific and Industrial Research Organisation (CSIRO), Epping, NSW (Australia). Australia Telescope National Facility
- McGill Univ., Montreal, QC (Canada)
- Univ. of Manchester, Macclesfield (United Kingdom). Jodrell Bank Observatory
- West Virginia Univ., Morgantown, WV (United States). Dept. of Physics
- National Radio Astronomy Observatory, Charlottesville, VA (United States)
- Eureka Scientific, Inc., Oakland, CA (United States)
- Stanford Univ., CA (United States). Dept. of Physics
- Univ. of Orleans (France). Lab. of Physics and Chemistry of Environment and Space; Paris Observatory (France). Nancay radio telescope; Paris Observatory (France). GEPI
- Univ. of California, Santa Cruz, CA (United States). Dept. of Astronomy & Astrophysics
- National Astronomical Observatories-CAS, Urumqi (China)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1357321
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Astronomy and Astrophysics
- Additional Journal Information:
- Journal Volume: 492; Journal Issue: 3; Journal ID: ISSN 0004-6361
- Publisher:
- EDP Sciences
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; pulsars; Gamma-rays; Ephemerides
Citation Formats
Smith, D. A., Guillemot, L., Camilo, F., Cognard, I., Dumora, D., Espinoza, C., Freire, P. C. C., Gotthelf, E. V., Harding, A. K., Hobbs, G. B., Johnston, S., Kaspi, V. M., Kramer, M., Livingstone, M. A., Lyne, A. G., Manchester, R. N., Marshall, F. E., McLaughlin, M. A., Noutsos, A., Ransom, S. M., Roberts, M. S. E., Romani, R. W., Stappers, B. W., Theureau, G., Thompson, D. J., Thorsett, S. E., Wang, N., and Weltevrede, P. Pulsar timing for the Fermi gamma-ray space telescope. United States: N. p., 2008.
Web. doi:10.1051/0004-6361:200810285.
Smith, D. A., Guillemot, L., Camilo, F., Cognard, I., Dumora, D., Espinoza, C., Freire, P. C. C., Gotthelf, E. V., Harding, A. K., Hobbs, G. B., Johnston, S., Kaspi, V. M., Kramer, M., Livingstone, M. A., Lyne, A. G., Manchester, R. N., Marshall, F. E., McLaughlin, M. A., Noutsos, A., Ransom, S. M., Roberts, M. S. E., Romani, R. W., Stappers, B. W., Theureau, G., Thompson, D. J., Thorsett, S. E., Wang, N., & Weltevrede, P. Pulsar timing for the Fermi gamma-ray space telescope. United States. https://doi.org/10.1051/0004-6361:200810285
Smith, D. A., Guillemot, L., Camilo, F., Cognard, I., Dumora, D., Espinoza, C., Freire, P. C. C., Gotthelf, E. V., Harding, A. K., Hobbs, G. B., Johnston, S., Kaspi, V. M., Kramer, M., Livingstone, M. A., Lyne, A. G., Manchester, R. N., Marshall, F. E., McLaughlin, M. A., Noutsos, A., Ransom, S. M., Roberts, M. S. E., Romani, R. W., Stappers, B. W., Theureau, G., Thompson, D. J., Thorsett, S. E., Wang, N., and Weltevrede, P. Mon .
"Pulsar timing for the Fermi gamma-ray space telescope". United States. https://doi.org/10.1051/0004-6361:200810285. https://www.osti.gov/servlets/purl/1357321.
@article{osti_1357321,
title = {Pulsar timing for the Fermi gamma-ray space telescope},
author = {Smith, D. A. and Guillemot, L. and Camilo, F. and Cognard, I. and Dumora, D. and Espinoza, C. and Freire, P. C. C. and Gotthelf, E. V. and Harding, A. K. and Hobbs, G. B. and Johnston, S. and Kaspi, V. M. and Kramer, M. and Livingstone, M. A. and Lyne, A. G. and Manchester, R. N. and Marshall, F. E. and McLaughlin, M. A. and Noutsos, A. and Ransom, S. M. and Roberts, M. S. E. and Romani, R. W. and Stappers, B. W. and Theureau, G. and Thompson, D. J. and Thorsett, S. E. and Wang, N. and Weltevrede, P.},
abstractNote = {Here, we describe a comprehensive pulsar monitoring campaign for the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope (formerly GLAST). The detection and study of pulsars in gamma rays give insights into the populations of neutron stars and supernova rates in the Galaxy, into particle acceleration mechanisms in neutron star magnetospheres, and into the “engines” driving pulsar wind nebulae. LAT's unprecedented sensitivity between 20 MeV and 300 GeV together with its 2.4 sr field-of-view makes detection of many gamma-ray pulsars likely, justifying the monitoring of over two hundred pulsars with large spin-down powers. To search for gamma-ray pulsations from most of these pulsars requires a set of phase-connected timing solutions spanning a year or more to properly align the sparse photon arrival times. We describe the choice of pulsars and the instruments involved in the campaign. Attention is paid to verifications of the LAT pulsar software, using for example giant radio pulses from the Crab and from PSR B1937+21 recorded at Nançay, and using X-ray data on PSR J0218+4232 from XMM-Newton. We demonstrate accuracy of the pulsar phase calculations at the microsecond level.},
doi = {10.1051/0004-6361:200810285},
journal = {Astronomy and Astrophysics},
number = 3,
volume = 492,
place = {United States},
year = {Mon Oct 27 00:00:00 EDT 2008},
month = {Mon Oct 27 00:00:00 EDT 2008}
}
Web of Science
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