The Identification Of The X-Ray Counterpart To PSR J2021+4026
Abstract
We report the probable identification of the X-ray counterpart to the γ-ray pulsar PSR J2021+4026 using imaging with the Chandra X-ray Observatory ACIS and timing analysis with the Fermi satellite. Given the statistical and systematic errors, the positions determined by both satellites are coincident. The X-ray source position is R.A. 20h21m30s.733, Decl. +40°26'46.04" (J2000) with an estimated uncertainty of 1."3 combined statistical and systematic error. Moreover, both the X-ray to γ-ray and the X-ray to optical flux ratios are sensible assuming a neutron star origin for the X-ray flux. The X-ray source has no cataloged infrared-to-visible counterpart and, through new observations, we set upper limits to its optical emission of i' > 23.0 mag and r' > 25.2 mag. The source exhibits an X-ray spectrum with most likely both a powerlaw and a thermal component. We also report on the X-ray and visible light properties of the 43 other sources detected in our Chandra observation.
- Authors:
-
- NASA Marshall Space Flight Center (MSFC), Huntsville, AL (United States)
- Stanford Univ., CA (United States)
- National Inst. of Nuclear Physics (INFN), Pisa (Italy); Univ. of California, Santa Cruz, CA (United States); Univ. of Pisa (Italy)
- Univ. of California, Santa Cruz, CA (United States); Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Univ. of Pavia (Italy)
- Univ. of California, Santa Cruz, CA (United States)
- Naval Research Lab. (NRL), Washington, DC (United States)
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- National Inst. of Astrophysics (Mexico)
- Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Istituto Nazionale di Fisica Nucleare (INFN), Pavia (Italy); Istituto Universitario di Studi Superiori (IUSS), Pavia (Italy)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1356779
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 743; Journal Issue: 1; Journal ID: ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Weisskopf, Martin C., Romani, Roger W., Razzano, Massimiliano, Belfiore, Andrea, Saz Parkinson, Pablo, Ray, Paul S., Kerr, Matthew, Harding, Alice, Swartz, Douglas A., Carramiñana, Alberto, Ziegler, Marcus, Becker, Werner, De Luca, Andrea, Dormody, Michael, Thompson, David J., Kanbach, Gottfried, Elsner, Ronald F., O'Dell, Stephen L., and Tennant, Allyn F. The Identification Of The X-Ray Counterpart To PSR J2021+4026. United States: N. p., 2011.
Web. doi:10.1088/0004-637X/743/1/74.
Weisskopf, Martin C., Romani, Roger W., Razzano, Massimiliano, Belfiore, Andrea, Saz Parkinson, Pablo, Ray, Paul S., Kerr, Matthew, Harding, Alice, Swartz, Douglas A., Carramiñana, Alberto, Ziegler, Marcus, Becker, Werner, De Luca, Andrea, Dormody, Michael, Thompson, David J., Kanbach, Gottfried, Elsner, Ronald F., O'Dell, Stephen L., & Tennant, Allyn F. The Identification Of The X-Ray Counterpart To PSR J2021+4026. United States. https://doi.org/10.1088/0004-637X/743/1/74
Weisskopf, Martin C., Romani, Roger W., Razzano, Massimiliano, Belfiore, Andrea, Saz Parkinson, Pablo, Ray, Paul S., Kerr, Matthew, Harding, Alice, Swartz, Douglas A., Carramiñana, Alberto, Ziegler, Marcus, Becker, Werner, De Luca, Andrea, Dormody, Michael, Thompson, David J., Kanbach, Gottfried, Elsner, Ronald F., O'Dell, Stephen L., and Tennant, Allyn F. Wed .
"The Identification Of The X-Ray Counterpart To PSR J2021+4026". United States. https://doi.org/10.1088/0004-637X/743/1/74. https://www.osti.gov/servlets/purl/1356779.
@article{osti_1356779,
title = {The Identification Of The X-Ray Counterpart To PSR J2021+4026},
author = {Weisskopf, Martin C. and Romani, Roger W. and Razzano, Massimiliano and Belfiore, Andrea and Saz Parkinson, Pablo and Ray, Paul S. and Kerr, Matthew and Harding, Alice and Swartz, Douglas A. and Carramiñana, Alberto and Ziegler, Marcus and Becker, Werner and De Luca, Andrea and Dormody, Michael and Thompson, David J. and Kanbach, Gottfried and Elsner, Ronald F. and O'Dell, Stephen L. and Tennant, Allyn F.},
abstractNote = {We report the probable identification of the X-ray counterpart to the γ-ray pulsar PSR J2021+4026 using imaging with the Chandra X-ray Observatory ACIS and timing analysis with the Fermi satellite. Given the statistical and systematic errors, the positions determined by both satellites are coincident. The X-ray source position is R.A. 20h21m30s.733, Decl. +40°26'46.04" (J2000) with an estimated uncertainty of 1."3 combined statistical and systematic error. Moreover, both the X-ray to γ-ray and the X-ray to optical flux ratios are sensible assuming a neutron star origin for the X-ray flux. The X-ray source has no cataloged infrared-to-visible counterpart and, through new observations, we set upper limits to its optical emission of i' > 23.0 mag and r' > 25.2 mag. The source exhibits an X-ray spectrum with most likely both a powerlaw and a thermal component. We also report on the X-ray and visible light properties of the 43 other sources detected in our Chandra observation.},
doi = {10.1088/0004-637X/743/1/74},
journal = {The Astrophysical Journal},
number = 1,
volume = 743,
place = {United States},
year = {Wed Nov 23 00:00:00 EST 2011},
month = {Wed Nov 23 00:00:00 EST 2011}
}
Web of Science
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