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arXiv · 1108.3987

The Identification of the X-ray Counterpart to PSR J2021+4026

Martin C. Weisskopf·Roger W. Romani·Massimiliano Razzano·Andrea Belfiore·Pablo Saz Parkinson·Paul S. Ray·Matthew Kerr·Alice Harding·Douglas A. Swartz·Alberto Carraminana·Marcus Ziegler·Werner Becker·Andrea De Luca·Michael Dormody·David J. Thompson·Gottfried Kanbach·Ronald F. Elsner·Stephen L. O'Dell·Allyn F. Tennant
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Abstract

We report the probable identification of the X-ray counterpart to the gamma-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. 20h21m30.733s, Decl. +40 deg 26 min 46.04sec (J2000) with an estimated uncertainty of 1.3 arsec combined statistical and systematic error. Moreover, both the X-ray to gamma-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' > 25.2mag. 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.

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Martin C. Weisskopf, Roger W. Romani, Massimiliano Razzano, Andrea Belfiore, Pablo Saz Parkinson, Paul S. Ray, Matthew Kerr, Alice Harding, Douglas A. Swartz, Alberto Carraminana, Marcus Ziegler, Werner Becker, Andrea De Luca, Michael Dormody, David J. Thompson, Gottfried Kanbach, Ronald F. Elsner, Stephen L. O'Dell, Allyn F. Tennant. 2011-08-19. The Identification of the X-ray Counterpart to PSR J2021+4026. https://doi.org/10.1088/0004-637x/743/1/74

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