Chandra Multi-wavelength Plane Survey

Authors
  • P. Zhao
  • J.E. Grindlay
  • J. Hong
  • M. Servillat
Publication date 2013
Journal Proceedings of the International Astronomical Union
Event IAU Symposium 290"Feeding compact objects: Accretion on all scales
Volume | Issue number 8 | S290
Pages (from-to) 157-160
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract Chandra Multi-wavelength Plane Survey (ChaMPlane) surveys the X-ray point sources discovered by the Chandra X-ray Observatory in the galactic plane in order to constrain the populations of faint (L x ≤ 1033 erg/s) accretion-powered sources in the Galaxy. This multi-wavelength survey includes data from the Chandra archive, as well as optical and infrared images and spectra. This paper summarizes a few selected highlights.
Document type Article
Note In Volume 8, S290 (August 2012) © 2013. - Part of Symposium: Feeding compact objects: Accretion on all scales.
Language English
Published at
https://doi.org/10.1017/S1743921312019436 (Final published version)
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