4.7 Article

RoboPol: AGN polarimetric monitoring data

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 501, Issue 3, Pages 3715-3726

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/staa3777

Keywords

polarization; galaxies: active; galaxies: jets; galaxies: nuclei

Funding

  1. 'RoboPol' project
  2. European Social Fund (ESF)
  3. Greek National Resources
  4. European Commission [PCIG10-GA-2011-304001, PIRSES-GA-2012-31578, PCIG-GA-2011-293531]
  5. NASA [NNX11A043G]
  6. NSF [AST-1109911]
  7. Polish National Science Centre [2011/01/B/ST9/04618, 2017/25/B/ST9/02805]
  8. European Research Council (ERC) under the European Union [771282]
  9. NASA Hubble Fellowship - Space Telescope Science Institute under NASA [HST-HF2-51444.001-A, NAS5-26555]
  10. Academy of Finland [317383, 320085, 322535]

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This study presents uniformly reprocessed and re-calibrated data from the RoboPol programme of optopolarimetric monitoring of active galactic nuclei (AGNs) between 2013 and 2017, covering a total of 5068 observations of 222 AGNs with Dec. > -25(circle). The current version of the RoboPol pipeline used to process and calibrate the entire data set is described, with average quantities summarizing optopolarimetric behaviour provided for each source observed and for the time interval followed.
We present uniformly reprocessed and re-calibrated data from the RoboPol programme of optopolarimetric monitoring of active galactic nuclei (AGNs), covering observations between 2013, when the instrument was commissioned, and 2017. In total, the data set presented in this paper includes 5068 observations of 222 AGN with Dec. > -25(circle). We describe the current version of the RoboPol pipeline that was used to process and calibrate the entire data set, and we make the data publicly available for use by the astronomical community. Average quantities summarizing optopolarimetric behaviour (average degree of polarization, polarization variability index) are also provided for each source we have observed and for the time interval we have followed it.

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