VizieR Online Data Catalog: Multiwavelength light curves of PG 1553+113 (Huang+, 2021)

We collected γ-ray data of PG 1553+113 from the Fermi-LAT data website obtained during 8yr from 2012-2020 January 1. See Section 2.1.

The Swift X-ray Telescope (XRT) is one of the instruments on the Neil Gehrels Swift observatory with a sensitive broadband detector for X-ray from 0.3-10keV. The data from 2012-2020 January 1 were retrieved from the High Energy Astrophysics Science Archive Research Center website. See Section 2.2.1.

UV/Optical Telescope (UVOT), covering wavelength range 170-600nm, 7 filters (v, b, u, uvw1, uvm2, uvw2 and white), with field of view 17'x17', is one of instruments on the Swift observatory. See Section 2.2.2.

XMM-Newton is an X-ray observatory, and its main instrument is the European Photon Imaging Camera, consisting of two MOS detectors and a pn camera, which operate in the 0.2-12.0keV energy range. Totally, 24 sets of observations of PG 1553+113 obtained from 2001-2020 were employed. See Section 2.3.

The 40m telescope at the Owens Valley Radio Observatory (OVRO), is monitoring more than 1800 blazars (Richards+ 2011, J/ApJS/194/29). We obtain the 15GHz data covering from 2012-2020 January from the public data archived website.

(1 data file).