Polarization and variability of compact sources measured in Planck time-ordered data

被引:2
|
作者
Rocha, G. [1 ,2 ]
Keskitalo, R. [3 ]
Partridge, B. [4 ]
Marscher, A. [5 ]
O'Dea, C. [6 ]
Pearson, T. J. [2 ,7 ]
Gorski, K. M. [1 ,8 ]
机构
[1] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[2] CALTECH, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[3] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA
[4] Haverford Coll, Astron Dept, 370 Lancaster Ave, Haverford, PA USA
[5] Boston Univ, Inst Astrophys Res, 725 Commonwealth Ave, Boston, MA 02215 USA
[6] Univ Manitoba, Winnipeg, MB, Canada
[7] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA
[8] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland
基金
加拿大自然科学与工程研究理事会; 美国国家航空航天局;
关键词
polarization; galaxies; active; black hole physics; formation; evolution; quasars; general; ACTIVE GALACTIC NUCLEI; RADIO JET; ASTROPY; SCALE; M87;
D O I
10.1051/0004-6361/202141995
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper introduces a new Planck Catalog of Polarized and Variable Compact Sources (PCCS-PV) comprising 153 sources, the majority of which are extragalactic. The data include both the total flux density and linear polarization measured by Planck with frequency coverage from 30 to 353 GHz, and temporal spacing ranging from days to years. We classify most sources as beamed, extragalactic radio sources; the catalog also includes several radio galaxies, Seyfert galaxies, and Galactic and Magellanic Cloud sources, including H II regions and planetary nebulae. An advanced extraction method applied directly to the multifrequency Planck time-ordered data, rather than the mission sky maps, was developed to allow an assessment of the variability of polarized sources. Our analysis of the time-ordered data from the Planck mission, tod2flux, allowed us to catalog the time-varying emission and polarization properties for these sources at the full range of polarized frequencies employed by Planck, 30-353 GHz. PCCS-PV provides the time-and frequency-dependent, polarized flux densities for all 153 sources. To illustrate some potential applications of the PCCS-PV, we conducted preliminary comparisons of our measurements of selected sources with published data from other astronomical instruments. In summary, we find general agreement between the Planck and the Institut de Radioastronomie Millimetrique (IRAM) polarization measurements as well as with the Metsahovi 37 GHz values at closely similar epochs. These combined measurements also show the value of PCCS-PV results and the PCCS2 catalog for filling in missing spectral (or temporal) coverage and helping to define the spectral energy distributions of extragalactic sources. In turn, these results provide useful clues as to the physical properties of the sources.
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页数:17
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