X-ray/radio data of high energy peaked BL Lacs (Giommi+, 2005)

Details X-ray/radio data of high energy peaked BL Lacs (Giommi+, 2005) X-ray/radio data of high energy peaked BL Lacs (Giommi+, 2005)

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..34340385g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/434/385. Originally published in: 2005A&A...434..385G

Computer Science

2

Bl Lac Objects, Surveys, X-Ray Sources, Radio Sources, Redshifts

Scientific paper

The fully identified complete sample including 150 extreme HBL BL Lacs is presented in Table 1 where we give the source name built with the catalog identification code SHBL (where S stands for "Sedentary" survey and HBL for High energy peaked BL Lacs) and the arcsecond precision optical coordinates of the source taken from the APM and COSMOS on-line services; we give also the RASS name, the X-ray flux (0.1-2.4keV), the radio flux (20cm, from the NVSS survey), and the optical apparent V magnitude (from APM and COSMOS) respectively; we give the redshift when available and the reference for the optical identification.
In Table 2 we report properties for five bright elliptical galaxies/low luminosity HBLs in the original sample of high fX/fr sources of Paper I (Giommi et al., 1999MNRAS.310..465G). In Table 3 the 19 rejected emission line AGNs together with their properties are presented.
(4 data files).

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