The X-ray to infrared energy distribution of the quasar PG 0026+129

Details The X-ray to infrared energy distribution of the quasar PG 0026+129 The X-ray to infrared energy distribution of the quasar PG 0026+129

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...330..178t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 330, July 1, 1988, p. 178-183. CNR-supported research.

Astronomy and Astrophysics

Astronomy

8

Energy Distribution, Infrared Sources (Astronomy), Optical Emission Spectroscopy, Quasars, Stellar Spectrophotometry, X Ray Sources, Active Galactic Nuclei, Energy Bands, Exosat Satellite, Heao 2

Scientific paper

PG 0026+129 was observed with EXOSAT in 1983 and 1984. No variation between the two epochs was detected. The energy distribution from 0.2 to 6 keV is well fitted by a power law of energy index alpha = 1.06 + or - 0.25 and with Galactic absorption. Quasi-simultaneous spectrophotometry in the UV and optical range, together with near-infrared photometry was obtained. The results are compared with previous observations. The overall energy distribution and its variability are briefly discussed.

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