VLBI Observations of the Most Radio-Loud, Narrow-Line Quasar SDSS J094857.3 + 002225

• Published in: Publications of the Astronomical Society of Japan 2006-10, Vol.58 (5), p.829-834
• Main Authors: Doi, Akihiro, Nagai, Hiroshi, Asada, Keiichi, Kameno, Seiji, Wajima, Kiyoaki, Inoue, Makoto
• Format: Article
• Language: English
• ISSN: 0004-6264; 2053-051X
• DOI: 10.1093/pasj/58.5.829

We observed the narrow-line quasar SDSS J094857.3 $+$ 002225, which is known to have the highest radio loudness in the narrow-line Seyfert 1 galaxies (NLS1s), at 1.7–15.4 GHz with the Very Long Baseline Array (VLBA). This is the first very-long-baseline interferometry (VLBI) investigation of a radio-loud NLS1. We independently discovered (1) very high brightness temperatures from its compactness in a VLBA image and (2) flux variation among the VLBA observation and our other observations with the VLBA and the Very Large Array (VLA). A Doppler factor larger than 2.7–5.5 was required to meet an intrinsic limit of brightness temperature in the rest frame. This is evidence for highly relativistic nonthermal jets in an NLS1. We suggest that the Doppler factor is one of the most important parameters in the determination of the radio loudness of NLS1s. The accretion disk of SDSS J094857.3 $+$ 002225 is probably in a very high state, rather than the high/soft state, by analogy with X-ray binaries with strong radio outbursts and superluminal jets, such as GRS 1915 $+$ 105.