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  • Morokuma, Tomoki (author)

OISTER optical and near-infrared monitoring observations of peculiar radio-loud active galactic nucleus SDSSJ110006.07+442144.3

  • Article/chapterEnglish2017

Publisher, publication year, extent ...

  • 2017-09-01
  • Oxford University Press (OUP),2017
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-148860
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-148860URI
  • https://doi.org/10.1093/pasj/psx075DOI

Supplementary language notes

  • Language:English
  • Summary in:English

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  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • We present monitoring campaign observations at optical and near-infrared (NIR) wavelengths for a radio-loud active galactic nucleus (AGN) at z = 0.840, SDSSJ110006.07+442144.3 (hereafter, J1100+4421), which was identified during a flare phase in late 2014 February. The campaigns consist of three intensive observing runs from the discovery to 2015 March, mostly within the scheme of the OISTER collaboration. Optical-NIR light curves and simultaneous spectral energy distributions (SEDs) are obtained. Our measurements show the strongest brightening in 2015 March. We found that the optical-NIR SEDs of J1100+4421 show an almost steady shape despite the large and rapid intranight variability. This constant SED shape is confirmed to extend to similar to 5 mu m in the observed frame using the archival WISE data. Given the lack of absorption lines and the steep power-law spectrum of alpha(upsilon) similar to -1.4, where f(v) proportional to v(alpha upsilon), synchrotron radiation by a relativistic jet with no or small contributions from the host galaxy and the accretion disk seemsmost plausible as an optical-NIR emission mechanism. The steep optical-NIR spectral shape and the large amplitude of variability are consistent with this object being a low.peak jet-dominated AGN. In addition, sub-arcsecond resolution optical imaging data taken with Subaru Hyper Suprime-Cam does not show a clear extended component and the spatial scales are significantly smaller than the large extensions detected at radio wavelengths. The optical spectrum of a possible faint companion galaxy does not show any emission lines at the same redshift, and hence a merging hypothesis for this AGN-related activity is not supported by our observations.

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Added entries (persons, corporate bodies, meetings, titles ...)

  • Tanaka, Masaomi (author)
  • Tanaka, Yasuyuki T. (author)
  • Itoh, Ryosuke (author)
  • Tominaga, Nozomu (author)
  • Gandhi, Poshak (author)
  • Pian, Elena (author)
  • Mazzali, Paolo (author)
  • Ohta, Kouji (author)
  • Matsumoto, Emiko (author)
  • Shibata, Takumi (author)
  • Akimoto, Hinako (author)
  • Akitaya, Hiroshi (author)
  • Ali, Gamal B. (author)
  • Aoki, Tsutomu (author)
  • Doi, Mamoru (author)
  • Ebisuda, Nana (author)
  • Essam, Ahmed (author)
  • Fujisawa, Kenta (author)
  • Fukushima, Hideo (author)
  • Goda, Shuhei (author)
  • Gouda, Yuya (author)
  • Hanayama, Hidekazu (author)
  • Hashiba, Yasuhito (author)
  • Hashimoto, Osamu (author)
  • Hayashida, Kenzo (author)
  • Hiratsuka, Yuichiro (author)
  • Honda, Satoshi (author)
  • Imai, Masataka (author)
  • Inoue, Kanichiro (author)
  • Ishibashi, Michiko (author)
  • Iwata, Ikuru (author)
  • Izumiura, Hideyuki (author)
  • Kanda, Yuka (author)
  • Kawabata, Miho (author)
  • Kawaguchi, Kenji (author)
  • Kawai, Nobuyuki (author)
  • Kokubo, Mitsuru (author)
  • Kuroda, Daisuke (author)
  • Maehara, Hiroyuki (author)
  • Mito, Hiroyuki (author)
  • Mitsuda, Kazuma (author)
  • Miyagawa, Ryota (author)
  • Miyaji, Takeshi (author)
  • Miyamoto, Yusuke (author)
  • Morihana, Kumiko (author)
  • Moritani, Yuki (author)
  • Morokuma-Matsui, Kana (author)
  • Murakami, Kotone (author)
  • Murata, Katsuhiro L. (author)
  • Nagayama, Takahiro (author)
  • Nakamura, Kazuki (author)
  • Nakaoka, Tatsuya (author)
  • Niinuma, Kotaro (author)
  • Nishimori, Takafumi (author)
  • Nogami, Daisaku (author)
  • Oasa, Yumiko (author)
  • Oda, Tatsunori (author)
  • Ohshima, Tomohito (author)
  • Saito, Yoshihiko (author)
  • Sakata, Shuichiro (author)
  • Sako, Shigeyuki (author)
  • Sarugaku, Yuki (author)
  • Sawada-Satoh, Satoko (author)
  • Seino, Genta (author)
  • Sorai, Kazuo (author)
  • Soyano, Takao (author)
  • Taddia, FrancescoStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)ftadd (author)
  • Takahashi, Jun (author)
  • Takagi, Yuhei (author)
  • Takaki, Katsutoshi (author)
  • Takata, Koji (author)
  • Tarusawa, Ken'ichi (author)
  • Uemura, Makoto (author)
  • Ui, Takahiro (author)
  • Urago, Riku (author)
  • Ushioda, Kazutoshi (author)
  • Watanabe, Jun-ichi (author)
  • Watanabe, Makoto (author)
  • Yamashita, Satoshi (author)
  • Yanagisawa, Kenshi (author)
  • Yonekura, Yoshinori (author)
  • Yoshida, Michitoshi (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Nippon Tenmon Gakkai obun kenkyu hokoku: Oxford University Press (OUP)69:50004-6264
  • In:Publications of the Astronomical Society of Japan: Oxford University Press (OUP)69:52053-051X

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