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The loud and the quiet: Searching for radio counterparts of two radio-weak BL Lac candidates with VLBI

Cao, Hong Min (författare)
Shangqiu Normal University,Chinese Academy of Sciences
Frey, Sándor (författare)
Magyar Tudomanyos Akademia,Hungarian Academy of Sciences
Gabányi, Krisztina E. (författare)
Magyar Tudomanyos Akademia,Hungarian Academy of Sciences
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Yang, Jun, 1979 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Cui, Lang (författare)
Chinese Academy of Sciences
Hong, X. Y. (författare)
Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences
An, Tao (författare)
Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences
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 (creator_code:org_t)
2018-10-04
2019
Engelska.
Ingår i: Monthly Notices of the Royal Astronomical Society: Letters. - : Oxford University Press (OUP). - 1745-3925 .- 1745-3933. ; 482:1, s. L34-L39
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • BL Lac objects are known to have compact jets inclined to our line of sight at a small angle, showing prominent radio emission. Two radio-weak BL Lac candidates with no counterparts in current radio surveys were recently reported by Massaro et al. Both sources were selected as candidate low-energy counterparts of unassociated Fermi γ -ray sources. We carried out very long baseline interferometry (VLBI) observations with the European VLBI Network (EVN) at 5 GHz to explore their radio properties at the milliarcsecond (mas) scale. One target, J1410+7405, is clearly detected with the EVN. Its measured 5-GHz flux density, 2.4 mJy, is consistent with recent interferometricmeasurementswith theKarlG. JanskyVery LargeArray, suggesting that the radio emission is confined to the inner ≲10-mas region. J1410+7405 is therefore identified as a radio-loud jetted active galactic nucleus, and its brightness temperature exceeds ~109 K. Its properties are similar to those of other γ -ray-detected BL Lac objects. On the other hand, the second target, J0644+6031, remains undetected with the EVN with a 6s brightness upper limit of 0.12 mJy beam-1. This source is thus radio-quiet, confirming its peculiarity, or possibly questioning its BL Lac nature.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Nyckelord

Galaxies: individual: J1410+7405
BL Lacertae objects: general
Galaxies: individual: J0644+6031
Galaxies: active
Quasars: general

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