SDSS J102727.90+305902.4 , the SIMBAD biblio

SDSS J102727.90+305902.4 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST06:46:34


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Title First 3 Authors
2010ApJ...708..427L viz 15       D               1 174 147 Type 2 active galactic nuclei with double-peaked [O III] lines: narrow-line region kinematics or merging supermassive black hole pairs? LIU X., SHEN Y., STRAUSS M.A., et al.
2010ApJ...716..866S viz 15       D               1 149 163 A search for binary active galactic nuclei: double-peaked [O III] AGNs in the Sloan Digital Sky Survey. SMITH K.L., SHIELDS G.A., BONNING E.W., et al.
2012ApJ...753...42C viz 15       D               1 82 81 Kiloparsec-scale spatial offsets in double-peaked narrow-line active galactic nuclei. I. Markers for selection of compelling dual active galactic nucleus candidates. COMERFORD J.M., GERKE B.F., STERN D., et al.
2012ApJS..201...31G viz 15       D               1 15561 75 Double-peaked narrow emission-line galaxies from the Sloan Digital Sky Survey. I. Sample and basic properties. GE J.-Q., HU C., WANG J.-M., et al.
2014ApJ...788...45T viz 16       D               1 224162 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2015ApJ...813..103M 335       D S   X C       7 43 98 The origin of double-peaked narrow lines in active galactic nuclei. I. Very large array detections of dual AGNs and AGN outflows. MULLER-SANCHEZ F., COMERFORD J.M., NEVIN R., et al.
2018MNRAS.474.1873W viz 16       D               1 35335 23 Spectral classification and composites of galaxies in LAMOST DR4. WANG L.-L., LUO A.-L., SHEN S.-Y., et al.
2018ApJ...867...66C viz 16       D               1 95 8 The origin of double-peaked narrow lines in active galactic nuclei. IV. Association with galaxy mergers. COMERFORD J.M., NEVIN R., STEMO A., et al.
2019MNRAS.484.4933R 17       D               1 88 28 Searching for dual AGN in galaxies with double-peaked emission line spectra using radio observations. RUBINUR K., DAS M. and KHARB P.

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