NVSS J165456+223820 , the SIMBAD biblio

NVSS J165456+223820 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:32:39


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Keywords
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Title First 3 Authors
2010ApJ...723.1119L viz 15       D               1 1041 41 On the populations of radio galaxies with extended morphology at z < 0.3. LIN Y.-T., SHEN Y., STRAUSS M.A., et al.
2010ApJS..191..254H viz 15       D               1 20101 235 A GMBCG galaxy cluster catalog of 55,424 rich clusters from SDSS DR7. HAO J., McKAY T.A., KOESTER B.P., et al.
2011ApJ...736...21S viz 15       D               1 195565 104 An optical catalog of galaxy clusters obtained from an adaptive matched filter finder applied to Sloan Digital Sky Survey Data Release 6. SZABO T., PIERPAOLI E., DONG F., et al.
2012MNRAS.421.1569B viz 15       D               2 18458 511 On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. BEST P.N. and HECKMAN T.M.
2012ApJ...756..116A viz 15       D               1 156 20 The lifetime and powers of FR IIs in galaxy clusters. ANTOGNINI J., BIRD J. and MARTINI P.
2015ApJ...807..178W viz 16       D               1 1191 98 Calibration of the optical mass proxy for clusters of galaxies and an update of the WHL12 cluster catalog. WEN Z.L. and HAN J.L.
2016MNRAS.460.3669Y viz 16       D               1 7138 25 Radio luminosity function of brightest cluster galaxies. YUAN Z.S., HAN J.L. and WEN Z.L.
2018AJ....155..188L viz 16       D               1 13497 1 An analysis framework for understanding the origin of nuclear activity in low-power radio galaxies. LIN Y.-T., HUANG H.-J. and CHEN Y.-C.
2020ApJS..247...53K viz 16       D               1 23378 20 Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N.
2021A&A...655A..17S viz 17       D               1 338578 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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