NVSS J085053+475348 , the SIMBAD biblio

NVSS J085053+475348 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST00:40:53

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2005MNRAS.362....9B viz 15       D               2707 245 A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey. BEST P.N., KAUFFMANN G., HECKMAN T.M., et al.
2009MNRAS.395..255M viz 15       D               1 397035 82 Compact groups in theory and practice - III. Compact groups of galaxies in the sixth data release of the Sloan Digital Sky Survey. McCONNACHIE A.W., PATTON D.R., ELLISON S.L., et al.
2010A&A...511A..53V viz 15       D               1 107940 39 The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. VOLLMER B., GASSMANN B., DERRIERE S., et al.
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.
2012MNRAS.421.1569B viz 15       D               3 18499 511 On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. BEST P.N. and HECKMAN T.M.
2013ApJ...765...62S viz 16       D               1 409 33 Constraining jet production scenarios by studies of narrow-line radio galaxies. SIKORA M., STASINSKA G., KOZIEL-WIERZBOWSKA D., et al.
2017MNRAS.466.4346M viz 16       D               1 1437 66 The nuclear properties and extended morphologies of powerful radio galaxies: the roles of host galaxy and environment. MIRAGHAEI H. and BEST P.N.
2018AJ....155..188L viz 16       D               1 13494 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.
2021A&A...655A..17S viz 17       D               1 338596 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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