NVSS J045226-173752 , the SIMBAD biblio

NVSS J045226-173752 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST23:21:16


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2000A&A...362..519D viz 159 110 A statistical study of emission lines from high redshift radio galaxies. DE BREUCK C., ROETTGERING H., MILEY G., et al.
2000A&AS..143..303D viz 680 171 A sample of 669 ultra steep spectrum radio sources to find high redshift radio galaxies. DE BREUCK C., VAN BREUGEL W., ROETTGERING H.J.A., et al.
2001AJ....121.1241D 58 71 Spectroscopy of ultra-steep-spectrum radio sources. DE BREUCK C., VAN BREUGEL W., ROETTGERING H., et al.
2002AJ....123..637D viz 266 166 Optical and near-infrared imaging of ultra-steep-spectrum radio sources: the K-z diagram of radio-selected and optically selected galaxies. DE BREUCK C., VAN BREUGEL W., STANFORD S.A., et al.
2008A&ARv..15...67M 15       D               2 222 321 Distant radio galaxies and their environments. MILEY G. and DE BREUCK C.
2010A&A...511A..53V viz 15       D               1 107473 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.
2013ApJ...769...79W viz 15       D               1 392 164 Galaxy clusters around radio-loud active galactic nuclei at 1.3 < z < 3.2 as seen by Spitzer. WYLEZALEK D., GALAMETZ A., STERN D., et al.
2014ApJ...786...17W viz 15       D               1 426 38 The galaxy cluster mid-infrared luminosity function at 1.3 < z < 3.2. WYLEZALEK D., VERNET J., DE BREUCK C., et al.
2016MNRAS.462..421H 16       D               2 8 4 Early quenching of massive protocluster galaxies around z = 2.2 radio galaxies. HUSBAND K., BREMER M.N., STOTT J.P., et al.
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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