NVSS J233458+154549 , the SIMBAD biblio

NVSS J233458+154549 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST10:40:38


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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
1999A&AS..135..299V 49 5 Infrared imaging of WENSS radio sources. VILLANI D. and DI SEREGO ALIGHIERI S.
2001AJ....121.1241D 58 71 Spectroscopy of ultra-steep-spectrum radio sources. DE BREUCK C., VAN BREUGEL W., ROETTGERING H., et al.
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2007MNRAS.375.1299V 68 46 Lyα excess in high-redshift radio galaxies: a signature of star formation. VILLAR-MARTIN M., HUMPHREY A., DE BREUCK C., et al.
2008A&ARv..15...67M 89       D       C       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...780..134S 78             C       1 7 15 A search for moderate-redshift survivors from the population of luminous compact passive galaxies at high redshift. STOCKTON A., SHIH H.-Y., LARSON K., 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.
2015ApJ...815...50S 468           X C       11 4 1 A compact group of galaxies at z = 2.48 hosting an AGN-driven outflow. SHIH H.-Y. and STOCKTON A.
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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