NVSS J011755+394432 , the SIMBAD biblio

NVSS J011755+394432 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST13:41:42


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Title First 3 Authors
1989AJ.....98..419V viz 1091 103 Structures, spectral indexes, and optical identifications of radio sources selected from the B3 catalogue. VIGOTTI M., GRUEFF G., PERLEY R., et al.
1998MNRAS.295..265B 14       D               1 39 62 A sample of 6C radio sources designed to find objects at redshift z>4. I. The radio data. BLUNDELL K.M., RAWLINGS S., EALES S.A., et al.
1999A&AS..135..299V 49 5 Infrared imaging of WENSS radio sources. VILLANI D. and DI SEREGO ALIGHIERI S.
1999A&AS..139..359V viz 1047 11 Multi-frequency study of the B3-VLA sample. II. The database. VIGOTTI M., GREGORINI L., KLEIN U., et al.
2001MNRAS.326.1563J 34 49 A sample of 6C radio sources designed to find objects at redshift z > 4 - II. Spectrophotometry and emission-line properties. JARVIS M.J., RAWLINGS S., LACY M., et al.
2001MNRAS.326.1585J 1 33 133 A sample of 6C radio sources designed to find objects at redshift z>4 - III. Imaging and the radio galaxy K-z relation. JARVIS M.J., RAWLINGS S., EALES S., et al.
2008A&ARv..15...67M 15       D               4 222 321 Distant radio galaxies and their environments. MILEY G. and DE BREUCK C.
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.
2013ApJ...769...79W viz 16       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 16       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.
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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