NVSS J082838+252827 , the SIMBAD biblio

NVSS J082838+252827 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:55:55

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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
1996ApJ...460...68E 36 71 A panoramic view of radio galaxy evolution from a redshift of 0 to a redshift of 4.3. EALES S.A. and RAWLINGS S.
2001MNRAS.323..417A 1 47 206 A submillimetre survey of the star formation history of radio galaxies. ARCHIBALD E.N., DUNLOP J.S., HUGHES D.H., et al.
2002MNRAS.335.1120W 50 34 Optical spectroscopy of radio galaxies in the 7C Redshift Survey. WILLOTT C.J., RAWLINGS S., BLUNDELL K.M., et al.
2003MNRAS.339..173W 74 176 Near-infrared imaging and the K -z relation for radio galaxies in the 7C Redshift Survey. WILLOTT C.J., RAWLINGS S., JARVIS M.J., et al.
2007ApJS..171..353S 1 69 226 The massive hosts of radio galaxies across cosmic time. SEYMOUR N., STERN D., DE BREUCK C., et al.
2008MNRAS.388..677W 15       D               1 72 11 Cosmological evolution of the Fanaroff-Riley type II source population. WANG Y. and KAISER C.R.
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.
2010ApJ...725...36D 203       D     X         6 74 95 The Spitzer high-redshift radio galaxy survey. DE BREUCK C., SEYMOUR N., STERN D., et al.
2012ApJ...749..169G 92       D       C       2 80 60 The mid-infrared environments of high-redshift radio galaxies. GALAMETZ A., STERN D., DE BREUCK C., et al.
2012A&A...548A..45D 15       D               1 128 26 Jet and torus orientations in high redshift radio galaxies. DROUART G., DE BREUCK C., VERNET J., 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.
2014MNRAS.438.1149G viz 15       D               1 355 78 The Wide-field Infrared Survey Explorer properties of complete samples of radio-loud active galactic nucleus. GURKAN G., HARDCASTLE M.J. and JARVIS M.J.
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.
2014A&A...566A..53D 15       D               4 71 81 Rapidly growing black holes and host galaxies in the distant Universe from the Herschel Radio Galaxy Evolution Project. DROUART G., DE BREUCK C., VERNET J., et al.
2017A&A...599A.123N 16       D               7 41 54 The SINFONI survey of powerful radio galaxies at z ∼ 2: Jet-driven AGN feedback during the Quasar Era. NESVADBA N.P.H., DE BREUCK C., LEHNERT M.D., et al.
2017A&A...600A.121N 23 15 Gas kinematics in powerful radio galaxies at z ∼ 2: Energy supply from star formation, AGN, and radio jets. NESVADBA N.P.H., DROUART G., DE BREUCK C., et al.
2021ApJS..255...22M viz 17       D               1 366 ~ An atlas of dynamical evolution models of 361 Fanaroff-Riley Type II radio sources. MACHALSKI J., KOZIEL-WIERZBOWSKA D. and GOYAL 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.
2021ApJ...922..197W viz 17       D               1 266 3 A novel method for estimating the ambient medium density around distant radio sources from their observed radio spectra. WOJTOWICZ A., STAWARZ L., MACHALSKI J., et al.
2023AstBu..78..443K viz 17       D               1 173 ~ Radio properties, radio spectra classification, radio variability parameters at a long time scale up to 30 years, radio loudness and radio luminosity estimate of high-redshift galaxies at z ≥ 1. KHABIBULLINA M., MIKHAILOV A., SOTNIKOVA YU., et al.

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