NVSS J134033+401731 , the SIMBAD biblio

NVSS J134033+401731 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.05CEST20:07:22


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Title First 3 Authors
2000MNRAS.312..139J 1 17 60 Multiwavelength observations of an evolved galaxy group: an end-point of galaxy merging?. JONES L.R., PONMAN T.J. and FORBES D.A.
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2007MNRAS.377..787B viz 4391 7 Properties of luminous red galaxies in the Sloan Digital Sky Survey. BARBER T., MEIKSIN A. and MURPHY T.
2009AJ....138..502M 15       D               1 47 15 An optical and X-ray study of the fossil group RX J1340.6+4018. MENDES DE OLIVEIRA C.L., CYPRIANO E.S., DUPKE R.A., et al.
2009ApJ...705.1336C viz 15       D               1 108 44 Probing the balance of AGN and star-forming activity in the local universe with ChaMP. CONSTANTIN A., GREEN P., ALDCROFT T., et al.
2010MNRAS.406..197B viz 15       D               1 137 13 Radio galaxies in the Sloan Digital Sky Survey: spectral index-environment correlations. BORNANCINI C.G., O'MILL A.L., GUROVICH S., et al.
2013ApJ...778..188T viz 16       D               1 617 17 Empirical links between XRB and AGN accretion using the complete z < 0.4 spectroscopic CSC/SDSS catalog. TRICHAS M., GREEN P.J., CONSTANTIN A., et al.
2015ApJ...807..178W viz 16       D               1 1191 98 Calibration of the optical mass proxy for clusters of galaxies and an update of the WHL12 cluster catalog. WEN Z.L. and HAN J.L.
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.
2020ApJS..247...53K viz 17       D               1 23374 20 Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N.

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