NVSS J141541-011105 , the SIMBAD biblio

NVSS J141541-011105 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST23:58:12


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Title First 3 Authors
2002MNRAS.329..227S viz 915 225 Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHz. SADLER E.M., JACKSON C.A., CANNON R.D., 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.
2005MNRAS.362....9B viz 15       D               2708 245 A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey. BEST P.N., KAUFFMANN G., HECKMAN T.M., et al.
2012MNRAS.421.1569B viz 15       D               2 18458 511 On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. BEST P.N. and HECKMAN T.M.
2015MNRAS.452.2087L viz 16       D               1 71490 449 Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. LISKE J., BALDRY I.K., DRIVER S.P., et al.
2016A&A...590A..29P viz 16       D               1 13088 7 Multifrequency studies of galaxies and groups. I. Environmental effect on galaxy stellar mass and morphology. POUDEL A., HEINAMAKI P., NURMI P., et al.
2019ApJS..244....3D viz 16       D               1 23803 ~ Circumventing the effects of projection and dust using inclination-independent infrared galaxy structure measurements: method, error analysis, and a new public catalog of near-infrared galaxy structures. DEVOUR B.M. and BELL E.F.
2022MNRAS.509.3966W viz 17       D               1 89291 61 Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies. WALMSLEY M., LINTOTT C., GERON T., et al.
2022MNRAS.513..439D viz 17       D               1 302202 70 Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions. DRIVER S.P., BELLSTEDT S., ROBOTHAM A.S.G., et al.

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