NVSS J131104-000255 , the SIMBAD biblio

NVSS J131104-000255 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:20:58

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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
2003MNRAS.344..307L viz 63299 194 The Millennium Galaxy Catalogue: 16 ≤BMGC< 24 galaxy counts and the calibration of the local galaxy luminosity function. LISKE J., LEMON D.J., DRIVER S.P., et al.
2009ApJ...692..511W viz 15       D               1 3632 20 Mergers of luminous early-type galaxies in the local universe and gravitational wave background. WEN Z.L., LIU F.S. and HAN J.L.
2011MNRAS.416..727C viz 15       D               1 3386 57 The Padova–Millennium galaxy and group catalogue (PM2GC): the group-finding method and the PM2GC catalogues of group, binary and single field galaxies. CALVI R., POGGIANTI B.M. and VULCANI B.
2013ApJ...762...77P viz 15       D               1 999 152 Superdense galaxies and the mass-size relation at low redshift. POGGIANTI B.M., CALVI R., BINDONI D., et al.
2013MNRAS.432.3141C viz 15       D               1 3210 26 The impact of global environment on galaxy mass functions at low redshift. CALVI R., POGGIANTI B.M., VULCANI B., et al.
2018AJ....155..188L viz 16       D               1 13497 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.
2018MNRAS.481.2458D viz 16       D               1 31575 ~ On the nature of small galaxy systems. DUPLANCIC F., COLDWELL G.V., ALONSO S., et al.
2020ApJS..247...53K viz 16       D               1 23378 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.
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.

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