Z 41-13 , the SIMBAD biblio

Z 41-13 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST18:40:07


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Title First 3 Authors
1975SoByu..47....3A 598 54 The galaxies of high surface brightness. ARAKELIAN M.A.
1981AJ.....86..820K 592 9 Accurate optical positions of Arakelian galaxies. KOJOIAN G., ELLIOTT R., BICAY M.D., et al.
1993ApJS...88..383L 579 102 H I 21 centimeter observations and I-band CCD surface photometry of spiral galaxies behind the Virgo cluster and toward its antipode. LU N.Y., HOFFMAN G.L., GROFF T., et al.
1998ApJS..119..277G viz 1085 28 A complete redshift survey to the Zwicky catalog limit in a 2hx15° region around 3C 273. GROGIN N.A., GELLER M.J. and HUCHRA J.P.
1999PASP..111..438F viz 14       D               1 19407 418 The updated Zwicky catalog (UZC). FALCO E.E., KURTZ M.J., GELLER M.J., 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.
2010ApJS..186..427N viz 15       D               1 14033 346 A catalog of detailed visual morphological classifications for 14,034 galaxies in the Sloan Digital Sky Survey. NAIR P.B. and ABRAHAM R.G.
2011MNRAS.416.2840L viz 15       D               1 72558 178 The 2M++ galaxy redshift catalogue. LAVAUX G. and HUDSON M.J.
2012MNRAS.421.1569B viz 15       D               3 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.
2012ApJS..199...26H viz 15       D               1 48926 517 The 2MASS Redshift Survey - Description and data release. HUCHRA J.P., MACRI L.M., MASTERS K.L., et al.
2013AJ....146..151O viz 15       D               1 10249 5 Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence. OH K., CHOI H., KIM H.-G., et al.
2015AJ....149..171T viz 16       D               1 49219 119 Galaxy groups: a 2MASS catalog. TULLY R.B.
2016A&A...588A..14T viz 16       D               2 84079 35 Friends-of-friends galaxy group finder with membership refinement. TEMPEL E., KIPPER R., TAMM A., et al.
2017ApJ...836..115O viz 16       D               1 838 4 Testing the presence of multiple photometric components in nearby early-type galaxies using SDSS. OH S., GREENE J.E. and LACKNER C.N.
2017MNRAS.471.2687B viz 16       D               1 7831 45 On the interdependence of galaxy morphology, star formation and environment in massive galaxies in the nearby Universe. BAIT O., BARWAY S. and WADADEKAR Y.
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.
2018A&A...618A..81T viz 16       D               1 50420 14 Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set. TEMPEL E., KRUUSE M., KIPPER R., et al.
2019ApJ...872..148C viz 16       D               1 15663 21 Radio sources in the nearby universe. CONDON J.J., MATTHEWS A.M. and BRODERICK J.J.
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.
2021ApJ...914..121A viz 17       D               1 43541 20 The NANOGrav 11 yr data set: limits on supermassive black hole binaries in galaxies within 500 Mpc. ARZOUMANIAN Z., BAKER P.T., BRAZIER A., et al.
2022ApJ...935..170A viz 17       D               1 44067 26 Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory. ABREU P., AGLIETTA M., ALBURY J.M., et al.
2023ApJS..267...41K viz 17       D               1 2026 ~ Minor Mergers Are Not Enough: The Importance of Major Mergers during Brightest Cluster Galaxy Assembly. KLUGE M. and BENDER R.
2023ApJS..269....3M viz 17       D               1 356397 ~ Siena Galaxy Atlas 2020. MOUSTAKAS J., LANG D., DEY A., et al.

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