IC 3171 , the SIMBAD biblio

IC 3171 , the SIMBAD biblio (34 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:52:49

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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
1986AJ.....91..204J 232 16 Radio continuum survey of the coma/A1367 supercluster. II. 1.5 GHz observations of 396 CGCG galaxies. JAFFE W. and GAVAZZI G.
1986MNRAS.219..511P 187 7 Taxonomical analysis of superclusters - II. The A 1367/Coma supercluster. PEREA J., MOLES M. and DEL OLMO A.
1995AJ....109..874B viz 1044 45 Kinematics and dynamics of the MKW/AWM poor clusters. BEERS T.C., KRIESSLER J.R., BIRD C.M., et al.
1999A&A...343...93G viz 425 20 On the local radio luminosity function of galaxies. II. Environmental dependences among late-type galaxies. GAVAZZI G. and BOSELLI A.
1999A&AS..140...89P viz 14       D               1 16703 9 Galaxy coordinates. II. Accurate equatorial coordinates for 17298 galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
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.
2000A&A...361..863G viz 1118 78 1.65 µm (H-band) surface photometry of galaxies. V. Profile decomposition of 1157 galaxies. GAVAZZI G., FRANZETTI P., SCODEGGIO M., et al.
2000A&AS..142...65G viz 560 25 1.65 µm (H-band) surface photometry of galaxies. III. Observations of 558 galaxies with the TIRGO 1.5 m telescope. GAVAZZI G., FRANZETTI P., SCODEGGIO M., et al.
2001ApJ...560..566K viz 14       D               4204 426 The K-band galaxy luminosity function. KOCHANEK C.S., PAHRE M.A., FALCO E.E., et al.
2001MNRAS.325..693H 210 52 X-ray luminosities of galaxies in groups. HELSDON S.F., PONMAN T.J., O'SULLIVAN E., 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.
2003AJ....126.2152R viz 15       D               15140 214 CAIRNS: the cluster and infall region nearby survey. I. Redshifts and mass profiles. RINES K., GELLER M.J., KURTZ M.J., et al.
2007ApJ...655..790C viz 15       D               13811 196 Groups of galaxies in the Two Micron All Sky redshift Survey. CROOK A.C., HUCHRA J.P., MARTIMBEAU N., et al.
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               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.
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.
2013A&A...560A..80P 15       D               1 88 8 The relationship between radio power at 22 and 43 GHz and black hole properties of AGN in elliptical galaxies. PARK S., SOHN B.W. and YI S.K.
2014ApJ...788...45T viz 15       D               1 224166 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2015AJ....149..171T viz 16       D               1 49219 119 Galaxy groups: a 2MASS catalog. TULLY R.B.
2015A&A...578A..61D viz 16       D               1 5680 7 Where are compact groups in the local Universe? DIAZ-GIMENEZ E. and ZANDIVAREZ A.
2015ApJ...812...89M viz 16       D               1 12670 7 ECO and RESOLVE: galaxy disk growth in environmental context. MOFFETT A.J., KANNAPPAN S.J., BERLIND A.A., et al.
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...837..120G viz 16       D               1 14404 66 LOSS revisited. I. Unraveling correlations between supernova rates and galaxy properties, as measured in a reanalysis of the Lick Observatory Supernova Search. GRAUR O., BIANCO F.B., HUANG S., et al.
2017ApJ...849...20E viz 16       D               1 9926 2 The baryonic collapse efficiency of galaxy groups in the RESOLVE and ECO surveys. ECKERT K.D., KANNAPPAN S.J., LAGOS C.D.P., 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.478.4336M viz 16       D               1 4285 3 Ultraviolet and optical view of galaxies in the Coma supercluster. MAHAJAN S., SINGH A. and SHOBHANA D.
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.
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.
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.
2021AJ....162..274L 334           X C       7 16 6 The ALFALFA almost dark galaxy AGC 229101: a 2 billion solar mass H I cloud with a very low surface brightness optical counterpart. LEISMAN L., RHODE K.L., BALL C., 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..269....3M viz 17       D               1 356397 ~ Siena Galaxy Atlas 2020. MOUSTAKAS J., LANG D., DEY A., et al.
2026ApJ..1000..108S 20       D               1 156 ~ A FAST Survey of H I Absorption in Low-power Radio Sources. SU Y., YU Q., FANG T., et al.

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