UGC 1065 , the SIMBAD biblio

UGC 1065 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST05:38:16


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Title First 3 Authors
1982ApJS...50..319T 563 53 Double galaxy investigations. I. Observations. TIFFT W.G.
1983A&A...121...26A 81 6 Pairs of spiral galaxies with magnitude differences greater than one. ARP H., GIRAUD E., SULENTIC J.W., et al.
1985Ap&SS.116..333P 34 1 Some spectrophotometric data for 31 galaxies from Karchentsev's list. PETROV G.T., KOVACHEV B.Z. and MINEVA V.A.
1986AJ.....91..255B 79 162 Star-formation rates in the nuclei of violently interacting galaxies. BUSHOUSE H.A.
1987ApJ...320...49B 120 274 Global properties of interacting disk-type galaxies. BUSHOUSE H.A.
1988ApJ...335...74B 248 144 IRAS observations of an optically selected sample of interacting galaxies. BUSHOUSE H.A., LAMB S.A. and WERNER M.W.
1990ApJ...355..393W 314 8 A redshift survey toward a proposed void of galaxies suggested by the distribution of Abell clusters. WILLICK J.A., BRODIE J.P. and BOWYER S.
1999A&AS..140...89P viz 14       D               1 16701 9 Galaxy coordinates. II. Accurate equatorial coordinates for 17298 galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
1999AJ....117.1668H 1731 89 The I-band Tully-Fisher relation for Sc galaxies: optical imaging data. HAYNES M.P., GIOVANELLI R., SALZER J.J., et al.
1999AJ....117.2039H viz 1272 119 The I-band Tully-Fisher relation for Sc galaxies: 21 centimeter H I line data. HAYNES M.P., GIOVANELLI R., CHAMARAUX P., et al.
1999ApJS..125..409C viz 13438 54 Arcsecond positions of UGC galaxies. COTTON W.D., CONDON J.J. and ARBIZZANI E.
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.
2005ApJS..160..149S viz 15       D               9541 372 A digital archive of H I 21 centimeter line spectra of optically targeted galaxies. SPRINGOB C.M., HAYNES M.P., GIOVANELLI R., et al.
2006AJ....132..197W viz 15       D               1 493 98 Tidally triggered star formation in close pairs of galaxies: Major and minor interactions. WOODS D.F., GELLER M.J. and BARTON E.J.
2009AJ....138.1938C viz 15       D               1 13325 92 The Extragalactic Distance Database: All Digital H I profile catalog. COURTOIS H.M., TULLY R.B., FISHER J.R., et al.
2013AJ....146...86T viz 16       D               1 9233 484 Cosmicflows-2: the data. TULLY R.B., COURTOIS H.M., DOLPHIN A.E., et al.
2015MNRAS.447.1531C viz 16       D               1 13577 26 Update on HI data collection from Green Bank, Parkes and Arecibo telescopes for the Cosmic Flows project. COURTOIS H.M. and TULLY R.B.
2016A&A...588A..14T viz 16       D               1 84076 35 Friends-of-friends galaxy group finder with membership refinement. TEMPEL E., KIPPER R., TAMM A., et al.
2016AJ....152...50T viz 16       D               1 20396 318 Cosmicflows-3. TULLY R.B., COURTOIS H.M. and SORCE J.G.
2017ApJ...837..120G viz 16       D               1 14403 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.
2018ApJ...861...49H viz 16       D               1 31269 293 The Arecibo Legacy Fast ALFA survey: the ALFALFA extragalactic H I source catalog. HAYNES M.P., GIOVANELLI R., KENT B.R., et al.
2019AJ....157..194H viz 59       D     X         2 926 ~ Total ALFALFA neutral hydrogen fluxes for extended sources. HOFFMAN G.L., DOWELL J., HAYNES M.P., et al.
2020MNRAS.494.1784A viz 17       D               1 47437 9 Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. ASMUS D., GREENWELL C.L., GANDHI P., et al.
2020ApJ...902..145K viz 17       D               1 10723 45 Cosmicflows-4: the catalog of ∼10,000 Tully-Fisher distances. KOURKCHI E., TULLY R.B., EFTEKHARZADEH S., et al.
2022ApJS..261...21Y viz 18       D               1 29961 6 Statistical Analysis of H I Profile Asymmetry and Shape for Nearby Galaxies. YU N., HO L.C., WANG J., et al.

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