Mrk 1377 , the SIMBAD biblio

Mrk 1377 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.07CEST07:06:23

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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
1982AJ.....87.1364K 104 11 Accurate optical positions for Markarian galaxies 1303-1399. KOJOIAN G., ELLIOTT R. and BICAY M.D.
1986ApJS...62..751M 1524 187 A catalog of Markarian galaxies. MAZZARELLA J.M. and BALZANO V.A.
1988Afz....28..476M 94 4 Spectra of galaxies with UV-continuum. VII. MARKARIAN B.E., ERASTOVA L.K., LIPOVETSKY V.A., et al.
1992A&AS...94..553K 549 49 Pairing properties of Markarian starburst galaxies. KEEL W.C. and VAN SOEST E.T.M.
1992PNAOJ...2..399T viz 464 5 Kiso survey for ultraviolet-excess galaxies. XV. TAKASE B. and MIYAUCHI-ISOBE N.
1995ApJS...98..369B viz 1309 34 A multifrequency radio continuum and IRAS faint source survey of Markarian galaxies. BICAY M.D., KOJOIAN G., SEAL J., et al.
1996A&AS..117..467G viz 22335 19 An image database. II. Catalogue between δ=-0deg and δ=70deg. GARNIER R., PATUREL G., PETIT C., et al.
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.
2003MNRAS.344..181C viz 467 4 The PDS versus Markarian starburst galaxies: comparing strong and weak IRAS emitter at 12 and 25 µm in the nearby Universe. COZIOL R.
2007ApJS..170...33P viz 15       D               1529 50 Markarian galaxies. I. The optical database and atlas. PETROSIAN A., McLEAN B., ALLEN R.J., et al.
2009MNRAS.398..109W viz 15       D               1 50356 37 The imperial IRAS-FSC redshift catalogue. WANG L. and ROWAN-ROBINSON M.
2011AJ....142..170H viz 15       D               1 15886 568 The Arecibo Legacy Fast ALFA survey: the α.40 H I source catalog, its characteristics and their impact on the derivation of the H I mass function. HAYNES M.P., GIOVANELLI R., MARTIN A.M., et al.
2014ApJ...788...45T viz 16       D               1 224162 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.
2015MNRAS.447.1531C viz 16       D               2 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.
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.
2017A&A...599A..71D viz 16       D               1 209270 41 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2017ApJ...849...20E viz 16       D               2 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.
2017ApJS..233...22S viz 16       D               1 533 334 xCOLD GASS: the complete IRAM 30 m legacy survey of molecular gas for galaxy evolution studies. SAINTONGE A., CATINELLA B., TACCONI L.J., 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.
2019ApJS..244...24L viz 17       D               2 15505 136 A z = 0 Multiwavelength Galaxy Synthesis. I. A WISE and GALEX atlas of local galaxies. LEROY A.K., SANDSTROM K.M., LANG D., 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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