2MASX J13443740+0033414 , the SIMBAD biblio

2MASX J13443740+0033414 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST17:19:10


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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
1986MNRAS.221..233P 523 142 A complete galaxy redshift sample - III. Methods and catalogue. PETERSON B.A., ELLIS R.S., EFSTATHIOU G., et al.
1998MNRAS.294..147M 335 29 UBVRI photometry of the Durham-AAT redshift survey. METCALFE N., RATCLIFFE A., SHANKS T., 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.
2010MNRAS.405..783M viz 15       D               1 5435 245 Galaxy Zoo: passive red spirals. MASTERS K.L., MOSLEH M., ROMER A.K., et al.
2012ApJS..201...31G viz 15       D               1 15561 75 Double-peaked narrow emission-line galaxies from the Sloan Digital Sky Survey. I. Sample and basic properties. GE J.-Q., HU C., WANG J.-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.
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.
2019ApJS..244....3D viz 17       D               1 23802 ~ 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.
2022ApJ...925...70Z viz 18       D               1 9296 5 The Relation between Morphological Asymmetry and Nuclear Activity in Low-redshift Galaxies. ZHAO Y., LI Y.A., SHANGGUAN J., et al.
2022A&A...666A.186D viz 18       D               1 194358 6 Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.

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