2MASX J03190773+0057214 , the SIMBAD biblio

2MASX J03190773+0057214 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST14:02:04

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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
1985AnTok..20..237T viz 555 18 Kiso survey for ultraviolet-excess galaxies. II. TAKASE B. and MIYAUCHI-ISOBE N.
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.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2009MNRAS.398..109W viz 15       D               1 50356 37 The imperial IRAS-FSC redshift catalogue. WANG L. and ROWAN-ROBINSON M.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
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.446.3749Y viz 16       D               3 3838 12 Box/peanut and bar structures in edge-on and face-on nearby galaxies in the Sloan Digital Sky Survey - I. Catalogue. YOSHINO A. and YAMAUCHI C.
2017MNRAS.466.2570B viz 16       D               1 587 84 SDSS-IV MaNGA - the spatially resolved transition from star formation to quiescence. BELFIORE F., MAIOLINO R., MARASTON C., et al.
2017AJ....154...86W viz 16       D               2 4613 272 The SDSS-IV MaNGA sample: design, optimization, and usage considerations. WAKE D.A., BUNDY K., DIAMOND-STANIC A.M., et al.
2018MNRAS.476.1765L viz 16       D               1 2080 86 SDSS-IV MaNGA: global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane. LI H., MAO S., CAPPELLARI M., et al.
2018MNRAS.477.4711G viz 16       D               1 2754 110 SDSS-IV MaNGA: stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties. GRAHAM M.T., CAPPELLARI M., LI H., et al.
2019MNRAS.483.2057F viz 17       D               1 4599 64 SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogues and implications for bulge properties and stellar angular momentum. FISCHER J.-L., DOMINGUEZ SANCHEZ H. and BERNARDI M.
2019MNRAS.487.5572M viz 17       D               1 4573 ~ Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies. MISHRA P.K., WADADEKAR Y. and BARWAY S.
2020MNRAS.492.6027E 87               F     3 12 27 The ALMaQUEST Survey - II. What drives central starbursts at z ∼ 0? ELLISON S.L., THORP M.D., PAN H.-A., et al.
2020MNRAS.492.4680W viz 17       D               1 2725 44 Ionized gas outflow signatures in SDSS-IV MaNGA active galactic nuclei. WYLEZALEK D., FLORES A.M., ZAKAMSKA N.L., et al.
2020ApJ...903..145L viz 17       D               3 46 34 ALMaQUEST. IV. The ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey. LIN L., ELLISON S.L., PAN H.-A., et al.
2021MNRAS.501.4777E 236       D     X   F     5 28 38 The ALMaQUEST Survey - V. The non-universality of kpc-scale star formation relations and the factors that drive them. ELLISON S.L., LIN L., THORP M.D., et al.
2021ApJ...908..165P 17       D               1 631 ~ SDSS-IV/MaNGA: can impulsive gaseous inflows explain steep oxygen abundance profiles and anomalously low-metallicity regions? PACE Z.J., TREMONTI C., SCHAEFER A.L., et al.
2022ApJS..262...36S viz 18       D               1 10074 23 SDSS-IV MaNGA: pyPipe3D Analysis Release for 10,000 Galaxies. SANCHEZ S.F., BARRERA-BALLESTEROS J.K., LACERDA E., et al.
2024ApJ...964..120P 100               F     1 46 ~ The ALMaQUEST Survey. XIII. Understanding Radial Trends in Star Formation Quenching via the Relative Roles of Gas Availability and Star Formation Efficiency. PAN H.-A., LIN L., ELLISON S.L., et al.

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