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2MASX J11484520+3547093 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST00:13:32 |
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 |
---|---|---|---|---|---|---|---|---|---|
1996A&AS..117..467G | 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 | 15 | D | 1 | 956205 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
2008MNRAS.390.1133B | 15 | D | 1 | 1597 | 48 | The anisotropic distribution of satellite galaxies. | BAILIN J., POWER C., NORBERG P., et al. | ||
2011MNRAS.416.2840L | 15 | D | 1 | 72554 | 178 | The 2M++ galaxy redshift catalogue. | LAVAUX G. and HUDSON M.J. | ||
2014ApJ...788...45T | 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. | ||
2016ApJS..222...16C | 16 | D | 1 | 399 | 17 | Herschel observations of Major merger pairs at z = 0: dust mass and star formation. | CAO C., XU C.K., DOMINGUE D., et al. | ||
2016A&A...588A..14T | 16 | D | 1 | 84076 | 35 | Friends-of-friends galaxy group finder with membership refinement. | TEMPEL E., KIPPER R., TAMM A., et al. | ||
2016ApJ...829...78D | 16 | D | 1 | 88 | 2 | Major-merger galaxy pairs at z = 0: dust properties and companion morphology. | DOMINGUE D.L., CAO C., XU C.K., et al. | ||
2019ApJ...872..148C | 17 | D | 1 | 15662 | 21 | Radio sources in the nearby universe. | CONDON J.J., MATTHEWS A.M. and BRODERICK J.J. | ||
2019MNRAS.489.5030F | 17 | D | 1 | 178 | ~ | From the outside looking in: what can Milky Way analogues tell us about the star formation rate of our own galaxy? | FRASER-MCKELVIE A., MERRIFIELD M. and ARAGON-SALAMANCA A. | ||
2022ApJS..261...34H | 18 | D | 1 | 181 | ~ | Close Major-merger Pairs at z = 0: Bulge-to-total Ratio and Star Formation Enhancement. | HE C., XU C.K., DOMINGUE D., et al. |