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2MASX J11065070+4751091 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST19:42:19 |
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. | |||||
2009MNRAS.398..109W | 15 | D | 1 | 50356 | 37 | The imperial IRAS-FSC redshift catalogue. | WANG L. and ROWAN-ROBINSON M. | ||
2012ApJS..201...31G | 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 | 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. | ||
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. | ||
2017MNRAS.471.2687B | 16 | D | 1 | 7831 | 45 | On the interdependence of galaxy morphology, star formation and environment in massive galaxies in the nearby Universe. | BAIT O., BARWAY S. and WADADEKAR Y. | ||
2019MNRAS.487.5572M | 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. | ||
2020ApJS..246...12Z | 17 | D | 1 | 25543 | 12 | Compact groups of galaxies in Sloan Digital Sky Survey and LAMOST spectral Survey. I. The catalogs. | ZHENG Y.-L. and SHEN S.-Y. | ||
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. |