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| SDSS J132615.53+345631.0 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:30:23 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
1990IRASF.C......0M 
|
14 | D | 1 | 26192 | 130 | IRAS Faint Source Catalogue, version 2.0. | MOSHIR M., et al. | ||
| 1991ApJS...76.1043P | 408 | 16 | The Case low-dispersion northern sky survey. XII. A region in southern Canes Venatici. | PESCH P., SANDULEAK N. and STEPHENSON C.B. | |||||
|
1995AJ....110.2009O
|
32173 | 32 | Galaxy properties at the North Galactic Pole. I. Photometric properties on large spatial scales. | ODEWAHN S.C. and ALDERING G. | |||||
|
2009MNRAS.395..255M
|
15 | D | 1 | 397037 | 82 | Compact groups in theory and practice - III. Compact groups of galaxies in the sixth data release of the Sloan Digital Sky Survey. | McCONNACHIE A.W., PATTON D.R., ELLISON S.L., et al. | ||
|
2009MNRAS.398..109W
|
15 | D | 1 | 22041 | 37 | The imperial IRAS-FSC redshift catalogue. | WANG L. and ROWAN-ROBINSON M. | ||
|
2014ApJ...788...45T
|
15 | D | 1 | 224166 | 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
|
16 | D | 1 | 209271 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
|
2018ApJ...861...49H
|
16 | D | 1 | 31270 | 293 | The Arecibo Legacy Fast ALFA survey: the ALFALFA extragalactic H I source catalog. | HAYNES M.P., GIOVANELLI R., KENT B.R., et al. | ||
|
2022ApJS..261...21Y
|
17 | D | 1 | 29963 | 6 | Statistical Analysis of H I Profile Asymmetry and Shape for Nearby Galaxies. | YU N., HO L.C., WANG J., et al. | ||
|
2022A&A...666A.186D
|
17 | D | 1 | 194359 | 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. |
