other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2MASX J04571847+0041196 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST06:26:59 |
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 |
---|---|---|---|---|---|---|---|---|---|
1999MNRAS.308..897L | 2402 | 75 | The QDOT all-sky IRAS galaxy redshift survey. | LAWRENCE A., ROWAN-ROBINSON M., ELLIS R.S., et al. | |||||
2000A&AS..144..475P | 14 | D | 1 | 16403 | 8 | Galaxy coordinates. III. Accurate positions for 17124 galaxies including 3301 new companions of UGC galaxies. | PATUREL G., PETIT C., GARNIER R., et al. | ||
2000MNRAS.317...55S | 14 | D | 1 | 16418 | 457 | The PSCz catalogue. | SAUNDERS W., SUTHERLAND W.J., MADDOX S.J., 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. | ||
2003A&A...412...57P | 809 | 148 | HYPERLEDA. II. The homogenized HI data. | PATUREL G., THEUREAU G., BOTTINELLI L., et al. | |||||
2003AJ....126.2152R | 15 | D | 15140 | 214 | CAIRNS: the cluster and infall region nearby survey. I. Redshifts and mass profiles. | RINES K., GELLER M.J., KURTZ M.J., et al. | |||
2009AJ....138.1938C | 15 | D | 1 | 13325 | 92 | The Extragalactic Distance Database: All Digital H I profile catalog. | COURTOIS H.M., TULLY R.B., FISHER J.R., 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. | ||
2019ApJS..244...24L | 17 | D | 2 | 15505 | 136 | A z = 0 Multiwavelength Galaxy Synthesis. I. A WISE and GALEX atlas of local galaxies. | LEROY A.K., SANDSTROM K.M., LANG D., et al. | ||
2020MNRAS.494.1784A | 17 | D | 1 | 47437 | 9 | Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. | ASMUS D., GREENWELL C.L., GANDHI P., et al. |