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| 2MASX J11343495+5704409 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST13:14:51 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1983Afz....19..639M | 117 | 67 | The second Byurakan spectral sky survey. I. The results of the area centred on alpha = 11h 30 m, delta = 59 00. | MARKARIAN B.E. and STEPANIAN J.A. | |||||
| 1984Afz....21..445S | 84 | 1 | Luminosity function of faint galaxies with UV-continuum. | STEPANIAN J.A. | |||||
| 1988AJ.....95.1678N | 113 | 5 | Accurate optical positions for 107 Byurakan objects and 11 blue stars from the "Second Byurakan Spectral Sky Survey (1)". | NELSON R.L., KOJOIAN G., SEAL J., et al. | |||||
2000A&AS..147..169B 
|
2737 | 21 | Accurate optical positions for 2978 objects from the Second Byurakan Survey (SBS) with the Digitized Sky Survey. | BICAY M.D., STEPANIAN J.A., CHAVUSHYAN V.H., 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. | ||
|
2005RMxAA..41..155S
|
3231 | 23 | The Second Byurakan Survey. General Catalogue. | STEPANIAN J.A. | |||||
|
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. | ||
|
2017A&A...599A..71D
|
16 | D | 1 | 209270 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
|
2022ApJ...925...70Z
|
18 | D | 1 | 9296 | 5 | The Relation between Morphological Asymmetry and Nuclear Activity in Low-redshift Galaxies. | ZHAO Y., LI Y.A., SHANGGUAN J., et al. | ||
|
2022A&A...666A.186D
|
18 | D | 1 | 194358 | 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. |
