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| NVSS J114549+052018 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST00:53:43 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2003A&A...412...45P 
|
15 | D | 1 | 956205 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
|
2005MNRAS.362....9B
|
15 | D | 2707 | 245 | A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey. | BEST P.N., KAUFFMANN G., HECKMAN T.M., et al. | |||
|
2012MNRAS.421.1569B
|
15 | D | 2 | 18499 | 511 | On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. | BEST P.N. and HECKMAN T.M. | ||
|
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. | ||
|
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. | ||
|
2018AJ....155..188L
|
16 | D | 1 | 13494 | 1 | An analysis framework for understanding the origin of nuclear activity in low-power radio galaxies. | LIN Y.-T., HUANG H.-J. and CHEN Y.-C. | ||
|
2018MNRAS.481.2458D
|
16 | D | 1 | 31576 | ~ | On the nature of small galaxy systems. | DUPLANCIC F., COLDWELL G.V., ALONSO S., et al. | ||
|
2019ApJS..244....3D
|
17 | D | 1 | 23802 | ~ | Circumventing the effects of projection and dust using inclination-independent infrared galaxy structure measurements: method, error analysis, and a new public catalog of near-infrared galaxy structures. | DEVOUR B.M. and BELL E.F. |
