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| LEDA 1373882 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:15:53 |
| 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 | 956189 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
|
2012MNRAS.421.1569B |
15 | D | 2 | 18458 | 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 |
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. | ||
| 2019MNRAS.487.5490P | 97 | D | F | 5 | 31 | ~ | Do AGN triggering mechanisms vary with radio power? - I. Optical morphologies of radio-intermediate HERGs. | PIERCE J.C.S., TADHUNTER C.N., RAMOS ALMEIDA C., et al. | |
|
2020ApJS..246....2A |
16 | D | 1 | 36251 | ~ | GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19). | ABDULLAH M.H., WILSON G., KLYPIN A., et al. | ||
|
2020ApJS..247...53K |
16 | D | 1 | 23378 | 20 | Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. | KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N. | ||
|
2022ApJ...925...70Z |
17 | D | 1 | 9297 | 5 | The Relation between Morphological Asymmetry and Nuclear Activity in Low-redshift Galaxies. | ZHAO Y., LI Y.A., SHANGGUAN J., et al. | ||
|
2024A&A...686A.223P |
18 | D | 1 | 1349 | ~ | What excites the optical emission in X-ray-selected galaxies? | PULATOVA N.G., RIX H.-W., TUGAY A.V., et al. | ||
| 2024A&A...688A..79M | 63 | D | X | 2 | 15 | ~ | AGN populations in the local Universe: Their alignment with the main sequence, stellar population characteristics, accretion efficiency, and the impact of AGN feedback. | MOUNTRICHAS G., RUIZ A., GEORGANTOPOULOS I., et al. |