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| NVSS J224552+002749 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:21:03 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2000MNRAS.318.1047M | 87 | 24 | The redshift distribution of FIRST radio sources at 1mJy. | MAGLIOCCHETTI M., MADDOX S.J., WALL J.V., et al. | |||||
2005MNRAS.362....9B 
|
15 | D | 2708 | 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. | |||
|
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. | ||
|
2012MNRAS.421.1569B
|
15 | D | 3 | 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. | ||
|
2018AJ....155..188L
|
16 | D | 1 | 13497 | 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.480..707P
|
16 | D | 1 | 4785 | 7 | The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: multiwavelength counterparts. | PRESCOTT M., WHITTAM I.H., JARVIS M.J., et al. | ||
|
2018ApJ...868...99F
|
16 | D | 1 | 19564 | 4 | Identifying tidal disruption events via prior photometric selection of their preferred hosts. | FRENCH K.D. and ZABLUDOFF A.I. | ||
|
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. |
