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| NVSS J112833+560840 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST08:51:12 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2007MNRAS.377..787B 
|
4391 | 7 | Properties of luminous red galaxies in the Sloan Digital Sky Survey. | BARBER T., MEIKSIN A. and MURPHY T. | |||||
|
2010A&A...511A..53V
|
15 | D | 1 | 107940 | 39 | The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. | VOLLMER B., GASSMANN B., DERRIERE S., et al. | ||
|
2012MNRAS.421.1569B
|
15 | D | 3 | 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. | ||
|
2013ApJ...765...62S
|
16 | D | 1 | 409 | 33 | Constraining jet production scenarios by studies of narrow-line radio galaxies. | SIKORA M., STASINSKA G., KOZIEL-WIERZBOWSKA D., et al. | ||
|
2017MNRAS.466.4346M
|
16 | D | 1 | 1437 | 66 | The nuclear properties and extended morphologies of powerful radio galaxies: the roles of host galaxy and environment. | MIRAGHAEI H. and BEST P.N. | ||
|
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. | ||
|
2020ApJS..247...53K
|
17 | D | 1 | 23374 | 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. | ||
|
2021A&A...655A..17S
|
17 | D | 1 | 338596 | 3 | The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. | STEIN Y., VOLLMER B., BOCH T., et al. |
