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| [VV2006] J122531.1+071552 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:14:16 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2004MNRAS.351...83L |
175 | 40 | A physical classification scheme for blazars. | LANDT H., PADOVANI P., PERLMAN E.S., et al. | |||||
|
2006A&A...455..773V |
108223 | 628 | A catalogue of quasars and active nuclei: 12th edition. | VERON-CETTY M.-P. and VERON P. | |||||
|
2010A&A...518A..10V |
15 | D | 1 | 168913 | 597 | A catalogue of quasars and active nuclei: 13th edition. | VERON-CETTY M.-P. and VERON P. | ||
|
2011ApJ...726...20M |
15 | D | 1 | 687 | 98 | X-ray emission from optically selected radio-intermediate and radio-loud quasars. | MILLER B.P., BRANDT W.N., SCHNEIDER D.P., et al. | ||
|
2011AJ....141..182K |
15 | D | 1 | 5750 | 38 | Correlations of quasar optical spectra with radio morphology. | KIMBALL A.E., IVEZIC Z., WIITA P.J., et al. | ||
| 2011A&A...533A..79M | 91 | D | C | 4 | 105 | 5 | Flux density measurements of a complete sample of faint blazars. | MANTOVANI F., BONDI M. and MACK K.-H. | |
|
2015A&A...577A..36M |
16 | D | 1 | 104 | 1 | A sample of weak blazars at milli-arcsecond resolution. | MANTOVANI F., BONDI M., MACK K.-H., et al. | ||
|
2020MNRAS.496..245Z |
16 | D | 1 | 736 | 34 | The Lx-Luv-Lradio relation and corona-disc-jet connection in optically selected radio-loud quasars. | ZHU S.F., BRANDT W.N., LUO B., et al. | ||
|
2021MNRAS.505.1954Z |
17 | D | 1 | 963 | 7 | The X-ray spectral and variability properties of typical radio-loud quasars. | ZHU S.F., TIMLIN J.D. and BRANDT W.N. | ||
|
2021A&A...655A..17S |
17 | D | 1 | 338578 | 3 | The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. | STEIN Y., VOLLMER B., BOCH T., et al. | ||
|
2022MNRAS.515.1358H |
17 | D | 1 | 511 | ~ | A cosmological distance measure using radio-loud quasars. | HUANG L. and CHANG Z.X. |