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| PMN J1938-4657 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST05:24:09 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1994ApJS...91..111W |
4374 | 324 | The Parkes-MIT-NRAO (PMN) Surveys: II. Source catalog for the Southern Survey (-87deg.5 < delta < -37deg). | WRIGHT A.E., GRIFFITH M.R., BURKE B.F., et al. | |||||
|
2004MNRAS.351...83L |
175 | 40 | A physical classification scheme for blazars. | LANDT H., PADOVANI P., PERLMAN E.S., et al. | |||||
|
2009A&A...495..691M |
15 | D | 2 | 3199 | 339 | Roma-BZCAT: a multifrequency catalogue of blazars. | MASSARO E., GIOMMI P., LETO C., et al. | ||
|
2010A&A...511A..53V |
15 | D | 1 | 107473 | 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.422.1527M |
15 | D | 2 | 6426 | 22 | ATPMN: accurate positions and flux densities at 5 and 8 GHz for 8385 sources from the PMN survey. | McCONNELL D., SADLER E.M., MURPHY T., et al. | ||
| 2012A&A...548A..32M | 114 | X | 3 | 17 | 6 | Flat-spectrum radio sources as likely counterparts of unidentified INTEGRAL sources. | MOLINA M., LANDI R., BASSANI L., et al. | ||
|
2015Ap&SS.357...75M |
16 | D | 1 | 3562 | 223 | The 5th edition of the Roma-BZCAT. A short presentation. | MASSARO E., MASELLI A., LETO C., et al. | ||
|
2016ApJS..224...26M |
16 | D | 1 | 2216 | 17 | A comprehensive statistical description of radio-through-gamma-ray spectral energy distributions of all known blazars. | MAO P., URRY C.M., MASSARO F., et al. | ||
|
2017ApJ...841..113M |
16 | D | 1 | 2944 | 1 | An investigation of blazars without redshifts: not a missing population at high redshift. | MAO P. and URRY C.M. | ||
|
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. |