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| 2MASS J17420150-6055122 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:30:08 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2009ApJS..184..138H |
15 | D | 2 | 20623 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
|
2010A&A...524A..64C |
15 | D | 1 | 1294 | 157 | The Palermo Swift-BAT hard X-ray catalogue. III. Results after 54 months of sky survey. | CUSUMANO G., LA PAROLA V., SEGRETO A., et al. | ||
|
2011MNRAS.417.2651M |
15 | D | 1 | 5893 | 47 | Optical properties of high-frequency radio sources from the Australia Telescope 20 GHz (AT20G) Survey. | MAHONY E.K., SADLER E.M., CROOM S.M., et al. | ||
|
2012ApJ...751...52E |
15 | D | 1 | 4327 | 67 | Reliable identifications of active galactic nuclei from the WISE, 2MASS, and ROSAT all-sky surveys. | EDELSON R. and MALKAN M. | ||
|
2013ApJS..206...17M |
15 | D | 2 | 26 | 11 | Searching for new γ-ray blazar candidates in the third Palermo BAT hard X-ray Catalog with WISE. | MASELLI A., MASSARO F., CUSUMANO G., et al. | ||
| 2017A&A...602A.124R | 100 | 9 | The nature of 50 Palermo Swift-BAT hard X-ray objects through optical spectroscopy. | ROJAS A.F., MASETTI N., MINNITI D., et al. | |||||
|
2023ApJS..265...32M |
17 | D | 1 | 323 | ~ | Powerful Radio Sources in the Southern Sky. I. Optical Identifications. | MASSARO F., WHITE S.V., GARCIA-PEREZ A., et al. | ||
| 2023ApJS..268...32M | 279 | D | X C | 6 | 100 | ~ | Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective. | MASSARO F., WHITE S.V., PAGGI A., et al. | |
| 2024ApJS..271....8G | 18 | D | 1 | 97 | ~ | Powerful Radio Sources in the Southern Sky. III. First Results of the Optical Spectroscopic Campaign. | GARCIA-PEREZ A., PENA-HERAZO H.A., JIMENEZ-GALLARDO A., et al. |