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| ICRF J014137.9-093001 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST08:56:14 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2010ApJ...718L..58I | 36 | 1 | 73 | Emergence of protoplanetary disks and successive formation of gaseous planets by gravitational instability. | INUTSUKA S.-I., MACHIDA M.N. and MATSUMOTO T. | ||||
|
2010ApJ...718..587M |
90 | D | X | 3 | 245 | 48 | High-frequency radio properties of sources in the Fermi-LAT 1 year point source catalog. | MAHONY E.K., SADLER E.M., MURPHY T., et al. | |
| 2010MNRAS.407..791G | 15 | D | 1 | 241 | 49 | Correlation of Fermi large area telescope sources with the 20-GHz australia telescope compact array radio survey. | GHIRLANDA G., GHISELLINI G., TAVECCHIO F., 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. | ||
|
2020MNRAS.494..923C |
16 | D | 1 | 3612 | ~ | WISE mid-infrared properties of compact active galactic nuclei selected from the high radio frequency AT20G survey. | CHHETRI R., KIMBALL A., EKERS R.D., et al. | ||
|
2020A&A...644A.159C |
16 | D | 1 | 4536 | 184 | The third realization of the International Celestial Reference Frame by very long baseline interferometry. | CHARLOT P., JACOBS C.S., GORDON D., et al. | ||
|
2022ApJS..260....4P |
17 | D | 1 | 7976 | 3 | Direction of Parsec-scale Jets for 9220 Active Galactic Nuclei. | PLAVIN A.V., KOVALEV Y.Y. and PUSHKAREV A.B. | ||
|
2023AJ....165..139D |
17 | D | 1 | 734 | 5 | The Celestial Reference Frame at K Band: Imaging. I. The First 28 Epochs. | DE WITT A., JACOBS C.S., GORDON D., et al. | ||
|
2024ApJS..274...28C |
18 | D | 1 | 4336 | ~ | Metrics of Astrometric Variability in the International Celestial Reference Frame. I. Statistical Analysis and Selection of the Most Variable Sources. | CIGAN P., MAKAROV V.V., SECREST N.J., et al. |