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| 2FGL J1836.8-0623c , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:25:54 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2012ApJS..199...31N |
15 | D | 1 | 2260 | 1282 | Fermi Large Area Telescope second source catalog. | NOLAN P.L., ABDO A.A., ACKERMANN M., et al. | ||
|
2012MNRAS.424.2832L |
15 | D | 1 | 1877 | 43 | Application of the Gaussian mixture model in pulsar astronomy – pulsar classification and candidates ranking for the Fermi 2FGL catalogue. | LEE K.J., GUILLEMOT L., YUE Y.L., et al. | ||
| 2012ApJ...756....5L | 77 | X | 2 | 61 | 123 | Search for spatially extended Fermi large area telescope sources using two years of data. | LANDE J., ACKERMANN M., ALLAFORT A., et al. | ||
|
2013MNRAS.428..220H |
15 | D | 1 | 473 | 19 | Gamma-ray active galactic nucleus type through machine-learning algorithms. | HASSAN T., MIRABAL N., CONTRERAS J.L., et al. | ||
| 2013ApJ...767...99B | 115 | X C | 2 | 21 | 17 | Observation of TeV gamma rays from the unidentified source HESS J1841-055 with the ARGO-YBJ experiment. | BARTOLI B., BERNARDINI P., BI X.J., et al. | ||
| 2013ApJ...773...77A | 15 | D | 1 | 105 | 91 | Constraints on the galactic population of TeV pulsar wind nebulae using Fermi large area telescope observations. | ACERO F., ACKERMANN M., AJELLO M., et al. | ||
| 2015A&A...574A..27H | 39 | X | 1 | 18 | 13 | Probing the gamma-ray emission from HESS J1834-087 using H.E.S.S. and Fermi LAT observations. | HESS COLLABORATION, ABRAMOWSKI A., AHARONIAN F., et al. | ||
|
2015ApJS..217....2M |
16 | D | 2 | 2199 | 42 | Refining the associations of the Fermi large area telescope source catalogs. | MASSARO F., D'ABRUSCO R., LANDONI M., et al. | ||
| 2017ApJ...839..129K | 40 | X | 1 | 67 | 11 | Extended Gamma-ray emission from the G25.0+0.0 region: a star-forming region powered by the newly found OB association? | KATSUTA J., UCHIYAMA Y. and FUNK S. |