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| 2HWC J1953+294 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:35:42 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2017ApJ...843...40A |
16 | D | 1 | 134 | 227 | The 2HWC HAWC Observatory gamma-ray catalog. | ABEYSEKARA A.U., ALBERT A., ALFARO R., et al. | ||
| 2018ApJ...861..134A | 96 | D | X | 3 | 112 | 38 | A very high energy γ-ray survey toward the Cygnus region of the Galaxy. | ABEYSEKARA A.U., ARCHER A., AUNE T., et al. | |
| 2018ApJ...866...24A | 682 | A | D | X | 18 | 36 | 20 | VERITAS and Fermi-LAT observations of TeV gamma-ray sources discovered by HAWC in the 2HWC catalog. | ABEYSEKARA A.U., ARCHER A., BENBOW W., et al. |
| 2019ApJ...878..126C | 227 | A | X | 6 | 12 | ~ | Multiwavelength investigation of pulsar wind nebula DA 495 With HAWC, VERITAS, and NuSTAR. | COERVER A., WILCOX P., ZHANG H., et al. | |
|
2020ApJ...905...76A |
17 | D | 1 | 89 | 89 | 3HWC: the third HAWC catalog of very-high-energy gamma-ray sources. | ALBERT A., ALFARO R., ALVAREZ C., et al. | ||
| 2022MNRAS.513.2884L | 17 | D | 1 | 26 | 3 | Prospect of detecting X-ray haloes around middle-aged pulsars with eROSITA. | LI B., ZHANG Y., LIU T., et al. | ||
|
2024ApJS..271...25C |
18 | D | 1 | 176 | ~ | The First LHAASO Catalog of Gamma-Ray Sources. | CAO Z., AHARONIAN F., AN Q., et al. | ||
| 2024ApJ...977L...3K | 18 | D | 1 | 70 | ~ | Quantitative Constraint on the Contribution of Resolved Gamma-Ray Sources to the Sub-PeV Galactic Diffuse Gamma-Ray Flux Measured by the Tibet ASγ Experiment. | KATO S., ANZORENA M., CHEN D., et al. | ||
| 2025ApJ...989..110F | 205 | D | X C | 4 | 112 | ~ | A Systematic Search for MeV-GeV Pulsar Wind Nebulae without Gamma-Ray Detected Pulsars. | FERMI-LAT COLLABORATION, ACHARYYA A., ADELFIO A., et al. | |
| 2026ApJ...997..367T | 200 | X C | 3 | 13 | ~ | The GeV γ-Ray Emission from the Pulsar Wind Nebula DA 495. | TANG J. and XIN Y. |