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| SNR G028.78-00.44 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:57:57 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017A&A...605A..58A | 16 | D | 1 | 156 | 61 | Galactic supernova remnant candidates discovered by THOR. | ANDERSON L.D., WANG Y., BIHR S., et al. | ||
| 2018ApJ...866...61D | 40 | X | 1 | 26 | 1 | Confirmation of two Galactic supernova remnant candidates discovered by THOR. | DOKARA R., ROY N., BEUTHER H., et al. | ||
| 2021A&A...647A..68D | 84 | X | 2 | 35 | ~ | Multiwavelength constraints on the unidentified Galactic TeV sources HESS J1427-608, HESS J1458-608, and new VHE γ-ray source candidates. | DEVIN J., RENAUD M., LEMOINE-GOUMARD M., et al. | ||
| 2021A&A...651A..85B | 168 | S C | 2 | 17 | 21 | A global view on star formation: The GLOSTAR Galactic plane survey. I. Overview and first results for the Galactic longitude range 28°<l<36°. | BRUNTHALER A., MENTEN K.M., DZIB S.A., et al. | ||
2021A&A...651A..86D 
|
17 | D | 1 | 254 | 16 | A global view on star formation: The GLOSTAR Galactic plane survey. II. Supernova remnants in the first quadrant of the Milky Way. | DOKARA R., BRUNTHALER A., MENTEN K.M., et al. | ||
| 2022ApJ...932..120A | 43 | X | 1 | 17 | 2 | Measurement of the Gamma-Ray Energy Spectrum beyond 100 TeV from the HESS J1843-033 Region. | AMENOMORI M., ASANO S., BAO Y.W., et al. | ||
| 2023A&A...671A.145D | 392 | A | D | S X C | 8 | 52 | 2 | A global view on star formation: The GLOSTAR Galactic plane survey VII. Supernova remnants in the Galactic longitude range 28° < l < 36°. | DOKARA R., GONG Y., REICH W., et al. |
| 2024AJ....168...42L | 448 | A | D | X C F | 9 | 69 | ~ | Investigation of Galactic Supernova Remnants and their Environment in 26.°6 < l < 30.°6, ∣b∣ ≤ 1.°25 Using Radio Surveys. | LUO T.-X., ZHOU P. and HE H.-N. |
