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| eFEDS J091610.1-002348 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST01:12:56 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2022A&A...661A...2L |
17 | D | 1 | 563 | 55 | The eROSITA Final Equatorial-Depth Survey (eFEDS). Catalog of galaxy clusters and groups. | LIU A., BULBUL E., GHIRARDINI V., et al. | ||
|
2022A&A...661A...4K |
17 | D | 1 | 543 | 25 | The eROSITA Final Equatorial-Depth Survey (eFEDS). Optical confirmation, redshifts, and properties of the cluster and group catalog. | KLEIN M., OGURI M., MOHR J.J., et al. | ||
|
2022A&A...661A...7B |
17 | D | 3 | 543 | 23 | The eROSITA Final Equatorial-Depth Survey (eFEDS). X-ray properties and scaling relations of galaxy clusters and groups. | BAHAR Y., BULBUL E., CLERC N., et al. | ||
|
2022A&A...661A..11C |
17 | D | 1 | 458 | 33 | The eROSITA Final Equatorial-Depth Survey (eFEDS). X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey. | CHIU I.-N., GHIRARDINI V., LIU A., et al. | ||
|
2022A&A...661A..14R |
17 | D | 1 | 21 | 7 | The eROSITA Final Equatorial-Depth Survey (eFEDS). A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint. | RAMOS-CEJA M.E., OGURI M., MIYAZAKI S., et al. | ||
| 2023A&A...671A..57S | 7 | 3 | Offset between X-ray and optical centers in clusters of galaxies: Connecting eROSITA data with simulations. | SEPPI R., COMPARAT J., NANDRA K., et al. | |||||
| 2025ApJ...985...78A | 19 | D | 1 | 22 | ~ | Gravity-selected Cluster Samples: A New Take on the Compton-y-Mass Relation. | ANDREON S. and RADOVICH M. | ||
| 2026A&A...705A.208A | 370 | D | X C | 7 | 16 | ~ | Gravity-selected galaxy clusters: A tight mass-richness relation and an unclear Compton Y-richness trend. | ANDREON S. and RADOVICH M. |