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| CIZA J1813.3-6127 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:50:12 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
2007ApJ...662..224K 
|
15 | D | 76 | 83 | A systematic X-ray search for clusters of galaxies behind the Milky Way. II. The second CIZA subsample. | KOCEVSKI D.D., EBELING H., MULLIS C.R., et al. | |||
|
2011A&A...536A...7P
|
15 | D | 1 | 1116 | 260 | Planck early results. VII. The Early Release Compact Source Catalogue. | PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al. | ||
|
2011A&A...536A...8P
|
15 | D | 1 | 200 | 362 | Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample. | PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al. | ||
|
2013ApJ...771..137M
|
15 | D | 1 | 177 | 9 | WMAP observations of Planck ESZ clusters. | MA Y.-Z., HINSHAW G. and SCOTT D. | ||
|
2017ApJ...843...76A
|
16 | D | 1 | 217 | 77 | The fraction of cool-core clusters in X-ray versus SZ samples using Chandra observations. | ANDRADE-SANTOS F., JONES C., FORMAN W.R., et al. | ||
| 2017ApJ...846...51L | 16 | D | 1 | 127 | 77 | X-ray morphological analysis of the Planck ESZ clusters. | LOVISARI L., FORMAN W.R., JONES C., et al. | ||
|
2020ApJ...892..102L
|
16 | D | 1 | 121 | 41 | X-ray scaling relations for a representative sample of Planck-selected clusters observed with XMM-Newton. | LOVISARI L., SCHELLENBERGER G., SERENO M., et al. | ||
|
2021ApJ...914...58A
|
17 | D | 1 | 184 | 9 | Chandra observations of the Planck early Sunyaev-Zeldovich sample: a reexamination of masses and mass proxies. | ANDRADE-SANTOS F., PRATT G.W., MELIN J.-B., et al. | ||
|
2022MNRAS.513.3013Y
|
17 | D | 2 | 1644 | 7 | Dynamical state of galaxy clusters evaluated from X-ray images. | YUAN Z.S., HAN J.L. and WEN Z.L. | ||
|
2023A&A...674A..48W
|
17 | D | 1 | 120 | 5 | Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters. | WICKER R., DOUSPIS M., SALVATI L., et al. |
