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| PLCKESZ G121.11+57.01 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:28:44 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2011MNRAS.414L..75H | 417 | K A | D | S X C F | 9 | 45 | 14 | Further Sunyaev–Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager. | HURLEY-WALKER N., BROWN M.L., DAVIES M.L., 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 | 2 | 200 | 362 | Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample. | PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al. | ||
| 2012ApJ...749...46M | 992 | K A | D | S X C | 25 | 5 | 9 | CARMA follow-up of the northern unconfirmed planck galaxy cluster candidates. | MUCHOVEJ S., LEITCH E., CULVERHOUSE T., et al. |
| 2013A&A...550A.128P | 207 | D | X | 6 | 47 | 24 | Planck intermediate results. II. Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters. | PLANCK COLLABORATION (The AMI Collaboration), ADE P.A.R., et al. | |
|
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. | ||
|
2021MNRAS.500..310D |
17 | D | 1 | 216 | 15 | Brightest cluster galaxies: the centre can(not?) hold. | DE PROPRIS R., WEST M.J., ANDRADE-SANTOS F., 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. | ||
|
2022A&A...665A..71O |
17 | D | 1 | 135 | 3 | The detection of cluster magnetic fields via radio source depolarisation. | OSINGA E., VAN WEEREN R.J., ANDRADE-SANTOS F., et al. |