
| Proposal ID | 094290 |
| Title | An XMM-Newton Study of New High-Redshift, High-Mass SZ-Selected Galaxy Cluster |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0942900101 |
| DOI | https://doi.org/10.57780/esa-g5p7e3o |
| Principal Investigator, PI | Dr John P. Hughes |
| Abstract | We propose a deep X-ray observation focused on spectral analysis of theintracluster medium in a high redshift (z=0.836), massive, SZ-selected cluster.The proposed target is the seventh highest signal-to-noise cluster in therecently published ACT sample of 4195 clusters, exceeded in its redshift rangeonly by El Gordo. ACT-CL J1407.0+10.48 is the fifth highest mass cluster at itsredshift or higher in this sample. The goal of the proposal is a comprehensivestudy of the hot intercluster medium to resolve the nature of this potentiallyexceptional system. |
| Publications | No publications found for current proposal! |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2025-01-04T13:42:57Z/2025-01-05T14:57:57Z |
| Version | 21.51_20241115_1113 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2026-01-31T00:00:00Z |
| Last Update | 2026-07-09 |
| Keywords | XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr John P. Hughes, 2026, 'An XMM-Newton Study of New High-Redshift, High-Mass SZ-Selected Galaxy Cluster', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-g5p7e3o |
| Rights | Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license. |