| Proposal ID | 092030 |
| Title | Observations of the JWST/GTO Merging Cluster PLCK G165.7+67.0 |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0920300201 |
| DOI | https://doi.org/10.57780/esa-q575peo |
| Principal Investigator, PI | Prof Brenda Frye |
| Abstract | The galaxy cluster PLCK G165.7+67.0 (z=0.35) is in the top 1 % brightest sourcesin the Planck sky, as a result of strong lensing of background star-forminggalaxies at z=2. The mass estimated from the lens model appears inconsistentwith the lack of X-ray detection in the ROSAT/RASS survey, but may be explainedby a non-equilibrium state of the cluster, as indicated by its bimodal galaxydistribution and extended radio halo, as well as the presence of two NarrowAngle Tail (NAT) galaxies. We request a 75ks XMM observation to determine thecluster???s dynamic state, which enables us to measure the position of the X-rayhalo(s) and to search for shocks. These complementary capabilities will greatlyaid the interpretation of the upcoming JWST observations of this cluster. |
| Publications | No publications found for current proposal! |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2023-11-26T19:32:44Z/2023-11-27T19:12:19Z |
| Version | 20.10_20230417_1156 |
| 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 | 2024-12-29T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Prof Brenda Frye, 2024, 'Observations of the JWST/GTO Merging Cluster PLCK G165.7+67.0', 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-q575peo |