Proposal ID | 090191 |
Title | Bridges of Intergalactic Gas Connecting ACT Cluster Pairs |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0901910101 |
DOI | https://doi.org/10.57780/esa-o8kbz62 |
Principal Investigator, PI | Prof Craig Sarazin |
Abstract | The nature and location of the missing baryons in the universe remains a majormystery. We propose joint Chandra and MUSTANG-2/GBT observations of two closepairs of galaxy clusters recently detected in SZ by ACT with possibleintergalactic gas filaments between them. The MUSTANG-2 and ACT SZ data will becombined to model the SZ on both large and small scales. Both the Chandra X-rayimage and SZ allow the separation of the cluster and the filament gas. Recently,X-ray and SZ observations have been used to study the filament between theclusters Abell 399 and 401. The combination of X-ray and SZ observations allowsthe density, temperature, pressure, and 3D shape of the filaments to bedetermined. These observations will help constrain the nature of the missing baryons in the universe. |
Publications | No publications found for current proposal! |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2022-06-03T17:41:09Z/2022-06-04T11:12:19Z |
Version | 20.08_20220509_1852 |
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 | 2023-07-12T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "Abell 399", "missing baryons", "close pairs", "act sz data", "cluster abell 399", "3d shape", "filament gas", "galaxy cluster", "intergalactic gas filaments", "chandra xray image" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Prof Craig Sarazin, 2023, 'Bridges of Intergalactic Gas Connecting ACT Cluster Pairs', 20.08_20220509_1852, European Space Agency, https://doi.org/10.57780/esa-o8kbz62 |