Name | 069290 |
Title | Cosmology from X-ray and Weak Lensing Observations of SZ Discovered Clusters |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692900101 |
DOI | https://doi.org/10.5270/esa-kkswedo |
Author | Dr Bradford Benson |
Description | We propose to complete X-ray observations of a sample of 20 intermediate redshift (0.3 < z < 0.5) massive clusters of galaxies discovered via the Sunyaev-Zel.dovich (SZ) effect by the South Pole Telescope (SPT). These clusters are uniformly selected by their SZ significance from 560 deg2 surveyed by the SPT, and are part of a ground-based weak lensing program using Magellan. The combined observations will calibrate X-ray and SZ observables to the lensing mass estimates with an overall 5% uncertainty for the ensemble of clusters. This result will improve SPT cluster mass estimates, which when applied to the 2500 deg ^2 SPT survey will allow a 5% constraint on the dark energy equation of state. To complete this sample, we need observations of 6 clusters requiring a total of 93 ksec. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2012-05-03T05:23:59Z/2012-05-31T18:20:35Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 | 2013-06-14T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2013-06-14T00:00:00Z, 069290, 17.56_20190403_1200. https://doi.org/10.5270/esa-kkswedo |