A dataset provided by the European Space Agency

Name 060487
Title Testing Cosmological SZE-X-ray-Multi-Wavelength Galaxy Cluster Surveys
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870331
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870332
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870333
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870334
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870335
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870336
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870337
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870338
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870339
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870340
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870341
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870342
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870343
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870344
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870345
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870346
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870347
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870348
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604870349
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873431
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873432
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873433
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873434
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873435
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873436
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873437
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873438
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873439
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873440
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873441
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873442
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873443
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873444
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873445
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873446
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873447
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873448
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873449
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873931
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873932
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873933
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873934
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873935
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873936
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873937
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873938
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873939
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873940
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873941
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873942
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873943
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873944
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873945
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873946
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873947
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873948
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604873949

DOI https://doi.org/10.5270/esa-13azing
Author Prof Hans Boehringer
Description Sunyaev-Zeldovich Effect (SZE) surveys have finally and successfully opened a
new window to study the cosmic large-scale structure in a more promising way
than previous methods. We have performed a coordinated SZE, X-ray, and
optical/MIR survey to best understand the potential of this new survey technique
and obtained the first exciting multi-wavelength detections. Here we propose to
extent the current small test area applying the new XMM-Newton mosaic mode,
which allows us to adapt our survey optimally to the depth of the SZE surveys
allowing for about 100 cluster detections with XMM.
Publication No observations found associated with the current proposal
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2009-10-31T01:58:52Z/2009-12-07T01:09:19Z
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 2010-12-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Hans Boehringer, 2010, 060487, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-13azing