A dataset provided by the European Space Agency

Name 076110
Title Securing the Detection of the Hot Roaming Baryons with the XMM-Newton
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761100101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761100201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761100301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761100401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761100701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761101001

DOI https://doi.org/10.5270/esa-s15kaot
Author European Space Agency
Description We propose a 1.6 Ms XMM-Newton ..Very Large Program. to settle unambiguously
one of the most controversial and open problems of modern astrophysics: the
existence of the missing baryons in a WHIM. We will do so by complementing the
first successful exploratory LETG observation of the z>0.4 blazar 1ESvirgul1553+113,
with additional 1.6 Ms of XMM-Newton RGS time, so more than doubling the S/N and
thus the absorption line equivalent width sensitivity of the currently available
LETG spectrum in the fundamental spectral region of the intervening oxygen. The
proposed observation will enable:(1) the solution to the missing-baryon problem;
(2) a robust estimate of the WHIM metallicity; (3) pioneering studiesof thermo-
and chemo-dynamics of the IGM with cosmic time and so of the diffuse-gas/galaxies interplay.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-07-29T19:57:33Z/2015-09-01T08:29:09Z
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 2015-09-07T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015, Securing The Detection Of The Hot Roaming Baryons With The Xmm-Newton, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-s15kaot