A dataset provided by the European Space Agency

Name 087261
Title Microlensing a Quasar.s Accretion Disk
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0872610901

DOI https://doi.org/10.57780/esa-7bbh6vc
Author Dr George Chartas
Description We propose a joint 6x30 ks Chandra and 6x40 ks XMM-Newton monitoring campaign of
the lens system RXJ1131 to reach the following goals: (1) Confirm and validate
the microlensing method of constraining the spin and inclination angle of a
z=0.658 lensed quasar. (2) Identify the origin of the soft excess, and (3)
compare these results to those obtained by employing the relativistic Fe line
method. The Chandra observations are crucial in resolving the 4 images,
unambiguously identifying a microlensing event, and providing the unlensed
source spectrum. XMM-Newton has the required effective area to provide
constraints on the soft and hard reflection components originating from the
disk.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-06-10T14:09:10Z/2021-12-30T18:46:13Z
Version 19.16_20210326_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 2023-01-14T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr George Chartas, 2023, 087261, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-7bbh6vc