A dataset provided by the European Space Agency

Name 088499
Title HYPerluminous quasars at the Epoch of ReionizatION (HYPERION)
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884990101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884990401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884990901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884991101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884991501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884991701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884992001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884992101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884992401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884992601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884992901
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884993901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884994001

DOI https://doi.org/10.57780/esa-7b9wyrz
Author European Space Agency
Description The growth of Supermassive Black Holes powering luminous quasars at the Epoch of
Reionization (EoR, z>6) is a hot topic in astrophysics. These quasars are being
characterized with large multiwavelength campaigns with current flagship
observatories. X-ray observations performed so far provided mostly < 15 counts
in 0.5-10 keV spectra and thus a poor characterization of their properties. We
propose HYPERION, a 2.3 Ms Multi-Year Heritage programme, to dramatically
improve data quality to 100 counts for 15 luminous quasars at EoR, delivering
unprecedented constraints on nuclear properties, accretion, ejection,
disc/corona complex. It will nicely complement observations at other wavelengths
enabling meaningful X-ray spectroscopic studies at EoR to begin.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-06-26T18:27:30Z/2023-01-16T16:38:26Z
Version 20.09_20221024_1724
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 2024-02-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2024, Hyperluminous Quasars At The Epoch Of Reionization Openparhyperionclosepar, 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-7b9wyrz