A dataset provided by the European Space Agency

Name 089105
Title BROAD-BAND X-RAY STUDY OF A PECULIAR HYPER-EDDINGTON AGN: IRAS04416+1215
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0891050101

DOI https://doi.org/10.57780/esa-wclzpdt
Author European Space Agency
Description We propose here a broadband X-ray study of a peculiar hyper-Eddington Active
Galactic Nucleus, namely IRAS 04416+1215, by observing it simultaneously with
NuSTAR (170ks) and XMM-Newton (40ks). IRAS 04416+1215 has one of the highest
Eddington-ratio in the local Universe (lambdaEdd=427), it represents a prototype
for the elusive class of hyper-Eddington AGN. The aim of these simultaneous
observations is to understand the behaviour of the primary power-law and the
reprocessed radiation in the regime of extreme accretion, as well as the
properties of soft-excess and the outflows. To this end, the combined large
effective area of XMM-Newton and high sensitivity of NuSTAR at high energy are
fundamental to constrain the spectral parameter of the proposed target.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-02-20T06:27:20Z/2022-02-20T18:05:40Z
Version 19.17_20220121_1250
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 2023-03-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Broad-Band X-Ray Study Of A Peculiar Hyper-Eddington Agn: Iras04416+1215, 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-wclzpdt