A dataset provided by the European Space Agency

Name 088135
Title Physics and Energetics of the Ultra Fast Outflow in IRAS F11119+3257
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881350101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881350201

DOI https://doi.org/10.57780/esa-g4cshz7
Author Dr Giorgio Lanzuisi
Description IRASF11119+3257 is an Ultra Luminous Infrared Galaxy (ULIRG) with post merger
morphology, hosting a type-1 QSO (LX 10^44 erg/s at z=0.189) with a persistent
UFO (v 0.25c) observed with both NuSTAR and Suzaku. It is also the first system
in which it was possible to connect the nuclear outflow with a galaxy-scale
molecular outflow, observed in OH and CO transitions. Despite its exceptional
properties, the source was never observed with XMM-Newton. We request a 110ks
XMM-Newton observation to study in detail the nuclear outflow properties and
energetics. We also request 53 ks of simultaneous NuSTAR observation, which is
crucial in order to constrain the blue wing of the UFO, and the absorption edges
and continuum above 10 keV.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-11-12T07:15:26Z/2021-11-13T17:57:17Z
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 2022-12-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Giorgio Lanzuisi, 2022, 088135, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-g4cshz7