A dataset provided by the European Space Agency

Name 055046
Title X-ray emission of a representative sample of local Luminous Infrared Galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550460901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550461001

DOI 10.5270/esa-slo0v0l
Author Dr Almudena Alonso-Herrero
Description We propose to observe with XMM-Newton 8 Luminous Infrared Galaxies (LIRGs, L_IR=10^11-10^12L_sun) and analyze existing X-ray data for another 7 LIRGs. Previous X-ray studies of local LIRGs are biased towards the most IR-luminous objects as well as those systems hosting a bright AGN. These 15 local LIRGs are representative of the LIRG class in terms of IR luminosity and nuclear activity. The proposed XMM observations together with existing multi-wavelength (UV to IR) data will allow to characterize the star formation history of these galaxies and relate it to their X-ray emission. A comprehensive multi-wavelength understanding of the extreme processes (star formation and AGN) taking place in local LIRGs is needed to improve the linkage of X-ray, UV and IR observations of deep cosmological fields.
Publication The X-ray emission of local luminous infrared galaxies . Pereira-Santaella, M., Alonso-Herrero, A., et all. . A&A . 535-93 . 2011 . 2011A&A...535A..93P ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Chandra Observations and Classification of Active Galactic Nucleus Candidates Correlated with Auger UHECRs . Terrano, William A., Zaw, Ingyin, . ApJ . 754-142 . 2012 . 2012ApJ...754..142T ,
An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission . Henley, David B., Shelton, Robin L., . ApJ . 773-92 . 2013 . 2013ApJ...773...92H ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission . Henley, David B., Shelton, Robin L., et all. . ApJ . 800-102 . 2015 . ...,
The X-Ray Zurich Environmental Study (X-ZENS). II. X-Ray Observations of the Diffuse Intragroup Medium in Galaxy Groups . Miniati, Francesco, Finoguenov, Alexis, et all. . ApJ . 819-26 . 2016 . 2016ApJ...819...26M ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured . Ricci, C., Bauer, F. E., et all. . MNRAS . 468-1273 . 2017 . 2017MNRAS.468.1273R ,
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies . Earnshaw, H. P., Roberts, T. P., et all. . MNRAS . 483-5554 . 2019 . 2019MNRAS.483.5554E ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-05-13T09:40:31Z/2009-04-19T03:41:36Z
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 2010-05-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-05-19T00:00:00Z, 055046, 17.56_20190403_1200. https://doi.org/10.5270/esa-slo0v0l