A dataset provided by the European Space Agency

Name 072777
Title RCAL: RGS effective area and Cross-calibration (PKS2155-304)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727770101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727770501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727770901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727771001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727771101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727771201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0727771301

DOI 10.5270/esa-pwek85k
Author Dr Fred Jansen XMM-Newton MM
Description
Publication Calibration and in-orbit performance of the reflection grating spectrometer onboard XMM-Newton . de Vries, C. P., den Herder, J. W., et all. . A&A . 573-128 . 2015 . 2015A&A...573A.128D ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund J., Miller, Matthew J., . ApJ . 822-21 . 2016 . 2016ApJ...822...21H ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Discovery of Galactic O iv and O v X-ray absorption due to transition temperature gas in the PKS 2155-304 spectrum . Nevalainen, J., Wakker, B., et all. . A&A . 605-47 . 2017 . 2017A&A...605A..47N ,
The Hard X-Ray Emission of the Blazar PKS 2155-304 . Gaur, Haritma, Chen, Liang, et all. . ApJ . 850-209 . 2017 . 2017ApJ...850..209G ,
X-ray spectral variability of blazars using principal component analysis . Gallant, D., Gallo, L. C., . MNRAS . 480-1999 . 2018 . 2018MNRAS.480.1999G ,
To be or not to be: the case of the hot WHIM absorption in the blazar PKS 2155-304 sight line . Nevalainen, J., Tempel, E., et all. . A&A . 621-88 . 2019 . 2019A&A...621A..88N ,
Variability studies and modelling of the blazar PKS 2155-304 in the light of a decade of multi-wavelength observations . Chevalier, J., Sanchez, D. A., et all. . MNRAS . 484-749 . 2019 . 201...,
Short-Term X-ray Variability during Different Activity Phases of Blazars S5 0716+714 and PKS 2155-304 . Kushwaha, Pankaj, Pal, Main, . Galax . 8-66 . 2020 . 2020Galax...8...66K ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-10-26T04:17:27Z/2014-10-29T05:50:01Z
Version PPS_NOT_AVAILABLE
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 2014-11-03T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-11-03T23:00:00Z, 072777, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-pwek85k