A dataset provided by the European Space Agency

Name 072444
Title Resolving AGN with PanSTARRS transients
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724440901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724441001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724441101

DOI https://doi.org/10.5270/esa-tmhzvqu
Author Prof Andy Lawrence
Description With PanSTARRS we have discovered a new class of slow, blue nuclear transients which we believe to be rare examples of background AGN microlensed by stars in foreground galaxies, amplified by a factor of 10--100. The background AGN should be somewhat resolved by the foreground lens, providing a unique new diagnostic of AGN size and structure - the UV, optical, IR, BLR, and X-ray regions should have differing evolutions during the event. This proposal is a first step towards understanding the structure of the X-ray source : testing the microlensing hypothesis, characterising the SED, and establishing the first two epochs in an expected gradual decline.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-08-12T02:33:10Z/2014-02-10T16:35:38Z
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 2015-03-04T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-03-04T23:00:00Z, 072444, 17.56_20190403_1200. https://doi.org/10.5270/esa-tmhzvqu