A dataset provided by the European Space Agency

Name 072444
Title Resolving AGN with PanSTARRS transients
URL

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

DOI 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 XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The broad-band SEDs of four 'hypervariable. AGN . Collinson, James S., Ward, Martin J., et all. . MNRAS . 474-3565 . 2018 . 2018MNRAS.474.3565C ,
The 'Big Dipper.: the nature of the extreme variability of the AGN SDSS J2232-0806 . Kynoch, Daniel, Ward, Martin J., et all. . MNRAS . 485-2573 . 2019 . 2019MNRAS.485.2573K ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
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