A dataset provided by the European Space Agency

Name 090023
Title The extreme X-ray weakness of PG 0043+039
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0900230301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0900230501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0900230601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0900230701

DOI https://doi.org/10.57780/esa-8hg9is9
Author European Space Agency
Description PG 0043+039 is the most X-ray weak quasar known. XMM-Newton observation in 2013
set a clear detection meaning a flux at least 3.8 times higher than in 2005. The
quasar remained extremely X-ray weak, with a peculiar spectral energy
distribution (SED) and a unique UV spectrum. This unique source deserves
further, deeper, observations, to establish its X-ray spectrum, its optical to
hard-X-ray SED and its variability. We aim at probing our hypothesis that PG
0043+039 is a genuine X-ray weak quasar and to test alternative scenarios
(ADAFs, missing corona, cyclotron-emission). We propose to observe PG0043+039
quasi-simultaneously (2 days) with XMM-Newton (20+100ks), NuSTAR (60ks), HST (2
orbits), 10m Hobby-Eberly and 10m SALT Telescope in South Africa.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-06-15T16:54:19Z/2022-07-11T01:56:10Z
Version 20.08_20220509_1852
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 2023-07-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, The Extreme X-Ray Weakness Of Pg 0043+039, 20.08_20220509_1852, European Space Agency, https://doi.org/10.57780/esa-8hg9is9