A dataset provided by the European Space Agency

Name 069417
Title Two relativistic Fe lines in one shot: the case of ESO323-G77 and ESO323-G81
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694170101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694170201

DOI 10.5270/esa-pelf2pt
Author Dr Giovanni Miniutti
Description A previous relatively short (24~ks) XMM-Newton observation of ESO~323--G77 revealed a remarkably rich X--ray spectrum both in absorption and emission. Despite its Seyfert~1 nature, the X--ray spectrum is highly absorbed and resembles that of a typical Compton--thin Seyfert~2 galaxy. Two ionized absorbers-emitters imprinting a series of blueshifted absorption and emission lines. The robust detection of a relativistic Fe K line with relatively large equivalent width (200~eV) makes this source even more interesting. ESO~323--G81 is also present in the field. A broad excess is detected in the 6--7~keV region possibly revealing the presence of a braod Fe K line in this object. We propose a 130~ks observation to study in details the properties of both sources.
Publication The properties of the clumpy torus and BLR in the polar-scattered Seyfert 1 galaxy ESO 323-G77 through X-ray absorption variability . Miniutti, G., Sanfrutos, M., et all. . MNRAS . 437-1776 . 2014 . 2014MNRAS.437.1776M ,
The ionized X-ray outflowing torus in ESO 323-G77: low-ionization clumps confined by homogeneous warm absorbers . Sanfrutos, M., Miniutti, G., et all. . MNRAS . 457-510 . 2016 . 2016MNRAS.457..510S ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The SUrvey for Pulsars and Extragalactic Radio Bursts - I. Survey description and overview . Keane, E. F., Barr, E. D., et all. . MNRAS . 473-116 . 2018 . 2018MNRAS.473..116K ,
The 26.3-h orbit and multiwavelength properties of the 'redback. millisecond pulsar PSR J1306-40 . Linares, Manuel, . MNRAS . 473-50 . 2018 . 2018MNRAS.473L..50L ,
Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? . Williams, James K., Gliozzi, Mario, . MNRAS . 480-96 . 2018 . 2018MNRAS.480...96W ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-01-17T12:11:52Z/2013-01-19T02:08:25Z
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 2014-02-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-02-07T00:00:00Z, 069417, 17.56_20190403_1200. https://doi.org/10.5270/esa-pelf2pt