A dataset provided by the European Space Agency

Name: Two relativistic Fe lines in one shot: the case of ESO323-G77 and ESO323-G81
Published: 2014-02-07T00:00:00Z

Proposal ID	069417
Title	Two relativistic Fe lines in one shot: the case of ESO323-G77 and ESO323-G81
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694170101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694170201
DOI	https://doi.org/10.5270/esa-pelf2pt
Principal Investigator, PI	Dr Giovanni Miniutti
Abstract	A previous relatively short (24~ks) XMM-Newton observation of ESO~323--G77revealed a remarkably rich X--ray spectrum both in absorption and emission.Despite its Seyfert~1 nature, the X--ray spectrum is highly absorbed andresembles that of a typical Compton--thin Seyfert~2 galaxy. Two ionizedabsorbers/emitters imprinting a series of blueshifted absorption and emissionlines. The robust detection of a relativistic Fe K line with relatively largeequivalent width (200~eV) makes this source even more interesting. ESO~323--G81is also present in the field. A broad excess is detected in the 6--7~keV regionpossibly revealing the presence of a braod Fe K line in this object. We proposea 130~ks observation to study in details the properties of both sources.
Publications	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 al. \| MNRAS \| 437-1776 \| 2014 \| 2014MNRAS.437.1776M \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 457-510 \| 2016 \| 2016MNRAS.457..510S \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.457..510S The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The SUrvey for Pulsars and Extragalactic Radio Bursts - I. Survey description and overview \|Keane E. F. Barr E. D. et al. \| MNRAS \| 473-116 \| 2018 \| 2018MNRAS.473..116K \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480...96W Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Changing-look active galactic nuclei \|Ricci Claudio Trakhtenbrot Benny \| NatAs \| 7-1282 \| 2023 \| 2023NatAs...7.1282R \| http://ui.adsabs.harvard.edu/#abs/2023NatAs...7.1282R From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Last Update	2025-01-27
Keywords	"relativistic fe lines", "xmm newton", "ev makes", "emitters imprinting", "relativistic fe", "eso323 g77", "G81.", "x ray spectrum", "emission lines", "broad excess", "robust detection", "XMM-Newton", "braod fe", "323 g81", "eso323 g81", "323 g77", "equivalent width", "kev region", "XMM", "ionized absorbers", "relatively short", "blueshifted absorption"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Giovanni Miniutti, 2014, 'Two relativistic Fe lines in one shot: the case of ESO323-G77 and ESO323-G81', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pelf2pt