A dataset provided by the European Space Agency

Name: STUDYING THE ENVIRONMENT OF LOW LUMINOSITY AGN
Published: 2022-01-26T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	087102
Title	STUDYING THE ENVIRONMENT OF LOW LUMINOSITY AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871020101
DOI	https://doi.org/10.57780/esa-7bmip5l
Principal Investigator, PI	Ms Yaherlyn Diaz
Abstract	Recent observations point out that Low-luminosity active galactic nuclei, suchLINERs and low power Seyfert galaxies, might have a different torusconfiguration compared to more powerful AGNs. The shape of the Compton humpobserved above 10 KeV is an excellent tool to study the geometry and thephysical features of the reflector. The purpose of this proposal is study a lowpowered (L/LEdd sim 10^-5) Seyfert galaxy NGC 5033, to study the characteristicsof the material surrounding the SMBH. We ask for observations with NuSTAR andXMM-Newton to study the relation between the accretion rate and properties ofthe reflector (torus covering fraction and column density) and to compare withexisting, similar quality data of a LINER with equal black hole mass and accretion rate.
Publications	Constraining the X-ray reflection in low accretion-rate active galactic nuclei using XMM-Newton NuSTAR and Swift \|Diaz Y. Hernu00e0ndez-Garcu00eda L. et al. \| A&A \| 669-114 \| 2023 \| 2023A&A...669A.114D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.114D Coronal properties of low-accreting AGNs using Swift XMM-Newton and NuSTAR observations \|Jana Arghajit Chatterjee Arka et al. \| MNRAS \| 524-4670 \| 2023 \| 2023MNRAS.524.4670J \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.4670J Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2020-12-10T06:20:31Z/2020-12-10T12:10:31Z
Version	21.51_20241115_1113
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	2022-01-26T00:00:00Z
Last Update	2026-07-09
Keywords	"NGC 5033", "torus configuration", "reflector torus", "XMM-Newton", "equal blackhole mass", "powerful agns", "ledd sim", "compton hump", "quality data", "NuSTAR", "accretion rate", "XMM", "low luminosity agn", "low powered", "column density", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Yaherlyn Diaz, 2022, 'STUDYING THE ENVIRONMENT OF LOW LUMINOSITY AGN', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-7bmip5l
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.