A dataset provided by the European Space Agency

Name: Quantifying the impact of galaxy-scale jets from the LOFAR Two-Metre Sky Survey
Published: 2021-01-11T00:00:00Z

Proposal ID	084426
Title	Quantifying the impact of galaxy-scale jets from the LOFAR Two-Metre Sky Survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844260101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844260201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844260501
DOI	https://doi.org/10.5270/esa-ia8zrgf
Principal Investigator, PI	Dr Judith Croston
Abstract	Our previous X-ray observations have provided some of the most direct evidenceso far for the galaxy-scale feedback role of AGN jets. However, until recentlyonly a small number of galaxy-scale jets were known. With the new LOFAR TwoMetre Sky Survey Data Release 1, we have been able for the first time to build arepresentative sample of galaxy-scale jets. Here we propose XMM-Newtonobservations of four galaxy-scale jets from this sample, two of which havespiral host galaxies, and all of which are predicted to be stronglyover-pressured with respect to their environments. We aim to detect shock-heatedgas and directly measure the cumulative energy deposition of these jets intotheir galaxy ISM, and therefore obtain the first population-wide view of galaxy-scale jet feedback.
Publications	Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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 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	2019-10-22T16:25:19Z/2019-11-14T08:50:51Z
Version	18.00_20191217_1110
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	2021-01-11T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "population wide", "XMM-Newton", "agn jets", "cumulative energy deposition", "metre sky survey", "xmm newton", "shock heated gas", "galaxy scale jets", "galaxy ism"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Judith Croston, 2021, 'Quantifying the impact of galaxy-scale jets from the LOFAR Two-Metre Sky Survey', 18.00_20191217_1110, European Space Agency, https://doi.org/10.5270/esa-ia8zrgf