A dataset provided by the European Space Agency

Name: High Resolution Spectroscopy of NGC 1399 at the Core of the Fornax Cluster
Published: 2009-10-02T00:00:00Z

Proposal ID	040062
Title	High Resolution Spectroscopy of NGC 1399 at the Core of the Fornax Cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400620101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400620201
DOI	https://doi.org/10.5270/esa-lpfxnst
Principal Investigator, PI	Prof Frederik Paerels
Abstract	We propose to obtain a high resolution spectrum of the giant elliptical galaxy NGC 1399 at the core of the Fornax Cluster. The RGS will fully resolve the soft X-ray emission line spectrum of the hot diffuse gas inthe galaxy. The properties of the hot gas can be determined without the usual ambiguities; spatial gradients will be constrained with the cross-dispersion image. We will likely detect the effect of resonance scattering on the spatial profile of the strongest Fe L emission line, which allows for a very powerful internal consistency test on our measurement of temperature, density, and abundances. It will also provide a strong constraint on the amplitude of the velocity field in the diffuse gas.
Publications	Elemental Abundances in the X-Ray Gas of Early-Type Galaxies with XMM-Newton and Chandra Observations \|Ji, Jun, Irwin, Jimmy A., et al. \| ApJ \| 696-2252 \| 2009 \| 2009ApJ...696.2252J \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696.2252J A Variable Black Hole X-ray Source in an NGC 1399 Globular Cluster \|Shih, I. Chun, Kundu, Arunav, et al. \| ApJ \| 721-323 \| 2010 \| 2010ApJ...721..323S \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721..323S HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion \|Zhang, Y.-Y., Andernach, H., et al. \| A&A \| 526-105 \| 2011 \| 2011A&A...526A.105Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A.105Z Suzaku and XMM-Newton Observations of the Fornax Cluster: Temperature and Metallicity Distribution \|Murakami, Hideyoshi, Komiyama, Madoka, et al. \| PASJ \| 63-963 \| 2011 \| 2011PASJ...63S.963M \| http://ui.adsabs.harvard.edu/#abs/2011PASJ...63S.963M The Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters \|Wik, Daniel R., Sarazin, Craig L., et al. \| ApJ \| 748-67 \| 2012 \| 2012ApJ...748...67W \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748...67W Comparison of approximately isothermal gravitational potentials of elliptical galaxies based on X-ray and optical data \|Churazov, E., Tremaine, S., et al. \| MNRAS \| 404-1165 \| 2010 \| 2010MNRAS.404.1165C \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.404.1165C The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey \|Corral, A., Della Ceca, R., et al. \| A&A \| 530-42 \| 2011 \| 2011A&A...530A..42C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...530A..42C Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Properties of the integrated spectrum of serendipitous 2XMM catalog sources \|Chaudhary, P., Brusa, M., et al. \| A&A \| 518-58 \| 2010 \| 2010A&A...518A..58C \| http://ui.adsabs.harvard.edu/#abs/2010A&A...518A..58C Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line \|Chaudhary, P., Brusa, M., et al. \| A&A \| 537-6 \| 2012 \| 2012A&A...537A...6C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A...6C A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton \|Frank, K. A., Peterson, J. R., et al. \| ApJ \| 764-46 \| 2013 \| 2013ApJ...764...46F \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764...46F Velocity width measurements of the coolest X-ray emitting material in the cores of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 429-2727 \| 2013 \| 2013MNRAS.429.2727S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.2727S Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact \|Schellenberger, G., Reiprich, T. H., et al. \| A&A \| 575-30 \| 2015 \| 2015A&A...575A..30S \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..30S Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence \|Pinto, Ciro, Sanders, Jeremy S., et al. \| A&A \| 575-38 \| 2015 \| 2015A&A...575A..38P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..38P Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC \|Mernier, F., de Plaa, J., et al. \| A&A \| 592-157 \| 2016 \| 2016A&A...592A.157M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A.157M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models \|Mernier, F., de Plaa, J., et al. \| A&A \| 595-126 \| 2016 \| 2016A&A...595A.126M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A.126M HIFLUGCS: X-ray luminosity-dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys \|Zhang, Yu-Ying, Reiprich, Thomas H., et al. \| A&A \| 599-138 \| 2017 \| 2017A&A...599A.138Z \| http://ui.adsabs.harvard.edu/#abs/2017A&A...599A.138Z AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis, sample selection and luminosity-mass scaling relation \|Schellenberger, G., Reiprich, T. H., \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S HICOSMO: cosmology with a complete sample of galaxy clusters - II. Cosmological results \|Schellenberger, G., Reiprich, T. H., \| MNRAS \| 471-1370 \| 2017 \| 2017MNRAS.471.1370S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1370S Improved measurements of turbulence in the hot gaseous atmospheres of nearby giant elliptical galaxies \|Ogorzalek, A., Zhuravleva, I., et al. \| MNRAS \| 472-1659 \| 2017 \| 2017MNRAS.472.1659O \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472.1659O CHEERS: The chemical evolution RGS sample \|de Plaa, J., Kaastra, J. S., et al. \| A&A \| 607-98 \| 2017 \| 2017A&A...607A..98D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A..98D Gas Sloshing Regulates and Records the Evolution of the Fornax Cluster \|Su, Yuanyuan, Nulsen, Paul E. J., et al. \| ApJ \| 851-69 \| 2017 \| 2017ApJ...851...69S \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...851...69S Solar abundance ratios of the iron-peak elements in the Perseus cluster \|Hitomi Collaboration, Aharonian, Felix, et al. \| Natur \| 551-478 \| 2017 \| 2017Natur.551..478H \| http://ui.adsabs.harvard.edu/#abs/2017Natur.551..478H Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies \|Mernier, F., de Plaa, J., et al. \| MNRAS \| 478-116 \| 2018 \| 2018MNRAS.478L.116M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478L.116M Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies \|Mernier, F., Werner, N., et al. \| MNRAS \| 480-95 \| 2018 \| 2018MNRAS.480L..95M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480L..95M The Recent Growth History of the Fornax Cluster Derived from Simultaneous Sloshing and Gas Stripping: Simulating the Infall of NGC 1404 \|Sheardown, Alex, Roediger, Elke, et al. \| ApJ \| 865-118 \| 2018 \| 2018ApJ...865..118S \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...865..118S Enrichment of the Hot Intracluster Medium: Observations \|Mernier, F., Biffi, V., et al. \| SSRv \| 214-129 \| 2018 \| 2018SSRv..214..129M \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214..129M Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr \|Ichikawa, Kohei, Ueda, Junko, et al. \| ApJ \| 870-65 \| 2019 \| 2019ApJ...870...65I \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...65I The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population \|Pratt, G. W., Arnaud, M., et al. \| SSRv \| 215-25 \| 2019 \| 2019SSRv..215...25P \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...25P Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu, Haonan, Pinto, Ciro, et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps \|Iodice, E., Sarzi, M., et al. \| A&A \| 627-136 \| 2019 \| 2019A&A...627A.136I \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A.136I X-ray spectra of the Fe-L complex \|Gu, Liyi, Raassen, A. J. J., et al. \| A&A \| 627-51 \| 2019 \| 2019A&A...627A..51G \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A..51G X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M The Fornax Deep Survey with VST. VIII. Connecting the accretion history with the cluster density \|Spavone, M., Iodice, E., et al. \| A&A \| 639-14 \| 2020 \| 2020A&A...639A..14S \| http://ui.adsabs.harvard.edu/#abs/2020A&A...639A..14S Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters \|Tian, Yong, Yu, Po-Chieh, et al. \| ApJ \| 910-56 \| 2021 \| 2021ApJ...910...56T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...56T A blind ATCA HI survey of the Fornax galaxy cluster. Properties of the HI detections \|Loni, A., Serra, P., et al. \| A&A \| 648-31 \| 2021 \| 2021A&A...648A..31L \| http://ui.adsabs.harvard.edu/#abs/2021A&A...648A..31L The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello, Fabio, Simionescu, Aurora, et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G 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 An XMM-Newton Early-type Galaxy Atlas \|Islam, Nazma, Kim, Dong-Woo, et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I High-resolution X-ray spectroscopy of astrophysical plasmas with X-ray microcalorimeters \|Ezoe, Yuichiro, Ohashi, Takaya, \| RvMPP \| 5-4 \| 2021 \| 2021RvMPP...5....4E \| http://ui.adsabs.harvard.edu/#abs/2021RvMPP...5....4E The cycle of metals in the infalling elliptical galaxy NGC 1404 \|Mernier, F., Werner, N., et al. \| MNRAS \| 511-3159 \| 2022 \| 2022MNRAS.511.3159M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.3159M A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra \|Wallbank, A. N., Maughan, B. J., et al. \| MNRAS \| 517-5594 \| 2022 \| 2022MNRAS.517.5594W \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.5594W CO(J = 1-0) Mapping Survey of 64 Galaxies in the Fornax Cluster with the ALMA Morita Array \|Morokuma-Matsui, Kana, Bekki, Kenji, et al. \| ApJS \| 263-40 \| 2022 \| 2022ApJS..263...40M \| http://ui.adsabs.harvard.edu/#abs/2022ApJS..263...40M O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy \|Fukushima, Kotaro, Kobayashi, Shogo B., \| ApJ \| 953-112 \| 2023 \| 2023ApJ...953..112F \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953..112F Hidden cooling flows in clusters of galaxies - III. Accretion on to the central black hole \|Fabian, A. C., Sanders, J. S., et al. \| MNRAS \| 524-716 \| 2023 \| 2023MNRAS.524..716F \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524..716F 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	2006-08-23T02:57:31Z/2006-08-24T17:40:24Z
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	2009-10-02T00:00:00Z
Keywords	"strongest fe", "hot gas", "resolution spectroscopy", "resonance scattering", "ngc 1399", "fornax cluster", "spatial profile", "diffuse gas", "hot diffuse gas", "velocity field", "spatial gradients", "resolution spectrum", "emission line", "cross dispersion image", "NGC 1399", "usual ambiguities"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Frederik Paerels, 2009, 'High Resolution Spectroscopy of NGC 1399 at the Core of the Fornax Cluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lpfxnst