A dataset provided by the European Space Agency

Name: High Resolution Spectroscopy of the Cluster of Galaxies A 1795
Published: 2001-10-31T00:00:00Z

Proposal ID	009782
Title	High Resolution Spectroscopy of the Cluster of Galaxies A 1795
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0097820101
DOI	https://doi.org/10.5270/esa-j5hmsog
Principal Investigator, PI	Dr Albert Brinkman
Abstract	We propose to observe the cluster of galaxies A 1795 to verify the capabilityof the RGS to analyse spatially resolved extended sources. A 1795 is anideal target for this since it has a FWHM of only 1.8 arcmin, allowinga high spectral resolution with the RGS and also an almost completecoverage of the cooling flow region within the cross-dispersion widthof the detector. In particular we will study the temperature andabundance distribution of the cooling flow region. The EPIC observationswill supplement this for the outer regions of the cluster, wherewe will study the abundance and temperature gradients as well asinvestigate the existence of non-thermal components.
Publications	Is the Gas in Cooling Flows Multiphase? \|Molendi, Silvano, Pizzolato, Fabio, \| ApJ \| 560-194 \| 2001 \| 2001ApJ...560..194M \| http://ui.adsabs.harvard.edu/#abs/2001ApJ...560..194M Metal abundances in the cool cores of galaxy clusters \|de Grandi, S., Molendi, S., \| A&A \| 508-565 \| 2009 \| 2009A&A...508..565D \| http://ui.adsabs.harvard.edu/#abs/2009A&A...508..565D Cross-calibrating X-ray detectors with clusters of galaxies: an IACHEC study \|Nevalainen, J., David, L., \| A&A \| 523-22 \| 2010 \| 2010A&A...523A..22N \| http://ui.adsabs.harvard.edu/#abs/2010A&A...523A..22N Galaxy Clusters in the Swift/BAT Era. II. 10 More Clusters Detected Above 15 keV \|Ajello, M., Rebusco, P., et al. \| ApJ \| 725-1688 \| 2010 \| 2010ApJ...725.1688A \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.1688A 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 Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita, K., \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan, A. J., Tanvir, N. R., et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L Studying the X-ray/UV Variability of Active Galactic Nuclei with data from Swift and XMM archives \|Turriziani, Sara, \| JPhCS \| 280-12005 \| 2011 \| 2011JPhCS.280a2005T \| http://ui.adsabs.harvard.edu/#abs/2011JPhCS.280a2005T New constraints on the X-ray spectral properties of type 1 active galactic nuclei \|Scott, A. E., Stewart, G. C., et al. \| MNRAS \| 417-992 \| 2011 \| 2011MNRAS.417..992S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.417..992S Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M A combined optical and X-ray study of unobscured type 1 active galactic nuclei - I. Optical spectra and spectral energy distribution modelling \|Jin, Chichuan, Ward, Martin, et al. \| MNRAS \| 420-1825 \| 2012 \| 2012MNRAS.420.1825J \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.1825J Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 536-11 \| 2011 \| 2011A&A...536A..11P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..11P 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 Two-phase ICM in the Central Region of the Rich Cluster of Galaxies A1795: A Joint Chandra, XMM-Newton, and Suzaku View \|Gu, Liyi, Xu, Haiguang, et al. \| ApJ \| 749-186 \| 2012 \| 2012ApJ...749..186G \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...749..186G The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M Cool core remnants in galaxy clusters \|Rossetti, M., Molendi, S., \| A&A \| 510-83 \| 2010 \| 2010A&A...510A..83R \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..83R The Axis Ratio Distribution of X-ray Clusters Observed by XMM-Newton \|Kawahara, Hajime, \| ApJ \| 719-1926 \| 2010 \| 2010ApJ...719.1926K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...719.1926K Star Formation Efficiency in the Cool Cores of Galaxy Clusters \|McDonald, Michael, Veilleux, Sylvain, et al. \| ApJ \| 734-95 \| 2011 \| 2011ApJ...734...95M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...734...95M Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies \|Zhang, Y.-Y., Lagana, T. F., et al. \| A&A \| 535-78 \| 2011 \| 2011A&A...535A..78Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...535A..78Z XMM-Newton/Sloan Digital Sky Survey: Star Formation Efficiency in Galaxy Clusters and Constraints on the Matter-density Parameter \|Lagana, Tatiana F., Zhang, Yu-Ying, et al. \| ApJ \| 743-13 \| 2011 \| 2011ApJ...743...13L \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...743...13L Measuring cluster temperature profiles with XMM/EPIC \|Arnaud, M., Neumann, D. M., et al. \| A&A \| 365-80 \| 2001 \| 2001A&A...365L..80A \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L..80A X-ray spectroscopy of the cluster of galaxies Abell 1795 with XMM-Newton \|Tamura, T., Kaastra, J. S., et al. \| A&A \| 365-87 \| 2001 \| 2001A&A...365L..87T \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L..87T UV observations of the galaxy cluster Abell 1795 with the optical monitor on XMM-Newton \|Mittaz, J. P. D., Kaastra, J. S., et al. \| A&A \| 365-93 \| 2001 \| 2001A&A...365L..93M \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L..93M The new emerging model for the structure of cooling cores in clusters of galaxies \|Bohringer, H., Matsushita, K., et al. \| A&A \| 382-804 \| 2002 \| 2002A&A...382..804B \| http://ui.adsabs.harvard.edu/#abs/2002A&A...382..804B XMM-Newton confirmation of soft X-ray excess emission in clusters of galaxies - The discovery of O VII emission from an extended warm baryonic component \|Kaastra, J. S., Lieu, R., et al. \| A&A \| 397-445 \| 2003 \| 2003A&A...397..445K \| http://ui.adsabs.harvard.edu/#abs/2003A&A...397..445K Improving the spatial resolution of XMM-Newton EPIC images by direct demodulation technique} \|Feng, Hua, Chen, Yong, et al. \| A&A \| 402-1151 \| 2003 \| 2003A&A...402.1151F \| http://ui.adsabs.harvard.edu/#abs/2003A&A...402.1151F Spatially resolved X-ray spectroscopy of cooling clusters of galaxies \|Kaastra, J. S., Tamura, T., et al. \| A&A \| 413-415 \| 2004 \| 2004A&A...413..415K \| http://ui.adsabs.harvard.edu/#abs/2004A&A...413..415K Elemental abundances in the intracluster medium as observed with XMM-Newton \|Tamura, T., Kaastra, J. S., et al. \| A&A \| 420-135 \| 2004 \| 2004A&A...420..135T \| http://ui.adsabs.harvard.edu/#abs/2004A&A...420..135T Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton \|Piffaretti, R., Jetzer, Ph., et al. \| A&A \| 433-101 \| 2005 \| 2005A&A...433..101P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...433..101P Effervescent heating: constraints from nearby cooling flow clusters observed with XMM-Newton \|Piffaretti, R., Kaastra, J. S., \| A&A \| 453-423 \| 2006 \| 2006A&A...453..423P \| http://ui.adsabs.harvard.edu/#abs/2006A&A...453..423P Constraining supernova models using the hot gas in clusters of galaxies \|de Plaa, J., Werner, N., et al. \| A&A \| 465-345 \| 2007 \| 2007A&A...465..345D \| http://ui.adsabs.harvard.edu/#abs/2007A&A...465..345D A catalog of galaxy clusters observed by XMM-Newton \|Snowden, S. L., Mushotzky, R. F., et al. \| A&A \| 478-615 \| 2008 \| 2008A&A...478..615S \| http://ui.adsabs.harvard.edu/#abs/2008A&A...478..615S Temperature structure of the intergalactic medium within seven nearby and bright clusters of galaxies observed with XMM-Newton \|Bourdin, H., Mazzotta, P., \| A&A \| 479-307 \| 2008 \| 2008A&A...479..307B \| http://ui.adsabs.harvard.edu/#abs/2008A&A...479..307B Soft X-Ray Excess Emission in Clusters of Galaxies Observed with XMM-Newton \|Nevalainen, J., Lieu, R., et al. \| ApJ \| 584-716 \| 2003 \| 2003ApJ...584..716N \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...584..716N High-Resolution X-Ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies \|Peterson, J. R., Kahn, S. M., et al. \| ApJ \| 590-207 \| 2003 \| 2003ApJ...590..207P \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...590..207P Smaug: A New Technique for the Deprojection of Galaxy Clusters \|Pizzolato, Fabio, Molendi, Silvano, et al. \| ApJ \| 592-62 \| 2003 \| 2003ApJ...592...62P \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...592...62P X-Ray Measurement of Dark Matter Temperature.. in A1795 \|Ikebe, Yasushi, Bohringer, Hans, \| ApJ \| 611-175 \| 2004 \| 2004ApJ...611..175I \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...611..175I XMM-Newton EPIC Background Modeling for Extended Sources \|Nevalainen, J., Markevitch, M., \| ApJ \| 629-172 \| 2005 \| 2005ApJ...629..172N \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...629..172N Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data \|Hicks, A. K., Mushotzky, R., \| ApJ \| 635-9 \| 2005 \| 2005ApJ...635L...9H \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...635L...9H On the Lack of a Soft X-Ray Excess from Clusters of Galaxies \|Bregman, Joel N., Lloyd-Davies, Edward J., \| ApJ \| 644-167 \| 2006 \| 2006ApJ...644..167B \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...644..167B Revisiting the Soft X-Ray Excess Emission in Clusters of Galaxies Observed with XMM-Newton \|Nevalainen, J., Bonamente, M., \| ApJ \| 656-733 \| 2007 \| 2007ApJ...656..733N \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...656..733N XMM-Newton study of soft excess X-ray emission in clusters of galaxies \|Kaastra, J. S., Lieu, R., et al. \| AdSpR \| 34-2504 \| 2004 \| 2004AdSpR..34.2504K \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..34.2504K Cold fronts in galaxy clusters \|Ghizzardi, S., Rossetti, M., \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G 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 A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis, Antonis, Nandra, K., \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G 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 Collisional interaction limits between dark matter particles and baryons in cooling flow. clusters \|Hu, Jian, Lou, Yu-Qing, \| MNRAS \| 384-814 \| 2008 \| 2008MNRAS.384..814H \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.384..814H Reflection-dominated X-ray spectra of narrow-line Seyfert 1 galaxies: Mrk 478 and EXO 1346.2+2645 \|Zoghbi, A., Fabian, A. C., \| MNRAS \| 391-2003 \| 2008 \| 2008MNRAS.391.2003Z \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.391.2003Z A search for X-ray flashes with XMM-Newton \|Law, Nicholas M., Rutledge, Robert E., \| MNRAS \| 350-1079 \| 2004 \| 2004MNRAS.350.1079L \| http://ui.adsabs.harvard.edu/#abs/2004MNRAS.350.1079L Detection of X-ray galaxy clusters based on the Kolmogorov method \|Gurzadyan, V. G., Durret, F., et al. \| EL \| 95-69001 \| 2011 \| 2011EL.....9569001G \| http://ui.adsabs.harvard.edu/#abs/2011EL.....9569001G An X-ray view of 82 LINERs with Chandra and XMM-Newton data \|Gonzalez-Martin, O., Masegosa, J., et al. \| A&A \| 506-1107 \| 2009 \| 2009A&A...506.1107G \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1107G Thermo-dynamic and chemical properties of the intra-cluster medium \|Leccardi, A., Rossetti, M., \| A&A \| 510-82 \| 2010 \| 2010A&A...510A..82L \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..82L On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters \|McDonald, Michael, Veilleux, Sylvain, et al. \| ApJ \| 721-1262 \| 2010 \| 2010ApJ...721.1262M \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721.1262M The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei \|Scott, A. E., Stewart, G. C., \| MNRAS \| 423-2633 \| 2012 \| 2012MNRAS.423.2633S \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.2633S 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 X-ray variability of 104 active galactic nuclei. 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H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 Cross-calibration of Suzaku/XIS and XMM-Newton/EPIC using galaxy clusters \|Kettula, K., Nevalainen, J., \| A&A \| 552-47 \| 2013 \| 2013A&A...552A..47K \| http://ui.adsabs.harvard.edu/#abs/2013A&A...552A..47K Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-131 \| 2013 \| 2013A&A...550A.131P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.131P A Good Mass Proxy for Galaxy Clusters with XMM-Newton \|Zhao, Hai-Hui, Jia, Shu-Mei, et al. \| ApJ \| 778-124 \| 2013 \| 2013ApJ...778..124Z \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778..124Z A tidal flare candidate in Abell 1795 \|Maksym, W. P., Ulmer, M. 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N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Are Boltzmann plots of hydrogen Balmer lines a tool for identifying a subclass of S1 AGN? \|Rafanelli, P., Ciroi, S., et al. \| AdSpR \| 54-1362 \| 2014 \| 2014AdSpR..54.1362R \| http://ui.adsabs.harvard.edu/#abs/2014AdSpR..54.1362R The optical emission lines of type 1 X-ray bright Active Galactic Nuclei \|La Mura, G., Berton, M., et al. \| AdSpR \| 54-1382 \| 2014 \| 2014AdSpR..54.1382L \| http://ui.adsabs.harvard.edu/#abs/2014AdSpR..54.1382L Relativistic Fe Kalpha line revealed in the composite X-ray spectrum of narrow-line Seyfert 1 galaxies - do their black holes have averagely low or intermediate spins? \|Liu, Zhu, Yuan, Weimin, et al. \| MNRAS \| 447-517 \| 2015 \| 2015MNRAS.447..517L \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447..517L XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . 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W., \| MNRAS \| 367-527 \| 2006 \| 2006MNRAS.367..527B \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367..527B Measurement of the Dark Matter Velocity Anisotropy in Galaxy Clusters \|Host, Ole, Hansen, Steen H., et al. \| ApJ \| 690-358 \| 2009 \| 2009ApJ...690..358H \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...690..358H Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters \|Vikhlinin, A., Markevitch, M., et al. \| ApJ \| 628-655 \| 2005 \| 2005ApJ...628..655V \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...628..655V Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Do the spectral energy distributions of type 1 active galactic nuclei show diversity? \|Scott, A. E., Stewart, G. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-06-26T01:13:57Z/2000-06-26T19:43:16Z
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	2001-10-31T00:00:00Z
Keywords	"resolution spectroscopy", "cooling flow region", "abundance distribution", "temperature gradients", "nonthermal components", "complete coverage", "cross dispersion width", "EPIC", "spectral resolution", "outer region", "ideal target"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2001, 'High Resolution Spectroscopy of the Cluster of Galaxies A 1795', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j5hmsog