A dataset provided by the European Space Agency

Name: A Very Deep XMM-Newton Study of the rho Oph Star Forming Region
Published: 2006-07-09T00:00:00Z

Proposal ID	030554
Title	A Very Deep XMM-Newton Study of the rho Oph Star Forming Region
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305541001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305541101
DOI	https://doi.org/10.5270/esa-gkxcpp5
Principal Investigator, PI	Prof Salvatore Sciortino
Abstract	We propose a 500 ks, 8 days long, EPIC observation of rho Oph. Due to itsdistance (virgul 140 pc), angular extent and strong absorption from a backgroundcloud rho Oph is the best target for an XMM-Newton study of the complexphenomena at work in star forming regions. It hosts a wide range of YSOs fromClass I and 0 to the Class II and III objects. About 90 YSOs ranging from ClassI to Class III with pn rate > 1 cnt/ks fall in the proposed EPIC fov. For allsuch YSOs we will obtain spectacular data that will allow breaking new groundsby studying variability on a variety of time scales (flares, rotationalmodulations, enigmatic long-term variations) and by characterizing spectravariations in search of the signature of accretion and/or circumstellar fluorescent plasma.
Publications	On the origin of NeII 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion \|Gudel, M., Lahuis, F., et al. \| A&A \| 519-113 \| 2010 \| 2010A&A...519A.113G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A.113G 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 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 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 Results from DROXO. II. Ne II and X-ray emission from rho Ophiuchi young stellar objects \|Flaccomio, E., Stelzer, B., et al. \| A&A \| 505-695 \| 2009 \| 2009A&A...505..695F \| http://ui.adsabs.harvard.edu/#abs/2009A&A...505..695F Results from Droxo. I. The variability of fluorescent Fe 6.4 keV emission in the young star Elias 29. High-energy electrons in the star.s accretion tubes? \|Giardino, G., Favata, F., et al. \| A&A \| 475-891 \| 2007 \| 2007A&A...475..891G \| http://ui.adsabs.harvard.edu/#abs/2007A&A...475..891G Results from DROXO. III. Observation, source list, and X-ray properties of sources detected in the Deep Rho Ophiuchi XMM-Newton Observation.. \|Pillitteri, I., Sciortino, S., et al. \| A&A \| 519-34 \| 2010 \| 2010A&A...519A..34P \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A..34P 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 Results from DROXO. I. The variability of fluorescent Fe 6.4 keV emission in the young star Elias 29. High-energy electrons in the star.s accretion tubes? \|Giardino, G., Favata, F., et al. \| A&A \| 495-899 \| 2009 \| 2009A&A...495..899G \| http://ui.adsabs.harvard.edu/#abs/2009A&A...495..899G 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 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 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 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 Results from DROXO. IV. EXTraS discovery of an X-ray flare from the Class I protostar candidate ISO-Oph 85 \|Pizzocaro, D., Stelzer, B., et al. \| A&A \| 587-36 \| 2016 \| 2016A&A...587A..36P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...587A..36P 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 High energy irradiated protoplanetary disks : the X-rays and FUV role in thermo-chemical modeling \|Aresu, Giambattista, \| PhDT \| 0-81 \| 2012 \| 2012PhDT........81A \| http://ui.adsabs.harvard.edu/#abs/2012PhDT........81A Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P Analysis of the Unconcentrated Background of the EPIC pn Camera on Board XMM-Newton \|Marelli, Martino, Molendi, Silvano, et al. \| ApJ \| 908-37 \| 2021 \| 2021ApJ...908...37M \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...908...37M 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero, E., Giordano, F., et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R 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 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	2005-03-08T14:51:59Z/2005-03-18T04:37:12Z
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	2006-07-09T00:00:00Z
Keywords	"angular extent", "time scales flares", "XMM-Newton", "rho oph", "xmm newton", "class ii", "complex phenomena", "spectacular data", "class iii", "XMM", "EPIC", "ysos ranging", "wide range", "epic fov", "pn rate", "deep xmm newton", "spectra variations", "term variations", "star forming region", "iii objects", "circumstellar fluorescent plasma", "rotational modulations", "140 pc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Salvatore Sciortino, 2006, 'A Very Deep XMM-Newton Study of the rho Oph Star Forming Region', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gkxcpp5