A dataset provided by the European Space Agency

Name 030554
Title A Very Deep XMM-Newton Study of the rho Oph Star Forming Region
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305540901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305541001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305541101

DOI 10.5270/esa-gkxcpp5
Author Prof Salvatore Sciortino
Description We propose a 500 ks, 8 days long, EPIC observation of rho Oph. Due to its distance (~ 140 pc), angular extent and strong absorption from a background cloud rho Oph is the best target for an XMM-Newton study of the complex phenomena at work in star forming regions. It hosts a wide range of YSOs from Class I and 0 to the Class II and III objects. About 90 YSOs ranging from Class I to Class III with pn rate > 1 cnt-ks fall in the proposed EPIC fov. For all such YSOs we will obtain spectacular data that will allow breaking new grounds by studying variability on a variety of time scales (flares, rotational modulations, enigmatic long-term variations) and by characterizing spectra variations in search of the signature of accretion and-or circumstellar fluorescent plasma.
Publication On the origin of [NeII] 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion . Gudel, M., Lahuis, F., et all. . A&A . 519-113 . 2010 . 2010A&A...519A.113G ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Results from DROXO. II. [Ne II] and X-ray emission from rho Ophiuchi young stellar objects . Flaccomio, E., Stelzer, B., et all. . A&A . 505-695 . 2009 . 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 all. . A&A . 475-891 . 2007 . 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 all. . A&A . 519-34 . 2010 . 2010A&A...519A..34P ,
An All-Sky Atlas of Radio-X-ray A...
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-07-09T00:00:00Z, 030554, 17.56_20190403_1200. https://doi.org/10.5270/esa-gkxcpp5