A dataset provided by the European Space Agency

Name 004175
Title Metallicity effects on stellar magnetic activity: Blanco 1 as a test case
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0041750101

DOI 10.5270/esa-xgahbje
Author Dr Giuseppina Micela
Description We propose a 50 ksec EPIC observation on Blanco 1, a metal rich high latitude open cluster, that for its characteristics is well suited to address some questions unsolved by previuos X-ray missions. Our objective is to determine the X-ray luminosity of late type cluster members aiming to understand how metallicity affects stellar magnetic activity and its time evolution. The achieved sensitivity will allow us also to determine the low-mass end of the Initial Mass Function of Blanco 1, that for its peculiar origin could be very different from that of other more typical open clusters and star formation regions.
Publication Properties of serendipitous X-ray flares discovered in XMM-Newton observations . Trenholme, Duncan, Ramsay, Gavin, . MNRAS . 355-1125 . 2004 . 2004MNRAS.355.1125T ,
XMM-Newton observation of the young open cluster Blanco 1. II. X-ray time variability and flares . Pillitteri, I., Micela, G., et all. . A&A . 430-155 . 2005 . 2005A&A...430..155P ,
Identifying XMM-Newton observations affected by solar wind charge exchange - Part II . Carter, J. A., Sembay, S., . A&A . 527-115 . 2011 . 2011A&A...527A.115C ,
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 ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
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 ,
XMM-Newton observations of the young open cluster Blanco 1. I. X-ray spectroscopy and photometry . Pillitteri, I., Micela, G., et all. ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-06-15T19:38:36Z/2002-06-16T10:09:46Z
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 2003-07-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-07-05T00:00:00Z, 004175, 17.56_20190403_1200. https://doi.org/10.5270/esa-xgahbje