A dataset provided by the European Space Agency

Name 067123
Title Studying Stellar Activity with a XMM-Kepler Joint Project
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671230101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671230201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671230301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671230401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671230601

DOI 10.5270/esa-tryvf91
Author Dr Giuseppina Micela
Description We propose to survey 3 sq. deg. of sky within the Kepler target area with 12 XMM pointing of 80 ksec each. We will take advantage of the unprecedented accuracy, duration and duty cycle of the white-light light-curves (LCs), obtained by Kepler on a large, statistically meaningful stellar sample. These allow us to reliably determine the rotational periods of slow rotators and to obtain simultaneous optical and X-rays observations. The proposed observations will allow us i) to derive the size of active regions in a large sample of stars (hundreds, spanning different activity regimes), ii) to constrain coronal heating mechanisms and iii) to explore the slow rotation regime in low mass stars, using a variety of diagnostics described in the proposal.
Publication 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Activity and rotation of the X-ray emitting Kepler stars . Pizzocaro, D., Stelzer, B., et all. . A&A . 628-41 . 2019 . 2019A&A...628A..41P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-06-09T04:49:15Z/2012-03-27T14:17:44Z
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 2013-04-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-19T00:00:00Z, 067123, 17.56_20190403_1200. https://doi.org/10.5270/esa-tryvf91