A dataset provided by the European Space Agency

Name: The XUV irradiation of the young exo-planets around V1298 Tau
Published: 2022-09-28T00:00:00Z

Proposal ID	088122
Title	The XUV irradiation of the young exo-planets around V1298 Tau
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881220101
DOI	https://doi.org/10.57780/esa-cizvhvg
Principal Investigator, PI	Dr Serena Benatti
Abstract	We propose joint XMM-Newton (30ks) and HST observations (3 orbits) of the nearbyK young star V1298 Tau (virgul20Myr) hosting four transiting exoplanets discoveredwith Kepler (K2), and included in a follow-up optical/IR campaign with HARPS-Nand GIANO-B@TNG. These young planets have radii between 5.6 and 10.3 R_Earth andthey are located between 0.08 and virgul0.3 AU from the host. They are stillexperiencing the contraction phase toward their final sizes and are subject tophotoevaporation effects at different rates. Our immediate objective is toreconstruct the full XUV spectrum, and to assess the spectral and timevariability of the host star. In this way we will characterize its activitylevel and the dose of high- energy radiation received by those very young planets.
Publications	X-Ray and Ultraviolet Emission of the Young Planet-hosting Star V1298 Tau from Coordinated Observations with XMM-Newton and Hubble Space Telescope \|Maggio, A., Pillitteri, I., et al. \| ApJ \| 951-18 \| 2023 \| 2023ApJ...951...18M \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951...18M 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2021-08-25T03:09:32Z/2021-08-25T13:42:52Z
Version	19.16_20210326_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	2022-09-28T00:00:00Z
Keywords	"time variability", "XMM", "xuv spectrum", "photoevaporation effects", "v1298 tau", "energy radiation received", "ir campaign", "contraction phase", "final sizes", "star v1298 tau", "kepler k2", "transiting exoplanets", "XMM-Newton", "xuv irradiation", "activity level", "HST", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Serena Benatti, 2022, 'The XUV irradiation of the young exo-planets around V1298 Tau', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-cizvhvg