A dataset provided by the European Space Agency

Name: ToO proposal on exoplanet atmospheres
Published: 2020-08-12T22:00:00Z

Proposal ID	085338
Title	ToO proposal on exoplanet atmospheres
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853380901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853381001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853381101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853381201 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853381301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853381401
DOI	https://doi.org/10.5270/esa-5rmsizn
Principal Investigator, PI	Dr NORBERT SCHARTEL (PS)
Abstract	XMM-Newton observations of the following exoplanets:1) WASP-12: 8 ks; 2) WASP-13: 5 ks; 3) WASP-39: 11 ks; 4) WASP-76: 5 ks;5) WASP-127: 5 ks; 6) KELT-8: 5 ks; 7) HAT-P-1: 5 ks; 8) HAT-P-12: 5 ks;9) HAT-P-32: 8 ks; 10) HD 201585: 5 ks; 11) KELT-7: 5 ks
Publications	The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab \|Alam Munazza K. Lu00f3pez-Morales Mercedes et al. \| AJ \| 160-51 \| 2020 \| 2020AJ....160...51A \| http://ui.adsabs.harvard.edu/#abs/2020AJ....160...51A CARMENES detection of the Ca II infrared triplet and possible evidence of He I in the atmosphere of WASP-76b \|Casasayas-Barris N. Orell-Miquel J. et al. \| A&A \| 654-163 \| 2021 \| 2021A&A...654A.163C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...654A.163C Hu03b1 and He I absorption in HAT-P-32 b observed with CARMENES. Detection of Roche lobe overflow and mass loss \|Czesla S. Lampu00f3n M. et al. \| A&A \| 657-6 \| 2022 \| 2022A&A...657A...6C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...657A...6C HORuS transmission spectroscopy and revised planetary parameters of KELT-7 b \|Tabernero H. M. Zapatero Osorio M. R. et al. \| MNRAS \| 515-1247 \| 2022 \| 2022MNRAS.515.1247T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.1247T Possible origin of the non-detection of metastable He I in the upper atmosphere of the hot Jupiter WASP-80b \|Fossati L. Pillitteri I. et al. \| A&A \| 673-37 \| 2023 \| 2023A&A...673A..37F \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..37F The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets \|Behr Patrick R. France Kevin et al. \| AJ \| 166-35 \| 2023 \| 2023AJ....166...35B \| http://ui.adsabs.harvard.edu/#abs/2023AJ....166...35B The elusive atmosphere of WASP-12 b. High-resolution transmission spectroscopy with CARMENES \|Czesla S. Lampu00f3n M. et al. \| A&A \| 683-A67 \| 2024 \| 2024A&A...683A..67C \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A..67C 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	2019-08-29T18:32:29Z/2020-02-08T17:41:16Z
Version	18.02_20200221_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	2020-08-12T22:00:00Z
Last Update	2025-01-27
Keywords	"wasp 127", "xmm newton", "XMM-Newton", "exoplanet atmospheres", "hd 201585", "XMM", "HD 201585", "wasp 76"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr NORBERT SCHARTEL (PS), 2020, 'ToO proposal on exoplanet atmospheres', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-5rmsizn