A dataset provided by the European Space Agency

Name 15174
Title Investigating an SPI and Measuring Baseline FUV Variability in the GJ 436 Hot-Neptune System
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15174;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-dfo6kzm
Author Loyd, R. O. Parke
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15174&mission=hst
Publication
  • Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
  • Flares, Rotation, Activity Cycles, and a Magnetic Star-Planet Interaction Hypothesis for the Far-ultraviolet Emission of GJ 436
  • HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars
  • The Hubble PanCET program: an extensive search for metallic ions in the exosphere of GJ 436 b
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2017-12-22T21:22:35Z/2018-02-23T08:50:00Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2018-02-23T12:51:43Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Loyd comma R. O. Parke, 2018, 'Investigating an SPI and Measuring Baseline FUV Variability in the GJ 436 Hot-Neptune System', 1.0, European Space Agency, https://doi.org/10.5270/esa-dfo6kzm