A new method to measure the spectra of transiting exoplanet atmospheres using multi-object spectroscopy
An HST/STIS Optical Transmission Spectrum of Warm Neptune GJ 436b
A Temperature Trend for Clouds and Hazes in Exoplanet Atmospheres
Disequilibrium Chemistry in Exoplanet Atmospheres Observed with the Hubble Space Telescope
Revisiting the Transit Timing and Atmosphere Characterization of the Neptune-mass Planet HAT-P-26 b
The metal-rich atmosphere of the exo-Neptune HAT-P-26b
Instrument
STIS/CCD, WFC3, WFC3/IR
Temporal Coverage
2016-01-25T18:21:28Z/2016-08-16T07:32:38Z
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.
European Space Agency, Sing comma David K., 2017, 'Charaterizing the atmosphere of the enlarged Neptune-mass planet HAT-P-26b', 1.0, European Space Agency, https://doi.org/10.5270/esa-5h1h5le