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 Population Analysis of 20 Exoplanets Observed from Optical to Near-infrared Wavelengths with the Hubble Space Telescope: Evidence for Widespread Stellar Contamination
A Temperature Trend for Clouds and Hazes in Exoplanet Atmospheres
Disequilibrium Chemistry in Exoplanet Atmospheres Observed with the Hubble Space Telescope
Exoplanet Ephemerides Change Observations (ExoEcho). I. Transit Timing Analysis of 37 Exoplanets Using HST/WFC3 Data
HST SHEL: Revealing Haze and Confirming Elevated Metallicity in the Warm Neptune HAT-P-26b
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
2016-08-16T00:23:56Z/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 et al., 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
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.