| Ref | Type | Facility | Instrum. | Npt | Comments |
| Kreidberg et al. 2018 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 20 | KREIDBERG ET AL 2018. We determined the planet's composition with two techniques: atmospheric retrieval based on the transmission spectrum and interior structure modeling based on the observed mass and radius.
We observed a single transit of WASP-107b with HST Wide Field Camera 3 (WFC3) instrument on UT 5-6 June 2017. The transit observation consisted of five HST orbits. At the beginning of each 96-minute orbit, we took an image of the target with the F130N filter (ex-posure time = 4.2 s). This direct image is used for wave-length calibration. For the remainder of the target visibility period, we obtained time series spectra with the G141 grism, which provides low-resolution spectroscopy over the wavelength range 1.1−1.7 microns. We used the NSAMP=6, SPARS25 readout mode (exposure time =112 s) to optimize the efficiency of the observations, as determined by the PandExo HST planning tool (Batalhaet al. 2017). As is standard for WFC3 observations of bright targets, we used the spatial scanning observing mode, which slews the telescope in the spatial direction over the course of an exposure. The scan rate was 0.12 arcseconds/sec.
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| Spake et al. 2018 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 49 | SPAKE ET AL 2018 On 32 May 2017, we observed a primary transit of WASP-107b with the WFC3 on board of the HST. Our observatons lasted 7 hours and we acquired 84 time series spectra with the G102 grism, which covers the 8000 to 11000 ansgtrongs wavelenght range. |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 14 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_28:11_39_50
Obs.Type:transit |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_28:11_58_19
Obs.Type:transit |
