| Ref | Type | Facility | Instrum. | Npt | Comments |
| Angerhausen et al. 2015 | phot | Stratospheric Observatory For Infrared Astronomy | HIPO | 2 | ANGERHAUSEN ET AL 2015 We observed HD 189733 b during a transit on SOFIA's flight number 134 on UT Oct 1 2013 aspart of a Cycle 1 GO program.
Observations were conducted in the FLIPO configuration (FLITECAM and HIPO operating simultaneously) in order to observein three optical and infrared bands at the same time: B and z' with HIPO and a narrow-bandfilter covering the Paschen spectral feature at 1.88 with FLITECAM. |
| Barnes et al. 2016 | spec | European Southern Observatorys 3.6 meter Telescope | HARPS Echelle Spectrograph | 15 | BARNES ET AL 2016 HD 189733b has been observed withharpsduring a num-ber of transit events. |
| Borsa et al. 2016 | spec | European Southern Observatorys 3.6 meter Telescope | HARPS Echelle Spectrograph | 7 | BORSA ET AL 2016 We divide the HARPS spectral range in 7 broadbands,calculating for each band the ratio between the area of the out-of-transit CCF and the area of the signal imprinted by the planet on it during the full part of the transit |
| Di Gloria et al. 2015 | spec | European Southern Observatorys 3.6 meter Telescope | HARPS Echelle Spectrograph | 7 | DI GLORIA ET AL 2015 HARPS spectrograph (R=115 000) at ESO 3.6-meter telescope. We perform differential spectroscopy to retrieve the transit spectrum and light curve of the planet, implementing corrections for telluric contamination and planetary orbital motion. W reduced HARPS spectrum covers the region between 380 nm and 690 nm with a spectral resolution of R ∼115 000 or 2.7 km s− |
| Desert et al. 2011 | spec | Spitzer Space Telescope satellite | Infrared Array camera (IRAC) | 1 | DESERT ET AL 2011 Here we focus on the data obtained during Visit 3 on 2007 November 25 at 3.6 (channel 1); its analysis is presented in this paper. We used IRAC 32x32 pixel subarray mode for visit 3, which lasted 4.5 hours with 1.8 h during transit. The primary goal of this last visit was to obtain an accurate measurement of the planetary radius at 3.6 microns. The subarray mode has a greater efficiency than the stellar mode in collecting photon. |
| Gibson et al. 2012 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 4 | GIBSON ET AL 2012 Observations used the G141grism, and we obtained slitless spectra from∼1.08 to 1.69 μm with a resolution of λΔ/λ∼130 at the central wavelength. |
| Pont et al. 2013 | spec | Hubble Space Telescope satellite | Advanced Camera for Surveys | 10 | PONT ET AL 2013 ACS camera on HST,using Grism G800L (0.6-1μm)The transit spectrum of HD 189733b has been measuredfrom 300 nm to 1μm with the STIS and ACS instruments
v ACS camera on HST,using Grism G800L (0.6-1╬╝m)
ACS camera on HST,using Grism G800L (0.6-1╬╝m)
PONT ET AL 2013 ACS camera on HST,using Grism G800L (0.6- 1 μm) |
| Pont et al. 2013 | spec | Hubble Space Telescope satellite | Near Infrared Camera and Multi-Object Spectrometer | 22 | PONT ET AL 2013 The transit spectrum of HD 189733b has been measured from 300 nm to 1 micron with the STIS and ACS instruments aboard HST , from 1 to 3 microns with HST WFC3 and NICMOS |
| Pont et al. 2013 | spec | Hubble Space Telescope satellite | Space Telescope Imaging Spectrograph | 16 | PONT ET AL 2013 The transit spectrum of HD 189733b has been measured from 300 PONT ET AL 2013 Five transits of HD 189733 were observed with STIS n two contexts, at low resolution from the present programme, and at medium resolution around the sodium doublet . The broad-band data showed a fea-tureless spectrum over the 300-600 nm range, with absorption rising blue wards. ( nm to 1μm with the STIS and ACS instruments |
| Pont et al. 2013 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 4 | PONT ET AL 2013 WFC3 camera on the refurbished HST as part of our programme, GO-11740, covering the wavelength interval 1.1 to 1.7μm. |
| Pont et al. 2013 | phot | Spitzer Space Telescope satellite | Infrared Array Camera (IRAC) | 7 | PONT ET AL 2013 The transit spectrum of HD 189733b has been measured from 300 nm to 1 micron with the STIS and ACS instruments aboard HST , from 1 to 3 microns with HST WFC3 and NICMOS |
| Pont et al. 2013 | phot | Spitzer Space Telescope satellite | Multiband Imaging Photometer (MIPS) | 1 | PONT ET AL 2013 The transit spectrum of HD 189733b has been measured from300 nm to 1 micron with the STIS and ACS instruments aboard HST , from 1 to 3 microns with HST WFC3 and NICMOS and in five infrered passbands between 3.6 and 24 microns with IRAC and MIPS on Spitzer |
| Sing et al. 2011 | spec | Hubble Space Telescope satellite | Space Telescope Imaging Spectrograph | 5 | SING ET AL 2011 We observed transits of HD 189733b with the HST STISG430L grating during 20 November 2009 and 18 May 2010 . The G430L dataset consists of about 200 spectra spanningthe two transit events covering the wavelength range 0.2892 to 0.5700 microns. |
| Sing et al. 2016 | spec | Hubble Space Telescope satellite | Near Infrared Camera and Multi-Object Spectrometer | 2 | SING ET AL 2016 |
| Sing et al. 2016 | spec | Hubble Space Telescope satellite | Space Telescope Imaging Spectrograph | 20 | SING ET AL 2016 In this survey, we observed all eight planets in the fulloptical wavelength range (0.3-1.01) using the Space Telescope Imaging Spectrograph (STIS) instrument. |
| Sing et al. 2016 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 29 | SING ET AL 2016 We analyzed the survey targets in conjunction with HST and Spitzer data from the two best-studied hot Jupiters to date, HD 209458b1 and HD 189733b5, giving a total of ten exoplanets in our comparative study with transmission spectra between 0.3 and 5 microns
|
| Sing et al. 2016 | phot | Spitzer Space Telescope satellite | Infrared Array Camera (IRAC) | 2 | SING ET AL 2016 The eight targets in the large HST survey were also all covered by Spitzer transit observations as part of an Exploration Science Programme obtained using the Infrared Array Camera (IRAC) instrument with the 3.6 and 4.5 channels in subarray mode |
| Swain et al. 2008 | spec | Hubble Space Telescope satellite | Near Infrared Camera and Multi-Object Spectrometer | 18 | SWAIN ET AL 2018 |
| Wyttenbach et al. 2015 | spec | European Southern Observatorys 3.6 meter Telescope | HARPS Echelle Spectrograph | 1 | WYTTENBACH ET AL 2015: HD 189733 (Bouchy et al. 2005) was observed with the HARPS echelle spectrograph (High-Accuracy Radial-velocity Planet Searcher) on the ESO 3.6 m telescope, La Silla, Chile |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_27:12_12_38
Obs.Type:transit |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_27:12_20_21
Obs.Type:eclipse |
