| Ref | Type | Facility | Instrum. | Npt | Comments |
| Bean et al. 2011 | spec | Magellan II Landon Clay Telescope | MMIRS | 36 | BEAN ET AL 2011 MMIRS We used an HK grism as the dispersive element and an HK filter to isolate the first-order spectra. Complete spectra from 1.23 to 2.48m with a dispersion of 6.6 were obtained for all the objects |
| Berta et al. 2012 | spec | Hubble Space Telescope satellite | WFC3 | 24 | BERTA ET AL 2012 WFC3 We observed three transits of GJ1214b on UT 2010 October 8, 2011 March 28, and 2011 July 23 with the G141grism on WFC3 infrared channel (HSTProposal GO-12251,PI: Z. Berta), obtaining simultaneous multiwavelength spectrophotometry of each transit between 1.1 and 1.7 mm. |
| Croll et al. 2011 | phot | Canada-France-Hawaii Telescope | WIRCam | 8 | CROLL ET AL 2011 : We observed the transit of GJ 1214b on four occasions with WIRCam on CFHT. For each transit we observed GJ 1214 in two bands nearly simultaneously by rapidly switching the WIRCam filter wheel back and forth between the two filters.
We observed GJ 1214 alternating between the J (1.25 microns) and Ks (2.15microns) filters on the evenings of 2010 June 27, 2010 August 15 and 2010 September 22.
On the evening of 2010 August 7 we observed GJ 1214 alternating between the Jand CH4On filters (1.69 microns) |
| Cáceres et al. 2014 | phot | The Southern Astrophysical Research Telescope | OSIRIS | 1 | CACERES ET AL 2014 : We observed a GJ 1214 b transit from UT 0:19 to 4:10 on the night of August 09, 2011 with the Ohio State Infrared Imager/Spectrometer (OSIRIS; Depoy et al. 1993) at the 4.1 m Southern Astrophysical Research (SOAR) Telescope at CerroPachon, Chile. A narrow-band (1%) filter centered on 2.14 was used. |
| Cáceres et al. 2014 | phot | The Southern Astrophysical Research Telescope | SOI | 1 | CACERES ET AL 2014 : A transit of GJ 1214 b was observed in the I-Bessel filter from UT 04:03 to 09:30 on the night of April 28, 2010 with the SOAR Optical Imager (SOI) at the SOAR telescope on Cerro Pachon
We observed GJ 1214 alternating between the J (1.25 microns) and Ks (2.15microns) filters on the evenings of 2010 June 27, 2010 August 15 and 2010 September 22.
On the evening of 2010 August 7 we observed GJ 1214 alternating between the Jand CH4On filters (1.69 microns) |
| de Mooij et al. 2012 | phot | Isaac Newton Groups Isaac Newton Telescope | WFC | 2 | DE MOOIJ ET AL 2012 A transit of GJ 1214b was observed in Sloanr-band (c=627 nm) on May 26, 2010 . On July 29, 2010, a transit of GJ 1214 was observed inI-band (c=822 nm) with the same instrument |
| de Mooij et al. 2012 | phot | Isaac Newton Groups William Herschel Telescope | LIRIS | 1 | DE MOOIJ ET AL 2012 : The Kc-band (2.27) observations were obtained with the Long-slit Intermediate Resolution Infrared Spectrograph (LIRIS; Acosta-Pulido et al. 2002) on the William Herschel Telescope (WHT) on the night of August17, 2010. The pixel-scale of the LIRIS detector is 0.2''/pixel, resulting in a field of view of the detector of 4.2 by 4.2 arcminutes. The same reference stars as for the NOTCam observations were used. |
| de Mooij et al. 2012 | phot | Max Planck Gesellschaft 2.2 meter Telescope at European Southern Observatory | GROND | 4 | DE MOOIJ ET AL 2012 : On the night of July 3, 2010, we obtained simultaneous observations of GJ1214b in the g (459 nm), r (622 nm), i (764 nm), and z-band (899 nm) with the GROND instrument (Greiner et al. 2008) on the 2.2 meter MPI/ESO telescope at La Silla in Chile. The field of view in each of the wavelength channels is 5.4' by 5.4', which is sufficient to observe both GJ1214 and a set of reference stars simultaneously.The observations started at 00:16 UT and lasted until 04:06 UT. During this time we obtained 280 frames in each of the four optical bands. The exposure time was varied from 20 to 30 seconds to avoid saturation of the CCDs. The average cycle time was 50 seconds. |
| de Mooij et al. 2012 | phot | Nordic Optical Telescope | NOTCam | 1 | DE MOOIJ ET AL 2012 wide fieldimaging optics and aKs-band filter (c=2.15m) were used |
| de Mooij et al. 2013 | phot | Isaac Newton Groups Isaac Newton Telescope | WFC | 1 | DE MOOIJ ET AL 2012 On the night of 2012 May 6, a transit of GJ1214b was observed in the g band (4962) with the WFC of the INT |
| de Mooij et al. 2013 | phot | Isaac Newton Groups William Herschel Telescope | ACAM | 1 | On the night of 2011 May 22, a transit of GJ1214b was observed in the g band (4996) with ACAM (Bennet al.2008) on the William Herschel Telescope (WHT) |
| de Mooij et al. 2013 | spec | Very Large Telescope (Antu) | FORS | 1 | DE MOOIJ ET AL 2013 FORS A second transit of GJ1214 was observed with (FORS) on the Very Large Telescope(VLT) on 2011 July 12 in the B-high filter (c=4543). |
| Désert et al. 2011 | phot | Spitzer Space Telescope satellite | Infrared Array Camera (IRAC) | 2 | DESERT ET AL 2011 : We report observations of two consecutive transits of the warm super-Earth exoplanet GJ 1214b at 3.6 and 4.5 microns with the Infrared Array Camera instrument on-board the Spitzer Space Telescope. The two transit light curves allow for the determination of the transit parameters for this system. We find these paremetersto be consistent with the previously determined values and no evidence for transit timing variations. The main investigation consists of measuring the transit depths in each bandpass to constrain the planet's transmission spectrum. |
| Gillon et al. 2014 | phot | La Silla Observatorys 60-cm TRAPPIST Telescope | TRAPPISTCam | 1 | GILLON ET AL 2014: In 2011, we observed seven transits of GJ 1214 b from Chile with the 60 cm robotic telescope TRAPPIST located at ESO La Silla Observatory.
We monitored all the transits with the telescope slightly defocused and in the I+z filter that has a transmittance > 90 % from 750 nm to beyond 1100 nm. |
| Gillon et al. 2014 | phot | Spitzer Space Telescope satellite | Infrared Array Camera (IRAC) | 4 | GILLON ET AL 2014: The surviving data consist of 12383 sets of 64 individual subarray images divided in 20 AOR s gathered by the IRAC detector at 4.5 microns with an integration time of 2 s, and calibrated by the Spitzer pipeline version S18.18.0. |
| Kreidberg et al. 2014 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 22 | KREIDBERG ET AL 2014 We obtained time-series spectroscopy from 1.1 to 1.7 m during each observation. The data were taken in spatial scanmode, which slews the telescope during the exposure and moves the spectrum perpendicular to the dispersion direction on the detector. The observations had the following design. At the beginning of each orbit, we took a direct image with the F130N narrowband filter to establish a wavelength zero-point. For the remainder of each orbit, we took spatially scanned exposures with the G141 grism. |
| Murgas et al. 2012 | spec | Gran Telescopio CANARIAS 10.4m telescope | OSIRIS | 3 | MURGAS ET AL 2012 We used the OSIRIS Red Tunable Filter (RTF): Tunable filter was set up at 658.0 nm, 661.2 nm, and 666.9 nm to get the desired wavelengths of 653.5 nm, 656.3 nm,and 662.0 nm at both the target and reference star, |
| Narita et al. 2013 | phot | Infrared Survey Facility | SIRIUS | 3 | NARITA ET AL 2013 SIRIUS INSTRUMENT http://www-ir.u.phys.nagoya-u.ac.jp/~irsf/sirius/index_e.html |
| Nascimbeni et al. 2015 | phot | Large Binocular Telescope Observatory | LBC | 2 | NASCIMBENI ET AL 2015 We mounted a BesselB and BesselR filter on the blue and red channel, respectively. |
| Rackham et al. 2017 | spec | Magellan I Walter Baade Telescope | IMACS spectrograph | 14 | RACKMAN ET AL IMACS Details for the three transit observations are provided in Table1. We carried out all observations in spectroscopic mode with no filter. We observed two transits with the f/4 camera and one with the f/2 camera; therefore we designed two with three criteria:(1)to include the widest spectral range for the target and comparison stars,(2)to include as many comparison stars as possible, and(3)to eliminate slit losses using extra-wide slits. We also used larger lengths for the slits in order to adequately sample the sky background |
| Wilson et al. 2014 | spec | Gran Telescopio CANARIAS 10.4m telescope | OSIRIS | 8 | WILSON ET AL 2014 GTC/OSIRIS Using the tuneable filter (TF) imaging mode on (OSIRIS) instrument installed on the 10.4 m GTC |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_3_2:9_41_9
Obs.Type:transit |
