| Ref | Type | Facility | Instrum. | Npt | Comments |
| Ricci et al. 2017 | phot | Multiple Observatories | Multiple Instruments | 2 | RICCI ET AL 2017 We also present 18 UDEM transits: six with the Vf ilter,five with the Rc filter, six in the Ic band and finally one in the z' band |
| Ricci et al. 2017 | phot | National Autonomous University of Mexico (UNAM) 0.84m Telescope at El Observatorio Astronomico Nacional/Sierra San Pedro Martir (OAN/SPM) | MEXMAN | 1 | RICCI ET AL 2017 The first telescope is the OAN-SPM 84cm. It provides a set of instruments that can be mounted according to the observational needs, among which Mexman, a wide-field imager already successfully tested for the observation and characterization of exoplanets using the transit method (Ricci et al.2015) Concerning TrES-3b, we obtained three complete light curves in the R band at OAN-SPM, and two in the I band. Except for the first I light curve, we used the defocused photometry method described in detail by Southworth et al. (2014) and in previous papers of the series. |
| Ricci et al. 2017 | phot | University of Monterrey (UDEM) 0.36m telescope at Observatorio de la Universidad de Monterrey | SBIG STL-1301E | 3 | RICCI ET AL 2017 The second telescope is the UDEM 36cm, a lx200 gps college telescope located close to the city of Monterrey, Mexico, and classed with a Minor Planet Center Code of 720. It is available for student training and has been active for almost 10 years in the field of exoplanetary transit observations. |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_28:10_36_53
Obs.Type:eclipse |
