| Ref | Type | Facility | Instrum. | Npt | Comments |
| Ricci et al. 2017 | phot | 0.51m KPNO Visitor Center Telescope (KPNO-VCT) at Kitt Peak National Observatory (KPNO) | CCD camera | 2 | RICCI ET AL 2017 : An additional follow-up at Kitt Peak National Observatorywas carried out by Sada et al. (2012), Filters B and z prime. TABLE 2 |
| 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 | 3 | RICCI ET AL 2017 : We carried out 4 observations of HAT-P-3b at OAN-SPM in nearly-full moon conditions, in 2014, over a period spanning five months using three filters: two with the R filter, one with the I filter and the final one with the V filter. Except for the first R observation, we were able to follow the target for roughly five hours. |
| Ricci et al. 2017 | phot | National Optical Astronomy Observatory (NOAO) 2.1 meter Telescope at Kitt Peak National Observatory (KPNO) | FLAMINGOS | 1 | RICCI ET AL 2017 : Moreover, we also aggregated 4 already published observations from Sada et al. (2012): two light curves from the Kitt Peak National Observatory (KPNO) 200cm telescope observed with the JH filter, one light curve from the KPNO Visitor CenterTelescope (KPNO-VCT) 51cm telescope with the B filter and one curve from the same telescope with the Sloan z′ filter. A log of HAT-P-3b observations is shown in Table 2 |
| Ricci et al. 2017 | phot | University of Monterrey (UDEM) 0.36m telescope at Observatorio de la Universidad de Monterrey | SBIG STL-1301E | 1 | RICCI ET AL 2017 : We also obtained 6 transits from UDEM taken with the Ic filter between 2009 and 2013 |
| Exoplanets-A (CASCADe) | spec | HST | WFC3 | 25 | Exoplanets-A reduction
CASCADE v. 1.0.0
Created:2021_2_18:7_23_45
Obs.Type:transit |
