This dataset was used in the analysis presented in Glusman et al. (2025) (arXiv:2509:08773), which investigates the occurrence rates of giant planets orbiting low-mass stars observed by TESS. It conta
The ionizing radiation generated by accreting supermassive black holes (SMBHs) can drive powerful outflows of gas that play a key role in galaxy evolution. These outflows are observed on a variety of
Target RA (J2000): 180.844345 and deg Target Dec (J2000): 49.25123 and deg Gaia GMag: 10.543 Programme ID: CH_PR110045 Programme Manager: SERRANO PI of observing programme: Benz
Target RA (J2000): 173.314209 and deg Target Dec (J2000): -60.07603 and deg Gaia GMag: 9.5 Programme ID: CH_PR149000 Programme Manager: OSBORN PI of observing programme: Benz
