HATS-54b-HATS-58Ab: Five New Transiting Hot Jupiters including One with a Possible Temperate Companion the HATSouth network is operated by a collaboration consisting of Princeton University (PU), the Max Planck Institute für Astronomie (MPIA), the Australian National University (ANU), and the Pontificia Universidad Católica de Chile (PUC). The station at Las Campanas Observatory (LCO) of the Carnegie Institute is operated by PU in conjunction with PUC, the station at the High Energy Spectroscopic Survey (H.E.S.S.) site is operated in conjunction with MPIA, and the station at Siding Spring Observatory (SSO) is operated jointly with ANU. Based in part on observations made with the MPG 2.2 m Telescope at the ESO Observatory in la Silla.

N. Espinoza, J. D. Hartman, G. Bakos, T. Henning, D. Bayliss, J. Bento, W. Bhatti, R. Brahm, Z. Csubry, V. Suc, A. Jordán, L. Mancini, T. G. Tan, K. Penev, M. Rabus, P. Sarkis, M. De Val-Borro, S. Durkan, J. Lázár, I. PappP. Sári

Research output: Contribution to journalArticlepeer-review

14 Scopus citations

Fingerprint

Dive into the research topics of 'HATS-54b-HATS-58Ab: Five New Transiting Hot Jupiters including One with a Possible Temperate Companion the HATSouth network is operated by a collaboration consisting of Princeton University (PU), the Max Planck Institute für Astronomie (MPIA), the Australian National University (ANU), and the Pontificia Universidad Católica de Chile (PUC). The station at Las Campanas Observatory (LCO) of the Carnegie Institute is operated by PU in conjunction with PUC, the station at the High Energy Spectroscopic Survey (H.E.S.S.) site is operated in conjunction with MPIA, and the station at Siding Spring Observatory (SSO) is operated jointly with ANU. Based in part on observations made with the MPG 2.2 m Telescope at the ESO Observatory in la Silla.'. Together they form a unique fingerprint.

Physics

Keyphrases