0000000001302382
AUTHOR
J.a. Munoz
CCDC 193057: Experimental Crystal Structure Determination
Related Article: L.Escriche, J.A.Munoz, R.Kivekas, R.Sillampaa, J.Casabo|2002|Eur.J.Inorg.Chem.||3258|doi:10.1002/1099-0682(200212)2002:12<3258::AID-EJIC3258>3.0.CO;2-P
The TESS Grand Unified Hot Jupiter Survey I. 10 planets
Hot Jupiters-short-period giant planets-were the first extrasolar planets to be discovered, but many questions about their origin remain. NASA's Transiting Exoplanet Survey Satellite (TESS), an all-sky search for transiting planets, presents an opportunity to address these questions by constructing a uniform sample of hot Jupiters for demographic study through new detections and unifying the work of previous ground-based transit surveys. As the first results of an effort to build this large sample of planets, we report here the discovery of 10 new hot Jupiters (TOI-2193Ab, TOI-2207b, TOI-2236b, TOI-2421b, TOI-2567b, TOI-2570b, TOI-3331b, TOI-3540Ab, TOI-3693b, TOI-4137b). All of the planets…
K2 light curve alternative analysis of ASASSN-18bt
On 2018 February 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnitude of B_max_=14.31, ASASSN-18bt is the nearest and brightest Supernovae Ia type (SNe Ia) yet observed by the Kepler spacecraft. Here we present the discovery of ASASSN-18bt, the K2 light curve, and prediscovery data from ASAS-SN and the Asteroid Terrestrial-impact Last Alert System. The K2 early-time light curve has an unprecedented 30-minute cadence and photometric precision for an SN Ia light curve, and it unambiguously shows a ~4 day nearly linear phase followed by a steeper rise. Thus, ASASSN-18bt joins a…
CCDC 193056: Experimental Crystal Structure Determination
Related Article: L.Escriche, J.A.Munoz, R.Kivekas, R.Sillampaa, J.Casabo|2002|Eur.J.Inorg.Chem.||3258|doi:10.1002/1099-0682(200212)2002:12<3258::AID-EJIC3258>3.0.CO;2-P