0000000001302382

AUTHOR

J.a. Munoz

showing 4 related works from this author

CCDC 193057: Experimental Crystal Structure Determination

2003

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

Dichloro-(6-phenyl-6-phospha-39-dithiabicyclo[9.2.2]pentadeca-1(13)1214-trien-69-diyl)-palladium(ii)Space GroupCrystallographyCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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The TESS Grand Unified Hot Jupiter Survey I. 10 planets

2022

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…

Photometryobservational astronomyRadial velocityAstrophysics and AstronomyExoplanetsPhysicsexoplanet astronomyWide-band photometryNatural SciencesInfrared photometrySpectroscopyWide band photometryOptical astronomy
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K2 light curve alternative analysis of ASASSN-18bt

2020

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…

observational astronomyPhotometryAstrophysics and AstronomySupernovaeStellar AstronomyPhysicsNatural SciencesOptical astronomy
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CCDC 193056: Experimental Crystal Structure Determination

2003

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

Space GroupCrystallographyCrystal SystemCrystal StructureCell ParametersDichloro-(6-phenyl-6-phospha-39-dithiabicyclo[9.3.1]pentadeca-1(15)1214-trien-69-diyl)-palladium(ii) acetonitrile solvateExperimental 3D Coordinates
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