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caballero@cab from superjupiters to exoearths

caballero@cab from superjupiters to exoearths. José Antonio Caballero 2010-2014: Ramón y Cajal (CSIC) 2007-2010: Juan de la Cierva (UCM) 2006-2007: Alexander von Humboldt (MPIA) 2006: WFC/INT support astronomer (ING) 2001-2006: “astrofísico residente” & FPU (IAC)

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caballero@cab from superjupiters to exoearths

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  1. caballero@cab fromsuperjupiterstoexoearths José Antonio Caballero 2010-2014: Ramón y Cajal (CSIC) 2007-2010: Juan de la Cierva (UCM) 2006-2007: Alexander von Humboldt (MPIA) 2006: WFC/INT supportastronomer (ING) 2001-2006: “astrofísico residente” & FPU (IAC) 2000: “estudiante de verano” (LAEFF) 1995-2000: Física (UCM) -10

  2. PhDthesis: Formation, evolution and multiplicity of browndwarfs and giantexoplanets(2006, Universidad de La Laguna) Chapter 10: Multiplicity of L dwarfs: binarity and habitable exoplanets Searchfortransitsaround L dwarfs – Study of radial-velocityplanetdetection – Astrobiology: orbitsynchronisation, atmosphericphysics, bacteriochlorophylla+b… caballero@cab -9

  3. Refereedpaperssince 01 Jan 2010 Thesubstellarmassfunction in the central region of the open clusterPraesepefromdeep LBT observations(Wang et al., submitted, A&A) Identification of bluehighpropermotionobjects in Tycho-2 and 2MASS catalogues using Virtual Observatorytools(Jiménez-Esteban, Caballero, Solano 2010, A&A) HRC-I/ChandraobservationstowardsOrionis(Caballero et al. 2010c, A&A) Themagnetically active, low-mass, triple star WDS 19312+3607 (Caballero et al. 2010b, A&A) Near-infraredlow-resolutionspectroscopy of Pleiades L-typebrowndwarfs(Bihain et al. 2010, A&A) Infrared and kinematicproperties of thesubstellarobject G 196-3B (Zapatero Osorio et al. 2010, ApJ) Reachingtheboundarybetweenstellarkinematicgroups and verywidebinaries. II.  Lib + KU Lib: a commonpropermotionsystem in Castor separatedby 1.0 pc(Caballero 2010c, A&A) Stars and browndwarfs in theOrioniscluster. II. A propermotionstudy(Caballero 2010b, A&A) Theoccultationevents of theHerbigAe/Be star V1247 Ori (Caballero 2010a, A&A Letters) Brown dwarfs and verylowmassstars in thePraesepe open cluster: a dynamicallyunevolvedmassfunction(Boudreault et al. 2010, A&A) Findingthemost variable stars in theOrionBeltwiththeAllSkyAutomatedSurvey(Caballero et al. 2010a, AN) caballero@cab -8a

  4. Proceedingssince01 Jan2010 Binarysystems: from 0.2 arcsecto 2 deg(Caballero, Doublestars) CARMENES: Calar Alto high-Resolutionsearchfor M dwarfswithExoplanetswith a visible and Near-infraredEchelleSpectrograph(Quirrenbach, Amado, Mandel, Caballero et al. 2010, SPIE) Optical and near-infraredstudy of thestellar and substellarpopulation of therecentlydiscovered open clustersAlessi 5 and Monocerotis(Boudreault & Caballero, CoolStars 16) Kinematics of ultra cooldwarfs: membership in movinggroups and associations(Montes & Caballero, CoolStars 16) Thestellar and substellarmassfunction in the central region of theold open clusterPraesepe(Wang et al., CoolStars 16) CARMENES: Towardsthedetection of exoearths(Caballero et al., CoolStars 16) Estimatingtheage of exoplanet’s host starsbytheirmembership in movinggroups and youngassociations(Montes, Caballero et al. 2010, ASPC) NAHUAL: a next-generationnear-infraredinstrumentforthe GTC (Martín et al. 2010, ASPC) CARMENES: technicaldetails(Caballero et al., PRVS) Music and Astronomy(Caballero et al. 2010, HSA5) Preliminaryresultson a virtual observatorysearchforcompanionstoLuytenstars(Caballero et al. 2010, HSA5) Anapplication of theMayrit catalogue: verywidebinaries in theOrioniscluster(Caballero 2010, HSA5) Formation, evolution and multiplicity of browndwarfs and giantexoplanets (Caballero2010, HSA5) caballero@cab -8b

  5. “De Mayrit al cielo”: • Orioniscluster • ( ~ 3 Ma, d ~ 385 pc) • InitialMassFunction • Brown dwarfs and “(isolated) planetary-massobjects” • Circum(sub)stellar discs • X-rays • Ha, Li I • Photometricvariability • Abundances • Propermotions • Spatialdistribution • Multiplicity… caballero@cab -7

  6. caballero@cab • Virtual Observatoryscience, e.g.Koenigstuhl 1AB: the (second) widestultracoolbinary •  = 77.76 ± 0.07 arcsec • d = 23 ± 2 pc • r = 1800 ± 170 AU • MA = 0.103 ± 0.006 Msol • MB = 0.079 ± 0.004 Msol • Highlight of theweek in A&A.Almostcover page! -6

  7. caballero@cab • Lecturer at theUniversidad Complutense de Madrid • From quarks to Cosmos (2007-08, 2008-09) • Astrophysics (2008-09, 2009-10) • Physics of the Solar System(2010-11; Master) • “Trabajo académicamente dirigido” (2009) & “Trabajo fin de Máster” (2010) -5

  8. Outreach: Rock’n’Astronomy caballero@cab -4

  9. caballero@cab • WSO-UV: WorldSpaceObservatory-UltraViolet • 1.7 m telescope • Russian-Spanish-Germanspacemission •  = 1210-6563 Å • Spanishcontribution: ISSIS (imaging and slit-lessspectroscopyinstrumentforsurveys) and groundsegment • Launch: 2014 -3

  10. caballero@cab • GO-IRS: GTC OpticalIntermediateResolutionSpectrograph • 10.4 m Gran Telescopio Canarias • University of Florida, China, Spain • 1000 MOS fibres in FoV = 15 arcmin + IFU • R = 20k, 10k, 5-2k;  = 0.37-1.00 m (or 0.45-1.25 m…) • Project scientist -2

  11. caballero@cab • CARMENES: Calar Alto high-Resolutionsearchfor M dwarfswithExoearthswithNear-infrared and opticalEchelleSpectrographs • 3.5 m telescope • 1 m/s radial-velocityaccuracywith a double-channelspectrograph • 11 German and Spanishinstitutions • Deputyproject manager -1

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