Tiempo asignado por el CAT

Semestre 2014B

William Herschel Telescope

Ref. CATIPNoches ConcedidasInstrumentoProgramaColaboradores
8-WHT2/14BGloria Sala Cladellas15 A (0.5hrs)ACAMWHT/ACAM identification spectroscopy of nova candidates in M31
21-WHT3/14BTariq Shahbaz1 D (II)visitanteIquEYE observations of the pulsar PSR J1023+0038
33-WHT5/14BJavier Zaragoza Cardiel3 GvisitanteUnveiling the gas kinematics of interacting/merging galaxies
37-WHT6/14BTariq Shahbaz1 A (4.5hrs)LIRISThe polarimetric signature of jets in X-ray binaries
51-WHT8/14BEduardo Martin Guerrero de Escalante1 D (I)ISISSpectroscopic characterization of low-latitude ultracool dwarfs
53-WHT10/14BIrene Agulli4 D (II)AF2Deep spectroscopy of dwarf galaxies in the Perseus cluster
58-WHT11/14BJose Alfonso Lopez Aguerri3 G (I)NAOMI/OASISUnveiling the evolution of bulges in lenticular galaxies
73-WHT13/14BRomano Corradi3 G (I)ISISThe chemistry of planetary nebulae with close binary central stars: clues to the abundance discrepancy problem?
82-WHT15/14BMaría Rosa Zapatero Osorio4 G (I)ISISPolarimetric characterization of the comet-like tails of disintegrating planets
91-WHT17/14BJulia de Leon Cruz3 A (II)LIRISNear-infrared spectra of asteroids from the Erigone collisional family
95-WHT18-B/14BDiego Tescaro2 D (2hrs)ACAMConstraining the Extragalactic Background Light through gamma-ray BL Lacs objects
103-WHT19/14BCarlos Allende Prieto3 AISISEarly Steps of the Milky Way: Old Stars as Tracers of the Formation and Evolution of the Galactic Halo.
104-WHT20/14BPeter Klagyivik4 GAF2The unusual frequency of eclipsing binaries in NGC 2264: Implication for cluster formation
123-WHT23/14BLuis Colina Robledo2 A (I)LIRISNear-IR study of the OH Megamaser Infrared luminous Galaxy
124-WHT24/14BGemma Busquet2 D (I)ISISUnveiling the L1157-B1 bow-shock structure through optical emisison lines
129-WHT25-B/14BPaulo Alberto Miles Páez2 D (II)LIRISHigh rotation and linear polarization: exploring the dusty atmospheres of ultracool dwarfs
132-WHT27/14BArtemio Herrero Davó1 A (II)LIRISEXPLORING THE POTENTIAL OF THE J-BAND FOR MASSIVE STARS ANALYSES
133-WHT28/14BArtemio Herrero Davó2 A (I)AF2Asking the neighbors about two apparently very massive stars in Cygnus OB2
144-WHT30/14BJosé Miguel Rodríguez Espinosa2 GISISDouble peaked AGNs: Binnary AGNs or kinematical efffects
150-WHT32/14BNicolas Lodieu1 G (I)LIRISAccretion and outflow properties in Class I brown dwarfs
163-WHT35-A/14BJavier Gorosabel Urkia1 A (1hrs)LIRISThe WHT to study short GRBs, the LT to monitor long GRBs, and the INT to identify FERMI GRBs: 3 telescopes for 3 sharp GRB science cases.
163-WHT36-B/14BJavier Gorosabel Urkia1 A (1hrs)PFIPThe WHT to study short GRBs, the LT to monitor long GRBs, and the INT to identify FERMI GRBs: 3 telescopes for 3 sharp GRB science cases.
163-WHT37-D/14BJavier Gorosabel Urkia1 A (1hrs)ISISThe WHT to study short GRBs, the LT to monitor long GRBs, and the INT to identify FERMI GRBs: 3 telescopes for 3 sharp GRB science cases.
163-WHT38-E/14BJavier Gorosabel Urkia1 A (1hrs)ACAMThe WHT to study short GRBs, the LT to monitor long GRBs, and the INT to identify FERMI GRBs: 3 telescopes for 3 sharp GRB science cases.
166-WHT39/14BManuel Linares Alegret1 A (4.5hrs) (I)ISISThe mass of the neutron star in PSR J2215+5135