about
Variable Stars in the Newly Discovered Milky Way Dwarf Spheroidal Satellite Canes Venatici IOn the Newly Discovered Canes Venatici II dSph GalaxyThe long-lived UV "plateau" of SN 2012awPulsating variable stars in the Coma Berenices dwarf spheroidal galaxyOn the Remote Galactic Globular Cluster NGC 2419SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phaseSTEP: the VST survey of the SMC and the Magellanic Bridge – I. Overview and first results★STREGA: STRucture and Evolution of the GAlaxy – I. Survey overview and first results★The Carina Project. I. Bright Variable StarsThe Carina Project. II. Stellar PopulationsRemoving static aberrations from the active optics system of a wide-field telescopeSupersolar Ni/Fe production in the Type IIP SN 2012ecThe Type IIP supernova 2012aw in M95: hydrodynamical modeling of the photospheric phase from accurate spectrophotometric monitoringRed and dead: the progenitor of SN 2012aw in M95Looking for building blocks of the Galactic halo: variable stars in the Fornax, Bootes I, Canes Venatici II dwarfs and in NGC 2419The Leo IV dwarf spheroidal galaxy: color-magnitude diagram and pulsating starsOn the distance of the globular cluster M4 (NGC 6121) using RR Lyrae stars. I. Optical and near-infrared period-luminosity and period-wesenheit relationsThe Capodimonte Deep Field. Presentation of the survey and first follow-up studiesData reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep FieldShapley Supercluster Survey: construction of the photometric catalogues andi-band data releaseOn a new near-infrared method to estimate the absolute ages of star clusters: NGC 3201 as a first test caseON THE ΔVbumpHBPARAMETER IN GLOBULAR CLUSTERSA new method to estimate the ages of globular clusters: the case of NGC 3201On the radial distribution of horizontal branch stars in NGC 2808The Carina project. VII. Toward the breaking of the age-metallicity degeneracy of red giant branch stars using the c_U, B, I_ indexConstraints on the formation of the globular cluster IC 4499 from multiwavelength photometry★Period change similarities among the RR Lyrae variables in Oosterhoff I and Oosterhoff II globular systemsReddening Distribution across the Center of the Globular Cluster ω CentauriThe M31 pixel lensing PLAN campaign: MACHO lensing and self-lensing signals
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description
hulumtues
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researcher
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wetenschapper
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հետազոտող
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
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Massimo Dall'Ora
@sl
P106
P21
P31
P496
0000-0001-8209-0449