PPT-SDSS-II SN survey:

Constraining Dark Energy with intermediate redshift probes Hubert Lampeitl University Portsmouth ICG In collaboration with HJ Seo T Giannantonio C Shapiro RC Nichol B Bassett WJ Percival T Davis . Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve . Majewski. (. UVa. ), Jennifer Johnson (OSU), Gail . Zasowski. (JHU), Leo . Girardi. (. Padova. ), Carlos Allende-. Prieto. (IAC), Ana Garcia-Perez (. White Dwarfs . in . SDSS . . Estimating the Mean Mass of Normal . DAs . and . DBs . Kepler. Scot . Kleinman. , Atsuko Nitta. B. árbara. Castanheira, . Detlev. Koester. Marcos Diaz . H. a. H. b. Yue . Shen. Carnegie Observatories. In collaboration with Brandon . Kelly (UCSB). M. otivation. T. he abundance (and clustering) of quasars are key to understand the evolution of quasars/SMBHs in the hierarchical structure formation paradigm . With thanks to the members of the Quasar Working Group, particularly Don Schneider, . Xiaohui. Fan, Michael Strauss, Pat Hall, Dan . Vanden. . Berk. , Sebastian Jester, and . Scott Anderson, also Adam Myers. Status and future developments. Luigi Boschetti, David Roy, . Chris Justice, Steve Stehman and Louis Giglio. Current version is C5 . . first global run of the product. . run on purpose with conservative thresholds. Fig. 2 SDSSLSST: Lightcurve of quadruple lens RXJ1131-12 fromoptical monitoring (Morgan et al. astro-ph/0605321). Here we predict the number distribution of lensed quasars in LSST. We assume Singular Followup. Paula Szkody. University of Washington. HotWiring. V. October 11, 2016. Survey . Results . (and . Followup. ) . depend on:. Limiting . magnitude . (aperture needed). FOV . (slit or multi-fiber). VG. So we want a color magnitude diagram for AGN so that by looking at the color of an AGN we can get its luminosity. But AGN have no fusion, why would we expect a color-magnitude relation?. The gas that accretes onto the black hole is still hot and so must follow the Blackbody Radiation law. . Ashley . Pagnotta. (very old novae), . Ben Oppenheimer (. chemistry of hot Jupiter atmosphere). , . MS + Dave . Zurek. . (. Magellanic. dwarf novae). . Adric. . Reidel. (young . red. dwarfs). Jackie . Brown dwarfs come of age. Fuerteventura, 21. st. May 2013. Plan. a. bit of history. the recent past . the state of the art. future challenges. The first wide area surveys. not digital. relatively simple data pipeline. @. SDSSurveys. Karen . Masters . Spokesperson for the Sloan Digital Sky . Survey-IV. Haverford College/University . of Portsmouth. @. KarenLMasters. Eighteen Years of . Sloan Digital . Sky Surveys. 14 . Ultra Metal - Poor (UMP ; [Fe/H] - 4 . 0 ) stars hold the key to the nucleosynthesis processes associated with first - generation stars in the Universe . However, only about two dozen UMP stars have b Report NoZKS15110048Page1of10Safety Data Sheets SDSsClientShenzhen Junered Battery IndCo LtdAdd of ClientNo506 Lot 3Block B Yintian Xifa Industrial ZoneXixiang TownBaoan DistrictShenzhenDescriptionAlk Keep labels on shipped containersLabel workplace containers where requiredChemical manufacturers and importers are required to provide labels on shipped containers with the following information produ