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: http://www.stsci.edu/~inr/thisweek1/2013/thisweek203.html
Дата изменения: Wed Nov 13 20:33:31 2013 Дата индексирования: Sat Mar 1 13:25:13 2014 Кодировка: Поисковые слова: moon |
Program Number | Principal Investigator | Program Title |
---|---|---|
12114 | Julianne Dalcanton, University of Washington | A Panchromatic Hubble Andromeda Treasury - I |
12115 | Julianne Dalcanton, University of Washington | A Panchromatic Hubble Andromeda Treasury - I |
12488 | Mattia Negrello, Open University | SNAPshot observations of gravitational lens systems discovered via wide-field Herschel imaging |
12519 | Raghvendra Sahai, Jet Propulsion Laboratory | Newly Discovered LMC Preplanetary Nebulae as Probes of Stellar Evolution |
12866 | Mark Swinbank, University of Durham | A Morphological Study of ALMA Identified Sub-mm Galaxies with HST/WFC3 |
12870 | Boris T. Gaensicke, The University of Warwick | The mass and temperature distribution of accreting white dwarfs |
12873 | Beth Biller, Max-Planck-Institut fur Astronomie, Heidelberg | Search for Planetary Mass Companions around the Coolest Brown Dwarfs |
12874 | David Floyd, Monash University | Quasar accretion disks: is the standard model valid? |
12880 | Adam Riess, The Johns Hopkins University | The Hubble Constant: Completing HST's Legacy with WFC3 |
12884 | Harald Ebeling, University of Hawaii | A Snapshot Survey of The Most Massive Clusters of Galaxies |
12890 | Edward M. Sion, Villanova University | The Unique Recurrent Nova T Pyxidis: The Decline and Transition to Quiescence |
12893 | Ronald L Gilliland, The Pennsylvania State University | Study of Small and Cool Kepler Planet Candidates with High Resolution Imaging |
12897 | Marc W. Buie, Southwest Research Institute | Pluto System Orbits in Support of New Horizons |
12902 | Matthew A. Malkan, University of California - Los Angeles | WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
12904 | Joel N. Bregman, University of Michigan | The Galactic Fountain Meets The Accreting Halo |
12922 | Jong-Hak Woo, Seoul National University | Calibrating black hole mass estimators using the enlarged sample of reverberation-mapped AGNs |
12934 | Clive N. Tadhunter, University of Sheffield | The importance warm outflows in the most rapidly evolving galaxies in the local Universe |
12967 | Abhijit Saha, National Optical Astronomy Observatory, AURA | Establishing a Network of DA White Dwarf SED Standards |
12978 | Daniel E. Welty, University of Chicago | Properties of Diffuse Molecular Gas in the Magellanic Clouds |
12982 | Nicolas Lehner, University of Notre Dame | Are the Milky Way's High Velocity Clouds Fuel for Star Formation or for the Galactic Corona? |
13004 | Margaret Meixner, The Johns Hopkins University | The Life Cycle of Dust in the Magellanic Clouds: Crucial Constraints from Zn and Cr depletions |
13017 | Timothy M. Heckman, The Johns Hopkins University | UV Spectroscopy of Lyman Break Galaxy Analogs: A Local Window on the Early Universe |
13045 | Asantha Cooray, University of California - Irvine | The Nature and Environment of a Luminous Starburst Galaxy During the Era of Reionization |
13046 | Robert P. Kirshner, Harvard University | RAISIN: Tracers of cosmic expansion with SN IA in the IR |
13050 | Remco van den Bosch, Max-Planck-Institut fur Astronomie, Heidelberg | The Most Massive Black Holes in Small Galaxies |
13063 | Adam Riess, The Johns Hopkins University | Supernova Follow-up for MCT |
13113 | C. S. Kochanek, The Ohio State University | ENERGY DEPENDENT X-RAY MICROLENSING AND THE STRUCTURE OF QUASARS |
13176 | Daniel Apai, University of Arizona | Extrasolar Storms: The Physics and Chemistry of Evolving Cloud Structures in Brown Dwarf Atmospheres |
13184 | Jelle Kaastra, Space Research Organization Netherlands | Deciphering AGN outflows: multiwavelength monitoring of NGC 5548 |
13286 | Ryan Foley, University of Illinois at Urbana - Champaign | Understanding the Progenitor Systems, Explosion Mechanisms, and Cosmological Utility of Type Ia Supernovae |
13502 | Steven Chesley, Jet Propulsion Laboratory | Search for the Binary Companion of Deep Impact Target 2002 GT |
GO 12866: A Morphological Study of ALMA Identified Sub-mm Galaxies with HST/WFC3
GO 12897: Pluto system orbits in support of New Horizons
GO 13063: Supernova follow-up for MCT Programs
![]() High redshift supernovae from HST observations in previous cycles |
CANDELS and CLASH are two of three Multi-Cycle Treasury Programs whose observations will be executed over HST Cycles 18, 19 and 20. Both programs have components that focus on the identification and subsequent follow-up of candidate high redshift supernovae. CLASH focuses on galaxy clusters (eg GO 12065 ), with 17-colour observations using ACS and WFC3. But while the cluster is centred on one camera, the second camera is being used to take deep images in fields offset by several arcminutes, and the multiple exposures obtained in those regions can be used to search for high redshift supernovae. CANDELS is a tiered wide-field imaging program that includes coverage of the two fields of the Great Observatory Origins Deep Survey (GOODS), centred on the northern Hubble Deep Field (HDF) in Ursa Major and the Chandra Deep Field-South in Fornax. In addition to deep HST data at optical and near-infrared wavelengths, those fields have been covered at X-ray wavelengths by Chandra (obviously) and XMM-Newton; at mid-infrared wavelengths with Spitzer; and ground-based imaging and spectroscopy using numerous telescopes, including the Kecks, Surbaru and the ESO VLT. This represents an accumulation of almost 1,000 orbits of HST time, and comparable scale allocations on Chandra, Spitzer and ground-based facilities. CANDELS is capitalising on this large investment, with new observations with WFC3 and ACS on both GOODS fields, and on three other fields within the COSMOS, EGS and UDS survey areas (see this link for more details). The existence of previous datasets permits searching for high-redshift supernovae, with the prime aim of measuring their properties at redshifts between z~1 and z~2. The present program is focused on a high-redshift candidate identified within the EGS field. |
GO 13176: Extrasolar Storms: The Physics and Chemistry of Evolving Cloud Structures in Brown Dwarf Atmospheres