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Дата изменения: Fri Jun 8 23:36:04 2007 Дата индексирования: Tue Oct 2 14:14:16 2012 Кодировка: Поисковые слова: solar corona |
ACS resumes observations with the Wide-Field Camera
Program Number | Principal Investigator | Program Title | Links |
10496 | Saul Perlmutter, Lawrence Berkeley National Laboratory | Decelerating and Dustfree: Efficient Dark Energy Studies with Supernovae and Clusters | Abstract |
10519 | Janet Simpson, NASA Ames Research Center | Testing the Stellar Coalescence and Accretion Disk Theories of Massive Star Formation with NICMOS | Abstract |
10551 | Shri Kulkarni, California Institute of Technology | Gamma-Ray Bursts from Start to Finish: A Legacy Approach | Abstract |
10632 | Massimo Stiavelli, Space Telescope Science Institute | Searching for galaxies at z>6.5 in the Hubble Ultra Deep Field | Abstract |
10633 | Nial Tanvir, University of Hertfordshire | GRB afterglows and host galaxies at very high redshifts | Abstract |
10763 | Shami Chatterjee, Harvard University | The Guitar Nebula: A Bow Shock that Traces ISM Turbulence and Accelerates Relativistic Particles | Abstract |
10795 | Timothy Heckman, The Johns Hopkins University | The Largest Galaxies in the Local Universe: New Light on Disk Galaxy Formation? | Abstract |
10802 | Adam Riess, Space Telescope Science Institute | SHOES-Supernovae, HO, for the Equation of State of Dark energy | Abstract |
10813 | David Bowen, Princeton University | MgII Absorption Line Systems: Galaxy Halos or the Metal-Enriched IGM? | Abstract |
10824 | Oleg Gnedin, The Ohio State University Research Foundation | Measuring the Shape and Orientation of the Galactic Dark-Matter Halo using Hypervelocity Stars | Abstract |
10825 | Bradford Holden, University of California - Santa Cruz | The Formation Epoch of Early-type Galaxies: Constraints from the Fundamental Plane at z=1.3 | Abstract |
10829 | Paul Martini, The Ohio State University | Secular Evolution at the End of the Hubble Sequence | Abstract |
10848 | Mark Lacy, Jet Propulsion Laboratory | Relating the host galaxies of type-2 quasars to their infrared properties | Abstract |
10851 | Raghvendra Sahai, Jet Propulsion Laboratory | Solving the Riddle of the Red Rectangle: Proper Motion Study of a Bipolar Nebula around a Binary | Abstract |
10852 | Glenn Schneider, University of Arizona | Coronagraphic Polarimetry with NICMOS: Dust grain evolution in T Tauri stars | Abstract |
10876 | Jean-Paul Kneib, Observatoire de Marseille | SL2S: The Strong Lensing Legacy Survey | Abstract |
10880 | Henrique Schmitt, Naval Research Laboratiry | The host galaxies of QSO2s: AGN feeding and evolution at high luminosities | Abstract |
10886 | Adam Bolton, Smithsonian Institution Astrophysical Observatory | The Sloan Lens ACS Survey: Towards 100 New Strong Lenses | Abstract |
10893 | Peter Garnavich, University of Notre Dame | Sweeping Away the Dust: Reliable Dark Energy with an Infrared Hubble Diagram | Abstract |
10905 | R. Tully, University of Hawaii | The Dynamic State of the Dwarf Galaxy Rich Canes Venatici I Region | Abstract |
10906 | Sylvain Veilleux, University of Maryland | The Fundamental Plane of Massive Gas-Rich Mergers: II. The QUEST QSOs | Abstract |
10920 | Charles Hoopes, The Johns Hopkins University | High-Resolution Imaging of Nearby Lyman Break Galaxy Analogs in the GALEX All-Sky Survey | Abstract |
GO 10802: SHOES-Supernovae, HO, for the Equation of State of Dark energy
GO 10852: Coronagraphic Polarimetry with NICMOS: Dust grain evolution in T Tauri stars
GO 10886: The Sloan Lens ACS Survey: Towards 100 New Strong Lenses