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ScienceProblem: GalaxyClustering PrimaryActor: astronomer ScienceGoal: Aim to address the evolution of galaxy populations in clusters. Comparison can then be made ...
Brown Dwarf Rough Notes AnitaRichards 12 Jan 2004 The parts of the workflow which I think we can do now or are about to be able to do, with some questions so ...
The European Astrophysical Virtual Observatory Project is a Phase A, three year study for the design and implementation of a VirtualObservatory for European astronomy ...
ScienceProblem: SolarStellarFlareComparison PrimaryActor: Astronomer ScienceGoal: Compare the atttributes of stellar and solar flares in order to determine the mechanism ...
ScienceProblem: STPSolarEventCoincidence PrimaryActor: Astronomer ScienceGoal: Identify models that use solar data to predict STP events with the greatest accuracy ...
ScienceProblem: SupernovaGalaxyEnvironment PrimaryActor: Astronomer, automated search engine ScienceGoal: Determine the galaxy environment of fields used in the ...
ScienceProblem: SolarCoronalWaves PrimaryActor: Astronomer ScienceGoal: There has been much debate recently about whether large scale coronal waves and chromospheric ...
ScienceProblem: OpticalNearIRGalaxyClusterSelection PrimaryActor: Research astronomer ScienceGoal: To create a catalogue of galaxy clusters using optical and near ...
ScienceProblem: MagneticStormOnset PrimaryActor: A solar terrestrial physicist studying the morphology of the tail of the Earth's magnetosphere during the onset of ...
ScienceProblem: DeepFieldSurveys PrimaryActor Astronomer ScienceGoal To establish the properties of faint extragalactic sources in the Hubble Deep Field (North ...
ScienceProblem: HiZQuasars PrimaryActor: Astronomer ScienceGoal: Discovery of very high redshift quasars in the range z 5 to 10. The most distant quasar currently ...
ScienceProblem: BrownDwarfSelection PrimaryActor: Astronomer ScienceGoal: Learn about the lower end to the stellar mass function by conducting a census of all brown ...
Spectra of the three new quasars at z 6. For SDSS J1148 5251, a spectrum taken at the Calar Alto 3.5 m is shown and binned to 1 Å pixel 1; for SDSS J1048 4637 and ...
FIG. 5.The discovery spectra of the three new z 5.8 quasars, taken with the ARC 3.5 m telescope and DIS spectrograph. The exposure time is 3600 s for each quasar ...
FIG. 1.The i z vs. z color magnitude diagram for the i dropout sample. Colors and magnitudes are plotted as asinh magnitudes measured by SDSS imaging. The symbols ...
Figure 1 A B J, R colour magnitude diagram for a typical high latitude UKST field used in the APM survey. Every detected B J, R matched pair of objects classified ...
Welcome to the home of AgWiki.VO. This is a web based collaboration area for ... VirtualObservatory topics in general Virtula Observatory developments and ...
The Future : EURO VO Planning A successor project to the AstrophysicalVirtualObservatory is now in the proposal stage, known as the EURO VO project. The AVO was ...