mosdef.astro.berkeley.edu
Team - The MOSFIRE Deep Evolution Field Survey
http://mosdef.astro.berkeley.edu/team
The MOSFIRE Deep Evolution Field Survey. Survey Parameters and Status. MOSDEF in the News. Co-PIs (in alphabetical order). Mojegan Azadi (UC San Diego). Tara Fetherolf (UC Riverside). William Freeman (UC Riverside). Gene Leung (UC San Diego). Ryan Sanders (UC Los Angeles). Tom Zick (UC Berkeley). Denison, former UCR grad). CfA, former UCB grad). U of Western Cape). Theme: based on Colinear by Automattic.
archive.stsci.edu
HST Treasury, Archival Legacy, and Large Programs
http://archive.stsci.edu/hst/tall.html
HST Treasury, Archival Legacy and Large Programs. Several special types of programs were created for the Hubble Space Telescope beginning in Cycle 11. Chief among these are the Treasury. Please consult the guidelines for contributing high-level science products. For more information. You may see a complete list of all high-level science products. Archived at MAST and also search for a variety of criteria to find HLSP of interest. You may also be interested in more information about download options.
stdatu.stsci.edu
HST Treasury, Archival Legacy, and Large Programs
http://stdatu.stsci.edu/hst/tall.html
HST Treasury, Archival Legacy and Large Programs. Several special types of programs were created for the Hubble Space Telescope beginning in Cycle 11. Chief among these are the Treasury. Please consult the guidelines for contributing high-level science products. For more information. You may see a complete list of all high-level science products. Archived at MAST and also search for a variety of criteria to find HLSP of interest. You may also be interested in more information about download options.
zfire.swinburne.edu.au
ZFIRE
http://zfire.swinburne.edu.au/index.html
A Keck/MOSFIRE spectroscopic survey of star-forming galaxies in rich enviornments during cosmic-noon. With the growing number of confirmed galaxy clusters at z 2, it is now possible to track how baryons cycle between stars, winds, and the ISM when cluster galaxies are still forming a large fraction of their stars. ZFIRE combines imaging from the Hubble Space Telescope. With deep spectroscopy from Keck Observatory.