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RESOLVE Survey | resolve.astro.unc.edu Reviews
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RESOLVE Survey
resolve.astro.unc.edu
Footprints
http://resolve.astro.unc.edu/pages/footprints.php
Skip to the navigation. Skip to the content. Skip to the news. RESOLVE-A (footprint demarcated by red dashed lines) embedded within ECO (entire plot showing current footprint, with ECO-B in preparation). Color indicates group halo mass from abundance matching. Dots mark galaxies brighter than M r. 175 in the ECO redshift range cz=2530-7470 km/s, which encompasses the RESOLVE redshift range cz=4500-7000 km/s. For the RESOLVE-B footprint click link below. B-semester RESOLVE footprint (62kB).
ECO Data Release 1
http://resolve.astro.unc.edu/news/20150731-ecoDR1.php
Skip to the navigation. Skip to the content. Skip to the news. ECO Data Release 1. Posted July 31, 2015. Basic properties of all ECO galaxies including stellar masses, colors, morphologies, and environmental properties have been released in Moffett et al. (2015). These measurements are combined with archival UV and HI data to analyze the environmental dependence of galaxy disk growth, with emphasis on disk regrowth in E/S0 galaxies. Click here for data. Click here for paper. ECO Data Release 1.
RESOLVE Publications
http://resolve.astro.unc.edu/pages/papers.php
Skip to the navigation. Skip to the content. Skip to the news. RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions. K D Eckert, S. J. Kannappan, D. V. Stark, A. J. Moffett, A. A. Berlind, and M. A. Norris, ApJ, accepted. RESOLVE Survey Photometry and Volume-limited Calibration of the Photometric Gas Fractions Technique. ECO and RESOLVE: Galaxy Disk Growth in Environmental Context. Analysis of Galaxy Halpha Kinematics Using SALT RSS Fabry-Perot Velocity Fields.
outreach
http://resolve.astro.unc.edu/pages/outreach.php
Skip to the navigation. Skip to the content. Skip to the news. Background on the RESOLVE Survey. A KIPP Pride High School student from Gaston, North Carolina looks at SOAR telescope data with UNC undergraduate David Hendel and Prof. Sheila Kannappan in UNCs Remote Observing Center. Education and Outreach Efforts. AIMs Astronomy Instructional Modules for Physics:. This series of modules is aligned to the North Carolina state high school physics standards. The FAQ. Module 5 - Red Recedes, Blue Approaches.
Data
http://resolve.astro.unc.edu/pages/data.php
Skip to the navigation. Skip to the content. Skip to the news. RESOLVE's optical spectroscopy campaign makes use of UNC guaranteed time on the SOAR. Telescopes, supplemented with NOAO-awarded SOAR, Gemini, and AAT time as well as Rutgers/SAAO partner SALT time. Our 21cm campaign depends on the Arecibo. Click here for RESOLVE DR1 photometry. All galaxies, UV/optical/near-IR) from Eckert et al. 2015. Click here for ECO DR1 catalog. All galaxies) from Moffett et al. 2015. GALEX completed priority MIS-depth ...
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RESOLVE Survey
Skip to the navigation. Skip to the content. Skip to the news. REsolved Spectroscopy Of a Local VolumE. For a non-technical description. Survey Selection and Completeness. For information on how RESOLVE is adding to this treasury. 1723, corresponding to the apparent magnitude limit of the SDSS redshift survey at the far side of the RESOLVE cz range. The r band is ideal for selection on the sum. Of stellar cold gas mass (Kannappan and Wei 2008), yielding an approximate survey mass limit of 10 9. The high-...
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