Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Kernphysik     Collection: Infrared Astrophysics     Display Documents



  history
ID: 395942.0, MPI für Kernphysik / Infrared Astrophysics
Galaxy And Mass Assembly (GAMA)
Authors:Driver, S. P.; Baldry, I. K.; Bamford, S.; Bland-Hawthorn, J.; Bridges, T.; Cameron, E.; Conselice, C.; Couche, W. J.; Croom, S.; Cross, N. J. G.; Dunne, L.; Eales, S.; Edmondson, E.; Ellis, E.; Frenk, C. S.; Graham, A. W.; Jones, H.; Hill, H.; Hopkins, A.; van Kampen, E.; Kuijken, E.; Lahav, O.; Liske, J.; Loveday, J.; Nichol, B.; Norberg, B.; Norberg, P.; Oliver, S.; Parkinson, H.; Peacock, J. A.; Phillips, S.; Popescu, C.; Prescott, M.; Proctor, R.; Sharp, R.; Staveley-Smith, L.; Sutherland, W.; Tuffs, R.; Warren, S.
Language:English
Date of Publication (YYYY-MM-DD):2008
Title of Series:IAU Symposium
Volume (in Series):254
Name of Conference/Meeting:The Galaxy Disk in Cosmological Context
Place of Conference/Meeting:Copenhagen, Denmark
(Start) Date of Conference/Meeting
 (YYYY-MM-DD):
2008-06-09
End Date of Conference/Meeting 
 (YYYY-MM-DD):
2008-06-13
Copyright:2008 International Astronomical Union
Review Status:not specified
Audience:Experts Only
Abstract / Description:The GAMA survey aims to deliver 250,000 optical spectra (3–7°A resolution) over 250 sq. degrees to spectroscopic limits of rAB < 19.8 and KAB < 17.0 mag. Complementary imaging will be provided by GALEX, VST, UKIRT, VISTA, HERSCHEL and ASKAP to comparable flux levels leading to a definitive multi-wavelength galaxy database. The data will be used to study all aspects of cosmic structures on 1kpc to 1Mpc scales spanning all environments and out to a redshift limit of z  0.4. Key science drivers include the measurement of: the halo mass function via group velocity dispersions; the stellar, HI, and baryonic mass functions; galaxy component mass-size relations; the recent merger and star-formation rates by mass, types and environment. Detailed modeling of the spectra, broad SEDs, and spatial distributions should provide individual star formation histories, ages, bulge-disc decompositions and stellar bulge, stellar disc, dust disc, neutral HI gas and total dynamical masses for a significant subset of the sample ( 100k) spanning both the giant and dwarf galaxy populations. The survey commenced March 2008 with 50k spectra obtained in 21 clear nights using the Anglo Australian Observatory’s new multi-fibre-fed bench-mounted dual-beam spectroscopic system (AA ).
External Publication Status:accepted
Document Type:Conference-Paper
Affiliations:MPI für Kernphysik/Group of W. Hofmann/Infrared Astrophysics (R. Tuffs)
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.