Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sitc.conf.4020r&link_type=abstract
SPICA joint European/Japanese Workshop, held 6-8 July, 2009 at Oxford, United Kingdom. Edited by A.M. Heras, B.M. Swinyard, K.G
Physics
Galaxies: Formation, Missions: Spica
Scientific paper
Source confusion occurs when sources are clustered to the order of the telescope beam size on the sky, and determines the useful depth to which to take large-area extragalactic surveys (cf. discussion in Raymond et al. these proceedings). Line, or spectral confusion occurs when multiple sources are observed by a spectrometer in a single telescope beam: the spectra from two or more ob jects are effectively scrambled.
In this poster we present the preliminary results of an investigation into how well redshifts can be estimated from deep spectroscopic surveys with SAFARI-type observations in which more than one source is observed in a single, spatial element.
Isaak Kate G.
Raymond Gwenifer
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