Motivation • 40 orbits of UDF observations with the ACS grism • Spectra for every source in the field. • Good S N continuum detections to I(AB) ~ 27; about 30% of UDF sources. • Spectral identification of every 4 - Gunn–Peterson trough - Document - PDFSEARCH.IO

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Date: 2004-10-25 16:02:54 Space Reionization Gunn–Peterson trough Quasar Lyman-alpha emitter Lyman-break galaxy Wilkinson Microwave Anisotropy Probe Redshift Astronomical spectroscopy Physical cosmology Astronomy Physics		Motivation • 40 orbits of UDF observations with the ACS grism • Spectra for every source in the field. • Good S/N continuum detections to I(AB) ~ 27; about 30% of UDF sources. • Spectral identification of every 4 Add to Reading List Source URL: www.stsci.edu Download Document from Source Website File Size: 561,16 KB Share Document on Facebook

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