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 - Lyman Good - Document - PDFSEARCH.IO

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	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 Document Date: 2004-10-25 16:02:54 Open Document File Size: 561,16 KB Share Result on Facebook Company ACS / Lilly / / RadioStation WMAP / / Technology alpha / Spectroscopy / S/N / / SocialTag Space Reionization Gunn–Peterson trough Quasar Lyman-alpha emitter Lyman-break galaxy Wilkinson Microwave Anisotropy Probe Redshift Astronomical spectroscopy Physical cosmology

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 4Add to Reading List