The NICMOS parallel program: Grism survey results and emission-line candidates

Details The NICMOS parallel program: Grism survey results and emission-line candidates The NICMOS parallel program: Grism survey results and emission-line candidates

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..470..364t&link_type=abstract

The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5). AIP Conference Proceedi

Computer Science

Databases

1

Observational Cosmology, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Origin, Formation, Evolution, Age, And Star Formation, Near Infrared

Scientific paper

In its parallel pointings, NICMOS has given us a unique window on the evolving Universe. We have analyzed the deep parallel NICMOS grism observations, covering more than 60 square arcminutes and down to continuum H1.6=22 in the deepest fields. With this slitless grism spectroscopy, NICMOS reveals 33 new line-emitting galaxies. In most cases, the single emission line is likely to be Hα at 0.7

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