Studying the Evolution of Field Galaxies Using NICMOS/HST Parallel Imaging and Grism Data

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We present results from our analysis of F160W NICMOS Parallel images. These data cover 9 sq. arcminutes and reach 3σ depths of H= 24.3 - 25.5 in a 0.6'' diameter aperture with integration times of 2,000 to 13,000 seconds. We derive the first deep H band galaxy counts. The slope of the counts for H< 20 is 0.31, consistent with various K-band measurements from the Keck telescopes. The measured number counts vs. magnitude relation is reasonably well fitted with no-evolution models with a low Ω value. The half-light radii of the galaxies declines steeply with apparent magnitude and reaches the NIC3 resoltion limit at H=23.5. Deep ground-based VRI imaging of one NICMOS field has revealed an extremely red galaxy with R-H = 6 and H of 18.8. Our analyses of the grism data show that we can reach 3σ flux limits of of 1× 10⁻¹⁶ to 2×10⁻¹⁷ ergs/sec/cm² for integration times of 2,000 to 21,000 seconds. We have detected a total of 33 emission line galaxies. The comoving number density is 2× 10⁻⁴ Mpc⁻³. The detected emission lines are probably Hα 6563Å. Thus, the derived star formation rates, without extinction correction, are 10 - 163 M per year for galaxies at redshifts between 0.7 and 1.9.