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The Wyoming Survey for H-alpha. I. Initial Results at z ~ 0.16 and 0.24
Daniel A. Dale, Rebecca J. Barlow, Seth A. Cohen +6
The Wyoming Survey for H-alpha, or WySH, is a large-area, ground-based, narrowband imaging survey for H-alpha-emitting galaxies over the latter half of the age of the Universe. The…
Variations in 24 micron morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: New insights into the Hubble sequence
G. J. Bendo, D. Calzetti, C. W. Engelbracht +7
To study the distribution of star formation and dust emission within nearby galaxies, we measured five morphological parameters in the 3.6 and 24 micron wave bands for 65 galaxies…
An Optical Survey of the Position Error Contours of Unidentified High Energy Gamma-Ray Sources at Galactic Latitude b >|20| degrees
S. D. Bloom, D. A. Dale, R. Cool +7
We present the most recent results of an optical survey of the position error contours ("error boxes") of unidentified high energy gamma-ray sources.
SINGS: The SIRTF Nearby Galaxies Survey
R. C. Kennicutt, L. Armus, G. Bendo +20
The SIRTF Nearby Galaxy Survey is a comprehensive infrared imaging and spectroscopic survey of 75 nearby galaxies. Its primary goal is to characterize the infrared emission of gala…
Optically faint counterparts to the ISO-FIRBACK 170 micron population: the discovery of cold, luminous galaxies at high redshift
S. C. Chapman, I. Smail, R. J. Ivison +3
We present Keck spectroscopy and UKIRT near-IR imaging observations of two 170micron-selected sources from the ISO-FIRBACK survey which have faint counterparts in the optical, and…
No Hubble Bubble in the Local Universe
R. Giovanelli, Daniel Dale, Martha Haynes +2
Zehavi et al. (1998) have suggested that the Hubble flow within 70/h Mpc may be accelerated by the existence of a void centered on the Local Group. Its underdensity would be ~20 %,…