▪ Abstract The properties of galaxies that are lower in surface brightness than the dark night
sky are reviewed. There are substantial selection effects against the discovery of galaxies …

▪ Abstract The physical properties of the faint blue galaxy population are reviewed in the
context of observational progress made via deep spectroscopic surveys and Hubble Space …

From the Nobel Prize–winning physicist Opinions on the large-scale structure of the early
universe range widely from primeval chaos to a well-ordered mass distribution. PJE Peebles …

The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …

The universe at faint magnitudes. I - Models for the galaxy and the predicted st ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …

We present star count data from the Sloan Digital Sky Survey for 5.8× 10 5 stars brighter
than g &arcmin;= 21 mag over 279 deg 2 in two samples north and south of the Galactic …

Infrared source counts at wavelengths 3 μm< λ< 10 μm cover more than 10 mag in source
brightness, reach 4 orders of magnitude in surface density, and reach an integrated surface …

A total of 86 galaxies have been detected at 60 microns in the high galactic latitude portion
of the IRAS minisurvey. The surface density of detected galaxies with flux densities greater …

A comparison of digital centering algorithms ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

Using a new multislit spectrograph, LDSS, we have obtained intermediate dispersion
spectroscopy for a new sample of 149 faint objects selected randomly from the magnitude …