activity
19972010
most citedStar-Formation Rates of Local Blue Compact Dwarf Galaxies I: 1.4 GHz and 60 um luminosities

82 citations · 698 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.CO2010

Dwarf-Galaxy Cosmology

Regina Schulte-Ladbeck, Ulrich Hopp, Elias Brinks +1

Dwarf galaxies provide opportunities for drawing inferences about the processes in the early universe by observing our "cosmological backyard"-the Local Group and its vicinity. Thi…

astro-ph.CO2009★ 3 cited

HI Observations of the Ca II absorbing galaxies Mrk 1456 and SDSS J211701.26-002633.7

Brian Cherinka, Regina Schulte-Ladbeck, Jessica Rosenberg

In an effort to study Damped Lyman Alpha galaxies at low redshift, we have been using the Sloan Digital Sky Survey to identify galaxies projected onto QSO sightlines and to charact…

astro-ph.IM2009

Educating the Next Generation of Leading Scientists: Turning Ideas into Action

Michael Wood-Vasey, Regina Schulte-Ladbeck, William Blair +12

The core of scientific research is turning new ideas into reality. From the school science fair to the search for the secrets of dark energy, high-quality research consists of scie…

astro-ph2008

Connecting high-redshift galaxy populations through observations of local Damped Lyman Alpha dwarf galaxies

Regina E. Schulte-Ladbeck

I report on observations of the z=0.01 dwarf galaxy SBS1543+593 which is projected onto the background QSO HS1543+5921. As a star-forming galaxy first noted in emission, this dwarf…

astro-ph2006★ 15 cited

Searching for Stars in Compact High-Velocity Clouds. II

U. Hopp, R. E. -Schulte-Ladbeck, J. Kerp

We address the hypothesis that High Velocity Clouds correspond to the "missing" dwarf galaxies of the Local Group predicted by cosmological simulations. To this end, we present opt…

astro-ph2006★ 5 cited

Galaxies in front of Quasars: Mrk 1456 and SDSS J114719.90+522923.2

Brigitte K"onig, Regina E. Schulte-Ladbeck, Brian Cherinka

The chance projection of the disk of Mrk~1456 onto a background QSO is similar to the case of SBS 1543+593/HS 1543+5921. Mrk~1456 is a luminous, late-type spiral at z ~ 0.05. Thoug…