Regina E. Schulte-Ladbeck
Affiliations: | University of Pittsburgh, Pittsburgh, PA, United States |
Area:
Astronomy and AstrophysicsGoogle:
"Regina Schulte-Ladbeck"Mean distance: 4658.33
Children
Sign in to add traineeJennifer J. Birriel | grad student | 2000 | University of Pittsburgh |
James E. Herald | grad student | 2000 | University of Pittsburgh |
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Publications
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Cherinka B, Schulte-Ladbeck RE. (2011) Ca II and Na i quasar absorption-line systems in an emission-selected sample of SDSS DR7 galaxy/quasar projections. I. Sample selection Astronomical Journal. 142 |
Schulte-Ladbeck R, Hopp U, Brinks E, et al. (2010) Dwarf-Galaxy Cosmology Advances in Astronomy. 2010: 930426 |
Cherinka B, Schulte-Ladbeck RE, Rosenberg JL. (2009) H i observations of the Ca II absorbing galaxies Mrk 1456 and SDSS J211701.26-002633.7 Astronomical Journal. 138: 1714-1723 |
Schulte-Ladbeck RE. (2008) Connecting high-redshift galaxy populations through observations of local Damped Lyman Alpha dwarf galaxies Proceedings of the International Astronomical Union. 4: 129-133 |
Hopp U, Schulte-Ladbeck RE, Kerp J. (2007) Searching for stars in compact high-velocity clouds - II Monthly Notices of the Royal Astronomical Society. 374: 1164-1168 |
König B, Schulte-Ladbeck RE, Cherinka B. (2006) Galaxies in front of quasars: Markarian 1456 and SDSS J114719.90+522923.2 Astronomical Journal. 132: 1844-1850 |
Schulte-Ladbeck RE, König B, Miller CJ, et al. (2005) Emission-line spectroscopy of Damped Lyαa systems: The case of ses 1543+593/HS 1543+5921 Astrophysical Journal. 625: L79-L82 |
Christensen L, Schulte-Ladbeck RE, Sánchez SF, et al. (2005) Abundances and kinematics of a candidate sub-damped Lymanα galaxy toward PHL 1226 Astronomy and Astrophysics. 429: 477-487 |
Schulte-Ladbeck RE, König B, Cherinka B. (2005) Chemical abundances in star-forming galaxies and damped Lyman alpha systems Proceedings of the International Astronomical Union. 1: 319-324 |
Schulte-Ladbeck RE, Rao SM, Drozdovsky IO, et al. (2004) The H II regions of the damped Lyα absorber SBS 1543+593 Astrophysical Journal. 600: 613-625 |