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astro-ph2008

An extended dust disk in a spiral galaxy; An occulting galaxy pair in ANGST

B. W. Holwerda, W. C. Keel, B. Williams +2

We present an analysis of an occulting galaxy pair, serendipitously discovered in ACS Nearby Galaxy Survey Treasury (ANGST) observations of NGC 253 taken with Hubble Space Telescop…

astro-ph2008

Spitzer's View of Edge-on Spirals

B. W. Holwerda, R. S. de Jong, A. Seth +4

Edge-on spiral galaxies offer a unique perspective on disks. One can accurately determine the height distribution of stars and ISM and the line-of-sight integration allows for the…

astro-ph2008

Structure and Evolution of the Opacity of Spiral Disks

B. W. Holwerda, R. A. Gonzalez, W. C. Keel +3

The opacity of a spiral disk due to dust absorption influences every measurement we make of it in the UV and optical. Two separate techniques directly measure the total absorption…

astro-ph2007

Structure and Evolution of the Opacity of Spiral Disks

B. W. Holwerda, R. A. González, W. C. Keel +3

The opacity of a spiral disk due to dust absorption influences every measurement we make of it in the UV and optical. Two separate techniques directly measure the total absorption…

astro-ph2007

Spitzer's View of Edge-on Spirals

B. W. Holwerda, R. S. de Jong, A. Seth +4

Edge-on spiral galaxies offer a unique perspective on disks. One can accurately determine the height distribution of stars and ISM and the line-of-sight integration allows for the…

astro-ph2007

Galaxy Structural Parameters in Source Extractor

B. W. Holwerda

Over the last decade, the Concentration, Asymmetry and Smoothness (CAS), as well as the M20 and GINI parameters have become popular to automatically classify distant galaxies in im…