Abstract / Description of output
We explore galaxy assembly over the last seven billion years by characterizing "normal" galaxies along the Hubble sequence, against strongly disturbed merging/interacting galaxies with the widely used CAS system of concentration (C), asymmetry (A), and 'clumpiness' (S) parameters, as well as visual classification. We analyze Hubble Space Telescope (HST) ACS images of similar to 4000 intermediate and high mass (M/M-circle dot > 10(9)) galaxies from the GEMS survey, one of the largest HST surveys conducted to date in two filters. We explore the effectiveness of the CAS criteria [A > S and A > 0.35] in separating normal and strongly disturbed galaxies at different, redshifts, and quantify the recovery and contamination rate. We also compare the average star formation rate and the cosmic star formation rate density as a function of redshift between normal and interacting systems identified by CAS.
Original language | English |
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Title of host publication | NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007 |
Editors | A Frebel, JR Maund, J Shen, MH Siegel |
Place of Publication | SAN FRANCISCO |
Publisher | ASTRONOMICAL SOC PACIFIC |
Pages | 235-238 |
Number of pages | 4 |
ISBN (Print) | 978-1-58381-656-1 |
Publication status | Published - 2008 |
Event | Frank N Bash Symposium on New Horizons Astronomy - Austin Duration: 14 Oct 2007 → 16 Oct 2007 |
Conference
Conference | Frank N Bash Symposium on New Horizons Astronomy |
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City | Austin |
Period | 14/10/07 → 16/10/07 |
Keywords / Materials (for Non-textual outputs)
- HIGH-REDSHIFT GALAXIES
- NEARBY