outline of talk
DESCRIPTION
Identifying and Classifying the Galaxies of the High Redshift Cluster 2192 Patricia Mutunga (with Fana Mulu) Advisors: Eric Wilcots Marc Verheijen. Outline of talk. Introduction Motivation The project Conclusion Acknowledgement. Motivation. - PowerPoint PPT PresentationTRANSCRIPT
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Identifying and Classifying the Galaxies of the High Redshift Cluster 2192
Patricia Mutunga (with Fana Mulu) Advisors: Eric Wilcots Marc Verheijen
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Outline of talk
•Introduction•Motivation•The project•Conclusion•Acknowledgement
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Motivation
Eric Wilcots - NSBP-students conferenceMarc and Eric - mini lecturesQuestions :How do galaxies form? Do clusters form from field galaxies? Have they evolved significantly since their formation? Is their morphological type an indication of their age?
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Introduction
This project entails the search for, and study of, galaxies in the rich cluster of galaxies Abell 2192 at very large distances ( i.e. at High Redshift).
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Abell 2192
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FLOW CHART FOR DATA PROCESSING
SExtractor
Separate stars & galaxies
GIPSY/copy
CCD mosaic image of Abell 2192
221 “postagestamp” images
Basic sample of 221 galaxies
Remove stars & other galaxies
GIPSY/blot
Geometric parameters
Master Table!
Photometric parameters
Morphologies
GIPSY/ellint
External knowledge
GIP
SY
/ellf
it
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The Project•CCD mosaic image of Abell 2192 - courtesy of Marc
•Executed SExtractor
•To separate the stars and galaxies
•Basic sample of 221 galaxies
•copy feature in GIPSY to make “postage stamp” images
•Blot feature in GIPSY to remove tars and other galaxies
•GIPSY and ellfit fitted in ellipses onto the galaxies to get
geometric parameters
•GIPSY and Ellint to get photometric parameters
•External knowledge-atlases and text books: morphologies
•All the steps led to The Master Table!
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GIPSY
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Ellint
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Examples
LP in R band LP in B band
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Geometric Parameters and Photometric parameters
• GIPSY and ellfit fitted in ellipses onto the galaxies to get geometric parameters• GIPSY and Ellint to get photometric parameters• External knowledge-atlases and text books: morphologies• All the steps led to The Master Table!
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Luminosity Profiles
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Luminosity Profiles
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Magnitude and Colour graph
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Radio detection
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Conclusions
•Our objective was reached.
•I learned a lot!
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Acknowledgements
•Thank God
•Thank Eric and Marc
•Fana too!
•All the REU students!
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copy feature in GIPSY to make “postage stamp” imagesBlot feature in GIPSY to remove tars and other galaxiesGIPSY and ellfit fitted in ellipses onto the galaxies to get geometric parametersGIPSY and Ellint to get photometric parametersExternal knowledge-atlases and text books: morphologiesAll the steps led to The Master Table!
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