Living fossils: A detailed view of distant Lyman break galaxies using ...

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Stellar masses Properties of UVLGs Specific star formation rate Berkeley - 5 Feb 2008 Roderik Overzier - Local LBG Analogs
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Page 1 and 2: Roderik Overzier (MPA) Tim Heckman
Page 3 and 4: Berkeley - 5 Feb 2008 Roderik Overz
Page 5 and 6: Are AGN (black hole growth) the res
Page 7 and 8: Lyman break galaxies: The typical g
Page 9 and 10: Important links between local galax
Page 11 and 12: How to interpret LBG kinematics and
Page 13 and 14: Strong Correlation between SFR and
Page 15 and 16: Far-UV Surface Brightness (L FUV /2
Page 17: SDSS Spectra indicate typical starb
Page 21 and 22: HST imaging program Cycles 15 & 16
Page 23 and 24: UVLG morphologies II Berkeley - 5 F
Page 25 and 26: UVLG morphologies IV Berkeley - 5 F
Page 27 and 28: Quantifying the Morphologies Low re
Page 29 and 30: Morphologies of star forming galaxi
Page 31 and 32: UDF depth COSMOS depth Berkeley - 5
Page 33 and 34: Collisional starbursts have been su
Page 35 and 36: Is there any evidence to suggest th
Page 37 and 38: Far-UV Surface Brightness (L FUV /2
Page 39 and 40: Faint-end slope of UV LF: but An in
Page 41: Summary • the GALEX/SDSS sample o

Living fossils: A detailed view of distant Lyman break galaxies using ...

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