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Published byElla Thøgersen Modified over 5 years ago
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OSIRIS Spectroscopy of Supercompact UV Luminous Galaxies
Thiago S. Gonçalves Caltech
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Caltech MPA, Garching Columbia JHU
Thiago S. Gonçalves Chris Martin Ted Wyder Roderik Overzier Columbia JHU Antara Basu-Zych David Schiminovich Matt O’Dowd Tim Heckman
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UVLGs: general characteristics
Heckman et al (2005), Hoopes et al. (2007) Detected by GALEX in the FUV with LFUV ≥ 2×1010 L, I1530 ≥ 109 L kpc-2 Low dust attenuation, young populations (Basu-Zych et al. 2007) Similar morphological indices to high- redshift LBGs
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Overzier et al
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UVLG0926 2hr exposures Pa-α emission line S/N map
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Velocity map σ map
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UVLG1434
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σ's similar to LBGs (Law et al. 2007)
Velocity map σ map σ's similar to LBGs (Law et al. 2007)
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Kinemetry (Krajnović et al, Shapiro et al)
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Summary Complementary data to understand UVLG dynamics: HST optical and IFU Opportunity to study Lyman Break analogs at higher S/N ratios and spatial resolution 4 more nights coming - so stay tuned!
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