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Multi-Wavelength SEDs of Herschel Selected Galaxies in the COSMOS Field
Nicholas Lee, D. B. Sanders, Caitlin M. Casey +14
We combine Herschel PACS and SPIRE maps of the full 2 deg^2 COSMOS field with existing multi-wavelength data to obtain template and model-independent optical-to-far-infrared spectr…
The role of galaxy interaction in the SFR-M relation: characterizing morphological properties of Herschel-selected galaxies at 0.2<z<1.5
Chao-Ling Hung, David B. Sanders, Caitlin M. Casey +13
Galaxy interactions/mergers have been shown to dominate the population of IR luminous galaxies (log(LIR)>11.6Lsun) in the local Universe (z<0.25). Recent studies based on the relat…
Resolved Giant Molecular Clouds in Nearby Spiral Galaxies: Insights from the CANON CO (1-0) Survey
Jennifer Donovan Meyer, Jin Koda, Rieko Momose +9
We resolve 182 individual giant molecular clouds (GMCs) larger than 2.5 10 \Msun in the inner disks of five large nearby spiral galaxies (NGC 2403, NGC 3031, NGC 473…
The Galactic Center Cloud G2 -- a Young Low-Mass Star with a Stellar Wind
Nick Scoville, Andi Burkert
We explore the possibility that the G2 gas cloud falling in towards \sgra is the mass loss envelope of a young TTauri star. As the star plunges to smaller radius at 1000 to 6000 \k…
Newly-quenched galaxies as the cause for the apparent evolution in average size of the population
C. M. Carollo, T. J. Bschorr, A. Renzini +10
Abridged. We use COSMOS to study in a self-consistent way the change in the number densities of quenched early-type galaxies (Q-ETGs) of a given size over the interval 0.2 < z < 1.…
Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
O. Ilbert, H. J. McCracken, O. Le Fevre +33
We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.2<z<4. We construct a deep K<24 sample of 220000 galaxies selec…