[PDF] Top 20 An Evolutionary Model for Submillimeter Galaxies

... High-resolution imaging of local ULIRGs has revealed the complex morphologies of these systems (Soifer et al. 2000, Goldader et al. 2002, Scoville et al. 2000), indicat- ing a merger-driven origin. This scenario is ... See full document

... estimates for H-ATLAS galaxies at similar redshifts. On the other hand, the amplitude of the cross-correlation is found to be a factor 1.62 ± 0.16 higher than expected from the standard model and also found ... See full document

... six submillimeter sources, which include a to- tal of 14 SMGs, to determine that & 75% of blends of multiple SMGs are not physically ...single-dish submillimeter sources is consis- tent with ... See full document

... our galaxies on the ...disk galaxies, they report bar radii of ∼1-10 kpc, which would put these high-redshift “bars” on the extreme short ...disk galaxies. This may be due to the gas content of the ... See full document

... servation, we find a redshift of z = 2.093. Our value is consis- tent with the CO(3–2) observation by Riechers et al. (in prep.), and we have adopted this value. SMA observation of the 880 µm dust continuum shows two ... See full document

... At high resolution, significant progress with the character- ization of the high-redshift ISM has been achieved through the observation of gravitationally lensed sources, as part of surveys conducted by the South Pole ... See full document

... and model the lensing for each transition indi- vidually, so even if we had attained detections for several galaxies individually we would be unable to determine the differential magnification on a case by ... See full document

... The collecting area and sensitivity of the Atacama Large Millimeter Array ( ALMA ) is transforming our view of the star- forming ISM in distant galaxies. While high-resolution studies of the dust continuum ... See full document

... As well as stacking the spectra, we can also create a rest-frame broad-band SED for a “typical” SMG (or at least “typical” of the brighter/bluer examples for which redshifts can be measured). Simpson et al. (2014) and ... See full document

... of galaxies in EAGLE is approximately correct, as shown by ...of galaxies in the post-starburst region is simply due to the smaller volume, and we address this point ...star-forming galaxies, as well ... See full document

... 52 submillimeter galaxies ( SMGs ) , identi fi ed using ALMA 870 μ m continuum imaging in a pilot program to precisely locate bright SCUBA-2-selected submillimeter sources in the UKIDSS Ultra Deep ... See full document

... every model estimate must play a ...of model components is that of the observer, who must determine that based on the required level of filtering that the models should impose on one another (see Section ... See full document

... high-redshift galaxies, whose submillimeter flux densities suggest large bolometric luminosities ( ∼ 10 13 L ) mostly emitted in IR wavebands, when SEDs of local ULIRGs were used as ...these galaxies ... See full document

... the galaxies that have even higher 850 μ m fl uxes, in Figure 9, we also show the clustering measurements of bright SMGs from the ...sequence galaxies at z ~ 2 have a gas depletion timescale of ∼ ... See full document

... where the constraints from different line measurements overlap ( e.g., Kaufman et al. 1999, 2006; Pound & Wol fi re 2008 ) . It is important to note that the PDR models assume that all the measured fl uxes are being ... See full document

... of galaxies in extreme environments and determine cosmological parameters of the ...learning model. Eventually we will apply our deep learning model to future upcoming redshift surveys such as LSST ... See full document

... of galaxies (for example: size, structure, mass, star-formation history, metallicity, age of the stellar populations) as well as their dynamics, interactions and their distribution across the Universe at different ... See full document

... of coordination and unavailability of common platform or knowledge base in the same domain. Evolutionary study of sorting algorithm or sorting problem is foundation of futuristic knowledge base for sorting problem ... See full document

... (SPT) model can then be used to predict the galaxy density-galaxy density-intrinsic alignment (ggI) bispectrum to tree level (fourth order in the linear matter ... See full document

... The IRAC images have a much broader point-spread function ( PSF ) than the i ¢ and J images, so selecting sources using the 4.5 μ m  image is prone to blending and some galaxies may be missed which are distinct ... See full document