[PDF] Top 20 Multi Wavelength Properties of Submillimeter Selected Galaxies

... 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

... Polystyrene latex spheres have a small (≤5 %) coefficient of variation in diameter and are often used as a proxy for monodisperse spherical aerosols. PSLs interact with light as predicted by Mie theory, and therefore ... See full document

... physical properties and astrophysics of these ...the properties of high-redshift ULIRGs relied on identi fi cations based on indirect tracers of the FIR / submilli- meter emission such as the radio, near-IR ... See full document

... MAMBO (Greve et al. 2004) and/or Bolocam (Laurent et al. 2005) detections at longer wavelengths, providing justification for a 3-parameter fit. In practice, however, such an approach is unlikely to yield robust ... See full document

... Polystyrene latex spheres have a small (≤5 %) coefficient of variation in diameter and are often used as a proxy for monodisperse spherical aerosols. PSLs interact with light as predicted by Mie theory, and therefore ... See full document

... these properties are similar to those of the ‘nor- mal’ star-forming galaxy population, signatures of tidal tails and asymmetric structures indicative of mergers are also more frequently found in SMGs or ... 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

... the galaxies that host Type Ia ...supernova properties and the physical properties of their host galaxies such as mass, metallicity, and star formation ...and multi-wavelength ... See full document

... wide wavelength range in this paper by analyzing a number of simulations (and different realizations of these simu- lations by varying the IMF and dust opacity curve, as we describe in §2), we defer a derivation of ... See full document

... collective multi-wavelength effort has enabled a steadily growing picture of the astrophysical details of SMGs ...astrophysical properties of the ensemble of SMGs, and also suggests a number of ... See full document

... massive galaxies, measur- ing their basic properties have been hampered by the coarse angular resolution of the single-dish telescopes, with beams of ∼ 15 00 ...bright submillimeter sources in the ... See full document

... infrared galaxies at high red- shift (z ∼1–6) with a nearly constant sensitivity in terms of dust mass or far-infrared luminosity (although the latter is sensitive to dust ...bright submillimeter sources ... See full document

... physical properties to low-redshift far-infrared-bright galaxies, emphasizing that these sources cannot be simply used as analogues to describe high-redshift ... See full document

... isolated galaxies with off- centre bars in our sample and other studies (Feitzinger 1980; Wilcots & Prescott 2004) is ...the galaxies being lopsided, the asymmetries in the dark matter halo could also ... See full document

... We combine our SMA compact and subcompact observations with single-dish data to achieve better recovery of structure at large spatial scales. For the dust continuum emis- sion, we use data from the Bolocam Galactic Plane ... See full document

... of wavelength more compactly in ...with wavelength for red galaxies indicates that they principally comprise one-component objects, ...elliptical galaxies, or two-component galaxies in ... See full document

... During her Masters degree studies, she spent one year at the Friedrich-Alexander University of Erlangen-Nuremberg, Erlangen, Germany, and was with the Fraunhofer Institute for Integrated Circuits, Erlangen. From 2002 to ... See full document

... particular wavelength, or en- ergy, will be absorbed by speci R c molecular struc- ...the wavelength of the S uorescent light emitted is always greater than the incident ... See full document

... For Lyα , we interpolate to our reference redshifts, using the results at z ∼ 0.3 from Cowie et al. (2010), 0.9 (Barger et al. 2012), ∼ 2.2 from Konno et al. (2016) and Sobral et al. (2017) and 3.1 and 3.7 from Ouchi et ... See full document

... local strong-AGN sources are the optically classified AGN-dominated galaxies and the local H ii + mild-AGN sources are star-forming-dominated galaxies with possible mild AGN contribution (Y13). The first ... See full document