Nanyao Y. Lu

TL;DR: Excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500 μm is reported, and it is found that submillimetre galaxies are located in dark matter haloes with a minimum mass, Mmin, which corresponds to the most efficient mass scale for star formation in the Universe.

TL;DR: In this article, the authors analyzed three fields from the Herschel Multi-tiered Extragalactic Survey (HerMES) programme in all three SPIRE bands (250, 350 and 500 μm) and derived parametrized galaxy number count models to a depth of ∼2 mJy beam−1, approximately four times the depth of previous analyses at these wavelengths, using a probability of deflection [P(D)] approach for comparison to theoretical number count model.

TL;DR: The spectra reported here typify the integrated emission from the interstellar medium of the majority of star-forming galaxies and could thus be used to obtain redshifts of highly extincted galaxies up to z=3 with SIRTF.

TL;DR: In this paper, the far-infrared emission of the starburst and underlying disk from the SPIRE maps was derived, and spatially-resolved farinfrared colors for the wind and halo were derived in terms of dust mass, dust temperature and global physical conditions.

TL;DR: In this paper, the authors incorporated the newest ISO results on the mid-infrared spectral energy distribution (SED) of galaxies into models for the number counts and redshift distributions of MIR surveys.