[PDF] Top 20 Luminosity functions of local infrared galaxies with AKARI : implications for the cosmic star formation history and AGN evolution

... bolometric infrared luminosities (L TIR,8−1000 µm ) of local galaxies have been estimated using a sim- ple polynomial presented by P´erault (1987), obtained assuming a simple blackbody ... See full document

... massive galaxies experience one or more phases of nuclear activity ...scenario of close connection between AGNs and their ...mass and galaxy bulge properties (stellar mass, velocity ... See full document

... investigated the X-ray emission from 2568 normal late-type galaxies over the redshift range z = 0 Y ...within the Chandra Deep Fields ...color and abso- lute V-band magnitudes, to ... See full document

... thank the anonymous referee for a helpful report which improved the ...Smith for allow- ing the pre-publication use of the H-ATLAS ...from the endowment of ... See full document

... period for lifespan determination Experiments where the IIS pathway was manipulated at different time points in life, both in ...2002) and Drosophila (Giannakou et al., 2007), have shown that in ... See full document

... XLFs for normal /starburst galaxies in GOODS for sources with X-ray counterparts, and fit the XLFs with linear models using ‘‘traditional’’ techniques, as well as Markov- ... See full document

... in the SFRs of AGN hosts depending on the type/luminosity of the AGNs in their samples and/or selection ...between the masses of their AGN ... See full document

... explanation of AGN obscuration does not involve the presence of the dusty torus, but rather a parsec-scale ...scenario the torus is identified with the outer region ... See full document

... In the first SUSHIES sample paper, Leloudas et al. (2015c) dis- cussed the spectroscopic properties of 17 H-poor and 8 H-rich SLSN host ...that the host galaxies of H-poor ... See full document

... thank the anonymous referee for insight that has substantially improved the quality of this ...DJR and DMA acknowledge the support of the UK Science and ... See full document

... growth of supermassive black holes and their host galaxies are thought to be linked, but the precise nature of this symbiotic relationship is still poorly ...observations and ... See full document

... to the tidal bridge between two galax- ies. It is known that the interaction between galaxies and/or galaxy activity phenomena may enhance the rate of star ...consequence ... See full document

... when the argument of a variable IMF is considered to explain the [α/Fe]–stellar mass relation, the proposed IMF is treated as a free parameter (Arrigoni et ...varied with exploratory ... See full document

... that the absence of type 1 AGN in these sam- ples of isolated galaxies is ...1.0 AGN among the 175 active galaxies in our sam- ples. The fraction of ... See full document

... pathological history, no language, intellectual or cultural barriers that could affect ...communication. The patient went to emergency service due to a two- week history of acute abdominal ... See full document

... studies of the relationship between host star- formation and AGN activity are an essential test of the de- gree and importance of galaxy-SMBH ... See full document

... explore the detailed physics behind these remarkable properties, Marconi et ...time- and metal- dependent convective hydrodynamic models to derive a theoretical calibration for the period – ... See full document

... reveals the knee for both populations. This fact allows us to compare the level of [ X / Fe ] in stars from each population formed before and after the main contribution ... See full document

... identification of lines for determining the redshifts was done independently from two methods by three of the ...authors. The 2D spectrum was visually scanned to search ... See full document

... ent formation processes at different epochs might have shaped the dwarf galaxy evolution (Lisker 2009), the transformation of low-luminosity star forming systems into ... See full document