95 citations · 275 across the 16 of their papers we have counts for
6 papers · 1 filter
The Evolution of the Visible and Hidden Star Formation in the Universe: Implication from the Luminosity Functions at FUV and FIR
Tsutomu T. Takeuchi, Veronique Buat, Denis Burgarella
Based on GALEX and IRAS/Spitzer datasets, we have found that both FUV and FIR luminosity functions (LFs) show a strong evolution from z=0 to z=1, but the FIR LF evolves much strong…
The Local Universe as Seen in Far-Infrared and in Far-Ultraviolet: A Global Point of View on the Local Recent Star Formation
V. Buat, T. T. Takeuchi, J. Iglesias-Paramo +23
We select far-infrared (FIR-60 microns) and far-ultraviolet (FUV-1530 A) samples of nearby galaxies in order to discuss the biases encountered by monochromatic surveys (FIR or FUV)…
Effects of dust scattering albedo and 2175 A bump on ultraviolet colours of normal disc galaxies
Akio K. Inoue, Veronique Buat, Denis Burgarella +3
We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a radiative transfer mo…
Search for high column density systems with gamma ray bursts
Hiroyuki Hirashita, Hiroshi Shibai, Tsutomu T. Takeuchi
We investigate the possibility to search for metal-poor high column density (> 10^{23} cm^{-2}) clouds at high redshift (z) by using gamma ray burst (GRB) afterglows. Such clouds c…
A Dust Emission Model for Very Young Galaxies: Expected Properties and Far Infrared Diagnostics
Tsutomu T. Takeuchi
Dust plays crucial roles in galaxy formation and evolution. In the early epoch of galaxy evolution dust is only supplied by supernovae (SNe). With the aid of a new physical model o…
Ultraviolet-to-Far Infrared Properties of Lyman Break Galaxies and Luminous Infrared Galaxies at z ~ 1
D. Burgarella, P. G. Perez-Gonzalez, K. D. Tyler +13
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected us…