Zobrazeno 1 - 10
of 256
pro vyhledávání: '"Yuan, F. T."'
Autor:
Yuan, F. -T., Argudo-Fernandez, M., Shen, S., Hao, L., Jiang, C., Yin, J., Boquien, M., Lin, L.
Publikováno v:
A&A 613, A13 (2018)
We investigate the star formation history and the dust attenuation in the galaxy merger Mrk848. Thanks to the multiwavelength photometry from the ultraviolet (UV) to the infrared (IR), and MaNGA's integral field spectroscopy, we are able to study thi
Externí odkaz:
http://arxiv.org/abs/1801.04860
Autor:
Yuan, F. -T., Buat, V., Burgarella, D., Ciesla, L., Heinis, S., Shen, S., Shao, Z., Hou, J. -L.
We use the Herschel SPIRE color-color diagram to study the spectral energy distribution (SED) and the redshift estimation of high-z galaxies. We compiled a sample of 57 galaxies with spectroscopically confirmed redshifts and SPIRE detections in all t
Externí odkaz:
http://arxiv.org/abs/1506.07397
Publikováno v:
2012A&A...548A.117Y
Merger processes play an important role in galaxy formation and evolution. To study the influence of merger processes on the evolution of dust properties and cosmic star formation rate, we investigate a local sample of major merger galaxies and a con
Externí odkaz:
http://arxiv.org/abs/1212.1956
An accurate estimation of the star formation-related properties of galaxies is crucial for understanding the evolution of galaxies. In galaxies, ultraviolet (UV) light emitted by recently formed massive stars is attenuated by dust, which is also prod
Externí odkaz:
http://arxiv.org/abs/1209.5844
We present the results of the near-infrared (IR) spectroscopy of nine IRAS galaxies (NGC 1266, NGC 1320, NGC 2633, NGC 2903, NGC 3034, Mrk 33, NGC 7331, NGC 7625, NGC 7714) with the ISLE imager and spectrograph mounted on the Okayama Astrophysical Ob
Externí odkaz:
http://arxiv.org/abs/1111.4522
Autor:
Yuan, F. -T., Takeuchi, T. T., Buat, V., Heinis, S., Giovannoli, E., Murata, K. L., Iglesias-Paramo, J., Burgarella, D.
AKARI/Infrared Camera (IRC) Point Source Catalog provides a large amount of flux data at {\it S9W} ($9\ {\rm \mu m}$) and {\it L18W} ($18\ {\rm \mu m}$) bands. With the goal of constructing Star-Formation Rate(SFR) calculations using IRC data, we ana
Externí odkaz:
http://arxiv.org/abs/1111.3814
Autor:
Buat, V., Giovannoli, E., Takeuchi, T. T., Heinis, S., Yuan, F. T., Burgarella, D., Noll, S., Iglesias-Paramo, J.
The nearby universe remains the best laboratory to understand physical properties of galaxies and is a reference for any comparison with high redshift observations. The all sky (or very large) surveys performed from the ultraviolet (UV) to the far-in
Externí odkaz:
http://arxiv.org/abs/1102.1571
Autor:
Takeuchi, T. T., Buat, V., Heinis, S., Giovannoli, E., Yuan, F. -T., Iglesias-Paramo, J., Murata, K. L., Burgarella, D.
The AKARI All-Sky Survey provided the first bright point source catalog detected at 90um. Starting from this catalog, we selected galaxies by matching AKARI sources with those in the IRAS PSCz. Next, we have measured total GALEX FUV and NUV flux dens
Externí odkaz:
http://arxiv.org/abs/0912.5051
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Akademický článek
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