A highly sensitive scanning far-infrared microscope with quantum Hall detectors

2003 ◽  
Vol 74 (9) ◽  
pp. 4209-4211 ◽  
Author(s):  
Kenji Ikushima ◽  
Hisato Sakuma ◽  
Susumu Komiyama
2003 ◽  
Vol 18 (1-3) ◽  
pp. 130-131 ◽  
Author(s):  
Kenji Ikushima ◽  
Hisato Sakuma ◽  
Susumu Komiyama

2001 ◽  
Vol 89 (7) ◽  
pp. 4037-4048 ◽  
Author(s):  
Y. Kawano ◽  
Y. Hisanaga ◽  
H. Takenouchi ◽  
S. Komiyama

2002 ◽  
Vol 81 (2) ◽  
pp. 382-384 ◽  
Author(s):  
N. G. Kalugin ◽  
G. Nachtwei ◽  
Yu. B. Vasilyev ◽  
S. D. Suchalkin ◽  
K. Eberl
Keyword(s):  

2002 ◽  
Vol 12 (1-4) ◽  
pp. 144-148 ◽  
Author(s):  
N.G Kalugin ◽  
Yu.B Vasilyev ◽  
S.D Suchalkin ◽  
G Nachtwei ◽  
B.E Sagol ◽  
...  

2002 ◽  
Vol 80 (1) ◽  
pp. 136-138 ◽  
Author(s):  
Y. Kawaguchi ◽  
K. Hirakawa ◽  
M. Saeki ◽  
K. Yamanaka ◽  
S. Komiyama

2002 ◽  
Vol 12 ◽  
pp. 489-492 ◽  
Author(s):  
G.R. Meurer ◽  
T.M. Heckman ◽  
M. Seibert ◽  
J. Goldader ◽  
D. Calzetti ◽  
...  

AbstractMany recent estimates of the star formation rate density at high redshift rely on rest-frame ultraviolet (UV) data. These are highly sensitive to dust absorption. Applying a correlation between the far-infrared (FIR) to UV flux ratio and UV color found in local starbursts to galaxy samples out toz∼ 3, one can account for most of the FIR background. However, the correlation is based on a sample that does not include the most extreme starbursts, Ultra Luminous Infrared Galaxies (ULIGs). Our new UV images of ULIGs show that their FIR fluxes are underpredicted by this correlation by factors ranging from 7 to 70. We discuss how ULIGs compare to the various types of high-zgalaxies: sub-mm sources, Lyman Break Galaxies, and Extremely Red Objects.


2001 ◽  
Vol 298 (1-4) ◽  
pp. 392-396 ◽  
Author(s):  
Y. Imanaka ◽  
T. Takamasu ◽  
G. Kido ◽  
G. Karczewski ◽  
T. Wojtowicz ◽  
...  

2010 ◽  
Vol 49 (3) ◽  
pp. 031201 ◽  
Author(s):  
Jeng-Chung Chen ◽  
Jingbin Zhang ◽  
Cheng-Chung Chi ◽  
Takeji Ueda ◽  
Susumu Komiyama

2014 ◽  
Vol 105 (18) ◽  
pp. 181103 ◽  
Author(s):  
Chiu-Chun Tang ◽  
D. C. Ling ◽  
C. C. Chi ◽  
Jeng-Chung Chen

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