scholarly journals Tunable Josephson junction far infrared source. Report No. 2151

1974 ◽  
Author(s):  
R.K. Elsley ◽  
A.J. Sievers
1983 ◽  
Vol 54 (12) ◽  
pp. 7078-7082 ◽  
Author(s):  
J‐C. Henaux ◽  
G. Vernet ◽  
R. Adde

1982 ◽  
Vol 258 ◽  
pp. 165 ◽  
Author(s):  
J. Fischer ◽  
R. R. Joyce ◽  
M. Simon ◽  
T. Simon

1979 ◽  
Vol 232 ◽  
pp. L183 ◽  
Author(s):  
B. McBreen ◽  
G. G. Fazio ◽  
M. Stier ◽  
E. L. Wright

1989 ◽  
Vol 120 ◽  
pp. 227-230
Author(s):  
C. Eiroa ◽  
M. Casali

ABSTRACT:Near-infrared images of the Serpens molecular cloud core have been carried out at UKIRT (Mauna Kea Observatory) using the infrared array camera, IRCAM. A large-scale diffuse nebulosity extending over the central part of the core is observed. Over 100 K-sources are detected in the 30 arc min2 cloud core. Some of them are PMS objects which were previously unknown. For the first time, a near-infrared counterpart of the far-infrared source Seroens FIRS1 has been detected. The 2.2 µm source appears as a point like object at the apex of an extended knotty, jet-like nebulosity oriented towards the northwest. In addition, a group of 11 stellar objects is seen in the position of the IR/radio source SVS4. These objects are embedded in a very faint nebulosity and form one of the densest clustering of young stars found in dark clouds.


2001 ◽  
Vol 204 ◽  
pp. 301-301
Author(s):  
H. Matsuhara ◽  
K. Kawara ◽  
Y. Sofue ◽  
Y. Taniguchi ◽  
Y. Sato ◽  
...  

We present the characteristics of far-infrared (FIR) brightness fluctuations at 90 μm and 170 μm in the Lockman Hole, which were surveyed with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO), and give constraints on the galaxy number counts down to 30 mJy at 90 μm and 50 mJy at 170 μm. The fluctuation power spectra of the FIR images are not dominated by IR cirrus, and are instead most likely due to star-forming galaxies. This analysis indicates the existence of strong evolution in the counts. Especially at 90 μm, the source density is much larger than that expected from the currently available galaxy count models. The galaxies responsible for the fluctuations also significantly contribute to the cosmic infrared background radiation recently derived from an analysis of the COBE data.


1979 ◽  
Vol 228 ◽  
pp. 439
Author(s):  
E. L. Wright ◽  
W. Decampli ◽  
G. G. Fazio ◽  
C. J. Lada ◽  
F. J. Low ◽  
...  
Keyword(s):  

1978 ◽  
Vol 221 ◽  
pp. L77 ◽  
Author(s):  
G. G. Fazio ◽  
C. J. Lada ◽  
D. E. Kleinmann ◽  
E. L. Wright ◽  
P. T. P. Ho ◽  
...  
Keyword(s):  

1975 ◽  
Vol 170 (1) ◽  
pp. 37P-38P ◽  
Author(s):  
G. J. White ◽  
L. T. Little ◽  
E. A. Parker ◽  
P. S. Nicholson ◽  
G. H. MacDonald ◽  
...  
Keyword(s):  

2000 ◽  
Vol 14 (25n27) ◽  
pp. 3104-3109 ◽  
Author(s):  
R. MIGLIORE ◽  
A. MESSINA ◽  
A. NAPOLI

We show that the quantum nature of a mesoscopic Josephson junction may be exploited for detecting low-intensity electromagnetic quantized fields. In particular we prove that intensity and phase of single-mode quantized coherent field may be reconstructed measuring amplitude and quantum noise of the first quantum Shapiro step occurring in the I-V characteristic of the ultrasmall Josephson junction.


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