HAWC: a far-infrared camera for SOFIA

Author(s):  
Doyal A. Harper ◽  
Christine A. Allen ◽  
Michael J. Amato ◽  
Troy J. Ames ◽  
Arlin E. Bartels ◽  
...  
Keyword(s):  
2015 ◽  
Vol 48 (8) ◽  
pp. 659-672 ◽  
Author(s):  
Yu Kwonkyu ◽  
◽  
Kim Seojun ◽  
Yoo Byeongnam ◽  
Bae Inhyuk

2004 ◽  
Author(s):  
Doyal A. Harper ◽  
Arlin E. Bartels ◽  
Sean C. Casey ◽  
David T. Chuss ◽  
Jessie L. Dotson ◽  
...  
Keyword(s):  

Author(s):  
Satoru Yokoi ◽  
Jun Takahashi ◽  
Shigetoshi Tokita

1998 ◽  
Author(s):  
Doyal A. Harper ◽  
Samuel H. Moseley, Jr. ◽  
Ian Gatley ◽  
Sean C. Casey ◽  
Rhodri Evans ◽  
...  
Keyword(s):  

Author(s):  
Chaitra Hegde ◽  
Zifan Jiang ◽  
Pradyumna Byappanahalli Suresha ◽  
Jacob Zelko ◽  
Salman Seyedi ◽  
...  

AbstractWith the recent COVID-19 pandemic, healthcare systems all over the world are struggling to manage the massive increase in emergency department (ED) visits. This has put an enormous demand on medical professionals. Increased wait times in the ED increases the risk of infection transmission. In this work we present an open-source, low cost, off-body system to assist in the automatic triage of patients in the ED based on widely available hardware. The system initially focuses on two symptoms of the infection fever and cyanosis. The use of visible and far-infrared cameras allows for rapid assessment at a 1m distance, thus reducing the load on medical staff and lowering the risk of spreading the infection within hospitals. Its utility can be extended to a general clinical setting in non-emergency times as well to reduce wait time, channel the time and effort of healthcare professionals to more critical tasks and also prioritize severe cases.Our system consists of a Raspberry Pi 4, a Google Coral USB accelerator, a Raspberry Pi Camera v2 and a FLIR Lepton 3.5 Radiometry Long-Wave Infrared Camera with an associated IO module. Algorithms running in real-time detect the presence and body parts of individual(s) in view, and segments out the forehead and lip regions using PoseNet. The temperature of the forehead-eye area is estimated from the infrared camera image and cyanosis is assessed from the image of the lips in the visible spectrum. In our preliminary experiments, an accuracy of 97% was achieved for detecting fever and 77% for the detection of cyanosis, with a sensitivity of 91% and area under the receiver operating characteristic curve of 0.91. Heart rate and respiratory effort are also estimated from the visible camera.Although preliminary results are promising, we note that the entire system needs to be optimized before use and assessed for efficacy. The use of low-cost instrumentation will not produce temperature readings and identification of cyanosis that is acceptable in many situations. For this reason, we are releasing the full code stack and system design to allow others to rapidly iterate and improve the system. This may be of particular benefit in low-resource settings, and low-to-middle income countries in particular, which are just beginning to be affected by COVID-19.


2021 ◽  
Author(s):  
Laurence O'Rourke ◽  
Thomas G. Müller ◽  
Nicolas Biver ◽  
Dominique Bockelée-Morvan ◽  
Sunao Hasegawa ◽  
...  

<p>Previous research on Asteroids (24) Themis and (65) Cybele have shown the presence of an absorption feature at 3.1 μm reported to be directly linked to surface water ice. We searched for water vapor escaping from these asteroids with the Herschel Space Observatory HIFI (Heterodyne Instrument for the Far Infrared) Instrument. While no H<sub>2</sub>O line emission was detected, we obtained sensitive 3σ water production rate upper limits of Q(H<sub>2</sub>O)< 4.1×10<sup>26</sup> molecules s<sup>−1</sup> for Themis and Q(H<sub>2</sub>O) <7.6 × 10<sup>26</sup> molecules s<sup>−1</sup> for the case of Cybele. Using a thermophysical model, we merged data from the Subaru/Cooled Mid-Infrared Camera and Spectrometer and the Herschel SPIRE (Spectral and Photometric Imaging Receiver) instrument with the contents of a multi-observatory database and thus derived new radiometric properties for these two asteroids. For Themis, we obtained a thermal inertia G = 20 <sup>+25</sup><sub>-10</sub> J m<sup>−2</sup> s<sup>−1/2</sup> K<sup>−1</sup>, a diameter 192 <sup>+10</sup><sub>-7</sub> km, and a geometric V-band albedo p<sub>V</sub>=0.07±0.01. For Cybele, we found a thermal inertia G = 25<sup>+28</sup><sub>-19</sub> J m<sup>−2</sup> s<sup>−1/2</sup> K<sup>−1</sup>, a diameter 282±9 km, and an albedo pV=0.042±0.005. Using all inputs, we estimated that water ice intimately mixed with the asteroids’ dark surface material would cover <0.0017% (for Themis) and <0.0033% (for Cybele) of their surfaces, while an areal mixture with very clean ice (Bond albedo 0.8 for Themis and 0.7 for Cybele) would cover <2.2% (for Themis) and <1.5% (for Cybele) of their surfaces. Based on these very low percentage coverage values, it is clear that while surface (and subsurface) water ice may exist in small localized amounts on both asteroids, it is not the reason for the observed 3.1 μm absorption feature.</p>


1999 ◽  
Vol 511 (2) ◽  
pp. 761-773 ◽  
Author(s):  
H. M. Latvakoski ◽  
G. J. Stacey ◽  
G. E. Gull ◽  
T. L. Hayward

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