Results 51 to 60 of about 4,303,458 (400)

Multiple-Collision Free-Electron Laser Compton Backscattering for a High-Yield Gamma-Ray Source

open access: yesApplied Sciences, 2020
We observed multiple-collision free-electron laser (FEL)-Compton backscattering in which a multi-bunch electron beam makes head-on collisions with multi-pulse FELs in an optical cavity, using an infrared FEL system in the storage ring NIJI-IV.
Norihiro Sei, Hiroshi Ogawa, QiKa Jia
doaj   +1 more source

Infrared Dichroism from the X-Ray Structure of Bacteriorhodopsin [PDF]

open access: yesBiophysical Journal, 2001
A detailed comparison with the three-dimensional protein structure provides a stringent test of the models and parameters commonly used in determining the orientation of the alpha-helices from the linear dichroism of the infrared amide bands, particularly in membranes.
Marsh, D., Pali, T.
openaire   +4 more sources

Mid-infrared variability of γ-ray emitting blazars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Using data from the Wide-field Infrared Survey Explorer, we studied the mid-infrared (mid-IR) 3.4 μm (W1-band) and 4.6 μm (W2-band) flux variability of γ-ray emitting blazars. Our sample consists of 460 flat spectrum radio quasars (FSRQs) and 575 BL Lacertae (BL Lac) objects.
Ayesha Anjum   +4 more
openaire   +2 more sources

Cosmogenic Neutrinos from Cosmic Ray Interactions with Extragalactic Infrared Photons [PDF]

open access: yesPhys.Rev.D73:043003,2006, 2005
We discuss the production of cosmogenic neutrinos on extragalactic infrared photons in a model of its cosmological evolution. The relative importance of these infrared photons as a target for proton interactions is significant, especially in the case of steep injection spectra of the ultrahigh energy cosmic rays.
arxiv   +1 more source

Reliability of Non-Contact Infrared Thermometers for Fever Screening Under COVID-19

open access: yesRisk Management and Healthcare Policy, 2022
Fan Lai,1,* Xin Li,1,* Qi Wang,1,* Yingjuan Luo,1 Xin Wang,1 Xiuhua Huang,1 Jiajia Zhang,1 Jieru Peng,1 Qin Wang,1 Li Fan,1 Wen Li,1 Junrong Huo,1 Tianjiao Liu,1 Yalan Li,2 Yonghong Lin,1 Xiao Yang1 1Chengdu Women’s and Children’s Central ...
Lai F   +15 more
doaj  

Impact of Low-Energy Cosmic Rays on Star Formation [PDF]

open access: yes, 2020
In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays ( < 1  
M. Padovani   +9 more
semanticscholar   +1 more source

THE INFRARED ARRAY CAMERA DARK FIELD: FAR-INFRARED TO X-RAY DATA [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2009
12 pages, ApJS ...
Krick, J. E.   +9 more
openaire   +5 more sources

Luminous infrared galaxies as plausible gamma-ray sources for GLAST and IACTs [PDF]

open access: yesAstrophys.J. 607 (2004) L99-L102, 2004
We argue that luminous infrared galaxies (LIGs) may constitute a newly detectable population of gamma-ray sources for the next generation of ground and space-based high energy telescopes. Additionally, we report for the first time upper limits on their fluxes using data obtained with the EGRET telescope.
arxiv   +1 more source

Simultaneous X-Ray and Infrared Observations of Sagittarius A*'s Variability [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract Emission from Sagittarius A* is highly variable at both X-ray and infrared (IR) wavelengths. Observations over the last ∼20 yr have revealed X-ray flares that rise above a quiescent thermal background about once per day, while faint X-ray flares from Sgr A* are undetectable below the constant thermal emission.
Daryl Haggard   +15 more
openaire   +9 more sources

Breaking the Radio - Gamma-Ray Connection in Arp 220 [PDF]

open access: yes, 2019
Recent analyses of the gamma-ray spectrum from the ultra-luminous infrared galaxy Arp 220 have revealed a discrepancy in the cosmic ray energy injection rates derived from the gamma-rays versus the radio emission. While the observed radio emission is consistent with the star formation rate inferred from infrared observations, a significantly higher ...
arxiv   +1 more source

Home - About - Disclaimer - Privacy