Results 41 to 50 of about 402,790 (249)

Mapping Hsp104 interactions using cross‐linking mass spectrometry

open access: yesFEBS Open Bio, EarlyView.
This study examines how cross‐linking mass spectrometry can be utilized to analyze ATP‐induced conformational changes in Hsp104 and its interactions with substrates. We developed an analytical pipeline to distinguish between intra‐ and inter‐subunit contacts within the hexameric homo‐oligomer and discovered contacts between Hsp104 and a selected ...
Kinga Westphal   +3 more
wiley   +1 more source

Total infrared luminosity estimation from local galaxies in AKARI all sky survey [PDF]

open access: yesA&A 592, A155 (2016), 2016
We aim to use the a new and improved version of AKARI all sky survey catalogue of far-infrared sources to recalibrate the formula to derive the total infrared luminosity. We cross-match the faint source catalogue (FSC) of IRAS with the new AKARI-FIS and obtained a sample of 2430 objects. Then we calculate the total infrared (TIR) luminosity $L_{\textrm{
arxiv   +1 more source

Dust covering factor, silicate emission and star formation in luminous QSOs [PDF]

open access: yes, 2007
We present Spitzer IRS low resolution, mid-IR spectra of a sample of 25 high luminosity QSOs at 2
arxiv   +1 more source

Ammonia and CO observations toward low-luminosity 6.7-GHz methanol masers [PDF]

open access: yesarXiv, 2010
To investigate whether distinctions exist between low and high-luminosity Class II 6.7-GHz methanol masers, we have undertaken multi-line mapping observations of various molecular lines, including the NH3(1,1), (2,2), (3,3), (4,4) and 12CO(1-0) transitions, towards a sample of 9 low-luminosity 6.7-GHz masers, and 12CO (1-0) observations towards a ...
arxiv  

A quick estimation of luminosity function based on the luminosity-distance diagram [PDF]

open access: yesarXiv, 2017
Based on the luminosity-distance diagram, we propose a method to quickly estimate the luminosity function for any certain astrophysical objects. Giving the mean distance between any two objects at a given luminosity range, we can find the relation between the mean distance and the luminosity, and consequently can obtain the luminosity function.
arxiv  

The Local [CII] 158 um Emission Line Luminosity Function [PDF]

open access: yes, 2016
We present, for the first time, the local [CII] 158 um emission line luminosity function measured using a sample of more than 500 galaxies from the Revised Bright Galaxy Sample (RBGS). [CII] luminosities are measured from the Herschel PACS observations of the Luminous Infrared Galaxies in the Great Observatories All-sky LIRG Survey (GOALS) and ...
arxiv   +1 more source

Comment on "Biases in the Quasar Mass-Luminosity Plane" [PDF]

open access: yesarXiv, 2010
Comment on "Biases in the Quasar Mass-Luminosity Plane"
arxiv  

Measurement of the Luminosity in the ZEUS Experiment at HERA II

open access: yes, 2013
The luminosity in the ZEUS detector was measured using photons from electron bremsstrahlung. In 2001 the HERA collider was upgraded for operation at higher luminosity.
Adamczyk, L.   +36 more
core   +1 more source

AAPM Medical Physics Practice Guideline MPPG 17.a: Quality management for mammography review workstation displays

open access: yesJournal of Applied Clinical Medical Physics, EarlyView.
Abstract The Mammography Quality Standards Act (MQSA) sets quality standards for displays used to interpret mammography images. With the shift to digital mammography and the widespread use of remote reading workstations (RWS), updated quality management (QM) programs are needed to ensure consistent image presentation and accurate interpretation.
Rebecca Milman   +12 more
wiley   +1 more source

Infrared Classification and Luminosities For Dusty AGN and the Most Luminous Quasars [PDF]

open access: yes, 2012
Mid-infrared spectroscopic measurements from the Infrared Spectrometer on Spitzer (IRS) are given for 125 hard X-ray AGN (14-195 keV) from the Swift Burst Alert Telescope sample and for 32 AGN with black hole masses from reverberation mapping. The 9.7 um silicate feature in emission or absorption defines an infrared AGN classification describing ...
arxiv   +1 more source

Home - About - Disclaimer - Privacy