Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
The CHIME fast radio burst project: system overview
Abstract The Canadian Hydrogen Intensity Map** Experiment (CHIME) is a novel transit
radio telescope operating across the 400–800 MHz band. CHIME is composed of four 20 m× …
radio telescope operating across the 400–800 MHz band. CHIME is composed of four 20 m× …
[KÖNYV][B] Physics and evolution of supernova remnants
J Vink - 2020 - Springer
When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …
1995, one of the things that I missed was a good textbook covering the various aspects of …
The Tianlai dish pathfinder array: design, operation, and performance of a prototype transit radio interferometer
ABSTRACT The Tianlai Dish Pathfinder Array is a radio interferometer designed to test
techniques for 21 cm intensity map** in the post-reionization universe as a means for …
techniques for 21 cm intensity map** in the post-reionization universe as a means for …
Low-frequency radio absorption in Cassiopeia A
Context. Cassiopeia A is one of the best-studied supernova remnants. Its bright radio and X-
ray emission is due to shocked ejecta. Cas A is rather unique in that the unshocked ejecta …
ray emission is due to shocked ejecta. Cas A is rather unique in that the unshocked ejecta …
Free–free absorption parameters of Cassiopeia A from low-frequency interferometric observations
Context. Cassiopeia A is one of the most extensively studied supernova remnants (SNRs) in
our Galaxy. The analysis of its continuum spectrum through low-frequency observations …
our Galaxy. The analysis of its continuum spectrum through low-frequency observations …
Map** the spectral index of Cassiopeia A: evidence for flattening from radio to infrared
V Domček, J Vink… - Monthly Notices of …, 2021 - academic.oup.com
Synchrotron radiation from supernova remnants is caused by electrons accelerated through
diffusive shock acceleration (DSA). The standard DSA theory predicts an electron spectral …
diffusive shock acceleration (DSA). The standard DSA theory predicts an electron spectral …
FRB 190520B–An FRB in a young supernova remnant?
JI Katz - Monthly Notices of the Royal Astronomical Society …, 2022 - academic.oup.com
ABSTRACT FRB 190520B, a repeating FRB near-twin of FRB 121102, has a dispersion
measure excess over the intergalactic and Galactic contributions of about 900 pc cm− 3 …
measure excess over the intergalactic and Galactic contributions of about 900 pc cm− 3 …
Spectrum and location of ongoing extreme particle acceleration in Cassiopeia A
J Woo, K Mori, CJ Hailey, E Spira-Savett… - The Astrophysical …, 2025 - iopscience.iop.org
Young supernova remnants (SNRs) are believed to be the origin of energetic cosmic rays
(CRs) below the" knee" of their spectrum at∼ 3 PeV (10 15 eV). Nevertheless, the precise …
(CRs) below the" knee" of their spectrum at∼ 3 PeV (10 15 eV). Nevertheless, the precise …
The two most recent thermonuclear supernovae in the Local Group: radio constraints on their progenitors and evolution
Young supernova remnants (SNRs) provide a unique perspective on supernova (SN)
progenitors and connect the late evolution of SNe with the onset of the SNR phase. Here we …
progenitors and connect the late evolution of SNe with the onset of the SNR phase. Here we …