2018
DOI: 10.48550/arxiv.1810.08197
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Science with an ngVLA: The ngVLA Reference Design

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
5

Relationship

0
5

Authors

Journals

citations
Cited by 6 publications
(1 citation statement)
references
References 0 publications
0
1
0
Order By: Relevance
“…In 2018, UWL, an ultra-wideband receiver covering 704-4032 MHz, was put into use in the Parkes Pulsar timing array project, and its timing accuracy was significantly improved (Hobbs et al 2020). The frequency coverage of a single radio telescope can range from centimeters to millimeters to meet the needs of extremely wide spectral-line observations, for example, the ngVLA project plans to cover the frequency range from 1.2 to 116 GHz by multiple UWB receivers (Selina et al 2018), with a maximum frequency ratio of 4:1 and a bandwidth of 36 GHz for a single receiver.…”
Section: Introductionmentioning
confidence: 99%
“…In 2018, UWL, an ultra-wideband receiver covering 704-4032 MHz, was put into use in the Parkes Pulsar timing array project, and its timing accuracy was significantly improved (Hobbs et al 2020). The frequency coverage of a single radio telescope can range from centimeters to millimeters to meet the needs of extremely wide spectral-line observations, for example, the ngVLA project plans to cover the frequency range from 1.2 to 116 GHz by multiple UWB receivers (Selina et al 2018), with a maximum frequency ratio of 4:1 and a bandwidth of 36 GHz for a single receiver.…”
Section: Introductionmentioning
confidence: 99%