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Chapman Scott C.
Professor
Dalhousie University
,
Instrument Development Center
电子邮件
CS889300
dal
ca
网站
https://www.scopus.com/authid/detail.url?authorId=24447889300
h-index
h10-index
h5-index
34708
引用
103
H-指数
根据储存在 Pure 的刊物以及来自 Scopus 的引用文献数量计算
8760
引用
52
H-指数
根据储存在 Pure 的刊物以及来自 Scopus 的引用文献数量计算
1581
引用
24
H-指数
根据储存在 Pure 的刊物以及来自 Scopus 的引用文献数量计算
1996 …
2023
每年的科研成果
综述
指纹
网络
科研成果
(478)
新闻 / 媒体
(4)
相似简介
(6)
指纹
深入其中 Chapman Scott C. 为活跃的研究主题。这些主题标签来自此人的成果。它们共同形成唯一的指纹。
分类
加权
按字母排序
Physics
Active Galactic Nuclei
61%
Adaptive Optics
21%
Andromeda Galaxy
15%
Antenna
12%
Bolometer
51%
Cosmic Microwave Background
37%
Dark Matter
23%
Dwarf Galaxy
25%
Dwarf Spheroidal Galaxies
19%
Early Universe
11%
Elliptical Galaxy
10%
Field of View
12%
Flux Density
52%
Galactic Evolution
16%
Galaxy Clusters
23%
Galaxy Evolution
19%
Globular Cluster
20%
Gravitational Lensing
17%
Gravitational Wave
10%
High Resolution
32%
High-Redshift Galaxy
15%
Hubble Space Telescope
24%
Interstellar Matter
23%
Luminosity Function
19%
Luminous Infrared Galaxies
24%
Lyman-Break Galaxies
21%
Metallicity
31%
Milky Way
17%
Molecular Gas
40%
Near Infrared
43%
Photometry
21%
Point Source
15%
Protoclusters
14%
Quasar
16%
Radio Galaxy
11%
Radio Sources
14%
Red Giant Branch
13%
Redshift Surveys
25%
Signal-to-Noise Ratio
14%
Space Infrared Telescope Facility
19%
Spectral Energy Distribution
45%
Spectrographs
37%
Stacking
21%
Star Formation
100%
Star Formation Rate
78%
Starburst Galaxy
15%
Stellar Mass
47%
Triangulum Galaxy
19%
Ultraluminous Infrared Galaxies
31%
Very Large Array
17%
Keyphrases
Active Galactic nuclei
13%
Andromeda
8%
Atacama
12%
Bolometer Arrays
7%
Common Users
7%
Cosmology
12%
Deep Fields
22%
Dust
11%
Dust Temperature
6%
Dwarf Galaxies
7%
Extragalactic Surveys
7%
Fainting
13%
Far-infrared
16%
Flux Density
6%
Galaxies
75%
Halo
11%
Herschel
10%
High-redshift
23%
High-resolution
8%
Hubble
6%
Interstellar Medium
7%
Keck
7%
Lensing
19%
Luminosity
20%
Massive Galaxies
7%
Metallicity
7%
Mid-infrared
8%
Milky Way
6%
Millimeter Wave
6%
Millimeter-submillimeter
10%
Molecular Gas
12%
Multi-wavelength
8%
Number Counts
6%
Protoclusters
7%
Radio
21%
SCUBA
12%
SCUBA-2
22%
South Pole Telescope
11%
Star Formation
17%
Star Formation Rate
16%
Star-forming
6%
Star-forming Galaxies
22%
Starburst
8%
Starburst Galaxies
7%
Stellar Masses
10%
Sub-mm
7%
Submillimeter
55%
Submillimeter Array
12%
Submillimeter Galaxies
49%
Ultra-deep Well
7%