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國立中央大學 首頁
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查看斯高帕斯 (Scopus) 概要
饒 兆聰
教授
天文研究所
https://orcid.org/0000-0001-8771-7554
電子郵件
cngeow
astro.ncu.edu
tw
網站
http://www.astro.ncu.edu.tw/people/faculty_bio.php?id=6
h-index
10747
引文
36
h-指數
按照存儲在普爾(Pure)的出版物數量及斯高帕斯(Scopus)引文計算。
2003
2025
每年研究成果
概覽
指紋
網路
研究計畫
(18)
研究成果
(176)
資料集
(35)
類似的個人檔案
(6)
指紋
查看啟用 Chow-Choong Ngeow 的研究主題。這些主題標籤來自此人的作品。共同形成了獨特的指紋。
排序方式
重量
按字母排序
Keyphrases
Luminosity
100%
Large Magellanic Cloud
56%
Light Curves
47%
Galaxies
33%
Galactic
33%
Classical Cepheids
30%
Palomar
30%
Color Relation
29%
Photometry
28%
Near-infrared
27%
RR Lyrae
26%
Metallicity
23%
Fundamental Mode
18%
Johannes Kepler
18%
Nonlinearity
16%
Multi-wavelength
16%
Pulsation
15%
Mid-infrared
15%
RR Lyrae Stars
14%
Synoptic Survey
14%
Galaxy Clusters
14%
Globular Clusters
13%
Observatory
13%
Small Magellanic Cloud
13%
Supernovae
13%
Hubble Constant
12%
Magellanic Clouds
12%
Distance Scale
11%
Cosmology
11%
Sunyaev-Zeldovich Effect
11%
Law
11%
Distance Modulus
10%
RR Lyrae Variables
10%
Mass Loss
9%
South Pole Telescope
9%
Spectral Energy Distribution
9%
Asteroids
8%
Ultra-long
8%
Line-of-sight Velocity
8%
Open Clusters
8%
Reddening
8%
Distance Measure
8%
X-ray
7%
Spiral Density Wave
7%
Variable Stars
7%
Infrared Observations
7%
Overtone
7%
Spectrograph
7%
Cepheid Distance
7%
Miras
7%
Physics
Transients
72%
Large Magellanic Cloud
70%
Light Curve
52%
RR Lyrae Variable Stars
39%
Photometry
35%
Cepheid Variable
35%
Metallicity
28%
Near Infrared
28%
Galaxy Clusters
18%
Small Magellanic Cloud
17%
Observatory
16%
Magellanic Clouds
15%
Hubble Constant
15%
Supernovae
14%
Globular Cluster
14%
Harmonics
13%
Gravitational Lensing
13%
X Ray
12%
Sky Surveys
11%
Variable Star
10%
Open Cluster
10%
Line of Sight
9%
Cepheid Distance
9%
Spectrographs
9%
Spectral Energy Distribution
9%
Physics
8%
Mira Variables
8%
Photosphere
8%
Neutron Star Mergers
8%
Hubble Space Telescope
8%
Stellar Pulsations
7%
Spiral Arms
7%
Radial-Velocity Method
6%
Field of View
6%
Neutron Stars
6%
Standard Candles
5%
Gravitational Wave
5%
James Webb Space Telescope
5%
Infrared Excess
5%