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| Document Title | Author Full Name | Author Short Name | Index | Corresponding | Address | ResearcherID | ResearcherID Author Name | ORCID | ORCID Author Name | Related Email |
|---|---|---|---|---|---|---|---|---|---|---|
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Ho, Luis C. | Ho, LC | 5 | Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China | mkim.astro@gmail.com; | |||||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Hwang, Ho Seong | Hwang, HS | 6 | Seoul Natl Univ, Dept Phys & Astron, 1 Gwanak Ro, Seoul 08826, South Korea | AAS-6010-2020 | HWANG, Ho | mkim.astro@gmail.com; | |||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Hwang, Ho Seong | Hwang, HS | 6 | Seoul Natl Univ, SNU Astron Res Ctr, Seoul 08826, South Korea | AAS-6010-2020 | HWANG, Ho | mkim.astro@gmail.com; | |||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Hwang, Ho Seong | Hwang, HS | 6 | Macquarie Univ, Australian Astron Opt, 105 Delhi Rd, N Ryde, NSW 2113, Australia | AAS-6010-2020 | HWANG, Ho | mkim.astro@gmail.com; | |||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Song, Hyunmi | Song, H | 7 | Chungnam Natl Univ, Dept Astron & Space Sci, Daejeon 34134, South Korea | mkim.astro@gmail.com; | |||||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Kim, Dohyeong | Kim, D | 8 | Pusan Natl Univ, Dept Earth Sci, Busan 46241, South Korea | 0000-0002-6925-4821 | Kim, Dohyeong | mkim.astro@gmail.com; | |||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Yang, Yujin | Yang, Y | 9 | Korea Astron & Space Sci Inst, Daejeon 34055, South Korea | mkim.astro@gmail.com; | |||||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Yang, Yujin | Yang, Y | 9 | Univ Sci & Technol, Daejeon 34113, South Korea | mkim.astro@gmail.com; | |||||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Jeong, Woong-Seob | Jeong, WS | 10 | Korea Astron & Space Sci Inst, Daejeon 34055, South Korea | 0000-0002-2770-808X | Jeong, Woong-Seob | mkim.astro@gmail.com; | |||
| Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models | Jeong, Woong-Seob | Jeong, WS | 10 | Univ Sci & Technol, Daejeon 34113, South Korea | 0000-0002-2770-808X | Jeong, Woong-Seob | mkim.astro@gmail.com; | |||
| Resource Allocation in Quantum-Key-Distribution Optical Data Center Networks | Chen, Bowen | Chen, BW | 1 | 교신저자 | Soochow Univ, Sch Elect & Informat Engn, Suzhou 215006, Peoples R China | bwchen@suda.edu.cn; | ||||
| Resource Allocation in Quantum-Key-Distribution Optical Data Center Networks | Ma, Weike | Ma, WK | 2 | Soochow Univ, Sch Elect & Informat Engn, Suzhou 215006, Peoples R China | bwchen@suda.edu.cn; | |||||
| Resource Allocation in Quantum-Key-Distribution Optical Data Center Networks | He, Bin | He, B | 3 | Soochow Univ, Sch Elect & Informat Engn, Suzhou 215006, Peoples R China | bwchen@suda.edu.cn; | |||||
| Resource Allocation in Quantum-Key-Distribution Optical Data Center Networks | Chen, Hong | Chen, H | 4 | Soochow Univ, Sch Elect & Informat Engn, Suzhou 215006, Peoples R China | bwchen@suda.edu.cn; | |||||
| Resource Allocation in Quantum-Key-Distribution Optical Data Center Networks | Jiang, Min | Jiang, M | 5 | Soochow Univ, Sch Elect & Informat Engn, Suzhou 215006, Peoples R China | bwchen@suda.edu.cn; |
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