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Enabling Milliarcsecond Astrophysics: Open access for the CHARA Array

Enabling Milliarcsecond Astrophysics: Open access for the CHARA Array
启用毫角秒天体物理学:CHARA 阵列的开放访问
批准号:
1636624
负责人:
Theo ten Brummelaar
金额:
$390.23万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2016
资助国家:
美国
项目状态:
已结题
起止时间:
2016-09-01 至 2022-08-31

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英文摘要
This program will provide observing time to the astronomical community using the Georgia State University Center for High Angular Resolution Astronomy (CHARA), as well as open access to archival CHARA data. Broader impacts of the work involve training of undergraduate and graduate students in instrumentation development, including a focused research opportunity for Georgia State undergraduates to participate in CHARA research. This proposal will also help fund upgrades to the CHARA Exhibit Hall on Mt. Wilson, which illustrates interferometry to the general public via displays of historical equipment and explanations of how the current system works. CHARA operates an optical/near infrared (OIR) interferometric array on Mount Wilson, CA. The CHARA Array has six 1-m aperture telescopes in a Y configuration providing 15 baselines from 33 to 331 meters and ten independent closure phase triangles. With the number and size of its telescopes, its imaging capabilities, the length of its baselines, the range of wavelength regimes and spectral resolutions covered by its beam combiners, the CHARA Array is a uniquely powerful facility for milliarcsecond imaging. This proposal defines a path to move optical interferometry from a rather small and experimental group to a broader user community.
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DOI: 10.1051/0004-6361/202037832
发表时间: 2020-06
期刊: arXiv: Solar and Stellar Astrophysics
影响因子: --
作者: [A. Chiavassa;K. Kravchenko;F. Millour;G. Schaefer;M. Schultheis;B. Freytag;O. Creevey;V. Hocd'e]
通讯作者: A. Chiavassa;K. Kravchenko;F. Millour;G. Schaefer;M. Schultheis;B. Freytag;O. Creevey;V. Hocd'e
Inspecting the Cepheid parallax of pulsation using Gaia EDR3 parallaxes: Projection factor and period-luminosity and period-radius relations
使用 Gaia EDR3 视差检查造父变星脉动视差:投影因子以及周期-光度和周期-半径关系
DOI: 10.1051/0004-6361/202141680
发表时间: 2021
期刊: Astronomy & Astrophysics
影响因子: 6.5
作者: [Trahin, B., Breuval, L., Kervella, P., Mérand, A., Nardetto, N., Gallenne, A., Hocdé, V., Gieren, W.]
通讯作者: Gieren, W.
DOI: 10.3847/1538-3881/ac141a
发表时间: 2021-09-01
期刊: ASTRONOMICAL JOURNAL
影响因子: 5.3
作者: [Ellis, Tyler G., Boyajian, Tabetha, Farrington, Christopher D.]
通讯作者: Farrington, Christopher D.
DOI: 10.1093/mnras/stx2515
发表时间: 2018
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [F. Kirchschlager, S. Wolf, R. Brunngräber, A. Matter, A.V. Krivov, A. Labdon]
通讯作者: A. Labdon
60
    A Leap in Sensitivity for CHARA/CLASSIC Optical Interferometry for Astronomy
    Collaborative Research: Imaging planet-forming disks around young Suns using a revolutionary infrared detector
    MRI: Development of Adaptive Optics Upgrade for the CHARA Array - Phase II
    Adaptive Optics for the CHARA Array
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