Astronomical imaging spectroscopy at far-infrared wavelengths

远红外波长的天文成像光谱

基本信息

  • 批准号:
    RGPIN-2016-06551
  • 负责人:
  • 金额:
    $ 7.07万
  • 依托单位:
  • 依托单位国家:
    加拿大
  • 项目类别:
    Discovery Grants Program - Individual
  • 财政年份:
    2020
  • 资助国家:
    加拿大
  • 起止时间:
    2020-01-01 至 2021-12-31
  • 项目状态:
    已结题

项目摘要

Approximately half of the radiant energy emitted by the universe falls in the far-infrared (FIR) spectral range (301000 µm) for two reasons: the first is that sources in the distant universe, galaxies in the local universe, or protostars in our own galaxy are often shrouded in dust and gas. The dust efficiently scatters and absorbs shorter wavelength radiation, which is subsequently re-radiated at longer wavelengths, both as continuum (dust) and line (ions, atoms, molecules) emission. The second reason is that distant galaxies do not decrease in IR brightness with increasing distance, because their emission is redshifted into the IR. Most of the FIR is inaccessible from the ground due to atmospheric absorption. Moreover, space borne instruments must operate at ~ 4 K to minimize their self-emission, which would otherwise dominate the weak astronomical signal. In previous FIR missions cooling was achieved by placing the entire telescope in a cryostat, limiting the diameters of primary mirrors to ~60 cm and resulting in relatively low spatial resolution. The Herschel Space Observatory broke this trend by employing a 3.5 m diameter passively cooled primary mirror located outside of the instrument payload, the instrument suite being cooled to ~4K. This design provided a major advance in spatial resolution and sensitivity, however, the latter remained limited by photon noise from the relatively warm (~80K) telescope. Potential gains in sensitivity of 2 -3 orders of magnitude exist by actively cooling large aperture telescopes as proposed for the ESA/JAXA SPICA mission. However, to realize these gains, the noise performance of the instruments themselves must be understood to a corresponding higher degree. This proposal has two components, the first is to continue to use data from Herschel/SPIRE in the study of the interstellar medium and the earliest stages of star formation, the time when molecular clouds fragment into cold and dense gravitationally bound cores. Starless cores can be probed by studying their thermal (continuum) emission, which provides information about the dust properties, and their line emission (or absorption), which provides information on the chemistry in these regions. Together they provide a unique window into the initial conditions of protostellar collapse. With its broad spectral coverage and intermediate resolution SPIRE is well suited to this task. The second component is to develop and evaluate the performance of a prototype of the spectrometer proposed for the SPICA/SAFARI instrument. A recently commissioned, large volume, low background, test facility cryostat will be used to study optical and thermal properties of key components of the spectrometer such as etalons, mechanisms and metrology. The ability to evaluate the performance of an integrated system at cryogenic temperatures will position Canada to be a partner of choice in future FIR space astronomy missions.
宇宙发射的辐射能大约有一半落在远红外(FIR)光谱范围内(301000µm),原因有两个:第一是遥远宇宙中的源、本地宇宙中的星系或我们银河系中的原恒星经常被尘埃和气体所笼罩。尘埃有效地散射和吸收较短波长的辐射,这些辐射随后以较长波长的形式重新辐射,作为连续体(尘埃)和线(离子、原子、分子)发射。第二个原因是,遥远星系的红外亮度不会随着距离的增加而降低,因为它们的辐射被红移到红外中。

项目成果

期刊论文数量(0)
专著数量(0)
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会议论文数量(0)
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Naylor, David其他文献

Using Sensor Networks to Study the Effect of Peripatetic Healthcare Workers on the Spread of Hospital-Associated Infections
  • DOI:
    10.1093/infdis/jis542
  • 发表时间:
    2012-11-15
  • 期刊:
  • 影响因子:
    6.4
  • 作者:
    Hornbeck, Thomas;Naylor, David;Polgreen, Philip M.
  • 通讯作者:
    Polgreen, Philip M.

Naylor, David的其他文献

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{{ truncateString('Naylor, David', 18)}}的其他基金

Fundamental Experimental and Numerical Convective Heat Transfer Research
对流传热基础实验和数值研究
  • 批准号:
    RGPIN-2020-04327
  • 财政年份:
    2022
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Fundamental Experimental and Numerical Convective Heat Transfer Research
对流传热基础实验和数值研究
  • 批准号:
    RGPIN-2020-04327
  • 财政年份:
    2021
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2021
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Fundamental Experimental and Numerical Convective Heat Transfer Research
对流传热基础实验和数值研究
  • 批准号:
    RGPIN-2020-04327
  • 财政年份:
    2020
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2019
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Fundamental Heat Transfer Research with Building Energy Applications
建筑能源应用的基础传热研究
  • 批准号:
    155420-2013
  • 财政年份:
    2018
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2018
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2017
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2016
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Analysis and optimization of a roof based building integrated photovoltaic/thermal system
屋顶建筑光伏光热一体化系统分析与优化
  • 批准号:
    485641-2015
  • 财政年份:
    2015
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Engage Grants Program

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相似海外基金

Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2021
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2019
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2018
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2017
  • 资助金额:
    $ 7.07万
  • 项目类别:
    Discovery Grants Program - Individual
Astronomical imaging spectroscopy at far-infrared wavelengths
远红外波长的天文成像光谱
  • 批准号:
    RGPIN-2016-06551
  • 财政年份:
    2016
  • 资助金额:
    $ 7.07万
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    5437-2011
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    2015
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Astronomical imaging spectroscopy at far infrared and submillimetre wavelenghts
远红外和亚毫米波长的天文成像光谱
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远红外和亚毫米波长的天文成像光谱
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远红外和亚毫米波长的天文成像光谱
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  • 财政年份:
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    $ 7.07万
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    Discovery Grants Program - Individual
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远红外和亚毫米波长的天文成像光谱
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    5437-2011
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    2011
  • 资助金额:
    $ 7.07万
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