“Herschel”的版本间差异

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*3.5m 目前口径最大的空间望远镜
*3.5m 目前口径最大的空间望远镜
*PACS, the Photodetector Array Camera and Spectrometer, a bolometer array photometer and a photoconductor array imagingspectrometer operating at a wavelenght range between 60 and 210 µm.:70 μm, 160 μm
*PACS, the Photodetector Array Camera and Spectrometer, a bolometer array photometer and a photoconductor array imagingspectrometer operating at a wavelenght range between 60 and 210 µm.:70 μm, 160 μm
*SPIRE (Spectral and Photometric Imaging Receiver) - the Spectral and Photometric Imaging Receiver, consisting of a 3-band(250,350,500 um) imaging photometer and a Imaging Fourier Transform Spectrometer and will operate at wavelengths between 200 and 670 µm.
*SPIRE (Spectral and Photometric Imaging Receiver) - the Spectral and Photometric Imaging Receiver, consisting of a 3-band(250,350,500 µm) imaging photometer and a Imaging Fourier Transform Spectrometer and will operate at wavelengths between 200 and 670 µm.
*HIFI (Heterodyne Instrument for the Far Infrared), a very high resolution heterodyne spectrometer

==相关科学数据==
*Stacked Average Far-Infrared Spectrum of Dusty Star-Forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer[https://arxiv.org/abs/1705.00734]

2017年5月3日 (三) 13:30的最新版本

space telescope

  • 3.5m 目前口径最大的空间望远镜
  • PACS, the Photodetector Array Camera and Spectrometer, a bolometer array photometer and a photoconductor array imagingspectrometer operating at a wavelenght range between 60 and 210 µm.:70 μm, 160 μm
  • SPIRE (Spectral and Photometric Imaging Receiver) - the Spectral and Photometric Imaging Receiver, consisting of a 3-band(250,350,500 µm) imaging photometer and a Imaging Fourier Transform Spectrometer and will operate at wavelengths between 200 and 670 µm.
  • HIFI (Heterodyne Instrument for the Far Infrared), a very high resolution heterodyne spectrometer

相关科学数据

  • Stacked Average Far-Infrared Spectrum of Dusty Star-Forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer[1]