Detectors of the New Projects at NAOC

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Presentation transcript:

Detectors of the New Projects at NAOC An Introduction Qian song Chinese National Astronomical Observatories

The most significant instruments run and will run at NAOC Optical LAMOST Xuntian Telescope Advanced Space-based Solar Observatory (ASO-S) Radio FAST SKA participant X-ray Einstein Probe

LAMOST MA mirror MB mirror Fibers Spectrographs CCDs Fiber Positioning Ma: reflecting corrector (24 sub-mirrors) ~ 4.9m Mb: spherical mirror (37 sub-mirrors) ~ 6.1m 4000 spectra of objects at once

Chinese Space Station (CSS) & Xuntian Telescope 2m telescope in the same orbit as the CSS orbit; docking with CSS for service & repair. CSS construction complete by 2022

Xuntian Telescope The major aspects of the survey: Science: 17500 ° imaging : 255-1000nm, ≥6 filters, ≥25.5 m 17500° spect: 255-1000nm, R≥200, ≥22-23 m 400° deep imaging & spect: at least 1 m deeper Science: Cosmology: dark energy, dark matter, gravity, large scale structures Active galactic necleus Galactic astronomy Galactic structure ……. The telescope : Field of view：1.1 º Image resolution：0.15″ Pixel number：2.7G Image quality of the slitless spectrograph：better than 0.3″ Spectral resolution of the slitless spectrograph ：R≥200

Advanced Space-based Solar Observatory (ASO-S) Science: exploring solar eruptions and their origins Payloads FMG full-disc vector magnetograph LST Lyman-alpha solar telescopes HXT hard X-ray imager Orbit solar synchronous Altitude 720 km Inclination: 98.2 degree Launch year 2022 Mission duration > 4 years

FMG: full-disc vector magnetograph

LST：Lyman-alpha Solar Telescopes To observe CMEs continuously from solar disk to a few solar radii, another payload LST will be on board. It comprises three telescopes observing in Lyman-alpha and white light: SDI (solar disk imager), SCI (solar coronagraph imager), and WST a full-disk white-light solar telescope for the purpose of calibration of SCI. SDI SCI

FAST

Einstein Probe (EP) Science: Transients and variable sources survey on the X-ray (0.5 – 4keV) Payloads WXT Wide-field X-ray telescope FXT Follow-up X-ray telescopes Orbit circular Altitude 600 km Inclination: ≤30° Launch year ~2022 Mission duration 5 years

WXT Optics MPO or LEIO Detector MCP FoV 60º×60° Angular resolution 4’ X-ray 0.5–4 keV Effective area 2cm 2 @0.7keV FXT Detector CCD FoV 1º×1º Effective area 60cm 2 @1keV

Thank you for your attention.