WINERED
(Warm Infrared Echelle Spectrograph)
(near-infrared non-cryogenic spectrograph)
WINERED (for Warm Infrared Echelle Spectrograph)
is a near infrared spectrograph on the
Magellan Telescopes' Clay Telescope
(Las Campanas Observatory, LCO),
having previously been used on the Araki Telescope at
Koyama Astronomical Observatory (KAO) and
the New Technology Telescope (NTT) at the La Silla Observatory (LSO).
WINERED has a cryogenically-cooled camera, but
non-cooled ("warm") optics including
an echelle grating with spectral resolution of 28,000
and an immersion grating with a resolution of 100,000.
(instrument,spectrograph,infrared,Japanese)
Further reading:
https://ui.adsabs.harvard.edu/abs/2022PASP..134a5004I/abstract
https://arxiv.org/abs/1501.03403
https://wasatchphotonics.com/applications/winered-astronomy-spectrograph/
https://www.lco.cl/technical-documentation/winered/
WaveL | Freq | Photon Energy | | |
0.9μm | 333THz | 1.4eV | begin | WINERED |
1.35μm | 222THz | 918meV | end | WINERED |
|
Referenced by page:
Magellan Telescopes
Index