... At lower redshifts, near-infrared spectroscopy (including slitless spectroscopy with WFC3 on HST) has enabled us to measure star formation rates at redshifts beyond one through the redshifted rest-frame optical lines. ...
... More recently, the ISO (Infrared Space Observatory) satellite, despite it's ghastly French detectors, discovered a large ... The DIRBE (Diffuse Infrared Background Experiment) detector on the COBE satellite has also recently picked up a diffuse ...
... It may just be too faint, people may have been looking in the wrong way, but most likely, it is just that all the light from things beyond redshift 6 is shifted into the infrared, and infrared detectors are not as sensitive as optical ones yet. ...
... work with both visible light and infrared radiation (wavelengths just a little ... with the GSAOI camera, we'll get infrared pictures as sharp as pictures from the ... an instrument called NIFS (Near-infrared Integral Field Spectrograph) for Gemini ...
... He starts with the hardest topic: direct imaging in the infrared with coronagraphy and interferometry. ... My favorite section is Jones's clear explanation of how to interpret infrared spectra of planets. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/JonesReviewPhysicsTodayv2.pdf -- 75.3 Кб -- 25.01.2010 Похожие документы
... sample of 60 micron Peaker galaxies have radio core luminosities which are intermediate between "normal" Seyferts (i.e. far-infrared selected Seyferts chosen without regard to far-infrared spectral energy distribution) and radio-loud ellipticals ...