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    41. http://www.mso.anu.edu.au/seminars/abstracts/20151216-1100.html
    ... state-of-art instruments which cover almost entire wavelength range in optical to mid-infrared and various spectral resolutions ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151216-1100.html -- 4.8 Кб -- 10.04.2016
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    42. http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html
    ... 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. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html -- 4.4 Кб -- 10.04.2016
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    43. Research Interests
    ... 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 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node27.html -- 5.5 Кб -- 02.10.2012
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    44. Research Interests
    ... 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. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node30.html -- 6.1 Кб -- 02.10.2012
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    45. GSAOI Latest Developments Page
    ... 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 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/latest/index.shtml -- 10.4 Кб -- 01.10.2012
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    46. http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf
    ... table (the primary quantity is given in bold): Photon Typical microwave Typical far infrared (Hz) (Angstroms) (metres) 0.20 100 10 = 10 ­6 (eV) 6.2 10 1.1 10 0.62 2.48 12.4 ­6 ­2 ­4 Typical near infrared Typical optical Typical UV Soft X-ray Hard X-ray ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf -- 117.5 Кб -- 04.08.2009
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    47. http://www.mso.anu.edu.au/~charley/papers/JonesReviewPhysicsTodayv2.pdf
    ... 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. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/JonesReviewPhysicsTodayv2.pdf -- 75.3 Кб -- 25.01.2010
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    48. http://www.mso.anu.edu.au/nifs/publications/2002a.pdf
    ... to permit measurements between strong near-infrared OH airglow emission lines where the near-infrared sky background is low ... near-infrared spectroscopy are studies of: § § § § § § § § § § § § § § Massive black holes in nearby galactic nuclei Nearby ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/nifs/publications/2002a.pdf -- 532.4 Кб -- 09.07.2002
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    49. Untitled1
    ... 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 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/07_research.html -- 73.5 Кб -- 02.10.2012
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    50. NIFS Performance Calculator
    ... Signal-to-noise ratio /aperture . This tool models the performance of the Gemini Near-infrared Integral-Field Spectrograph (NIFS) . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/nifs/predictions/performance.shtml -- 32.6 Кб -- 10.04.2016
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