... These estimates should include the effect of the earth's atmosphere, but not the spectrum of the target (the effe ct of the target spectrum should be taken into account as part of any model-fitting/mapping process, i.e. the target spectrum is part of the ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel2_apr02_letter.pdf -- 36.2 Кб -- 11.01.2008 Похожие документы
... These estimates should include the effect of the earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken into account as part of any model-fitting/mapping process, i.e. the target spectrum is part of the ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel4_feb03_letter.pdf -- 45.0 Кб -- 11.01.2008 Похожие документы
... These estimates should include the effect of the earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken into account as part of any model-fitting/mapping process, i.e. the target spectrum is part of the ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel5_apr03_letter.pdf -- 44.9 Кб -- 11.01.2008 Похожие документы
... These estimates should include the effect of the earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken into account as part of any model-fitting/mapping process, i.e. the target spectrum is part of the ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel3_nov02_letter.pdf -- 45.2 Кб -- 11.01.2008 Похожие документы
... These estimates should include the effect of the Earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken TABLE 6 OI_VIS (Revision 1) Label OI_REVN .. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/OIFITS_PASP.pdf -- 70.0 Кб -- 11.01.2008 Похожие документы
... 1 INTRODUCTION The Atacama Large (sub-)Millimetre Array (ALMA) will calibrate and correct the effects of the Earth's atmosphere on the phase of the observed radiation by a combination of two techniques: (i) Frequent (every 20200 s, depending on the ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2009/ALMAMemo588.pdf -- 908.6 Кб -- 25.11.2009 Похожие документы
... 11 For a V=16 star with a flat electromagnetic spectrum in the visible region, we could approximate the number of photons (F1) reaching the earth's atmosphere as: F1 = 2 ( m1 - m2 ) / 5 F 100 Where F2 = 9480 photons cm-2 s-1 nm-1, m1=16 and m2=0 ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.OldDocs/INT-403-ENG-0006.pdf -- 377.3 Кб -- 28.04.2010 Похожие документы
... 1 INTRODUCTION: Astronomical measurements carried out with ground-based telescopes are corrupted by optical aberrations introduced by the Earth's atmosphere. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROI.Tip-tiltSystems/INT-402-MIS-0034.pdf -- 323.2 Кб -- 04.05.2007 Похожие документы
... Method The on-axis gain of a radio telescope is the constant of proportionality (assuming a completely transparent Earth's atmosphere) between the flux density of a point source, S , and the measured antenna temperature, T A , when the point source is on ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2006/ptcspn47.pdf -- 1524.5 Кб -- 25.11.2009 Похожие документы
... For ground-based long-baseline optical and infrared interferometers, the Earth's atmosphere introduces random path-length uctuations of many tens of microns with a timescale as short as a few milliseconds. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-162-letter.ps -- 1693.2 Кб -- 20.02.2013 Похожие документы