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    11. http://hea-www.harvard.edu/~bradw/cv/papers/rxj1856.ps.gz
    ... methods 1 and 2 correspond formally to a radius over distance ratio (angular size) of R1 =D 100 ј 4:12 # 0:68 km per 100 pc ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/rxj1856.ps.gz -- 172.7 Кб -- 10.06.2002
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    12. http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords4.4.ps
    ... nominal focal length of the mirror is then needed to convert to actual angular size ... In practice, the angular size may be directly encoded in a WCS CDELT header ... The corresponding angular sizes are also given, but the actual angular size will be ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords4.4.ps -- 1242.2 Кб -- 16.03.1999
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    13. http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords.ps
    ... nominal focal length of the mirror is then needed to convert to actual angular size ... In practice, the angular size may be directly encoded in a WCS CDELT header ... The corresponding angular sizes are also given, but the actual angular size will be ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords.ps -- 1255.1 Кб -- 23.04.1999
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    14. http://hea-www.harvard.edu/~kim/pap/2012_YoungE_ISM_published.pdf
    ... As before, we select r = 30 in an angular size. ... This angular size corresponds approximately to one effective radius, re = 25 and 40 in NGC 720 and NGC 3923, respectively (from ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_YoungE_ISM_published.pdf -- 875.1 Кб -- 03.05.2012
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    15. ECT: Resources for Teachers
    ... Sighting Angular Size - Project for 4-6 grades to gain an understanding of angular measurement and how it is used for things such as surveying and astronomy. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ECT/allresources.html -- 67.4 Кб -- 01.10.2012
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    16. http://hea-www.harvard.edu/x-ray-clusters/papers/nocf-conf.pdf
    ... The angular size range in which the 400d X-ray detection is sensitive encompasses the entire range of core-radii expected for the high-redshift clusters (c.f. shaded histogram in Fig. 3b). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/x-ray-clusters/papers/nocf-conf.pdf -- 480.1 Кб -- 21.11.2006
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    17. http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf
    ... We calculate angular size distances in our cosmological model using the ANGSIZ code of Kayser et al. (1997). 4 No. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf -- 528.5 Кб -- 14.09.2005
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    18. http://hea-www.harvard.edu/~slane/ref/ps/RBS.ps
    ... Of course, both the finite angular size and the finite 3 energy resolution of the detector will result in a distribution of energies associated with a particular scattering material. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~slane/ref/ps/RBS.ps -- 85.2 Кб -- 31.01.2011
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    19. http://hea-www.harvard.edu/~kim/pap/2006_N3379_N4278_XLF.pdf
    ... Moreover, the large angular size (D25 ј 26 0 ) of NGC 5128 makes it hard to effectively remove contamination by foreground and background X-ray sources, which, given the depth of the exposure, account for about half of the detected sources ( Voss ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2006_N3379_N4278_XLF.pdf -- 358.3 Кб -- 06.12.2010
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    20. http://hea-www.harvard.edu/~slane/ref/ps/SPIE2_91.ps
    ... Of course, both the finite angular size and the finite energy resolution of the detector will result in a distribution of energies associated with a particular scattering material. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~slane/ref/ps/SPIE2_91.ps -- 93.9 Кб -- 31.01.2011
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