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    21. http://hea-www.harvard.edu/~pgreen/Papers/um425_03.pdf
    ... In the SIS model for the lensing mass, and using the minimum flux redshift for zl, the observed image separation of 6 > 5 12 We calculate angular size distances in our cosmological model using the ANGSIZ code of Kayser, Helbig, & Schramm (1997). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/um425_03.pdf -- 975.1 Кб -- 01.04.2005
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    22. http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords3.ps
    ... Instrument System Size at Focal Plane Angular Size \Delta p , \Delta ps (mm) \Delta ... which correspond to somewhat different angular sizes than the imaging case because ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords3.ps -- 851.6 Кб -- 18.02.1997
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    23. http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf
    ... Given the typical angular size of relaxed clusters, this requires a field of view (FOV) of 5 arcmin on a side. ... Source Extent: Either point like or extended, if extended, an approximate angular size. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011
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    24. http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf
    ... Throughout, we assume the following cosmological parameters for distance-dependent quantities: m = 0.3, = 0.7, and H0 = 72 km s-1 Mpc-1 , 1580 which yields an angular size scale of 5.5 kpc arcsec redshift of our system (z 0.44). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf -- 1028.8 Кб -- 02.02.2010
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    25. http://hea-www.harvard.edu/~kim/pap/2005_M33_I.pdf
    ... M33's proximity, angular size, and low line-of-sight column density provide unique ... data compiled by Dickey & Lockman (1990). angular size of M33 allows the observation ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2005_M33_I.pdf -- 431.8 Кб -- 06.12.2010
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    26. http://hea-www.harvard.edu/~bradw/cv/papers/CXwinds.pdf
    ... All other things being equal, the number of detected CX counts goes as the inverse square of the distance to a star, but the angular size of the emission region scales as 1/d so that the number of detected photons per radial bin (counts per arcsecond) is ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/CXwinds.pdf -- 67.0 Кб -- 23.01.2001
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    27. http://hea-www.harvard.edu/~bradw/cv/papers/CXwinds.ps
    ... other things being equal, the number of detected CX counts goes as the inverse square of the distance to a star, but the angular size of the emission region scales as so that the 1/d number of detected photons per radial bin (counts per arcse­ cond) is ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/CXwinds.ps -- 184.8 Кб -- 23.01.2001
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    28. http://hea-www.harvard.edu/vlp_m33_public/rt08a.pdf
    ... constant K of the spectral fit as follows: K= 10-14 2 4 DA ne nH dV , (1) http://cxc.harvard.edu/toolkit/pimms.jsp where DA is the angular size distance to the source in (cm), and ne and nH are the electron and hydrogen densities per cm-3 , respectively ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/vlp_m33_public/rt08a.pdf -- 1183.9 Кб -- 09.06.2008
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    29. The Lynxx
    ... The pixel size of the Lynxx's chip gives it the capability of very high angular resolution. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node56.html -- 5.1 Кб -- 01.10.2012
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    30. Guess My Shape - Links
    ... Zini's Activities - Some fun lessons on shapes and sizes with pages to print out for ... A fun game for younger students to learn to differentiate between size and shape ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ECT/Guess/resources.html -- 7.9 Кб -- 01.10.2012
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