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    1. http://www.stsci.edu/ftp/meetings/galaxy-morphology/im.ps
    ... A Test of Galaxy Evolutionary Models Via Angular Sizes M. Im S. Casertano, R. E. Griffiths, & K. U. Ratnatunga (The Johns ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/meetings/galaxy-morphology/im.ps -- 225.3 Кб -- 07.09.1994
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    2. Cosmology with the HST Medium Deep Survey
    ... be measured is, of course, a function of both angular size and apparent magnitude ... 1990) predict luminous galaxies of large angular size at high redshift: such objects ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/griffithsr.html -- 40.2 Кб -- 15.06.2005
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    3. HARD X
    ... by satellite size and weight restrictions, provide only crude angular resolution, of ... point spread function depends upon the angular size of the single smallest mask ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/desai.htm -- 17.6 Кб -- 21.04.2010
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    4. STScI Preprint #1218
    ... In this way we have derived an absolute size of the ring R abs = (6.23 0.08) 10 17 cm and an angular size R" = 808 17 mas, which give a distance to the supernova d(SN 1987A) = 51.4 1.2 kpc and a distance modulus m-M(SN 1987A)=18.55 0.05. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1218/prep1218.html -- 4.9 Кб -- 23.05.2000
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    5. http://www.stsci.edu/stsci/meetings/space_detectors/pdf/desai.pdf
    ... by satellite size and weight restrictions, provide only crude angular resolution, of ... point spread function depends upon the angular size of the single smallest mask ...
    [ Текст ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/pdf/desai.pdf -- 326.1 Кб -- 30.08.2001
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    6. The Vega Debris Disk: A Surprise from Spitzer
    ... The disk is well resolved, and its angular size is much larger than found previously. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2005ApJ...628..487S.html -- 5.6 Кб -- 21.01.2016
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    7. http://www.stsci.edu/~marel/decadal/sc/320.pdf
    ... only a few Mpc, and their projected angular sizes decrease rapidly below 0.1" beyond ... up to much higher redshifts, since the angular size scale changes very slowly above ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/320.pdf -- 1618.8 Кб -- 19.02.2009
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    8. Extragalactic Cepheid Distances by Calibrated Period - Luminosity-Color
    ... to Cepheids are derived by matching the photometric angular size of photosphere inferred by a surface brightness-color SC ... and theoretical results, this IR relation was found to be an ideal reference for inferring unbiased stellar angular sizes ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/dibenep.html -- 13.2 Кб -- 15.06.2005
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    9. http://www.stsci.edu/hst/fgs/documents/papers/1999Chicago.AAS.pdf
    ... Measuring the angular size of extended objects. · Relative astrometry at the 0.2 mas level (mV < 14.5). ... the FGS has also been used to determine the angular sizes of Active Galactic Nuclei (AGNs), asteroids, and extragalactic star ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/fgs/documents/papers/1999Chicago.AAS.pdf -- 499.6 Кб -- 23.08.2004
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    10. http://www.stsci.edu/science/preprints/prep1218/prep1218.bib
    ... SIZE=-1><SUB>abs</SUB></FONT>&nbsp;=&nbsp;(6.23&plusmn;0.08) &times;10<FONT SIZE=-1><SUP>17</SUP></FONT>&nbsp;cm and an angular size R"&nbsp;=&nbsp;808&plusmn;17&nbsp;mas, which give a distance to the supernova d(SN 1987A)&nbsp;=&nbsp;51.4&plusmn;1.2&nbsp ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1218/prep1218.bib -- 2.8 Кб -- 07.10.1998
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