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    11. Andy Fruchter's Homepage
    ... Among these are images of GRB 990123, a burst which reached an apparent visual magnitude of V=9 (bright enough to be observed with a pair of binoculars), yet was at a distance of some 10 billion light years. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~fruchter/ -- 5.2 Кб -- 01.10.2012
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    12. Figure of Merit
    ... magnitude determination: find the star in the truth file that falls nearest to the position of each star in my photometric ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/stetsonp.dir/section3_3.html -- 9.7 Кб -- 18.04.1994
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    13. NStars1A: Photometric searches - 2MASS and optical colours
    ... The catalogue lists F, B J and V magnitudes, and includes some sources as faint as 19th magnitude in R, although it is not complete at those magnitudes. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/nstarsu1.html -- 7.5 Кб -- 08.06.2007
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    14. http://www.stsci.edu/hst/fgs/documents/isrs/fgs_isr25.pdf
    ... Fig. 1a shows the amount of correction in magnitudes owing to the PMT deadtime which needs to be applied to the instrumental magnitudes as derived from the measured counts as a function of visual Johnson magnitude. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/fgs/documents/isrs/fgs_isr25.pdf -- 57.3 Кб -- 23.08.2004
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    15. WFC3 Instrument Handbook
    ... 7.8 . IR Sensitivity . 7.8.1 Limiting Magnitudes . 7.8.1 Limiting Magnitudes . ... Table 7.10 presents the predicted limiting-magnitude performance of the WFC3 IR channel and compares it with that of the NIC3 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/hst/wfc3/documents/handbooks/currentIHB/c07_ir09.html -- 17.8 Кб -- 12.04.2016
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    16. http://www.stsci.edu/stsci/meetings/planets/abs/prog36.html
    ... The positions, magnitudes, and colors of all stars to approximately visual magnitude 15 will be measured. ... proper motions and parallaxes of all stars to 15 magnitude, with magnitude dependent accuracy of positions, proper motions and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/planets/abs/prog36.html -- 3.3 Кб -- 22.10.1996
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    17. WFC3 Instrument Handbook
    ... 6.8 . UVIS Sensitivity . 6.8.1 Limiting Magnitudes . 6.8.1 Limiting Magnitudes . ... Table 6.10 presents the predicted limiting-magnitude performance of WFC3 and compares it with that of the ACS camera. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/hst/wfc3/documents/handbooks/currentIHB/c06_uvis09.html -- 24.7 Кб -- 12.04.2016
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    18. STIS Instrument Handbook
    ... The integrated magnitude limit gives the total magnitude from all stars (or galaxies, or diffuse objects) of spectral type O which can appear in the MAMA field of view. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/design/documents/handbooks/currentIHB/c14_imref34.html -- 283.9 Кб -- 12.04.2016
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    19. CSPICE Routines: VNORMG_C
    ... magnitude of that component indicates that a numeric overflow would occur when it is squared, or if it indicates that an underflow would occur when squared (falsely giving a magnitude of zero) then the following expression is used: vnormg_c = v1max ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~sontag/spicedocs/cspice/vnormg_c.html -- 5.5 Кб -- 17.12.2005
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    20. Target Count Rates
    ... The quantity AB is a color-dependent correction from V magnitude to AB magnitude at frequency . ... AB is defined as a color-dependent correction from V magnitude to AB magnitude at frequency . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand4/ch6_exposuretime4.html -- 34.1 Кб -- 04.09.2001
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