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    91. Mode = ACQ/PEAKXDConfig = COS/NUV
    ... The middle stripe ( MEDIUM ) is preferred because the flight software only stores the cross-dispersion offset between the location of the calibration spectrum and the optimal location of the science spectrum for that stripe. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelp21/ch14_cos09.html -- 16.2 Кб -- 24.05.2013
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    92. http://www.stsci.edu/documents/dhb/webvol2/c21_wfpc1errors.fm7.html
    ... The absolute sensitivity calculation in WF/PC-1 is done assuming a flat spectrum (constant flux per wavelength); if the spectrum of the source is not flat, the STSDAS synphot package can be used to recalibrate the flux (see Chapter 3). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c21_wfpc1errors.fm7.html -- 4.8 Кб -- 10.02.1998
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    93. Standard Patterns for Substepping and Background Measurement
    ... 3), N spectrum is the number of spectrum bins (col. 2), and ratio is from column 4. The minimum STEP-TIME is 0.2 sec. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/ghrs/GHRS_46.html -- 3.4 Кб -- 14.02.1996
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    94. Results for Side 1 (1100-1350 )
    ... The baseline spectrum is the one obtained on SMS 94098, and the five subsequent spectra were divided by the baseline spectrum with binning intervals of 10 (for details see ISR 69 ). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/instrument_news/GHRS/Ghrs_isr/ghrs_isr071/GHRS071_5.html -- 3.6 Кб -- 30.05.1996
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    95. The Spitzer discovery of a galaxy with infrared emission solely due to AGN
    ... the 5-37 ЮМm Spitzer/IRS spectrum and broad wavelength spectral energy distribution ... The spectrum shows a redshifted (z = 0.14 ТБ 0.005) silicate emission feature with ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011A&A...531A.137H.html -- 5.3 Кб -- 21.01.2016
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    96. Mode = ACQ/PEAKXDConfig = COS/NUV
    ... The middle stripe ( MEDIUM ) is preferred because the flight software only stores the cross-dispersion offset between the location of the calibration spectrum and the optimal location of the science spectrum for that stripe. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelpCy20/ch14_cos09.html -- 15.3 Кб -- 31.05.2012
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    97. COS Instrument Handbook
    ... The spectrum is collapsed along the dispersion direction, its centroid is calculated ... A target spectrum is recorded for the user-specified time using a sub-array tailored ... The spectrum is collapsed along the dispersion direction. 3. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/cos/design/hst/cos/documents/handbooks/current/ch08.Acquisitions06.html -- 12.3 Кб -- 12.04.2016
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    98. HST Spectral Maps of Accretion Disks in Cataclysmic Binaries
    ... The spectrum of the disk region containing the gas stream (Fig.2b) is noticeably different from the disk spectrum at the same radius for a range of radii. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/baptistar.html -- 12.0 Кб -- 15.06.2005
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    99. Results
    ... of the PC image of 0142 in the upper left, and its power spectrum in the upper right ... of a star is shown in the lower left and its power spectrum is in the lower right ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nisensonp.dir/section3_3.html -- 7.5 Кб -- 16.04.1994
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    100. Fluxes and Standard Magnitudes
    ... where m is in the STMAG system which is based on a spectrum with constant flux per unit wavelength set to roughly match the Johnson system at V. The more conventional systems are based on Vega's spectrum. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch8_calibration8.html -- 14.9 Кб -- 29.08.2000
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