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1. http://xmm.vilspa.esa.es/sas/7.0.0/doc/omgrism.ps.gz
... The task makes use of a source-list produced by running omdetect on the same image. ... Parameter Mand Type Default Constraints set yes string OM image le with grism spectra aligned with respect to the columns of the image ( output from omg- prep). xmmsas 20060628 1801-7.0.0 XMM-Newton Science Analysis System Page: 2 sourcelistset yes string Source list ( output from omdetect) outset yes string Output spectra le region le no string Name of the ASCII (input) ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/omgrism.ps.gz -- 49.6 Кб -- 28.06.2006
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2. ESO - VLT/Instrument Interfaces
... Science . ... Science Users Information > Observing Facilities > Instrumentation Development > VLT/Instrument Interfaces . ... APEX Visitor Instrument . ... The interfaces between the VLT Unit Telescopes and the scientific instruments to be operated at the VLT Cassegrain, Nasmyth and Coudц© foci are well defined. ... Interface and numerous other relevant information for instrument builders is available in the "Requirements for Scientific Instruments on the VLT Unit Telescopes" , ESO doc. no. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/facilities/develop/interfacesvlt.html -- 31.4 Кб -- 10.04.2016
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3. Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/dolenskym1.html -- 9.4 Кб -- 12.06.2006
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/dolenskym1.html -- 9.4 Кб -- 15.05.1998
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4. WFC3 Instrument Handbook
WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Chapter 8: Slitless Spectroscopy with WFC3 > 8.5 Extraction and Calibration of Spectra . ... A spectral extraction software package, called aXe , is available to extract, flat-field, wavelength- and flux-calibrate WFC3 grism spectra. ... Extraction of WFC3/IR slitless spectra depends on an accurate determination of the diffuse background light that is observed in all grism exposures. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/hst/wfc3/documents/handbooks/currentIHB/c08_slitless6.html -- 9.6 Кб -- 12.04.2016
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5. Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/ -- 73.9 Кб -- 09.04.2016
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6. Background Corrections
Next: *imcalc* - Obtain a Up: Calibration Previous: Exposure Map . Background maps are provided by the standard processing for all ROSAT and Einstein instruments. For the PSPC and IPC these are in three standard bands: soft, hard, and broad (Table 6.2). ... N.B.: ROSAT PSPC background maps in SASS 5-6 or higher are generated by smoothing a source-subtracted, exposure corrected image (see the ROSAT Data Products Guide). ... imcalc* - Obtain a background subtracted image for ROSAT PSPC Data . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node116.html -- 8.0 Кб -- 01.10.2012
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7. Procedures for Observations
... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/proc_ob.html -- 7.9 Кб -- 16.02.2000
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8. http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session7/pavlov_ELW.pdf
... Europa lander", Moscow >12.02.2009 Outline Planetary instruments for in-situ chemical analysis Laser-induced plasma spectroscopy: principle, instrumentation, features GENTNER proposal of the LIBS instrument for the Europa lander mission State-of-the-art of the instrument Page 2 von Hoerner & Sulger GmbH Int. Symp. ... Page 3 von Hoerner & Sulger GmbH Int. Symp. ... Europa lander", Moscow >12.02.2009 Laser-Induced Breakdown Spectroscopy (LIBS): Principle Page 5 von Hoerner & Sulger GmbH Int. Symp. ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session7/pavlov_ELW.pdf -- 1074.7 Кб -- 02.03.2009
[ Текст ]  Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session7/pavlo