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http://www.apo.nmsu.edu/arc35m/Instruments/NICFPS/.
http://www.apo.nmsu.edu/arc35m/Instruments/NICFPS/.
1. IKI IPL home page
You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...
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2. Astronomy Plus CCD Images of Galaxies
. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu
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Ссылки http://zebu.uoregon.edu/galaxy.html -- 4.8 Кб -- 10.03.2004
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3. Chandra Images for SNR J0537.8-6910
True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Distance: 50kpc( distance to LMC, Westerlund(1990) ) . ... Radio Images Page . ... Exposure uf . ... Exposure uf Exposure time of unfiltered event file . Exposure f Exposure time of filtered event file . The whole remnant is covered by chip ACIS-S3(CCD_ID=7) . ... Event 2 FITS File . ... see fit detail page for more about the fit. see chandra spectrum page for region used. ... Chandra Supernova Remnant Catalog . ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0537.8-6910/ -- 10.7 Кб -- 27.02.2014
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4. Ghost Images
Common ghost images result from internal reflections in the filters and in the field-flatteners. Two filter ghosts, caused by double (and quadruple) reflection inside the filter, are visible below and to the right of the star in Figure 5.13 . ... An additional ghost is caused by an internal reflection inside the MgF 2 field flattener lens immediately in front of each CCD ( Figure 5.14 ). ... Figure 5.14: Saturated Stellar Image Showing Field Flattener Ghost on WF2. ...
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Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand4/ch5_psf11.html -- 5.9 Кб -- 04.09.2001
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5. IBIS: Technical Description
The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...
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Ссылки http://www.arcetri.astro.it/science/solar/IBIS/IBIS_description.html -- 33.6 Кб -- 13.12.2015
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6. IRAF/STECF imaging linear polarimetry simulation and reduction package
... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data for ACS, FOC, NICMOS and WFPC2. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... hstpolsim -- Produce simulated polarization input data frames for HST instruments from images of the total signal, the linear polarization and the position angle of the polarization vectors. ...
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Ссылки http://www.eso.org/~jwalsh/softpol/ -- 8.2 Кб -- 02.02.2001
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7. ST-ECF IRAF package
... Several HST instruments both current and decommisioned have provided imaging linear polarimetry capabilities. ... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... For reduction of data from imaging linear polarization instruments other than from HST, the instrument