... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 . ... 1.3 NICMOS Proposal Preparation . ... 1.5 The NICMOS Instrument Team at STScI . ... 2.3 NICMOS Instrument Design . ... 4.1 Filters and Optical Elements . ... 4.1.2 Out-of-Band Leaks in NICMOS Filters . ... Camera 1, Filter F090M . Camera 1, Filter F095N . Camera 1, Filter F097N . Camera 1, Filter F108N . Camera 1, Filter F110M . Camera 1, Filter F110W . Camera 1, Filter F113N . ...

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• Space Telescope Imaging Spectrograph Instrument Handbook
• ACS Instrument Handbook for Cycle 20
• WFC3 Instrument Handbook

... We have developed a new extraction software package called aXe that was specifically designed to handle the ACS spectrophotometric data. ... The aXe software was designed to extract spectra in a consistent manner from all the slitless spectroscopy modes provided by the Advanced Camera for Surveys (ACS) that was installed on the Hubble Space Telescope in February 2002. ... The extraction process is a set of well isolated steps that can be individually applied and tweaked by the user (Figure 1 ). ...

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• On the Need for Input Data Control in Pipeline Reductions
• Using XML and Java for Astronomical Instrument Control
• A Spectroscopy Exposure Time Calculator for IRAF

... Example of an association table . Example of a CCD reduction table . ... CCD commands . ... Command parameters (1) . ... Checklist of necessary table files . ... DO commands . ... Observation Summary Table with file classifications appended in column :EXPTYPE and :OPATH as defined and applied in Table . ... Columns for star-catalog table files . ... Passband columns of the instrument table file . ... Detector columns of the instrument table file . ... Instrument table file for a simple CCD setup . ...

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• Echelle Spectra
• An example of selection criteria
• Loading the Telescope and Instrument Specifications

... 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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• Data Quality Control and Instrument Modeling
• pyQC: overview
• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)

... MODE = PrimePartialW2 / Instrument configuration CALIBRATION_ MODE _1 = PrimePartialW2 / Mode used to calibrate events from CCD 1 CALIBRATION_ MODE _2 = PrimeFullWindow / Mode used to calibrate events from CCD 2 CALIBRATION_ MODE _3 = PrimeFullWindow / Mode used to calibrate events from CCD 3 CALIBRATION_ MODE _4 = PrimeFullWindow / ... The DATA_MODE_n parameters indicate the data mode (determined by the oal ) the n-th CCD was in during the exposure. ...

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... 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 name is `SPECIAL'. ...

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• Near IR Astronomy with the ESO VLT
• VLT Status and Instruments
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

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• DOK-2 Results Page
• Instrumentation for Fundamental and Applied Space Projects

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

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• INTERBALL/ELECTRON EXPERIMENT
• ASPI experiment
• ENERGETIC PARTICLE EXPERIMENT DOK-2

... 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. ...

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• Observing capabilities
• Fasti Rationale
• NICMOS3 Detector for Spectroscopy

... На самом деле, когда я писал эту -- -- программу, мне хотелось потренироваться в проведении интервью по -- -- правилам SADT методологии. ... Логическое описание блоков SADT модели. ... Основное предназначение этих классов - хранить перечень посуды и -- -- инструментов, соответствующих различным блокам SADT модели. ...

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• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.A"
• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.DLG"
• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM\JAM.DLG"

Next: A wavelet Up: No Title Previous: Introduction . Figure: Data characterization using wavelets. The time axis is common to the raw data and the wavelet map (background), for which the vertical axis is analogous to an inverse frequency (Section 10). The Mexican hat wavelet (Section 3) used for the background wavelet map (Section 5) measures the magnitudes of local maxima (blue-grey shades) and minima (yellow/red shades) as a function of time and duration. ...

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• Dynamic HTML in Communicator
• Long description of example illustrating background calculation
• Long description of example of cell background calculation

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 . ...

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• Notes on IPC and PSPC Spectral Fitting
• Example - Creating a QPOE file from CD ROM Data
• Example - Retrieve Unscreened Data from CDROM

It is easy to incorporate information from an instrument or the telescope into your scripts. ... mess with the getKeyVar statements because getKeyVar returns None in debug mode, making the commands run, which is perfect. import TUI .TCC.TCCModel import TUI .Inst. DIS .DISModel from TUI .Inst. DIS .StatusConfigInputWdg import StatusConfigInputWdg InstName = DIS class ScriptClass(object): Simple script to configure DIS . def __init__(self, sr): Display ...

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• coordConv
• TUI:Introduction
• TUI:Scripts:Scripting Tutorial:Send Commands

OptInt PmWiki . Pm Wiki / . ... Wiki Style Examples . Wiki styles | ... PmWiki uses WikiStyles for styling text with color and other attributes. PmWiki 2.0 introduced the ability to control the styling further and to even place styles on blocks. ... In addition, an author can define a style "shortcut" by using the define= property. For example, to define a style of %red% , one can use: . define=mystyle color=red% Here is some %mystyle% red text created using a style shortcut. ...

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• OptInt PmWiki : PmWiki / Wiki Style Examples
• Astrophysics Group OIFITS: A Data Exchange Standard for Optical (Visible/IR)
• Understanding Infrared emission from galaxies

... Meade Instruments Corporation . ... Section 3: File Menu . ... Displays the dialog to open an existing image: . ... Saves the current image as a new file name or new file type, or both. ... This can be useful to prevent having 20 or more images open at once, and saves having to close them manually. ... This is done by creating a text file with the same name as the image file. ... Note that Image Information is saved within the FITS file, so there will not be a text file to accompany these files. ...

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• Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
• Meade Instruments Corporation - Pictor Manual Part 16
• Meade Instruments Corporation - Pictor Manual Part 13

... PmWiki . Summary: PmWiki group header. ... Summary: Styling text for colour and other attributes:) See also Wiki Styles Plus and Wiki style colors . ... PmWiki 2.0 introduced the ability to control the styling further and to even place styles on blocks. ... This text is %color=red% red, %color=blue% blue, %% and normal (black). ... For example, to define a style of %red% , one can use: . define=mystyle color=red% Here is some %mystyle% red text created using a style shortcut. ... Group . ...

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• Module pyrap.quanta pyrap v0.3 documentation
• Contents
• Pulsar Group Main/Psrfits

Lessons learned from the Thirty Meter Telescope site testing Tony Travouillon Sebastian Els, Angel Otarola, Reed Riddle, Matthias Schoeck, Warren Skidmore TMT.XXX.PRE.05.0XX.DRF01 1 Introduction TMT and its Site testing. Important choice before going on site. ... Considerations during analysis of the data. TMT.XXX.PRE.05.0XX.DRF01 2 Some Background about the TMT Site Testing TMT is a 30m, segmented, RitcheyChretien telescope design. ... ASCA Cloud Cover Analysis So how do we do it in practice? ...

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• http://site2010.sai.msu.ru/static/doc/Site2010-Summary.pdf

... NASA's newest Great Observatory, the Chandra X-Ray Observatory (CXO) -- formally known as the Advanced X-Ray Astrophysics Facility (AXAF) -- launched on July 23, 1999 and represents such an advance. ... Hughes Danbury Optical Systems (HDOS), now Raytheon Optical Systems Incorporated, figured and polished the x-ray optics; Optical Coating Laboratory Incorporated (OCLI) coated the polished optics with iridium; and Eastman Kodak Company (EKC) mounted and aligned the optics and provided the optical...

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• The Focal Plane Instruments
• The X-ray Optics
• Gravitational Wave Background from Individual Galaxies

... Stellar Evolution . Nucleosynthesis in Stars . The Evolution of Star Clusters . JAVA Physics Lab . Alternative Energies Class . Steve Kevan's Physics 251 Class . ... Talk on Solid State Physics of CCD detectors . Talk on Cosmological Issues . ... Digital Spectra of Stars . NETexperts E-mail List . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu ...

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• Galaxy Gallery Page III
• The Galaxy Gallery Page VII: Infrared Imaging
• CCD Astronomy Magazine Article Page 3

... Animation . Arrow . ... I created the first animation by running Script-Fu / Animators / Fire on the head of an arrow. ... I merged the animation with the background image, and specified a final X offset of -128 (the background is 128 pixels wide). This results in an animation with a nice moving background. Note that you can also use a background that is wider than the image, as long as you specify the width of the background for the final X offset if you want the final animation to loop. ...

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• GIMP animations: merge-anim example 1
• GIMP animations: merge-anim examples
• GIMP animations: merge-anim example 3