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. ...

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• Updates to the STIS Calibration Software, Reference Files, and OTFR Pipeline

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

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• NICMOS Data Calibration and Analysis

... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...

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• A Method for Minimizing Background Offset Errors When Creating Mosaics
• Automated Software for Slitless Spectroscopy Analysis and Quasar Selection
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in

... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Calibration & Background Calibration Background Analysis . ... Back to Background Analysis Page . The XMM-Newton Extended Source Analysis Software package (XMM-ESAS) is developed at the NASA/GSFC XMM-Newton Guest Observer Facility (GOF) in cooperation with the XMM-Newton SOC and the Background Working Group. ... http://xmm.esac.esa.int/sas/current/doc/esas/index.html . ...

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• XMM-Newton SAS: Watchout Page
• XMM-Newton SAS: Software requirements
• XMM-Newton Science Analysis Software

... This example uses an error array to determine the errors in the radial profile. task: imcnts . ... xs imcnts err=vigsnr_err expo=xdata$snr_exp.pl expthr=95.0 bkgdex=xdata$snr_exp bkgdth=95.0 bkgderr=vigsnr_err # Run the imcnts task with the appropriate parameters source image file : vigsnr # vigsnr.imh source region descriptor: a 300 300 0 50 n=5 # 5 annuli centered at 300 , 300 , 0 and 50 pixels min/max radius background image file or cts/pixel: cr # From the same ...

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• The ST-4
• Background Corrections
• The Lynxx Tools

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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. Aristarchus was extremely clever and also figured out a way to determine the ratio of distances between the earth and the moon and the earth and the sun. While wrong, at least he reasoned that the sun was much farther from the earth than the moon. Just Try and Follow this! . Summary of Greek Science .

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Next: Results of follow-up spectroscopy Up: Spectral observations and data Previous: Spectral observations and data . ... The reduction of the originally two-dimensional CCD data included standard steps such as: bias and dark subtraction, flat-fielding, cosmic-ray removal. ... In the final spectra showing emission lines, redshifts and line fluxes are measured applying Gaussian fitting. ... The line [O II ] 3727 ? ... For all spectra, the individual emission line fluxes of the H , [N II ] 6548,6583 ? ...

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• Background - Frequently Asked Questions - Apache HTTP Server
• Wavelength calibration
• Background Correction

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• Background Material for the Phase Correction Project
• World Coordinate Systems (WCS) in FITS
• ccontsubtract CentralProcessor 0.11 documentation

... Russian KOI8 . Scientists of Laboratory of radio astrophysics develop algorithms and software. ... design of statistical estimations methods of average and smoothing; . fitting algorithms design; . development of the data processing system FADPS (Flexible Astronomical Data Processing System); . design of visualisating and interactive data reduction programs for initial observational data ( fgr (Russian KOI-8) ) and continuum radio sources spectra (spg); . ...

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... Report on Cosmic Call 1999 . ... Cosmic Call Sessions . ... This Report outlines methodology, hard- and software, which were developed to transmit first public Interstellar messages from Evpatoria Deep Space Center (EDSC), and describes four Cosmic Call Sessions, which were fulfilled in EDSC on May 24 and June 30 - July 1, 1999. ... Each Cosmic Call consists of two parts. ... Dutil Message, . ... The software for gathering all messages and creating the Cosmic Call stream, was written on C language. ...

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• Processing Pictures - "InformChaos" Software

ALMA | ... Phase Correction Algorithms | ... On this page, we describe what the phase correction algorithms set out to do and the framework we have developed to optimally use all of the available information. ... We are developing a Bayesian framework to combine all the information we have about the current and future meterological conditions (which are naturally accommodated as priors in a Bayesian scheme) with detailed physical models of the atmosphere. ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• ALMA WVR phase correction algorithms and software Bojan Nikolic web pages (r.
• Inference of Coefficients for Use in Phase Correction

idl software documentation (phil's idl routines ) . ... aofits header format for the mock spectrometers (idl mas routines) . psrfits format for mock spectrometers .pdev file format for mock spectrometers . Description of idl spectral line header for interim correlator data . ... etc.. software modification history. generic idl routines. idl routines for correlator data . ... idl routines for wapp spectral line fits data . ... idl routines for mock spectrometer .pdev files (pdevxxx routines) . ...

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• azencRackGearRunout
• Progress Report on Software Spectrometer Development for GALFA
• Phil's public html listings

... The example demontsrates a way how to use the coefficients arrays and the Software . Let us suppose that we have a direction in the S/C frame, determined by the angles u1, u2, where: u1 - angle between vector and X axis (polar angle) u2 - angle on the YZ plane from Y axis (anticlockwise); . ... We use the file 950909t1 (the beginning data 9.09.06), which line 2 interval beginning : date 10.10.95 , time 1.926 thousands of sec, the interval duration is 4.583 thousand of sec. ...

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• Software for Attitude Determination

... Science Users Information > Data Handling and Products > Science Data Products Forum . ... Science Software . ... Science Data Products Forum . ... The ESO Science Data Products Forum is a platform for sharing ideas,methods, software and data to assist with the production of science data products from ESO telescopes. ... Software, calibration data or documents up to 100MB in size can be attached to any post.This forum is not meant to distribute scientific results or data products to the community. ...

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• IRAF/STECF 2-D spectrum point source / background decomposition package
• ESO - The Scisoft Software Collection
• ESO - Science Software

Bigbang Forum Message . ... Post . ... Solution . ... Post Message | Back to Thread Topics | ... OK - a friend explained it to me this way... for example - the background microwave radiation which originated shortly after the big bang. Take a mirror and reflect that radiation directly back the way it came. - hitch a ride on :) . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Brilliant! Thanks - an Astronomy Net Blackholes2 Forum Message
• Just A Little Background On Dick - an Astronomy Net Exploration Forum Message
• The Astronomy Shop - Software - by Astronomy Net

Next: The root filesystem Up: Overview of the Directory Previous: Overview of the Directory . This chapter is loosely based on the Linux filesystem standard, FSSTND, version 1.2 (see the bibliography, [ Qui95 ]), which attempts to set a standard for how the directory tree in a Linux system is organized. ... This chapter does not explain all files in detail. ... The major parts are the root, /usr љ , /var љ , and /home љ filesystems (see figure 2.1 ). ... Figure 2.1: Parts of a Unix directory tree. ...

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• Simon Jeffery's Software Store
• Showing and setting time
• WWW Links.....

... Matrix of Transformation | ... Software | ... The software includes: . attidf.for - a FORTRAN subroutine to get a matrix M (named PA in the subroutine text) to transform any vector from the S/C coordinate system to the GSE coordinate system: . V GSE = M * V S/C . To transform a vector from the GSE coordinate system to the S/C coordinate system transpose the matrix M: . ... We want to know the direction of this vector in the GSE frame for date: 30.05.1997, time 1h.0min.0sec. ut. ...

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• Tail Probe | Additional Information
• Tail Probe | Matrix of Transformation Tail Probe | Matrix of Transformation
• Shift

TransNix is the software that will control the three different processors involved in the detector control and in the low-level data handling. ... the DSP 56001 processor, that sends to the detector chip the clock wave patterns; . ... the host computer, responsible of writing the raw data on disk, and communicating between the TransNix and the high level software (XNIR); in the laboratory versions, it will be based on an Intel processor, using Linux as operative system,. ...

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• SDSSmosaic
• Software Page
• First Occultation with the TNG

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... To improve the quality of ionograms and to carry out on automatic ionogram processing we have developed a special software, which can be arbitraly devided into the following main parts: . ... Ionogram processing software on the basis of image processing; . Interactive ionogram processing software. ... Here we present ionogram samples for different kinds of chirp sounding . ... Capabilities and samples | ...

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