Next: Auxiliary Data Up: Spectral Analysis Previous: Convolution and Deconvolution . Interactive continuum determination can be done with the command NORMALIZE/SPECTRUM as mentioned above. There are commands to measure the position of spectral features. ... Measurements of line strengths and equivalent widths can be obtained with the command INTEGRATE/LINE . ... The fitting package permits the determination of line parameters and additional modelling of the data. ...

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Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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... User Guide ] Task: velplot Purpose: Interactively plot spectra and slices from Miriad Images. Categories: image analysis VELPLOT is an interactive task to analyse spectra, position- velocity slices, and integrated velocity maps from Miriad images. ... Also makes velocity and velocity dispersion images. ... The output from each option can be plotted, printed, or written out as Miriad images of velocity-averaged maps, position- velocity maps, or ascii spectra respectively. ...

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• clplot
• ANALYSIS tasks
• Index

... In order for FOS to have observed a target, that target must, naturally, have been located in the instrument aperture. ... An FOS Onboard target acquisition: Used either a Binary Acquisition (ACQ/BINARY), a Peakup or Peakdown (ACQ/PEAK), an interactive acquisition (INT ACQ), an early FOS Image (ACQ) or a firmware acquisitions (ACQ/FIRMWARE). ... The overwhelming majority of FOS target acquisitions used the onboard acquisition modes ACQ/BINARY and ACQ/PEAK. ... High wavelength accuracy. ...

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• Photometric Analysis
• FOS Data Handbook
• ACS Data Handbook

Next: Analysis Tools for Nebular Emission Lines . ... 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. ... The direct image is used to locate objects of interest, to find the position of the appropriate spectra in the grism image, to determine the optimal extraction technique to use, and to calibrate the wavelength range of the extracted spectra. ... Figure 1: The NICMOSlook User Interface . ...

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• Calculating the Position and Velocity Components of HST
• Data Modeling and Analysis
• Interactive Fitting of EUVE Emission Line Spectra

XMM-Newton Science Analysis System Page: 1 orbit March 18, 2004 Abstract Create a FITS timeseries \HK-like" le from the ODF Spacecraft Reconstructed Orbit File. ... Both sets of values will be written into a standard OGIP-compliant FITS binary extension table with a TIME column value, derived from a start, stop and sampling interval time, each speci ed by the user. ... StartANDEndNotInODFRange (error) Start AND End times selected not congruent with input ODF obs times. ... 7 Output Files 1. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/orbit.ps.gz

Tail Probe is one of the satellites of the INTERBALL program. ... Collection of the orbital elements | ... Flight situation analysis during operations scheduling . ... Two stages of the orbital situation analysis are presented: . ... The satellites motion calculation during the flight situation analysis is based on the orbital elements, determined by the Ballistic center at KIAM RAN. The modified (by backward integration) orbital elements are usedduring the aposteriory situation analysis. ...

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• INTERBALL AURORAL PROBE SITUATION ANALYSIS
• Two points (INTERBALL-1 and MAGION-4) observations of magnetopause motion
• About modification of the INTERBALL orbital elements

The National Astronomy and Ionosphere Center/Arecibo Observatory is seeking a programmer for the astronomy (radio and radar) program. Under general supervision, develop, maintain, and document spectral line data reduction and analysis software for astronomical research at the Arecibo Observatory. ... The National Astronomy and Ionosphere Center/Arecibo Observatory is operated by Cornell University under a cooperative agreement with the U.S. National Science Foundation. ... Arecibo Observatory . ...

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• Test of Position Switching with a Specified Off Position
• ON/OFF (Position Switching)

... Pre-university education . ... For the year Samara State Aerospace University moved up in the ranking of Vladimir Potanin Foundation from the 44th to the 10th place and added three positions in the ranking of universities reputation Expert RA in the field of Engineering, natural and exact sciences . Samara State Aerospace University has significantly improved its position in the ranking of universities of Vladimir Potanin Charitable Foundation at the end of academic year 2014-2015. ...

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• SSAU rose in the world ranking of universities Webometrics for 1379 positions
• "ANSYS EKM - efficient engineering analysis data management in new product

... Posts tagged ?time series? ... Tags: AstroStat , computer science , job announcement , job market , time series , UC Berkeley . Category: Job , News | ... arxiv:0906.3662] The Statistical Analysis of fMRI Data by Martin A. Lindquist . ... ArXiv] Statistical Analysis of fMRI Data? Tags: data aquisition , experimental design , fMRI , ICA , image analysis , image processing , localization , modeling , pipeline , preprocessing , similarities , Spatial , temporal , time series , voxel . ... 2008? ...

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• ChaMPlane data_archive_.html
• *tvmark* - Mark pixel positions on the display
• IRAF/PROS

reconstruction with Fast Simulation M. Iwasaki University of Oregon At the Sitges meting: tt 6jets 4jets analysis · Charged/Neutral cluster separation with Track- cluster matching · Reconstruction performance in Energy flow analysis · B-tag effect After the meeting: · In FastMC, set the cluster position resolution determined by FullMC · Study Cluster width with FullMC · ...

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• http://zebu.uoregon.edu/~uochep/docs/docs99/Aug99-root.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks00/Iwasaki.pdf
• http://zebu.uoregon.edu/1999/ph161/mflood.html

Chair of solid state physics . ... The most important concepts of the modern crystallography, crystal symmetry and methods of crystal structure determination are considered. ... The main experimental aims of X-ray diffraction study of classic crystal structure and real structure are analyzed. ... Crystal lattice. ... The main diffraction schemes in representation of a reciprocal lattice: Laue method, powder diffraction method, oscillation method, X-ray diffraction on powder sample and single crystal. ...

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• X-Ray Structural Analysis

... This document and the attached postscript figure document an analysis that I did to determine the optimum midpoint and required ranges for both the rotator and azimuth for the 2.5 M telescope. ... I simulate a series of drift scans on the sky for tracks that cover the northern survey area. These tracks cover the range in survey latitude of -60 to +60 degrees, spaced by 10 degrees. ... Along each track the azimuth, elevation, and position angle of the CCD is computed at 1 minute intervals. ...

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• Astrophysical Research Consortium - Apache Point Observatory
• TUI:Tidbits:Entering Sexagesimal Positions
• SDSS Slit-plate Deformation

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

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• Positions and Proper Motions

... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• Armagh Observatory
• Postgraduate Positions

... Exploring the physics of Type Ia supernovae through spectral analysis . ... Their progenitor scenario as well as the details of the explosion mechanism remain a mystery. ... It produces a supernova spectrum for a given luminosity, photospheric velocity, time since explosion and several elemental abundances. Tweaking these parameters to produce a spectrum that fits an observed spectrum is a complex, as of yet, manual task. ... The search space is large and complex. ...

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• COALA - Natsuko Izutani
• COALA - Luke Shingles

... Polarizer efficiency is defined as , where and are the respective measured signals for a polarizer oriented parallel and perpendicular to the axis of a fully polarized beam... angle 12.2 . Polarizer position angle as measured from the NICMOS Aperture Offset Angle of , about the aperture center toward the +U3 axis.. IDL 14.1 . IDL (Interactive Data Language) is an interactive analysis and visualization program written by Research Systems, Inc.... resolution. ...

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• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster

... This file GMRT_FLS_dr1.1.dat 95 3944 GMRT FLS sourcelist of 3944 sources -------------------------------------------------------------------------------- Byte-by-byte Description of file : GMRT_FLS_dr1.1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations ... ------------------------------------------------------------------ 1- 24 A24 --- Name IAU designation of source 27- 28 I2 h RAh Centroid position right ...

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• http://www.mrao.cam.ac.uk/projects/surveys/GMRT/ELAIS-N1/ReadMe
• http://www.mrao.cam.ac.uk/projects/surveys/7C_G/ReadMe_CDS
• http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf

Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences PUL Analysis Center Pulkovo IVS Analysis Center (PUL) 2009 Annual Rep ort Zinovy Malkin, Natalia Miller, Elena Popova Abstract This report briefly presents the PUL IVS Analysis Center activities during 2009 and plans for the coming year. The main topics of the investigations of PUL staff in that period were ICRF related studies, computation and analysis of EOP series, and VLBI2010 related issues. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/bezmenov.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm09c.pdf

... ALMA . ... ARC Staff at ESO . ... The European ALMA Regional Centre (ARC) provides the interface between the ALMA project and the European science community. ... Below you can read the latest Announcements from the European ARC Network.. ... The call for 1-mm Very Long Baseline Interferometry (VLBI) proposals to use phased ALMA at Band 6 in Cycle 4, in collaboration with the Event Horizon Telescope Consortium (EHTC), will be released to coincide with the ALMA Cycle 4 Call for Proposals in March 2016...

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• ESO - Calendars and Calculators
• OYSTER Lab
• Position of RS Pup in the Galaxy (Arstist's Impression) | ESO