... This paper describes various methods for the analysis of spectroscopic data, particularly as they relate to wavelength calibration of echelle-format spectra. ... Keywords: spectroscopy, Hough transform, wavelet transform, robust regression, echelle, wavelength calibration . ... Wavelet transform can be useful in complementing robust techniques for multiresolution analysis, and Section 4 presents an application of the Mexican hat transform to the detection of spectral features. ...

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• QPSIM: An IRAF/PROS Tool for Source Simulation
• Calculating the Position and Velocity Components of HST
• Automated Software for Slitless Spectroscopy Analysis and Quasar Selection

... HST . ... Data . ... HST Peer Review Process . ... HST Overview . ... Retrieving HST Data . ... Image Quality . ... Software Tools . ... Q.: Where can I find the newest version of the NICMOS reduction software CALNICA and CALNICB? ... Q.: I get this error from calnicb: tprint all1_asn.fits # Table all1_asn.fits[1] Mon 07:48:25 16-Mar-98 # row MEMNAME MEMTYPE MEMPRSNT # 1 N3V701Q1M EXP-TARG yes 2 N3V701Q1M EXP-TARG yes 3 N3V701Q1M EXP-TARG yes 5 N3V701Q1M EXP-TARG yes 6 all1 PROD-TARG yes . ...

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• NICMOS Background
• COS/FUV Lifetime Position 3 Line Spread Functions and Cross-dispersion Spread
• Index

The FITS archive & data processing pipelines . ... The archived data are broad band images (BBI) and long-slit spectra (LSS) plus their associated template and calibration files. The data in HFA can enter into the HyperLeda processing pipeline and the results can be freely downloaded. ... Definition of the file system (structure of the archive) . ... The coordinate systems must be updated when the data (pixel data, other keywords, related tables) are altered (eg. rebinning of the image). ...

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• echelle
• Background Correction

XMM-Newton Science Analysis System Page: 1 orbit November 22, 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/6.0.0/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/7.0.0/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/orbit.ps.gz

Next: The STScI NICMOS Calibration Up: No Title Previous: CONICA: The high resolution . The STScI NICMOS Calibration Pipeline . Introduction . ... Dark Current Subtraction . ... Input Data . ... Scalar Background Subtraction . 2-D Background Subtraction . ... Status and Goals of the NICMOS Calibration Plan . ... Photometry . ... Photometric Performance of NICMOS . ... NICMOS Photometry. ... ST-ECF Grism Spectrum Software for NICMOS Grism Data . ... Analysis . ... STScI NICMOS Software . ...

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• STScI NICMOS Software
• NICMOS Software at the University of Arizona
• ST-ECF Grism Spectrum Software for NICMOS Grism Data

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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Global VLBI data processing results . ... In this paper we briefly describe the QUASAR software for VLBI data processing created in IAA RAS. The estimation parameters and results of global solution obtained with QUASAR software are shown. The first results of involving QUASAR software into IAA EOP service for EOP and station positions calculation are discussed. ... VLBI, data processing, global parameter, EOP. ...

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• LAB Ephem. Astronomy-ERA
• Keywords_32
• Keywords_284

Program: TRACE Purpose: TRACE plots image values at user given positions as function of distance to a plot centre (in 2-d (sub)sets). Category: ANALYSIS, PLOTTING File: trace.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (, subset): Only one subset is allowed. ... XYBOX= Give size of box around one pixel: [3,3] The resulting value at a selected position is an average of the pixels in the defined box around that position. ... POSITION= Give position x, y: Physical values are allowed. ...

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• Source Fitting and Positions
• Event-driven Tasks and Graphical User Interfaces
• World Coordinate Systems (WCS) in FITS

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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• Shades and Apparitions: Toward an Inventory of Cold Hydrogen Clouds
• sefdPolB_dec07
• ON/OFF (Position Switching)

For all keywords that contain a red and a blue value, the blue value comes first. ... The full pathname, but without the trailing "b.fit" and "r.fit", that would be given to the next exposure if the basename argument is not given to the expose command. ccdHeaters=float,float . ... bluelambda2=float [M] . The center wavelength for the given grating: the 1 or 2 indicates the grating bay. The bluelambda and redlambda keywords match one set of these, depending on the position of the turret. ...

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• Mirror Controller Actor
• TUI:Telescope:User Catalogs
• MCP Menu documentation

Contents] [Prev page] [Next page] [Index] . ... Positioning HTML Content Using Styles . Positioning HTML Content Using the <LAYER> Tag . ... Absolute Positioning . ... Creating Positioned Blocks of Content Dynamically . Writing Content in Positioned Blocks . ... Positioning the Flower Layers . Positioning and Moving the Fish and Poles . Defining the onLoad Handler for the BODY Element . ... Adding Another Layer to Contain the Reverse Fish Image . ... The Initialization Functions . ...

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• Colors and backgrounds
• Keyword arguments and default arguments
• Long description for example illustrating absolute positioning

... This chapter deals with analyzing source positions and spatial structure and with image calibration. ... See Table 6.1 for the dimensions of ROSAT and Einstein images: . ... ROSAT . ... Einstein . ... imcnts* - Find background subtracted counts for a point source . ... imexamine* - General analysis of image containing many sources . ... Radial Profiles and Projections . imcnts* - Radial Profile of an extended source at the field center . ... imcnts* - Azimuthal profile of an extended source . ...

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• *imexamine* - General analysis of image containing many sources
• The Lynxx Tools
• Spatial Region Coordinates

Software Forum Message . Forums: . ... Discussion Forums | Astronomy Software Discussion | Post . ... Star Positions.. Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Where Is ETX 90EC Focal Plane Positioned? - an Astronomy Net Meade Equipment
• I Think What You're Saying Is Not A Deeply-considered Position - an Astronomy
• Modern Optical Design And Analysis Software, AstroGuide Listing

... 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
• The HST Guide Star Catalog

The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the following articles and reports, which are available online . Mills, D.L. Internet time synchronization: the Network Time Protocol. ... Mills, D.L. Network Time Protocol (Version 3) specification, implementation and analysis. ...

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• Astronomical Links
• Net Search
• Sternberg Astronomical Institute

On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

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• Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA
• OptInt PmWiki : Production Software PDR To Do List | History
• OptInt PmWiki : Analysis Software

Pulkovo NEO Page . Central Astronomical Observatory at Pulkovo . ... NEA Accuracy Estimation . Positions of the asteroids that have been sent by observers to the Minor Planet Center are automatically processed by means of calculation of (O-C) values with the help of the EPOS software package created at Pulkovo Observatory. ... Here attention is paid to observations of the near-Earth asteroids. This work was initiated by Dr. O.Bykov at Pulkovo Astronomical Observatory. ...

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• Pulkovo NEO Page: Ephemeris Support

... 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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• ESO - How do I interpret the SEQ TIME keyword values?
• FORS Sec Std and Abs Phot Project
• Jeremy R. Walsh's Home Page

... 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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• CHIANTI: A Database for Astrophysical Emission Line Spectroscopy
• SDSSmosaic
• NICMOS3 Detector for Spectroscopy

... During all period of our investigations Dr. N.Sumzina from the Institute of Applied Astronomy of RAS had prepared the Numbered Minor Planet positions from MPC Database for our processing with kind permission of the Director of Minor Planet Center Prof. Braian Marsden. ... Our extensive processing of the MPC data allows us to conclude that CCD observations of the Numbered and Unnumbered Minor Planets have the errors, sometimes very crude. ...

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