... GPI Data Pipeline 1.0 documentation . GPI IFS Data Handbook . Processing GPI Data, Step by Step . ... Wavelength Calibration . ... Using Wavelength Calibrations in the GPI Pipeline . ... Similar to other near-IR spectrographs, GPI uses the well calibrated emission lines of a Xenon lamp (Argon also works for Y-band). ... Most data reduction recipes for raw GPI data will begin by loading a wavelength calibration using the pipeline primitive Load Wavelength Calibration . ...

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• FOS/BL Wavelength Correction Description
• MKFRINGEFLAT: Make Fringe Flats for the STIS CCD Long Wavelength Fringing
• Wavelength Measurements on GHRS Spectra Acquired With FOS

... The first task assumes the searching for chemical composition and sizes of particles which give the wavelength dependence of the extinction efficiencies close to the observed dependence of . Figure 7: Wavelength dependence of the extinction efficiency factors for homogeneous spherical particles of different sizes consisting of astronomical silicate and amorphous carbon. The dashed segment shows the approximate wavelength dependence of the mean galactic extinction curve at optical wavelengths. ...

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• Linear polarization: wavelength dependence
• Optical constant database - Level: data

Next: Rebinning Up: Wavelength calibration Previous: Line search and . ... SET/MOS wlcmtd=IC CALIBRATE/MOS . ... In case you know the central wavelength and the mean dispersion of the grism you used you have to correct the central wavelength for the offset between the center of the CCD and the reference slitlet used by OFFSET/MOS . ... SET/MOS wcenter=central wavelength SET/MOS avdisp=mean linear dispersion SET/MOS wlcmtd=LC CALIBRATE/MOS . ... and adds to .tbl ( linpos ) the columns . ... slit . ...

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• Rebin to wavelength scale
• Wavelength Calibration

... Observatory . ... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > There are few ThAr lines in my wavelength calibration spectra, what do I do? ... Observing Facilities . ... Observing with ESO Telescopes . ... Data Pipelines and Calibrations . ... ESO Data . ... In order to obtain a good wavelength solution with CRIRES, you should have at least two or three ThAr lines visible on each detector, preferably well spaced, at least for a 2nd order polynomial. ...

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• ESO - I heard about problems with the X-shooter wavelength calibration. Where
• ESO - The spectrum of my MOS flux standard star is shifted in wavelength by
• ESO - Where can I find a line-list to use for the wavelength calibration of my

... The minimum precision occurs at x = 0.1 and is approximately equal to precision(1d0)-1. subroutine getBBfluxPerMetre(angstromValues, kelvin, powerValues) real(double), intent(in) :: angstromValues(:), kelvin real(double), intent(out) :: powerValues(size(angstromValues)) end subroutine getBBfluxPerMetre function bbFluxPerMetre(angstroms, kelvin) result(power) real(double), intent(in) :: angstroms, kelvin real(double) :: power end function bbFluxPerMetre . ...

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• Wavelength calibration

Main Page Data Structures File List Data Fields Globals . Data for OI_WAVELENGTH FITS table. ... int . ... char . ... float * . eff_wave . ... eff_band . Data for OI_WAVELENGTH FITS table. int _oi_wavelength::revision . char _oi_wavelength::insname[FLEN_VALUE] . int _oi_wavelength::nwave . float* _oi_wavelength::eff_wave . float* _oi_wavelength::eff_band . The documentation for this struct was generated from the following file: . ...

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• read_fits.c File Reference
• exchange.h File Reference
• write_fits.c File Reference

... People . Posts tagged ?wavelength? ... One of the biggest culprits is the unit of energy, [keV], Continue reading ?keV vs keV [Eqn]? Tags: Angstrom , Boltzmann , EotW , Equation , Equation of the Week , erg , Kelvin , keV , Planck , temperature , units , wavelength . ... 1 Comment . ... Entries RSS . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Alfred Inselberg on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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• The AstroStat Slog multi-wavelength
• Comments on: Grating Dispersion [Equation of the Week] By: vlk By: hlee

Filter : 7 Wavelength : -0.7023 FP1 V: -399.0 FP2 V: -315.0 Abs Wavelength : +7090.2002 Stokes: I LCVR1 Ret : 360.0 LCVR2 Ret : 360.0 LCVR1 Volt : 1.907 LCVR2 Volt : 1.935 Filter : 7 Wavelength : -0.6355 FP1 V: -354.0 FP2 V: -302.0 Abs Wavelength : +7090.2700 Stokes: I LCVR1 Ret : 360.0 LCVR2 Ret : 360.0 LCVR1 ...

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• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2013.1.02/17Aug2013/observing_logs/SN.1.05-JJ_aug17.ibis
• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2013.1.02/17Aug2013/observing_logs/SN.1.01-LF_aug17.ibis
• http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2013.1.03/30Aug2013/observing_logs/observation.ibis

... The calibration of astrophysical spectra in wavelength based on calibration lamp data suffers from different kinds of uncertainties. Besides inaccuracies in the observational phase, common data reduction practice adds ``pixelation'' errors, due to the fact that the centering method does not use the correct PSF. These model mismatch errors depend, for a given feature, on the sub-pixel location of the line center (David & Verschueren, private communication). ...

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• Zero-Points of FOS Wavelength Scales
• The LWS Interactive Analysis (LIA) Package
• ASpect: A Multi-Wavelength Spectrum Analysis Package for IRAF

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Tips on holding a viewing night . ... Multi-Wavelength View of the Interstellar Medium in the Large Magellanic Cloud . ... The Large Magellanic Cloud (LMC) has been surveyed in optical emission lines, X-rays, radio continuum, H I , and CO lines. ... Keywords: Magellanic Clouds - galaxies: ISM - ISM: general - ISM: structure - ISM: bubbles - supernova remnants . ... Structures of the Interstellar Medium in the LMC ...

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• Australia Telescope Compact Array Home Page
• Axis names recognized by GIPSY
• Radio Images of Jupiter

Multi-Wavelength investigations of the Sun and modern problems of solar activity . ... Conference participants: . ... Altyntsev A.T. altyntsev@iszf.irk.ru . ISZF . ... Ussuriysk Astrophysical Observatory RAS . ... Pulkovo Observatory . ... Vasil'eva V.V. solar@narzan.com . MAS Pulkovo Observatory . ... Crimean Astronomical Observatory . ... grechnev@iszf.irk.ru . ... vgrig@iszf.irk.ru . ... Grigor'eva S.A. sgrig@iszf.irk.ru . ... Gubin A.V. gubin@iszf.irk.ru . ... ivanoff@iszf.irk.ru . ...

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To a special Solar Physics issue on the Bastille Day Event: . ... Multi-scale temporal features of the 14 July 2000 meter-wavelength dynamic radio spectrum compared with TRACE data . ... Figure 1 (100 KB). SOHO/EIT (a) and LASCO/C2 (b) images show the region of the eruptive flare event of 14 July 2000 and related halo CME. ... Figure 2 (47 KB). ... Figure 3 (115 KB). Medium-scale dynamic spectrum (a), 204 MHz metric (b) and 3000 MHz microwave (c) profiles of the "Bastille Day" event. ...

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Multi-Wavelength investigations of the Sun and modern problems of solar activity . ... Conference participants: . ... Altyntsev A.T. altyntsev@iszf.irk.ru . ISZF . ... Ussuriysk Astrophysical Observatory RAS . ... Pulkovo Observatory . ... Vasil'eva V.V. solar@narzan.com . MAS Pulkovo Observatory . ... Crimean Astronomical Observatory . ... grechnev@iszf.irk.ru . ... vgrig@iszf.irk.ru . ... Grigor'eva S.A. sgrig@iszf.irk.ru . ... Gubin A.V. gubin@iszf.irk.ru . ... ivanoff@iszf.irk.ru . ...

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• Fabry-Perot Interferometer: Data cubes
• RATAN-600 antenna

.

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• Photovoltaics: Efficiency and Cost Effectiveness
• The Galaxy Gallery Page 6: Comparative Morphology
• Solar Energy

. Wavelength (nm) . To an expert (like me), every bump and wiggle in a spectrum like this tells a story of what the gas is made of, how it’s moving, and how hot it is. Strength of light at this wavelength . Previous slide . Next slide . Back to first slide . View graphic version .

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• The Maths
• Filter Throughput Curves
• Ziggy Telescope Simulator

... spectrum . ffit . ... grids . ... These commands read in a grid of model spectra. ... Values for the parameters are taken from the input models themselves, to avoid mixups. The syntax of the command arguments is precise. model{ . ... If there is only one spectrum to fit, one should set default parameters for the secondary which lie within the model grid, with <L_2/L> being a very small value. ... The output is saved in a file <file.fit> , where <file> was the name of the spectrum being fitted. ...

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• Spectrum v1 - Examples
• Simon Jeffery's Software Store: PHOT library
• Armagh Observatory

... The following table gives the sensitivity of field center, distortion, and image size to various misalignments of the optical elements in the 2.5 m telescope. ... The repointing is done so as to keep the center of the focal plane pointed to the same position on the sky. ... Field shift (this is the mean shift in object positions in the focal plane before repointing the telescope) . ... Image properties are measured for an array of points in the focal plane. ...

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• G191-B2B
• Feige 66
• BD+75 325

... Астронет | ... рда.) область сантиметровых волн (длин волн) . ... рда.) сантиметровый диапазон (длин волн) . ... рда.) область декаметровых волн (длин волн) . ... рда.) декаметровыи диапазон (длин волн) . ... рда.) область дециметровых волн (длин волн) . ... рда.) дециметровый диапазон (длин волн) . ... рда.) область метровых волн (длин волн) . ... рда.) метровый диапазон (длин волн) . ... рда.) область миллиметровых волн (длин волн) . ... рда.) область субмиллиметровых волн (длин волн) . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Страница 25
• Астронет > NGC 1512: A Panchromatic View

... Bionic eyes. If our eyes could see in different wavelength bands, this is what the Sun would look like. ... Visible light, crucial to photosynthesis, is a type of radiation. ... At the heart of this revolution is the recognition that light travels as a wave. ... Dreams of Fields . ... By the time the fields go from strong to weak and back to strong, the wave has moved a certain distance, known as the wavelength. ... Red light, blue light, infrared light, ultraviolet light, radio waves, x-rays ? ...

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... R2022 Date Received: 2004-Sep-28 07:22:59 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Planetary Radar Radar Solar System 80 Hours Radar Mapping of the Moon at 70-cm Wavelength Using Arecibo and the GBT We request 80 hours of observing time at Arecib o and the GBT to complete a 70-cm wavelength, dual circular p olarization, radar image mosaic of the near side of the Mo on. ... Part of the observing run. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/CampbelltagR2102tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/CampbelltagR2955tp.pdf
• bmwidthVsLambda