... 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 . ...

... 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. ...

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 . ...

... 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. ...

... 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 . ...

... 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) . ...

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: . ...

Filter : 2 Wavelength : -0.6221 FP1 V: -139.0 FP2 V: +24.0 Abs Wavelength : +8541.4326 Stokes: I LCVR1 Ret : 360.0 LCVR2 Ret : 360.0 LCVR1 Volt : 1.640 LCVR2 Volt : 1.689 Filter : 2 Wavelength : -0.3662 FP1 V: +4.0 FP2 V: +65.0 Abs Wavelength : +8541.6934 Stokes: I LCVR1 Ret : 360.0 LCVR2 Ret : 360.0 LCVR1 Volt : ...

... 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). ...

... 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 ...

Multi-Wavelength investigations of the Sun and modern problems of solar activity . SAO RAS . ... 8-87878-46436 (the secretary of director of SAO RAS) . Phones in SPb Branch of SAO RAS: . 8-812-7234038 (the secretary in SPb Branch of SAO RAS) . ... 8-87878-46571 (in SAO RAS) and 8-812-3882346 (in SPb Branch of SAO RAS) . ... To Bogod Vladimir Mihailovich vbog@gao.spb.ru and also vbog@sao.ru . ... Copyright © 2006 SAO RAS . ... RAS | ... MAO RAS | ...

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 . ...

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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... 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. ...

... 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) . ...

... 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 ? ...

... RR2102 Date Received: 2005-May-24 07:32:55 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Planetary Radar Radar Solar System 18 Hours Radar Mapping of the Moon at 70-cm Wavelength Using Arecibo and the GBT We request 18 hours of observing time at Arecib o and the GBT over the coming trimester to (1) continue to compile a ... Part of the observing run. ...

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. ...