Next: Refining the Dispersion Up: Getting the Dispersion Previous: Determination of the . Midas.. ... PLOT/RESIDUAL . displays the residuals (column :RESIDUAL in table line.tbl ) as a function of wavelength. ... plots the dispersion relation and the residual value as a function of the wavelength. Note that PLOT/RESIDUAL and PLOT/DELTA display the rms of the residuals. It is also possible to display, for all rows, the residuals for a given line of wavelength ``wavelength'' with: . ...

Еще в разделе: (Показать все результаты (>2326) - www.sao.ru/ )

• Wavelength calibration
• Identify the lines in one of the rows of the spectrum
• Getting the Dispersion Solution

Next: Determination of atmospheric parameters Up: Optical spectrum of IRAS04296 Previous: Radial velocity of the . From comparison of observed and synthetic spectra of IRAS04296 we revealed some strong absorptional features whose positions coincide with known diffuse interstellar bands (DIBs) (Jenniskens et al., ... In Fig. 5 we illustrate the presence of DIB's by showing a spectral region of IRAS04296 . ...

Еще в разделе: (Показать все результаты (>689) - jet.sao.ru/ )

• Radio sources identfification
• Atlas and list of identified lines
• Laboratory of spectroscopy and photometry of extragalactic objects : Devices

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. ...

Еще в разделе: (Показать все результаты (>234) - www.stecf.org/ )

• NICMOS Data Calibration and Analysis

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 . ...

Еще в разделе: (Показать все результаты (>1662) - www.adass.org/ )

• Identification and Analysis of Binary Star Systems using Probability Theory
• ADASS 2003 Conference Proceedings
• Robust Data Analysis Methods for Spectroscopy

... We also identified two other spectrally unique terrains, corresponding to the northern polar ice cap, and to the southern winter polar hood. Comparisons with mineral spectra indicate the possibility of different H 2O- or OH-bearing (i.e., hydroxides and/or hydrates) minerals existing both in northern Acidalia and in the nearby intermediate albedo terrain. Hydrated minerals do not appear to be spectrally important components of the southern hemisphere dark terrains imaged by HST in 1997. ...

Еще в разделе: (Показать все результаты (>17560) - www.stsci.edu/ )

• Checking Whether Your Data Needs to Be Recalibrated
• Identification of Erroneous Doppler Compensation for Moving Targets
• ACS Instrument Handbook for Cycle 20

Next: Identifications and Efficiency Up: THE DEEP X-RAY RADIO Previous: Source Classification . ... For some sources which did not have NVSS positions before the time of optical observations, arcsecond positions from the Texas survey (Douglas et al. 1996) and NED (typically based on VLA data) were used. ... All X-ray/radio sources without counterparts on the survey plates were imaged at either the KPNO 0.9m or the CTIO 0.9m telescopes. ... Previously Identified Sources . Sample Properties . ...

Еще в разделе: (Показать все результаты (>45106) - www.eso.org/ )

• Allocate/load STARTABLE
• Adding plot variables
• Identifications and Efficiency

Next: Flux calibration Up: Generation from In-Orbit Data Previous: Generation from In-Orbit Data Contents . The calibration is based in the identification of spectral features in the observed spectra of F-type stars for the UV grism and BPM 16274 for the Visible one. ... The CCF table is obtained by applying the polynomial to a monotonic array representing the pixels array in the extracted spectrum. Michael Smith 2011-09-20 ...

Еще в разделе: (Показать все результаты (>7893) - xmm.vilspa.esa.es/ )

• Procedure
• Home Page
• Description

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Equatorial coronal hole (top left), polar CH (top right), quiet Sun (bottom left) and quiet Sun with TCHs (bottom right) with the positions of all the corresponding identified brightening pixels over-plotted. ... We found that in comparison to the quiet Sun, the boundaries of coronal holes are abundant with brightening events including areas inside the coronal holes where closed magnetic field structures are present. ...

Еще в разделе: (Показать все результаты (>1456) - star.arm.ac.uk/ )

• Research Activity and Funding Trends
• ISS and an unidentified satellite | International Year of Astronomy in Ireland
• Performance

... The package AMPLE (Adaptable Minor Planet Ephemerides) is dedicated to solving a number of problems concerning minor planets with the aid of IBM-type personal computer. ... Obtaining selection of orbital elements and/ or photometric parameters of minor planets in conformity with imposed restrictions. ... The orbital elements of all minor planets used in AMPLE for 2015 have been determined in IAA on the ground of available observations in the catalogue of observations of the Minor Planet Center. ...

Еще в разделе: (Показать все результаты (>437) - www.ipa.nw.ru/ )

. email: rgonzale@naic.edu

Еще в разделе: (Показать все результаты (>3801) - www.naic.edu/ )

ASKAP Early Science Workshop ASKAPEnnitegrrngtiommissionrnfication I g nee i a Con & Ve i i g Adam MacLeod ASKAP System Engineer Oct 2015 ASKAP ASKAP Commissioning -ASKAP Commissioning Plan V2.0 about to be released. Identifies three major activities: - Integration & Verification - Commissioning - Early Science -Also identifies: - Relationships between activities - Relationships between the teams Commissioning Strategy - An iterative process as PAF Systems and backend capabilities are rolled out. ...

Еще в разделе: (Показать все результаты (>6676) - www.atnf.csiro.au/ )

• http://www.atnf.csiro.au/computing/software/gipsy/sub/grslct.dc3
• http://www.atnf.csiro.au/research/WALLABY/Wallaby2011/SIM-FEST2011-RJurek.pdf
• Task Version Identification

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

Еще в разделе: (Показать все результаты (>52) - vega.inp.nsk.su/ )

• Astronomical Catalogues
• The HST Guide Star Catalog

... Comparison of a synthetic radio image and quaтАж . ... Title: Comparison of a synthetic radio image and quasar 3C 48 . Description: Comparison of a synthetic radio image (left panel) derived from the movie "Movie 1" and a VLBI image of the qusar 3C 48 (the second quasar discovered). ... Comparison of a synthetic radio image and quasar 3C 48 Comparison of a synthetic radio image (left panel) derived from the movie "Movie 1" and a VLBI image of the qusar 3C 48 (the second quasar discovered). ...

Еще в разделе: (Показать все результаты (>408) - www.mso.anu.edu.au/ )

• Identifier Index
• PPT Slide
• Siding Spring Survey

... 251G: GUEINOV O.KH. and ZEL'DOVICH YA.B. Collapsed stars in binary systems. abstract from ADS when it exists. Total number of objects found: 7 . Currently displayed are the first identifier in SIMBAD and the object type. By clicking on the [Dic CAT] anchor, you get the informations from the nomenclature dictionnary for the corresponding catalogue. ... Emission-line Star.. Dic HD] #2.. ... Semi-regular pulsating Star.. ... Spectrocopic binary.. Dic SKY#] #4.. ... Wolf-Rayet Star.. ...

Еще в разделе: (Показать все результаты (>275) - xray.sai.msu.ru/ )

... are preliminary IAU-style names for ChaMP objects. Finalization of names awaits the final systematization of optical coordinates and source identification. ... The yellow regions highlight atmospheric telluric bands at ~6900A and ~7600A. The optical ID, X-ray ID, classification, and redshift are given at the top of each plot, and a series of lines are shown that are often found in sources of that given classification. ... HS limit? ... g' band magnitude; calibrated SExtractor Kron mag or limit . ...

Еще в разделе: (Показать все результаты (>1613) - hea-www.harvard.edu/ )

• The AstroStat Slog identification
• Spectroscopic Data
• HST/FOS Atlas of AGN and Quasars

... 1100 FTT/NAS . ... 1120 Camera . ... 1140 Camera Mount & Enclosure . ... 1170 Test Equipment . ... 1200 FLC . ... MRO-PLA-CAM-0000-0106 FTT/NAS & FLC Development Plan . ... MRO-ICD-CAM-1000-0109 "FTT/NAS,FLC-UTE" FTT/NAS & FLC to Enclosure ICD . MRO-ICD-CAM-1000-0110 "FTT/NAS,FLC-NOT" FTT/NAS & FLC to optical table ICD . MRO-ICD-CAM-1000-0111 "FTT/NAS,FLC-UT" FTT/NAS & FLC to UT optical ICD . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIFastTipTilt/DocMan) ...

Еще в разделе: (Показать все результаты (>1214) - www.mrao.cam.ac.uk/ )

• OptInt PmWiki : Doc Man
• The quasar fraction in a sample of giant radio sources
• Emily Curtis

... General Catalog of Variable Stars (GCVS database, Version 2012 Feb.) ... The cross-identification tables of the General Catalogue of Variable Stars (GCVS) contain all GCVS (including extragalactic variables from vol.V), NSV (New catalogue of Suspected Variable stars) and Supplement to the NSV stars as well as stars from the name-lists of variable stars nos. 67 - 80; it also makes it possible to find out identifications between the GCVS and the NSV catalogue. ... I-III) names are included. ...

Еще в разделе: (Показать все результаты (>57) - sai.msu.ru/ )

• General Catalogue of Variable Stars: What's new.

DIS-III Spectra Other information . ... LOW Blue . ... MED Blue . ... HIGH Blue . ... Lines / mm . ... 5.03е /pix . 2.43е /pix . 2.26е /pix . 1.23е /pix . 0.84е /pix . 0.62е /pix . ... 7.0 е /pix . 3.05е /pix . 3.15е /pix . ... 1.17е /pix . ... Spacial scale for Blue gratings are: 0.42 arc-sec/pixel . ... 300 lines/mm . Low Blue . ... Med Blue . ... 0.9 " slit . ... unidentified . ... Offset Directions for DIS Using Various Interfaces as viewed by the Slit Camera . ...

Еще в разделе: (Показать все результаты (>479) - www.apo.nmsu.edu/ )

• Astrophysical Research Consortium - Apache Point Observatory
• ar_lamps
• Untitled Document

Modules | ... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... Allows "anonymous" user access to authenticated areas . ... This module provides authentication front-ends such as mod_auth_basic to authenticate users similar to anonymous-ftp sites, i.e. have a 'magic' user id 'anonymous' and the email address as a password. ... Anonymous . ... Anonymous user [ user ] .. ... Specifies whether the user must specify an email address as the password. ...

Еще в разделе: (Показать все результаты (>8535) - www.arcetri.astro.it/ )

• CHIANTI atomic database
• mod_version - Apache HTTP Server

Peremennye Zvezdy", . ... Min . ... 2MASS J16480306-6715178 . ... The variable star catalogued as ASAS 164802 6715.2 by Pojmanski (2002) was found to display two types of eclipsing variability by Pilecki and Szczygiel (2007). ... The comparison stars (identified in the finding chart) used were: . ... The data for Star A and B has been obtained using Comp Star 2 between HJD 2455709.956 and 2455710.089 and between 2455718.005 and 2455718.096. All other data was obtained using Comp Star 1. ...

Еще в разделе: (Показать все результаты (>22172) - www.astronet.ru/ )

• Астронет > Identify this Phenomenon
• How to Identify that Light in the Sky
• Identify this Phenomenon