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http://www.arcetri.astro.it/science/chianti/chianti_5.1/ch_v3.html.
http://www.arcetri.astro.it/science/chianti/chianti_5.1/ch_v3.html.
1. QSO Absorption Lines and Other Cosmological Probes
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Ссылки http://zebu.uoregon.edu/1997/ph410/l22.html -- 12.7 Кб -- 10.03.1997
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2. Broadening of Si VIII lines observed in the Solar polar coronal holes
... We study the variation of the line width and electron density as a function of height above two coronal holes from forbidden spectral lines of Si VIII. The spectra were obtained with the Solar Ultraviolet Measurements of Emitted Radiation spectrometer flown on the Solar and Heliospheric Observatory spacecraft. ... The electron density shows a decrease from 1.1 10 8 cm -3 to 1.6 10 7 cm -3 over the same distance. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract291.html -- 3.3 Кб -- 23.07.1998
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3. High Line ? Solar Observing ? Amateur Astronomers Association of New York
... Observing . ... Home Observing High Line ? Solar Observing . ... High Line . High Line - Solar Observing . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... The AAA hosts solar observing on the High Line one Tuesday afternoon each month from April through August. ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
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Ссылки http://www.aaa.org/observing/solar-observing-on-the-high-line/ -- 97.2 Кб -- 10.04.2016
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4. Spectral-Line Observing
... We will consider the rms, (K), for observations with a receiver of system temperature, T , frequency resolution, per polarization, and total integration time per observing cycle, . ... For ``in-band'' frequency switching, the line under investigation is always in the observing band. ... Position Switching or ``Out-of-Band'' Frequency Switching: Here the line is only observed for one half of the time, with noise being present all of the time. ...
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Ссылки http://www.naic.edu/~astro/guide/node15.html -- 10.0 Кб -- 22.02.2012
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5. Spectral Line Processing and RPFITS files
Next: Spectral Line Processing and Up: Spectral Line Data Reduction Previous: ATCA Spectral Line Correlator . ... The ATCA allows you to observe two frequency setups simultaneously ifsel allows you to load just one of them by setting ifsel=1 or ifsel=2 . ... The RPFITS file does not contain the rest frequency of the spectral line observed, so you need to give this at some stage during data reduction - the earlier the better. The rest frequency can be entered (via restfreq , in GHz) in atlod . ...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node137.html -- 6.6 Кб -- 10.04.2016
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6. Line parameter measurements
Next: Results of follow-up spectroscopy Up: Data reduction Previous: Reduction of the Calar . In the final spectra, redshifts and line fluxes are measured within MIDAS, applying Gaussian fitting to the emission lines. To determine redshifts for individual galaxies, averages are taken over the prominent individual emission lines (mostly H , H , [O III ] 4959,5007 ?) The line [O II ] 3727 ? ... For all spectra, the individual emission line fluxes of the H , [N II ] 6548,6583 ? ...
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Ссылки http://www.sao.ru/precise/Laboratory/Publications/2000/HSSIII/node8.html -- 6.0 Кб -- 08.02.2000
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7. CHIANTI atomic database
... 1998, ApJ , 503, 467 % Observed energy levels (6,7,8): from the line list of Thomas Neupert, 1994, ApJS, 91, 461 % Observed energy levels (level 9): from the line list of Young, Landi Thomas, 1998, A , 329, 291 % Observed energy levels (level 15): from the line list of Brosius, Davila Thomas, 1998, ApJS, 119, 255 % Observed energy levels (level 37): from the line ...
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Ссылки http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/fe/fe_17.html -- 5.2 Кб -- 15.09.2005
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8. Command line interface to libAIR and water vapour column retrieval Bojan
... Bojan Nikolic web pages (r. 329) . ... Since version 0.12, libAIR comes with a simple command line interface to the routines which retrieve the water vapour and the phase correction coefficient. Currently only the very simplest model is supported, in which the all of pressure, temperature and water vapour column are free parameters, and they are inferred from the four observed water vapour radiometer readings. ... Command line interface to libAIR and water vapour column retrieval . ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/libaircmdline.html -- 10.4 Кб -- 04.04.2016
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9. Interactive Fitting of EUVE Emission Line Spectra
... An interactive IRAF task for the analysis of Extreme Ultraviolet Explorer ( EUVE ) emission line spectra is presented. The line flux in extracted spectra may be measured by multiple techniques, including fitting individual lines. ... To aid in identifying lines, the positions of known lines may be marked on the spectrum during the fitting process. Also, model EUVE spectra may be constructed and overlaid using plasma emissivities and source emission measures supplied by the user. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/abbottm.html -- 8.6 Кб -- 03.11.2000
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10. Absorption line spectra of the UV bright z=2.4 QSO HE 1122-1649
... We present ultraviolet and optical spectra of the bright (V=16.5), high-redshift ( ) QSO HE1122 - 1649 (Reimers et al. 1995a,1995b). ... Keywords: absorption lines . ... The combined data are shown in Figure 1. ... The Ly profile reveals an absorbing subcomponent at in agreement with results from heavy element absorption lines detected in the high resolution optical data. ... Figure: Velocity profiles of heavy element absorption lines arising in the damped Ly system as seen in the optical data. ...
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Ссылки http://www.stsci.edu/stsci/meetings/shst2/koehlers.html -- 14.3 Кб -- 15.06.2005
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11. http://hea-www.harvard.edu/QEDT/Papers/phl909.ps
Emission Line Diagnostics in a ``No UV Bump'' Quasar PHL909 Smita Mathur, Belinda Wilkes, Martin Elvis and Jonathan McDowell Abstract PHL909 is a quasar with unusually low ultraviolet luminosity (blue bump strength C UV=IR = \Gamma0:20 compared to an average value of 0:4 (McDowell et al. ... The intrinsic continuum of PHL909 ( i.e. as seen by the BELR ) may thus be similar to the `standard' continuum, with a big blue bump, reddened along the line of sight. ...
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Ссылки http://hea-www.harvard.edu/QEDT/Papers/phl909.ps -- 136.1 Кб -- 09.09.1994
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12. ESO - How can I correct telluric absorption lines in the Reflex science end
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How can I correct telluric absorption lines in the Reflex science end products? ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Data Products Forum . ... A software tool to fit and correct the telluric lines directly in your science spectra without the needs of using an observed telluric standard star is available at http://www.eso.org/sci/software/pipelines//skytools/ . ...
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Ссылки http://www.eso.org/sci/data-processing/faq/how-can-i-correct-telluric-absorption-lines-in-the-reflex-science-end-products.html -- 23.0 Кб -- 10.04.2016
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13. Fabry-Perot Interferometer: Gallery Old
... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...
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Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 Кб -- 02.10.2012
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14. http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/README
... 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., ...
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Ссылки http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/README -- 7.8 Кб -- 26.03.2000
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15. The Acceleration of the Aurora
The "ring of fire" seen by satellite cameras around the polar caps (picture below) is probably created by electrons leaking from the tail's plasma sheet, whose magnetic field lines form a somewhat imperfect trap. ... One possible explanation involves the close association between auroral arcs and electric currents which flow along field lines between the ionosphere and distant space ( Birkeland currents ). ... That produces an extra resistance to the flow of current. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/waurora2.html -- 8.5 Кб -- 21.12.2007
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16. Slim Line Series - Weather Stations - Products
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Meade 4M Community . ... Meade Instruments . ... Telescopes . LX850 Series . ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado Accessories . ... Weather Stations . ... Slim Line Series . ... Dealer Locator . ... Become a Meade Dealer . ... Slim Line Weather Stations (3) . ...
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Ссылки http://www.meade.com/products/weatherstations/slimline.html?dir=asc&order=price -- 90.5 Кб -- 10.04.2016
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17. SKY-MAP.ORG
SKY-MAP.ORG
18. Line (ImageJ API)
... java.lang.Object ij.gui.Roi ij.gui.Line . ... public class Line . ... int . ... protected double . ... Constructor Detail public Line (int ox1, int oy1, int ox2, int oy2) . Creates a new straight line selection using the specified starting and ending offscreen integer coordinates. public Line (double ox1, double oy1, double ox2, double oy2) . Creates a new straight line selection using the specified starting and ending offscreen double coordinates. public Line (int sx, int sy, ImagePlus imp) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/gui/Line.html -- 37.4 Кб -- 02.12.2010
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19. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/e0102_plucinsky.pdf
Chandra X-Ray Observatory CXC 1E0102.2-7219 as a Standard Candle for X-ray Astronomy Paul Plucinsky, Joseph DePasquale, Steven Snowden Paul Plucinsky 1 ICWG June 2006 Chandra X-Ray Observatory CXC Why Use E0102 as a Calibration Source for X-ray Astronomy? ... Paul Plucinsky 2 ICWG June 2006 Chandra X-Ray Observatory Gratuitous Pretty Pictures of E0102 S3 Summed Data ~100 ks True Color Image CXC Paul Plucinsky 3 ICWG June 2006 Chandra X-Ray Observatory Spectral Model: Calibration vs. ...
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Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/e0102_plucinsky.pdf -- 1215.8 Кб -- 19.06.2006
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20. Globular clusters with anomalously small masses, figures
... The relationship of the mass and the observed galactocentric distance R -- (a), and that of the mass and the total dissipation velocity n taken from Gnedin, Ostriker (1997) -- (b). The dotted line in diagram (a) shows the "cone of survival" according to the paper by Surdin and Arkhipova (1998) . ... The solid line is a regression stright line for the main sequence of clusters, and the dotted line parallel to it separates the sequence of clusters of anomalously small mass shown by open triangles. ...
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Ссылки http://ip.rsu.ru/~marsakov/paper8/p8fg1_1.htm -- 2.9 Кб -- 02.02.2007
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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