... V.E.Antonov, T.E.Antonova, I.T.Belash, A.E.Gorodetskii, E.G.Ponyatovskii . ... V.E.Antonov, T.E.Antonova, I.T.Belash, V.G.Tissen . ... B.Zhang, H.J.Bauer, M.Baier, F.E.Wagner, V.E.Antonov, T.E.Antonova . ... M.Baier, R.Wordel, F.E.Wagner, V.E.Antonov, T.E.Antonova . ... G.Schneider, M.Baier, F.E.Wagner, V.E.Antonov, T.E.Antonova, Yu.Kopilovskii, E.Makarov . ... B.Zhang, I.Dugand?i?, H.J.Bauer, M.Baier, F.E.Wagner, V.E.Antonov, T.E.Antonova, S.M.Filipek . ... LHPP ISSP RAS © 2004 All rights reserved ...

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• Spectroscopy of Semiconductors and Dielectrics
• Laboratory for Spectroscopy of Molecular Structures
• Laboratory of spectroscopy of defect structures ISSP RAS

is split into spectral colours, corresponding to wavelength. Red light has long wavelengths, blue light has short wavelengths. from hot objects are continuous , like a rainbow . atoms only emit light of specific colours, revealing their fingerprints as a line spectrum . atoms in front of a hot object absorb light at these colours, giving an absorption spectrum . are predominantly absorption spectra . next

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• Index of /preprints/2014/654/spectroscopy Rats-kepler - A variability survey of
• Armagh Observatory Preprint No. 305
• Armagh Observatory Preprint No. ???

We would like to announce the release of Version 3.03 of the CHIANTI database for astrophysical spectroscopy. This now extends the database to include the 1 - 50 wavelength region. The additions to the database are described in a paper `CHIANTI - an atomic database for emission lines, IV - Extension to X-ray Wavelengths' by K.P. Dere, E. Landi, G. Del Zanna, and P.R. Young and accepted for publication by the Astrophysical Journal Supplement Series. ... Atomic Data Updates (April 30, 2001) . ...

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• CHIANTI atomic database

. Name . Last modified . Size . Description . Parent Directory . - . DRD26a_ESPRESSO-Paranal_ICD_VLT-ICD-ESO-13529-5412_Issue_4.docx . 31-Mar-2016 15:31 . 31M . Thumbs.db . 31-Mar-2016 11:24 . 228K .

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• ESO - Thesis Topic: Use of CO rotational vibrational absorption spectroscopy to
• Spectroscopy
• ESO - ESO Working Group on the Future of Multi-Object Spectroscopy

... In Spiral . Between spiral . ... Center of vortices . ... to density exterema . ...

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• The peculiar post-AGB supergiant IRAS04296+3429: optical spectroscopy and its
• Laboratory of spectroscopy and photometry of extragalactic objects : Devices
• NES Stellar Spectroscopy Laboratory

Detector of hydrogen isotopes (ISIV) . ... Measurements of hydrogen isotopes content in surface layer of a solid (provided that the content is more than 0.01 %). ... Content of hydrogen isotopes of a sample is measured by nondestructive technique of direct measurements in the surface layer. ... Measurable hydrogen isotopes content ? ~0.01 wt. ... Area surface of sample ??????????????????????????????????????? ~10 cm 2 . ... G. Dolnikov +7(495)333-25-66, ggd@iki.rssi.ru . ...

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• ATR-spectroscopy aboard landers MATROS
• Space Research Institute (IKI) Seminar
• Instrumentation for Fundamental and Applied Space Projects

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Astrophysics graduate student programs . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Parkes radio telescope webcam . ... A detailed activity for studying different types of spectra in the laboratory using a spectroscope will be posted up here shortly. ... Absorption Spectroscopy uses Macromedia Shockwave in a web browser to simulate spectra from discharge tubes of different...

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• Spectroscopy
• Galaxy Lunch - Laboratory Spectroscopy for Herschel, ALMA and the Cologne
• Multi-object spectroscopy of the field surrounding PKS 2126-158 - discovery of

On 19/20 October 1995 we used GRIM II to attempt spectroscopy of the 2.3 micron CO absorption band in stellar clusters. ... Read Noise Our typical backgrounds in 60s were about 100 DN (about 500 e), and so for faint objects our noise is utterly dominated by the read noise of about 110 e. We can think of three ways to improve this situation: integrate longer; reduce the read noise; or implement multiple reads. ... Flats The quartz lamps were too dim for flats. ...

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... Астронет | ... Карта неба | ... планета Астронет | ... Водородное небо . ... Пояснение: Межзвездное пространство заполнено чрезвычайно разреженными газовыми облаками, состоящими в основном из водорода. ... NASA Web Site Statements, Warnings, and Disclaimers . ... Публикации с ключевыми словами: sky map - hydrogen - interstellar medium - звездные карты - водород - Межзвездная среда . Публикации со словами: sky map - hydrogen - interstellar medium - звездные карты - водород - Межзвездная среда . ...

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• Астронет > Neutron Mars
• Астронет > Hydrogen burning cycles
• Астронет > Ne and Al cycles of hydrogen burning

MFS . Data archive MFS . ... Data archive HSFA . ... Catalogue of solar flares . Atlas MFS . Data archive MFS [FTS, AVI] . Data MFS-2009 . Data MFS-2010 . Data MFS-2011 . Data MFS-2012 . Flares archiv with asymmetry absorption . ... Catalogue of prominence 2011 . Catalogue of prominence 2012 . ... Data MFS-2013 . Data MFS-2014 . Data MFS-2015 . ...

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• Solar Optical spectroscopy -Links

. Sorry, this page is still under construction

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• amdres

... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...

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• Infrared Spectroscopy Data Reduction with ORAC-DR
• Robust Data Analysis Methods for Spectroscopy
• Slitless Multiobject Spectroscopy with FOSC Type Instruments

Main parameters of Gamma Ray Spectrometer . Parts of GRS facility . ... Gamma Ray Spectrometer [GRS] with cooled germanium detector . ... Spectroscopy of gamma-ray emission from Mars in 16000 channels at the energy range 300-8000 keV; . Neutron Spectrometer - [NS] . ... High Energy Neutron Detector - [HEND] . ... Scintillation detector for fast neutrons at energies 1,0 ?10,0 MeV, for gamma-rays at energy range 60 keV ? 2 MeV and for hard X-rays at energy range 30 keV ? 1 MeV; . ...

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• Scientific tasks of GRS and HEND

... EQUINOX = 2000.0 . DATE-OBS= '1993-04-19T11:23:36' . RA_PNT = 214.4982041667 . ... OBJECT = 'NGC 5548' . ... GRNDMD01= 'SPECTROSCOPY' . DETECT01= 'BLUE ' . APERID01= 'A-1 ' . FGWAID01= 'H19 ' . ... GRNDMD02= 'SPECTROSCOPY' . DETECT02= 'BLUE ' . APERID02= 'A-1 ' . FGWAID02= 'H13 ' . ... GRNDMD03= 'SPECTROSCOPY' . DETECT03= 'BLUE ' . APERID03= 'A-1 ' . FGWAID03= 'H19 ' . ... GRNDMD04= 'SPECTROSCOPY' . DETECT04= 'BLUE ' . APERID04= 'A-1 ' . ...

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• NGC 4151
• NGC 4395
• NGC 1399

... As a result of the BTA spectroscopy of a faint optical source (R=23), earlier identified at the BTA with a compact ( RC J0311+0507 from the sample of objects with ultra-steep radio spectra (RATAN-600), a radio galaxy with a strong narrow emission line, the most likely identification of which is the Lyman-alpha hydrogen at redshift of z=4.514. This is the second radio galaxy, discovered at a redshift of more than 4.5 - a real candidate for the most powerful radio objects of the Early Universe. ...

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• SAO RAS home page
• Hardware sector, archive 2001
• The study of star formation in KDG61 and KDG64

предыдущая . ... На рисунке представлена схема ядерных реакция по превращению водорода в гелий, которые могут происходить при весьма высоких темпеартурах - более 60 млн. град. Роль катализаторов в этом случае играют ядра неона, натрия, магния и алюминия. Циклы превращения относительно просты и обозначены в том же стиле, как и для CNOF цикла . ... Около серых линий распада ядер проставлены времена жизни. В двух ключевых случаях захват протона ведет к образованияю ядра гелия. ...

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• Hydrogen burning cycles

Microsymposium 40, abstract 88, 2004 (A4 format) GAMMA RAYS FROM MAJOR ELEMENTS BY THERMAL NEUTRON CAPTURE REACTIONS: EXPERIMENT AND SIMULATION FOR PLANETARY GAMMA-RAY SPECTROSCOPY. ... Then the calculation can be restarted by producing gamma rays and let them trans- GAMMA RAYS FROM MAJOR ELEMENTS BY THERMAL NEUTRON CAPTURE REACTIONS: N. Yamashita et al. port and react, with initial energies determined the outside multiplication and initial locations wh neutron capture reaction took place. ...

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• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf

. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .

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... Spectroscopy for Everyone! Tom Field . Thursday, Sep 8, 2011 at 8:00 PM . ... However, until the last few years, spectroscopy has been too expensive and difficult for all but a few amateurs. Today, though, new tools make spectroscopy accessible to almost all of us. ... This will be our first web-talk, in which the speaker will be giving a live talk from a remote site (in this case, Seattle). ... Speaker Bio . ... Sep . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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Lectures . ... Home Lectures Lecture Series 2011-2012 Lecture Series 2011-2012 ? тАЬThe Mystery of Beta Lyrae: Astronomical Spectroscopy for AmateursтАЭ ? Fred Chromey . ... Lecture Series 2011-2012 . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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