... Many extragalactic objects for which radial velocities are desired display strong emission lines. ... EMSAO, a companion to the cross-correlation task XCSAO (Kurtz et al. 1992), was written to find emission lines automatically, compute redshifts for each identified line, and combine them into a single radial velocity. ... Figure: This EMSAO Summary page shows line centers and fit information for a night sky spectrum. ... To test EMSAO adequately, a lot of emission line spectra were needed. ...

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• RVSAO 2.0 - A Radial Velocity Package for IRAF
• Keeping Bibliographies using ADS
• Interactive Fitting of EUVE Emission Line Spectra

A full explanation of the motion of trapped particles would be too abstract and mathematical for this level, but some basic ideas may be described on an intuitive level. The magnetic force on a moving particle is always perpendicular to the motion, as well as to the magnetic field lines. That is why the basic pattern is motion in a circle, around a magnetic field line. ... The best-known periodic motion is the back-and-forth swing of a pendulum, say of a weight suspended by a string (drawing). ...

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• Auroral Images
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• Frames of Reference: The Basics

... Returns UT1 in seconds, with UTC input in seconds. ut12gst ( utc _real [, ut1 _real ]) Function. Returns GST in hours, inputs are in seconds. hourangle ( gst _real , ra _real ) Function. Return hourangle in hours, with inputs also in hours. zenithangle ( ha _real , dec _real ) Function. Return zenithangle in degrees with inputs ha in hours and dec in degrees. mirrorangle ( ha _real , dec _real ) Function. ... Return horizon coordinates for input azimuth and elevation angle in degrees. ...

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• HISTORY productExplorer
• Date conversion functions
• pet.py: the python plot engine for trendPlotter

... For example, IKI is located near Kaluzhskaya station of the orange colored line (line number 6). [pic] To help you find your way, there are several multicolored metro maps in every car, and a loud speaker that announces the name of the station at every stop. ... After you got out the train doors, turn right and proceed to the escalator (moving staircases) in the direction of your train movement. ... Enter the Kaluzhskaya metro station, go downstairs and take the train on the RIGHT side. ...

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• Motion in a Circle
• Magnetic Field Lines -- History
• Frames of Reference: The Basics

Previous Editions of the M111: . ... OutReach Training and Program . September Public Night . Welcome all ye weary travelers to a new type of M111 "On Line". ... Back to top.. ... When I logged our last outreach programs I couldn't help but notice that Warren Rupp Observatory is NUMBER FIVE in the worldwide standings in public outreach programs! ... If you'd like to train in astronomy outreach, just contact any of our members and we'll be happy to train you to do public outreach! ...

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I. Installation . ... AMPLE package distributive (created with program InstallShield for Microsoft Visual C++) has been downloaded on FTP server of IAA RAS as archive Ample.zip. ... Note: If the window "file download" appears, select Open... switch button, then press OK button. ... The shortcut for AMPLE will be linked with this folder, and auxiliary files will be created here during AMPLE work. ... When running AMPLE all auxiliary and new configuration files are created in the WORK folder. ...

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... Corresponding authors will receive an e-mail with a PDF file of paged proof for checking and correction. The file can be read and edited using Adobe Acrobat Reader (version 9 and higher) which can be free downloaded via the Internet ( http://get.adobe.c om/reader/ ). ... You can use text correction tools to make corrections (after selecting the necessary text fragment). ... For users of Adobe Reader 9: . ... to insert text without replacing the existing text, use the "Insert text at cursor" tool. ...

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• New LBV Stars in the Andromeda Galaxy
• New data on the cpmplex field structure of chemically peculiar stars
• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology

... Activity 3: Measuring the Position of the Sun in the Sky . Purpose: To give students the opportunity to measure the position of the Sun in the sky using simple tools and methods. ... Alternatively, you may have students devise their own methods of relative measurement and apply them to measuring the position of the Sun in the sky. ... Rangi is the sky, and when the Sun is near Rangi's head it is summer in New Zealand. ... Read the Maori story to students. ... back to Teachers' Newsletter Main Page ...

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• ASP: Up, Up, and Away
• ASP: An Ancient Universe - Changes in the Universe
• ASP: Running the Line: The Astronomy of Mason and Dixon

... 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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• Astronomical Catalogues
• Index of /~inest/astrolib/Sun/kursoviki/lines-c

... Russian Aviation and Space Agency liaison Sergei Ripkin, during the crew's welcome home ceremony May 27 f rom a change in crew to a new ride home, Expedition 6 members ­ International Space Station Commander Kenneth Bowersox, ISS Science Officer Donald Pettit and Flight Engineer Nikolai Budarin ­ were "all about teamwork and flexibility," said ISS Program Manager Bill Gerstenmaier. ... Bowersox later said that Pettit was "born to be a Space Station Science Officer." ...

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• S71-43477
• JSC Space Center Roundups
• NASA - JSC History Portal

... There are two main tasks in the package, XCSAO and EMSAO. XCSAO cross­correlates the Fourier transform of an object's spectrum against the transforms of a set of template spectra with known spectral shifts to obtain a velocity and error. EMSAO finds emission lines in a spectrum and computes the observed centers, getting individual shifts and errors for each line as well as a single velocity combining all of the lines. ... It combines spectra, shifting them to a common redshift. ...

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• http://www.stecf.org/software/ASTROsoft/DER_SNR/der_snr.pro
• http://www.stecf.org/software/PYTHONtools/astroasciidata/manual/asciidata_0.01.ps.gz
• http://www.stecf.org/software/PYTHONtools/astroasciidata/manual/asciidata_0.01.pdf

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

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• Spherical and Practical Astronomy
• Introduction to Astronomy
• Lunar eclipce explanation page of Computer Ephemeris (DE200/LE200).

... Tonight's Sky . ... The Magazine . ... Observing . ... Magazine . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... The end of the line for our planet . ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

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• Mars returns to glory | Astronomy.com
• MAVEN spacecraft returns first Mars observations | Astronomy.com
• Saturn spacecraft returns to the realm of icy moons | Astronomy.com

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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• http://www.uafo.ru/msg/zr_2014_08.doc

This is to help you migrate from Mail::Bulkmail 2.x to Mail::Bulkmail 3.x change use Mail::Bulkmail 2.05 to use Mail::Bulkmail 3.03 "/path/to/conf/file"; change $bulk->allow_duplicates(1); to $bulk->Trusting('duplicates' => 1) (should be in the conf file as Trusting @= duplicates) change $bulk->safe_banned(1) to $bulk->Trusting('banned' => 0); (should just not be specified, since it defaults to 0. ... Headers from message (HFM) is no longer supported. ...

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• http://hea.iki.rssi.ru/conf/hea2007/scripts/gen_validatorv2.js~
• JavaScript Form Validator Documentation
• High Energy Astrophysics Department at IKI RAN

SKY-MAP.ORG

37. http://xray.sai.msu.ru/~polar/html/black_hole_coll/kharkov_zaja

38. Bookmarks of Yakiv Pavlenko changed on Jul 1, 2015

39. XWare > APOD

40. Future of the Galaxy