... HST . ... HST Overview . ... Move of COS FUV Spectra to Lifetime Position 3 and Revisions to CalCOS to Support Spectral Extraction at the New Position -------------------------------------------------------------- Move of COS FUV Spectra to Lifetime Position 3 and Revisions to CalCOS to Support Spectral Extraction at the New Position On February 9th, 2015 the COS FUV spectra were successfully moved to Lifetime Position 3 (LP3) (except for G130M/1055 and G130M/1096 which remain at Lifetime Position 2...

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• COS Data Handbook
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... February 20, 1998 . Hale-Bopp: A Continuing Tail . ... Clearly the comet still has a substantial tail , blown by the solar wind , that points generally away from the sunward direction. ... As Hale-Bopp recedes from the sun its activity will subside but astronomers are still uncertain as to how long its tails will last. After a swing through the outer solar system and the Oort cloud , Hale-Bopp will pass through the inner solar system again ... around the year 5400. ... About APOD > . ...

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• APOD: 2001 February 23 - M55 Color Magnitude Diagram
• APOD: 2016 February 5 - Massive Stars in NGC 6357
• APOD: 2015 February 19 - Palomar 12

... gradients dependencies on solar wind parameters and IMF; . ... fate of thermal plasma at the dayside magnetopause. velocity-dispersed injections of the thermal and superthermal ions from LLBL at cusp and cleft (lowest energy VDIS-2 events); . ... outer cusp processes, role of outer cusp indentation, plasma entry (laminar reconnection, turbulent diffusion, others), role of turbulent boundary layer; . how is the magnetosheath plasma heated near magnetopause and cusp? . ... cusp/cleft wave emissions. ...

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• IB_MAG5 February 2000 during operations scheduling
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Full derivation of the projectile motion equations Acceleration is defined as the rate of change of velocity. So, by definition... dv a= dt For the projectile motion case, acceleration is constant. ... To undo differentiation, you need to integrate. ... The right hand is just the integral of the differential of v - i.e. it takes you back to v. For the left hand side, to integrate a constant, multiply it by whatever variable you are integrating against (in this case, t) and add a constant. ...

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• http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L02/lecture02.pdf
• http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L09/Lecture09.pdf

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

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• The AstroStat Slog Blog Archive [Jobs] postdoc position at UC Berkeley
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... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• Armagh Observatory
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• JLE Dreyer

The VIRGO project is a physics experiment; its aim is the detection of gravitational waves. ... It has not yet been possible to detect directly the gravitational waves: it remains one of the major challenges of experimental physics. ... Interferometric antennas for gravitational waves Gravitational waves distort space-time: along two perpendicular directions, the distances between fixed points will increase (resp. decrease), at the arrival of a gravitational wave. ... Publications from our Group . ...

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• Luna 20
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EPM-ERA2012 Lunar Ephemeris and selenodynamical parameters from LLR data(1970-2012) M.V. Vasilyev, E.I.Yagudina IAA RAS, St-Petersburg, Russia Reflector at the Moon The reflector 's positions at the Moon surface 3.5 m telescope at Apache station INTRODUCTION MODERN EPHEMERIDES: 1. ... IAA RAS, Russia-EPM-ERA2012 The present analysis of (17580) LLR observations, (time interval 1970, March - 2012, February) Model ( brief description). The dynamical model EPM-ERA has been developed by G.A. Krasinsky. ...

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• http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20090209lua.txt
• http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20080221lua.txt
• (Untitled)

Software Forum Message . Forums: . ... Discussion Forums | Astronomy Software Discussion | Post . ... Star Positions.. Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... Leonid CHEKHOV (Steklov Institute and Poncelet lab, Moscow) . ... Ivan DYNNIKOV (MSU, Moscow) . ... Oleg KARPENKOV (Poncelet lab, Moscow) . ... Gleb KOSHEVOY (CEMI and Poncelet lab, Moscow) . Serguei LANDO (Poncelet lab, Moscow) . ... 16:00-16:50 S. Natanzon: Klein topological field theories . ... 16:00-16:50 G. Duchamp: On some interactions between Combinatorics, Computer Science and Physics . ... evening Conference dinner . ... 14:45-15:30 O. Karpenkov: Energies of knots and of certain graphs . ...

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Positions of the carriage and focus, 2013. ... South . ... South+Flat reflector . ... Focus . ... 910 . ... 890 . March . ... Feed cabin N2. 02/2013: carriage 1131000 - old position; 2861000 - new location (when the adjusting device close to the center). ... found 18.02.2013 . ... 12516 from 7r (19.04) . ... 2863000 carriage . ... Positions of the carriage and focus, 2012. ... beginning of March - 898 mm . ...

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On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

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• Astrophysics Group FIRST
• OptInt PmWiki : Workstation | History

... The Figure shows the parallactic angle in relation to the source position at (RA,DEC), the zenith of the telescope at (LST,AoLatitude), the hour Angle HA, and the azimuth direction AZ (in the picture the source has already transitted). ... Now suppose that a second feed was placed 1 beam width away from the central horn parallel to the azimuth arm. ... Figure 1. shows the parallactic angle rate versus azimuth angle for declinations 8 through 28 (spaced 1 degree steps from Arecibo's latitude). ...

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... Category: UTILITY File: pplot.c Author: M.G.R. Vogelaar Keywords: GRDEVICE= Graphics device [list of all graphics devices] INSET= Give a (sub)set to extract a profile: Examples: You want a profile in frequency (velocity) direction: The set n3198h has axes RA, DEC, FREQ. ... 2) INSET=n3198h f 3:76 80 Because you entered a profile direction you are prompted: Give position in (RA,DEC): enter: POSITION=0 0 and a profile in the frequency direction is sampled at grids 3 to 76 and 80! ...

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• kpvslice: interactive position-velocity slicing
• SVS_Prog
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These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...

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... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm14e.pdf

... Fall 2005 . Fall 2004 . Winter 2005 . Spring 2005 . Summer 2005 . Fall 2003 . Winter 2004 . Spring 2004 . Summer 2004 . Fall 2002 . Winter 2003 . Spring 2003 . Summer 2003 . ... The Swift gamma-ray burst explorer was launched on Nov. 20, 2004 from Cape Canaveral, Florida. ... A number of models describing exotic forms of matter, generically referred to as dark energy (not to be confused with dark matter), have been proposed to explain this acceleration. ...

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• ESO Press Release 06/96, 16 February 1996

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA Exposure Time Calculator Help v1.0

... Dale A. Gardner . NASA Astronaut (deceased) . ... NASA EXPERIENCE: б  Gardner was selected as an Astronaut Candidate by NASA in January 1978, reporting to the Johnson Space Center in July 1978.б  In August 1979, he completed a one-year training and evaluation period, making him eligible for assignment as a mission specialist astronaut .б  He subsequently served as the Astronaut Project Manager for the flight software in the shuttle onboard computers leading up to the first ...

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• Astronaut Bio: Stephen G. Bowen (2/2013)
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• Cosmonaut Bio: Vinogradov Pavel Vladimirovich

... 1 XMM-Newton CCF Release XMM- CCF -REL-109 Page: 2 100 200 300 0.00 0.01 0.02 0.03 0.04 CCD1 ( 4.5e­05+/­3.2e­07)*day+0.00067+/­0.00013 adc /tr 100 200 300 0.00 0.01 0.02 0.03 0.04 CCD2 ( 4.9e­05+/­4.1e­07)*day+­0.0013+/­0.00015 adc /tr 100 200 300 0.00 0.01 0.02 0.03 0.04 CCD3 ( 4.8e­05+/­3.7e­07)*day+­0.0012+/­0.00014 adc /tr 100 200 300 0.00 0.01 0.02 0.03 0.04 CCD4 ( 4.1e­05+/­3.5e­07)*day+ 0.0023+/­0.00013 adc /tr 100 200 ... The degradation rate has also been adjusted per CCD. ...

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• srcinfov: compute position of SouRCe in Field Of View
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