The NICFPS:Dither:Extended Source script allows you to a set of take pairs of dithered source/sky exposures. These pairs of exposures are taken over various points of a small 5-point dither pattern. ... dither point 1 on source . dither point 1 on sky . ... For more information see NICFPS:Dither:Point Source . ... As the script runs the status of each dither point is updated. ... This differs from the NICFPS:Dither:Point Source script, whose dither pattern is aligned with the detector. ...

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• Other Sources of Information
• lsst.tcc: python/tcc/cmd/__init__.py Source File
• lsst.tcc: include/tcc/axeLim.h Source File

Gamma-rays from the GC . M.Chernyakova (DIAS), D.Malyshev (DIAS), F.Aharonian (DIAS, MPIK), R.M.Crocker(MPIK), D.I.Jones(MPIK) 1 10°x10° Count and TS maps (>300 GeV) Gamma-rays from the GC 2 TS maps of the GC at different energies 300 MeV ­ 3GeV 3 GeV ­ 30 GeV 30 GeV ­ 300 GeV Gamma-rays from the GC 3 4 Gamma-rays from the GC Lightcurve 5 Gamma-rays from the GC Source spectrum Model X-ray and low-energy emission come from the central object, probably SMBH accretion disk. ...

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• http://hea.iki.rssi.ru/integral06/papers/E36_Stephen01-07May07_17:57:56.pdf
• High Energy Astrophysics Department at IKI RAN

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...

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• Project SUBMILLIMETRON
• GUS Resources
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... Galaxy Evolution home . Cavendish Astrophysics . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . ... Radio sources are among the most powerful of the family of Active Galactic Nuclei (AGN). ... The overall properties of radio sources are well predicted by analytical models of self-modifying evolution of the radio source which we have developed, and many of the more unusual structures observed can be reproduced using computational models. ...

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• OptInt PmWiki : MROIDelayLine / Trolley Software
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• The 7C(G) survey

... Tested with -- Suse 10.0 Should work with -- Suse 10.0 , 10.1 Novell/ Suse Enterprise 9.3 or 10 when available Slackware 11 when available Any other recent distribution with 2.6.13 or higher kernel and udev Will not work with -- Slackware 10.2 or earlier Any distribution using 2.4 series kernels or lacking udev Dependencies -- Among others, but source code included: libusb Motif or Lesstif fxload Coming soon -- No support for LPT cameras in 2.6 series kernels. ...

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Lectures . ... Home Lectures Lecture Series 2010-2011 Lecture Series 2010-2011 ? Greening the Earth Using Space Resources? by Greg Matloff . ... Lecture Series 2010-2011 . ... 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 . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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• Moon from the High Line ? Amateur Astronomers Association of New York
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• High Line ? Amateur Astronomers Association of New York

... Visited 8168 times - Selected 52 months ago . ... Visited 4099 times - Selected 51 months ago . ... Visited 5378 times - Selected 51 months ago . ... Visited 4661 times - Selected 51 months ago . ... Visited 5590 times - Selected 51 months ago . ... Visited 5997 times - Selected 51 months ago . ... Visited 5377 times - Selected 51 months ago . ... Visited 9073 times - Selected 52 months ago . ... Visited 5524 times - Selected 52 months ago . ... Visited 4289 times - Selected 183 months ago . ...

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• The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. - an Astronomy

. Comment on J1325-4301 . Our image, limited by the short observing time, shows symmetrical structure elongated in the NE-SW direction which is not useful to study the details of this complex source. High dynamic range images of this source are published by Tingay et al. (1998). VLBApls home page . Last modified: 16 Oct 2000

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... This book uses many authentic sources such as factual texts, newspaper articles, features and TV schedules, instruction manuals, everyday signs, stories, quizzes, emails and diary entries. ... Чернила для принтера HP HP Photosmart 425. цвета: Cyan, Magenta, Yellow, Black, емкость баночек - по 100 мл. ...

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• Market Leader Elementary: Test File - Lewis Lansford - Lewis Lansford 12296407

... This version contains libc 4.6.27, Linux kernel 1.2.8 (plus source for many other versions in the source tree, including version 0.01 :^), and XFree86 3.1.1. ... This is what you'll find in the subdirectories below (or in the case of the installation disks, in the ./slakware subdirectory): ./bootdsks.144, ./rootdsks.144, bootdsks.12, rootdsks.12: Boot/install disks for 1.44M and 1.2M floppy drives. ... Based around the 1.2.8 Linux kernel, and concepts from the Linux filesystem standard. ...

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• XFree86/OS2 project
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• The same source code used for Fortran 77 and Fortran 90?

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• Laboratory static Fourier-spectrometer
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... One striking feature is a small source of almost pure H 2 line emission, which is located near one of the compact sources in Orion reported by O'Dell and collaborators (HST-18 = 203-504). ... H-H objects, Proplyds, Orion Bar, H 2 . ... We obtained a series of images across the bright rim of the Orion Bar near the peaks of mm-wave molecular line emission with NICMOS cameras 1-3 (NIC1, NIC2, NIC3) in several filters on 1998 February 18. ... The suggestion of an H-H object does not seem compelling. ...

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• The Structure and Composition of High Redshift Radio Galaxies
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As of 1.3, the Apache source directories have been re-organised. This re-organisation is designed to simplify the directory structure, make it easier to add additional modules, and to give module authors a way of specifying compile time options or distribute binary modules. ... The non-module source files have moved from src into src/main . ... Configure . ... For example, say it is called mod_demo.c. The archive for this module should consist of two files, in a suitable directory name. ...

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• Definitions of terms used to describe Apache modules
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What about Energy Storage? ... Battery Farms: . Acres of batteries; charged by transmission lines during periods of low demand . Returned to transmission lines during periods of high demand . ... Fused Silica has 25 times the energy storage per kg than lead-acid batteries . ... Very high energy density storage per kg . ... Not economically viable unless shipped large distances from point of production . Compressed Air . ... Have to cool the air as its compressed energy intensive . ...

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• http://zebu.uoregon.edu/~uochep/talks/talks04/grbs_v2.pdf
• Physics 410/510 Observational Cosmology
• Energy and the Environment: Resources for a Networked World

In calculating the NIFS sensitivity, we adopt a read noise of 5 e - , a dark current of 0.01 e - s -1 pix -1 , and a maximum exposure time of 3600 s. Grating . ... e/pix) . ... OH Cont. (e/pix) . ... NIFS should achieve signal-to-noise ratios of ~ 10 per spectral pixel in a 0.1" 0.1" aperture for single 1800 s exposures on uniform, extended, continuum sources with surface brightnesses of J = 15.4, J = 15.0, H = 14.8, and K = 13.5 mag arcsec -2 using the Z , J , H , and K gratings, respectively. ...

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• Pink Black Holes: Technical Details
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. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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• The Canadian S2 Correlator - Principles of Radio Interferometry

Stellarium 0.12.3 . ... FileљStructure . FileљList . ... core . modules . Meteor.hpp . ... 46 љ Meteor ( const StelCore *, double v); . ... 64 љ Vec3f position; . 65 љ Vec4f color; . ... 67 љ : position( Vec3f (pos[0], pos[1], pos[2])), color(color) {} . 68 љ VERTEX_ATTRIBUTES( Vec3f Position , Vec4f Color); . ... 75 љ Vec3d obs; // observer position in meteor coord. system . ... 88 љ double xydistance; // distance in XY plane (orthogonal to meteor path) from observer to meteor . ...

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• Stellarium: core/RefractionExtinction.hpp Source File
• Stellarium: gui/StelGuiItems.hpp Source File
• Stellarium: core/StelGeodesicGrid.hpp Source File

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Launches Chronology . ... Automatic Space Systems . ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• S.P.Korolev RSC Energia - MARTIAN MISSION
• S.P. KOROLEV ROCKET & SPACE CORPORATION ENERGIA

. New sources emerge and old sources fade as the LAT's view extends into higher energies. Credit: NASA/DOE/Fermi LAT Collaboration and A. Neronov et al.

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B97C571EE-51FB-4DD5-82F9-001DCCFF4C27%7D
• January 2006 resources | Astronomy.com
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