. Next: Pulse Widths Up: Integrated and single pulse Previous: Integrated and single pulse .   . Huge variations from pulse to pulse . Integrating several 100 forms a stable profile . Integrated profiles differ widely . Basic model includes core + cone . Slice in different ways to get various profiles .     . Figure 54: Integrated pulse profiles . Jon Bell . Thu Dec 19 15:15:11 GMT 1996

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• Frequency Frame Alignment
• Integrated and single pulse profiles
• Unix Shell and Text Editor

... 2012 March 13 . The M81 Galaxy Group Through the Integrated Flux Nebula . ... Explanation: Large galaxies and faint nebulae highlight this deep image of the M81 Group of galaxies. First and foremost in the wide-angle 12-hour exposure is the grand design spiral galaxy M81 , the largest galaxy visible in the image. ... This whole galaxy menagerie is seen through the faint glow of an Integrated Flux Nebula , a little studied complex of diffuse gas and dust clouds in our Milky Way Galaxy . ...

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• APOD: 2008 May 12 - The M81 Galaxy Group Through the Integrated Flux Nebula
• APOD: 2006 September 20 - The International Space Station Expands Again
• APOD: 2007 June 25 - The International Space Station Expands Again

... Integrated superconducting submm receivers and spectrometers. ... Development, study and optimization of the superconducting phase locked Local Oscillator for integrated spectrometer. ... Superconducting Integrated Submm Spectrometer for Laboratory Applications. ... Development, study and optimization of the superconducting phase locked Local Oscillator . ... The objective is to develop and study a superconducting Local Oscillator (LO) for an integrated submm spectrometer . ...

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• Lab234 - Technology for fabrication of superconducting integrated circuits
• Atmospheric influence on the different radioengineering systems functioning.
• Lab234 - Superconducting Integrated Submm Spectrometer for Laboratory

... We can investigate projection of this distribution onto the celestial sphere in two ways: in terms of lines of constant SN frequencies per one square degree for all galaxies from the sample (Figure 36 ), and in terms of constant GW amplitudes at a given SN frequency per square degree (Figure 44 ). ... Figure 45: The sky distribution of the total supernova frequency from nearby galaxies in terms of lines of equal frequencies per square degree. ...

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• E-P transitions for different orbits

Gain curves for various receivers and freq (ps) ( .pdf ) are plotted versus zenith angle. (last updated 22nov05) . ... The colors are for different receivers. For the same receiver, different frequency measurements use different plotting symbols. ... The solid line has averaged over azimuth, the dashed line has taken the maximum azimuth value for each measurement (all at a za of 10 degrees). ... For more info on the gain curve fits and their location see gain curves fits at ao . ...

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• http://www.naic.edu/~phil/optics/compute/lnfeedphase.html
• pdev_birdies_25jun07
• pshiftTest_04oct12

... Archives . ... If you do not mind the time predictor, it is hard to believe that this is a light curve, time dependent data. ... It?s hard to say this data set is designed for time series analysis apart from the complication in statistical inference due to measurement errors. How to design the statistical study with measurement errors, huge gaps in time, and unequal time intervals is complex and unexplored. ... The following is R output without measurement errors. ... Chandra Blog . ...

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• The AstroStat Slog measurement error
• The AstroStat Slog Blog Archive my first AAS. V. measurement error and EM
• The AstroStat Slog error propagation

ASTP PROJECT . On July 17, 1975, for the first time in the history of mankind, space vehicles belonging to different nations - the Soviet and the American space vehicles Soyuz-19 and Apollo - have performed rendezvous and docking to deploy into an integrated orbital complex. ... Appointed Project Managers were: for the Soviet part - K.D. Bushuev, a Corresponding Member of the USSR AS, for the American part - Doctor G. Lanny. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• INTERNATIONAL SPACE STATION
• S.P.Korolev RSC Energia - LAND LAUNCH SYSTEM

Results from a series of long-term numerical integrations of orbits centred on that of C/1995 O1 (Hale-Bopp) are presented. Initially, 33 orbits taken from various sources were integrated in realistic models of the solar system for various time-scales about the present in the range (-3, +2) Myr and analyzed to assess the probability of different dynamical outcomes, such as a sungrazing state or the number of orbits since it was captured from a long-period orbit in the Oort cloud. ...

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• Influence of Climate Variables on Tree-Ring Widths of Different Species
• Astro-Art Fun at Windmill Integrated Primary School, Dungannon | International
• ULTRACAM Observations of Subdwarf B Stars

... We have developed an integrated system that performs astronomical observations in Near Infrared bands operating two-dimensional instruments at the Italian National Infrared Facility's ARNICA and LONGSP . ... The user interface is organized as widget-based X11 client. ... 1993; Di Giacomo et al. 1993). ... Moreover, if the interprocess communication interface includes support for networking, the software immediately becomes network distributed software. ... DESQview/X User Guide 1993, Quarterdeck . ...

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• ADASS 2002 Conference Proceedings
• Object Oriented Near Real Time Packet Distribution as Part of the FIRST
• Image Reconstruction with Few Strip-Integrated Projections: Enhancements by

Since the light from galaxies represents the integrated contribution of its consitutient stars, then we can learn about stellar populations in galaxies by modelling their light by summing up individual stellar spectra for different kinds of stars. ... The data cover the wavelength range 3500 - 9000 angstroms. ... Retrieve Digital Stellar Spectra Click on the appropriate spectral type. ... Note that the designation V means main sequence, IV means subgiants, III means giants, I means supergiant. ...

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ES Visitor lane ESO Business Lane Planetarium exit Visitors counting device Donations box Receptionist Ticket printer Brochure holder for ~12-15 brochures ( integrated ) 3 Hanging info screens Guided tours meeting point 2 W all Clocks 4 shop shelves + storage (170 different items) Visitor Ticket kiosks Planetarium preshow ( mounted from ceiling) ESOshop Point of Sale Translation device charging stations ( ...

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• P2PP V2.4 Integration Test Plan
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• ESO - I want to process MOS data of the same target from different nights

As it is in Ephemerides task, O?C can be calculated with different accuracy. ... It presents three modes of accuracy. One can calculate position of a minor planet by the formulae of elliptic motion starting from the fundamental set of elements for given minor planet. ... Also there is possibility to calculate positions taking into account perturbations from different sets of perturbing bodies by numerical integration ( Integration mode). ... Accuracy of integration is equal to 10**(?10) AU. ...

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• ENGAMPLE
• Keywords_114

Next: Sky Subtraction Up: Construction of Flat Previous: Standard construction . For a number of projects where very deep integrations and accurate flat fields are required, and the targets are point sources or much smaller than the frame size, the sky background itself can be used to calculate the flat field. ... Use STATISTICS/IMAGE to calculate the image median, and COMPUTE/IMAGE to divide by this to get the normalised flat field. ...

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• The 7C(G) survey
• Flat-Fielding
• Spectra of Kallas Riech (1980) sources

Some recent results ( see ) attracted the attentions of astronomers working on field which could benefits from photon counting techniques with high speed and spatial resolutions as adaptive optics. ... Fasti has been designed to be fast and largerly configurable. ... The data rate attined in the best case (30 Mhz), give no impossible load to the digital acquisition in the photon counting mode, since data are 1 bit only, they can be parallelized, giving a maximum speed of about 940.000 32 bit word/sec. ...

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... The M81 Galaxy Group Through the Integrated Flux Nebula . ... Large galaxies and faint nebulae highlight this deep image of the M81 Group of galaxies. First and foremost in the wide-angle 12-hour exposure is the grand design spiral galaxy M81, the largest galaxy visible in the image. ... Colorful NGC 1579 resembles the better known Trifid Nebula, but lies much farther north in planet Earth's sky, in the heroic constellation Perseus. ... The Seagull Nebula . ... Warped Spiral Galaxy ESO 510 13 . ...

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• An Orion of a Different Color
• Астронет > An Orion of a Different Color
• The M81 Galaxy Group Through the Integrated Flux Nebula

... Clearing the library. Note the different flooтАж . Sidebar Left . Sidebar Top . ... Title: Clearing the library. Note the different floor levels. There were at least 4 different levels of underfloor in the library. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

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• Things are very different for small planets
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... Purpose: The purpose of this program is to monitor the sensitivity, wavelength and detector calibrations of Side 2. Description: Four times per year (twice in Cycle 6) the following observations will be done: . ... SENSITIVITY MONITORING . ... Fraction of GO Programs Supported: All GHRS programs using gratings G160M (19%), G200M (7%), and G270M (15%). ... Observation: Internal-16 orbits (8 orbits for each of the 2 executions. Note: the internal orbits are full orbits). ...

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• Proposal ID 6897: GHRS Cycle 6: CRIMP1-- Condensed-Regimen Integrated
• ST ScI Preprint #1364
• WFC3 Instrument Handbook

. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

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• Using a different printer
• Example of using a different printer
• Different types of file

... Information about a variety of different calendars for different cultures (e.g., Christian, Jewish, Muslim, Chinese, Hindu etc.) ... In addition, the Chinese had two different ways of interpreting and observing celestial events. One way the Chinese used astronomy was known as lifa; it was a discipline that aimed to understand the regularities and the predictable events in the celestial system through careful, observations, measurements and records. ... back to Teachers' Newsletter Main Page ...

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• ASP: Steering by Different Stars? Astronomers and the Dark-Sky Movement
• ASP: Good Astronomy Activities on the WWW
• ASP: An Ancient Universe - Changes in Stars

... A detector map is used to provide a grid of positions over which to calculate and flux weight the ARF. The default detector map is 'flat' which has a weighting of 1.0 for each detector map pixel and is rectangular having sides which just encompass the region specified in the DSS. Only detector map pixels falling within the source region are included in the ARF calculation, e.g. for a circular source box, the pixels in the corners of the detector map will be ignored. ... flat : . ...

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• Integrated probability
• Integrated Gaussian probability
• Integrated Poisson probability