. Fig. 8. The annual distribution of the UVAI camera visibility windows onboard the Auroral probe.

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STScI . ... You can install this with easy_install or pip. ... If you will be installing on Linux or Macintosh, you also need pip and the compiler packages for your system. ... To install stsci_python, type these commands into a cmd window: c:\python27\Scripts\easy_install stsci.distutils . ... STSCI_PYTHON is now distributed as several separate packages, so that it can more readily fit into the pypi/pip/easy_install ecosystem. ... On Linux or Macintosh, use this command: pip install --download . ...

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XMM-Newton CCF Release Note XMM-CCF-REL-183 EPIC-pn spectral response R. D. Saxton 11 November 2004 1 CCF components Name of CCF VALDATE Blocks changed XSCS ag EPN QUANTUMEF 0015.CCF 2000-01-01 FRACTION CHANNEL, FRACTION ENERGY QE TOTAL, EBINS FRACTION NO EPN REDIST 0009.CCF 2000-01-01 NOISE PARAMS, PARTEVENT PARAMS THRESH LOSS NO 2 Changes Recent calibration work has shown that the Epic-pn redistribution function is in practice narrower than that represented in the current matrices. ...

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XmCCD ----- The programs provided here offer a Linux graphical user interface to astronomical and scientific CCD cameras. SBIG has provided the library used here. It is essentially the same library used by commercial software for control of their cameras under Windows. ... This distribution includes source code to utilize the Santa Barbara Instrument Group (SBIG) shared library libsbigudrv.so with a Motif-based graphical user interface program to control SBIG astronomical CCD cameras. ...

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... Posts tagged ?distribution? ... No time for reading the whole article? ... Continue reading ?Guinness, Gosset, Fisher, and Small Samples? ... Category: arXiv , Fitting , Frequentist , Quotes , Stat | ... Continue reading ?chi-square distribution [Eqn]? ... 2008? Tags: bimodality , distribution , Fourier , GRB , K-S test , kurtosis , Nested Sampling , quantification , skewness , wavelet . ... Data-Driven Goodness-of-Fit Tests by L. Mikhail . ... ArXiv] Data-Driven Goodness-of-Fit Tests, Aug. ...

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• *ftpplot* - Distribution of FFT coefficient values

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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... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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Searching for GRB -GWB coincidence during LIGO science runs Isabel Leonor University of Oregon LIGO-G050216-00-Z Motivation almost 40 years since GRBs were discovered past 15 years has been time of important clues isotropic and inhomogeneous distribution (BATSE); first optical, x-ray, radio counterparts; redshift measurements; association with core-collapse supernovae yet important ...

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• http://zebu.uoregon.edu/~uochep/talks/talks04/S2S3GR~2.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks04/grbs_v2.pdf

... Previous: Determination of Variable Time Delay in Uneven Data Sets . ... It is shown that the likeness of the periodogram and the LS-spectrum (both estimators of the power spectrum are widely used in the spectral analysis of time series), depends on the properties of the spectral window corresponding to the distribution of time points. ... Present day theory and practice of the spectral analysis of unequally spaced time series are based on two approaches. ...

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James Gordon . ... Latex . ... Installation of Latex is platform dependent, but details of possible distributions and installation instructions can be found at . http://www.latex-project.org/ftp.html . ... TexnicCentre is possibly the most user friendly IDE for the creation of Latex documents. ... Gedit . Gedit is a standard text editor, and comes with good syntax highlighting for Latex documents . ... Almost certainly included, a command like latex file.tex or pdflatex file.tex should work . ...

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... Here are listed all extragalactic supernovae discovered since SN 1885A (S AND) and their annual distribution is shown. As of SN 2000ek 1791 supernovae have been discovered. YEAR . SNe . ... 1885 . ... 163 . ... 160 . ... 140 . ...

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... Public . Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Publications with ESO Data . ... ESO-MIDAS . ... The short statement of the GNU license is included in every MIDAS file; the full text is included as a separate file in the ESO-MIDAS Release. ... Manual pages,installation guides and other documentation are generally released together with the source code and can also be obtained from the ESO-MIDAS ftp account (see below). ...

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GTK+ 2.0 Tutorial . ... This program will create a 200x200 pixel window and has no way of exiting except to be killed by using the shell. #include <gtk/gtk.h> int main( int argc, char *argv[] ) { GtkWidget *window; gtk_init (&argc, &argv); window = gtk_window_new (GTK_WINDOW_TOPLEVEL); gtk_widget_show (window); gtk_main (); return 0; } . ... All programs will of course include gtk/gtk.h which declares the variables, functions, structures, etc. that will be used in your GTK application. ... gtk-debug . ...

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... The dates are shown along the X axis, . The time on the orbit counted from ascending node of the each turn is shown along the Y axis. ... The geomagnetic local time is shown along the Y axis. ...

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Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Description of algorithm
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... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...

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... The predictive power of current models (the so-called meteor forecasting) has given us the exact timing of the Leonid storms of 2001 and 2002 to the nearest hour and are now used to predict the arrival times of major annual showers such as the Perseids . ... Towards this goal, the Observatory has installed a sky-monitoring system, consisting of one medium angle (MA) and two wide-angle (WA) video cameras linked to software designed to detect motion. ... Bright Taurid Meteor . ... Meteors on Mars . ...

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. Controls for the ARCTIC imaging camera are distributed among two windows: . The ARCTIC window displays status and allows configuring ARCTIC. The status portion is always displayed. The configuration controls are hidden by default. The ARCTIC Expose window controls and displays exposure sequences. See also the ARCTIC documentation at APO .

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