... off]" 4086 "expected [1 | ... 4] 4087 '%Fs' : declared with void parameter list 4088 '%Fs' : pointer mismatch : parameter %d, parameter list %d 4089 '%Fs' : different types : parameter %d, parameter list %d 4090 different 'const/volatile' qualifiers 4091 no symbols were declared 4092 untagged enum/ struct / ...

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... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2015 May 31 . Supernova 1994D and the Unexpected Universe . Image Credit: High-Z Supernova Search Team , HST , NASA . Explanation: Long ago, far away, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... About APOD | ...

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... CentralProcessor 0.11 documentation . ... MergedSource ############################## tasks.tasklist = [ MergedSource , CalcUVWTask, TCPSink ] # record only 9 beams , discard the rest (determined by the # beam configuration (see the main ingest pipeline documentation page) tasks. MergedSource .params.maxbeams = 9 # channel distribution for each rank tasks. MergedSource .params.n_channels.0 = 216 tasks. MergedSource .params.n_channels.1 = 216 tasks ... MergedSource . ...

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... December 30, 1998 . Supernova 1994D and the Unexpected Universe . Credit: High-Z Supernova Search Team , HST , NASA . Explanation: Far away, long ago, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... The large number and great distances to supernovae measured in 1998 have been interpreted as indicating that we live in a previously unexpected universe . ... About APOD > . ... NASA Technical Rep.: ...

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... Default . ... The descriptions below focus on the meaning of each filename parameter, leaving the exact details of the inferred default value to be explained in the algorithm section. evlist . ... file . The response matrix file (OGIP-compliant format). ... If a spectrum file is not provided ( withspectrum =no) this parameter specifies the INDEX number of a source in the source description list (parameter srclist ), and thereby the incidence angle and selection regions for the response matrix. ...

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Astronomy Picture of the Day . ... 30.12.1998 . ... Credit: High-Z Supernova Search Team , HST , NASA Explanation: Far away, long ago, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... The large number and great distances to supernovae measured in 1998 have been interpreted as indicating that we live in a previously unexpected universe . ... Publications with keywords: cosmology - universe - supernova . ...

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Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

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Figure 1a. This figure shows the secondary tilts required to correct for transverse flexures of both the telescope truss and the secondary mirror mounts as the telescope changes altitude. ... The circles show the x-tilts of the secondary needed to minimize telescope coma and the squares show the y-tilts required. ... The small negative slope which seen in the y-tilt data is possibly real. ... However, the y-tilt data are very consistent with the y-tilts measured on August 14 (Figure 1a). ...

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stable spacetime manifold Expected to propagate at speed of light Expected to have 2 independent polarizations Sources ­ ­ ­ ­ http ://www.johnstonsarchive.net/relativity/pictures.html Unmodeled bursts Binary Coalescence Periodic Sources Stochastic Background http ://mucholderthen.tumblr.com/post/55970198303/gravitational-waves-patterns-in-space-time-a 3 LIGO-VIRGO Interferometer Gaussian Noise: Coherent Signal vs. ...

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... We cannot use for this purpose equivalent widths and profiles of HI lines (well known criteria of atmospheric conditions for normal supergiants), since these lines are strongly distorted in the spectrum of IRAS04296 as seen in Fig. ... Figure: Upper: iron abundance FeI (circles) and FeII (crosses) calculated for IRAS04296+3429 with model parameters , and using lines with different excitation potentials EP of a low level; bottom: the same as a function of the equivalent width W . ...

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Introduction to Hardware Signal Injections Peter Shawhan, Isabel Leonor, Szabi MАrka (LIGO/Caltech, U. of Oregon, LIGO/Caltech) LSC Meeting March 19, 2003 LSC Meeting, 19 March 2003 Shawhan, Leonor, Marka LIGO-G030112-00-D Uses of Hardware Signal Injections Complete end-to-end test of detector and analysis Verify that detector does not distort si gnal in unexpected ways Verify that search algorithm can detect signals ! ...

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