Changeset 40078

Timestamp:

Jul 5, 2017, 5:19:23 PM (9 years ago)

Author:

eugene

Message:

bigger test

File:

• trunk/doc/release.2015/ps1.analysis/test.tex (modified) (3 diffs)

trunk/doc/release.2015/ps1.analysis/test.tex

@@ -1 +1 @@
 \documentclass[iop,floatfix]{emulateapj}
+%\documentclass[preprint2]{aastex}
 \RequirePackage{color} % this is required for {code}
 \RequirePackage{code}
 \input{astro.sty}
-
-\usepackage[T1]{fontenc}% (2) specify encoding
 
 % Pick a terse version of the title here;
@@ -42 +41 @@
 Big test here.
 
-Testing \code{code_foo}.
-
-Testing \IPPstage{chip stage_test}.
-
-Testing \IPPdbtable{rawImage_test}.
-
-Testing \IPPdbcolumn{rawImage.datetime_test}.
-
+Testing \code{\code_foo}.
+
+Testing \IPPstage{\IPPstage : chip stage_test}.
+
+Testing \IPPdbtable{\IPPdbtable : rawImage_test}.
+
+Testing \IPPdbcolumn{\IPPdbcolumn : rawImage.datetime_test}.
+
+<<<<<<< .mine
+Testing \IPPmisc{\IPPmisc : another_check}.
+=======
 Testing \IPPprog{pantasks_client}.
 
@@ -67 +69 @@
 
 % Testing \url{http://by.source}
-
-% Testing \foocode{http://eugene@ifa.source}
+>>>>>>> .r40075
+
+Testing \url{http://by.source}
+
+Testing \url{http://eugene@ifa.source}
 
 \section{FOOBAR}\label{sec:intro}
 
+
 % Testing \foocode{AM_I_GOOD}
 
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+read \cite[][Paper I]{chambers2017} today.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+Over 3 billion astronomical sources have been detected in the more
+than 22 million orthogonal transfer CCD images obtained as part of the
+Pan-STARRS\,1 $3\pi$ survey.  Over 85 billion instances of those
+sources have been automatically detected and characterized by the
+Pan-STARRS Image Processing Pipeline photometry software,
+\code{psphot}.  This fast, automatic, and reliable software was
+developed for the Pan-STARRS project, but is easily adaptable to
+images from other telescopes.  We describe the analysis of the
+astronomical sources by \code{psphot} in general as well as for the
+specific case of the 3rd processing version used for the first public
+release of the Pan-STARRS $3\pi$ survey data.
+
+\bibliographystyle{apj}
+\bibliography{lib}{}
+
 \end{document}