Changeset 39888 for trunk/doc/release.2015/ps1.datasystem/datasystem.tex

Timestamp:

Dec 18, 2016, 4:32:26 PM (10 years ago)

Author:

eugene

Message:

update authors and refs

File:

• trunk/doc/release.2015/ps1.datasystem/datasystem.tex (modified) (8 diffs)

trunk/doc/release.2015/ps1.datasystem/datasystem.tex

@@ -50 +50 @@
 K. W. Hodapp,\altaffilmark{\IfA}
 R. Jedicke,\altaffilmark{\IfA}
+N. Kaiser,\altaffilmark{\IfA}
 R.-P. Kudritzki,\altaffilmark{\IfA}
 N. Metcalfe,\altaffilmark{\DUR}
@@ -56 +57 @@
 % T. Grav,\altaffilmark{\IfA}
 % J. N. Heasley,\altaffilmark{\IfA}
-% N. Kaiser,\altaffilmark{\IfA}
 % G. A. Luppino,\altaffilmark{\IfA}
 % D. G. Monet,\altaffilmark{\USNO}
@@ -621 +621 @@
 
 The Chip processing stage consists of: reading the raw image into
-memory, appyling the detrending steps (see~\note{Waters et al}),
+memory, appyling the detrending steps \citep[see][]{waters2017},
 stiching the individual OTA cells into a single chip image, detection
-and characterization of the sources in the image (see~\note{Magnier et
-  al}), and output of the various data products.  These include the
-detrended chip image, variance image, and mask image, as well as the FITS
-catalog of detected sources.  The PSF model and background model are
-also saved, along with a processing log.  A selection of summary
-metadata describing the processing results are saved and written to
-the processing database along with the completion status of the
-process.  Finally, binned chip images are generated (on two scales,
-binned by 16 and 256 pixels) for use in the visualization system of
-the processing monitor tool.
+and characterization of the sources in the image
+\citep[see][]{magnier2017b}, and output of the various data products.
+These include the detrended chip image, variance image, and mask
+image, as well as the FITS catalog of detected sources.  The PSF model
+and background model are also saved, along with a processing log.  A
+selection of summary metadata describing the processing results are
+saved and written to the processing database along with the completion
+status of the process.  Finally, binned chip images are generated (on
+two scales, binned by 16 and 256 pixels) for use in the visualization
+system of the processing monitor tool.
 
 \subsection{Camera Calibration}
@@ -660 +660 @@
 system.  For PS1, this is used to generate synthetic w-band photometry
 for areas where no PS1-based calibrated w-band photometry is
-available.  For more details, see \note{Magnier et al}.
+available.  For more details, see \cite{magnier2017c}.
 
 In addition to the astrometric and photometric calibrations, the
@@ -683 +683 @@
 exposure.  This processing is called `warping'; the warp analysis
 stage is run on all exposures before they are processed further.  For
-details on the warping algorithm, see \note{Waters et al paper}.
+details on the warping algorithm, see \cite{waters2017}.
 
 The output products from the Warp stage consist of the skycell images
@@ -696 +696 @@
 stacks also fill in coverage gaps between different exposures,
 resulting in an image of the sky with more uniform coverage than a
-single exposure.  See~\note{Waters paper} for details on the stack
+single exposure.  See~\cite{waters2017} for details on the stack
 combination algorithm.
 
@@ -735 +735 @@
 
 The stack photometry algorithms are described in detail in
-\note{Magnier et al}.  In short, sources are detected in all 5 filter
+\cite{magnier2017b}.  In short, sources are detected in all 5 filter
 images down to the $5\sigma$ significance.  The collection of detected
 sources is merged into a single master list.  If a source is detected
@@ -1080 +1080 @@
 
 \bibliographystyle{apj}
-% \bibliography{lib}{}
+%\bibliography{lib}{}
 \input{datasystem.bbl}
 
+
 \end{document}