Changeset 39853 for trunk/doc/release.2015/ps1.detrend/detrend.tex
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trunk/doc/release.2015/ps1.detrend/detrend.tex
r39852 r39853 125 125 %% http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2007ASPC..364..153M&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf 126 126 \section{Introduction and Survey Description} 127 128 This is the third in a series of seven papers describing the Pan-STARRS1 129 Surveys, 130 the data reduction techiques and the resulting data products. This paper (Paper III) 131 describes the details of the pixel processing algorithms, including 132 detrending, warping, and adding (to create stacked images) and subtracting 133 (to create difference images) and resulting image products and their 134 properties. 135 \citet[][Paper I]{chambers2017} provides an overview of the Pan-STARRS System, the 136 design and execution of the Surveys, the resulting image and catalog data 137 products, a discussion of the overall data quality and basic 138 characteristics, and a brief summary of important results. 139 %Magnier et al. 2017 (Paper II) 140 %Pan-STARRS Data Processing Stages 141 \citet[][Paper II]{magnier2017c} 142 describes how the various data processing stages are organised and 143 implemented 144 in the Imaging Processing Pipeline (IPP), including details of the 145 the processing database which is a critical element in the IPP 146 infrastructure. 147 %Waters et al. 2017 (Paper III) 148 %Pan-STARRS Pixel Processing : Detrending, Warping, Stacking 149 %\citet[][Paper III]{waters2017} 150 %Magnier et al. 2017 (Paper IV) 151 %Pan-STARRS Pixel Analysis : Source Detection 152 \citet[][Paper IV]{magnier2017a} 153 describes the details of the source detection and photometry, including 154 point-spread-function and extended source fitting models, and the 155 techniques for ``forced'' photometry measurements. 156 %Magnier et al. 2017 (Paper V) 157 %Pan-STARRS Photometric and Astrometric Calibration 158 \citet[][Paper V]{magnier2017b} 159 describes the final calibration process, and the resulting photometric and 160 astrometric quality. 161 The Pan-STARRS1 filters and photometric system has already been described 162 in detail in \cite{2012ApJ...750...99T}. 163 %Flewelling et al. 2017 (Paper VI) 164 %Pan-STARRS 1 Database and Data Products 165 \citet[][Paper VI]{flewelling2017} 166 describes the details of the resulting catalog data and its organization 167 in the Pan-STARRS database. 168 % 169 % 170 \citet[][Paper VII]{huber2017} 171 %Huber et al. 2017 (Paper VII) 172 describes the Medium Deep Survey in detail, including the unique issues and 173 data products specific to that survey. The Medium Deep Survey is not part 174 of Data Release 1. (DR1) 127 175 128 176 … … 1354 1402 pixels are masked. The large fraction of this masking is due to 1355 1403 regions that fall within the vignetted region. Defining the diameter 1356 of the unvignetted region to be 3 degrees, and excluding pixels that 1357 fall beyond this point reduces the static masking fraction to 9.7\%. 1404 of the unvignetted region to have be 3 degrees, and excluding pixels 1405 that fall beyond this point reduces the static masking fraction to 1406 9.7\%. 1358 1407 1359 1408 Unfortunately, due to the design of the OTAs and readout cells, a … … 1373 1422 across the field of view. Dynamic masking adds an additional $2-3\%$ 1374 1423 on average, with advisory burntool masking contributing the largest 1375 single component. 1424 single component. Table \ref{tab:mask fraction} contains estimates of 1425 the mask fraction in the GPC1 detector footprint by the sources of the 1426 masking for the 3 degree field of view, as well as for a larger 3.25 1427 degree field of view that allows addition unvignetted regions in the 1428 corners to contribute. 1429 1430 \begin{deluxetable}{lcc} 1431 \tablecolumns{3} 1432 \tablewidth{0pc} 1433 \tablecaption{Mask Fraction by Mask Source} 1434 \tablehead{\colhead{Mask Source}&\colhead{3 Degree FOV}&\colhead{3.25 Degree FOV}} 1435 \startdata 1436 No pixel & 4.44\% & 9.47\% \\ 1437 Detector defect & 6.37\% & 7.91\% \\ 1438 CTE issue & 2.62\% & 3.13\% \\ 1439 \enddata 1440 \label{tab:mask fraction} 1441 \end{deluxetable} 1442 1443 1376 1444 1377 1445
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