Changeset 39868 for trunk/doc/release.2015/ps1.datasystem/datasystem.tex
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- Dec 15, 2016, 3:48:40 PM (10 years ago)
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trunk/doc/release.2015/ps1.datasystem/datasystem.tex
r39865 r39868 1 %\documentclass[iop,floatfix]{emulateapj}1 \documentclass[iop,floatfix]{emulateapj} 2 2 % \documentclass[iop,floatfix,onecolumn]{emulateapj} 3 \documentclass[12pt,preprint]{aastex}3 % \documentclass[12pt,preprint]{aastex} 4 4 % \pdfoutput=1 5 5 … … 29 29 % list and (2) re-order the list at the bottom (and comment-out as needed) 30 30 \def\IfA{1} 31 \def\CfA{2} 32 \def\MPIA{3} 31 \def\LSST{2} 33 32 \def\Princeton{3} 34 \def\ USNO{4}35 \def\ JHU{1}33 \def\DUR{4} 34 \def\CfA{5} 36 35 37 36 % This example has a first author from UH: 38 37 \author{ 39 38 Eugene A. Magnier,\altaffilmark{\IfA} 40 IPP Team, 39 K.~C. Chambers,\altaffilmark{\IfA} 40 H.~A. Flewelling,\altaffilmark{\IfA} 41 J.~C. Hoblitt,\altaffilmark{\LSST} 42 M. E. Huber,\altaffilmark{\IfA} 43 % R. H. Lupton,\altaffilmark{\Princeton} 44 P.~A. Price,\altaffilmark{\Princeton} 45 W.~E. Sweeney,\altaffilmark{\IfA} 46 C. Z. Waters,\altaffilmark{\IfA} 41 47 %PS Builder List 48 L. Denneau,\altaffilmark{\IfA} 49 P. Draper,\altaffilmark{\DUR} 50 K. W. Hodapp,\altaffilmark{\IfA} 51 R. Jedicke,\altaffilmark{\IfA} 52 R.-P. Kudritzki,\altaffilmark{\IfA} 53 N. Metcalfe,\altaffilmark{\DUR} 54 C.~W. Stubbs,\altaffilmark{\CfA} 42 55 % W.~S. Burgett,\altaffilmark{\IfA} 43 % K.~C. Chambers,\altaffilmark{\IfA}44 % L. Denneau,\altaffilmark{\IfA}45 % P. Draper,\altaffilmark{\DUR}46 % H.~A. Flewelling,\altaffilmark{\IfA}47 56 % T. Grav,\altaffilmark{\IfA} 48 57 % J. N. Heasley,\altaffilmark{\IfA} 49 % K. W. Hodapp,\altaffilmark{\IfA}50 % M. E. Huber,\altaffilmark{\IfA}51 % R. Jedicke,\altaffilmark{\IfA}52 58 % N. Kaiser,\altaffilmark{\IfA} 53 % R.-P. Kudritzki,\altaffilmark{\IfA}54 59 % G. A. Luppino,\altaffilmark{\IfA} 55 % R. H. Lupton,\altaffilmark{\Princeton}56 % E. A. Magnier,\altaffilmark{\IfA}57 % N. Metcalfe,\altaffilmark{\DUH}58 60 % D. G. Monet,\altaffilmark{\USNO} 59 61 % J.~S. Morgan,\altaffilmark{\IfA} 60 62 % P. M. Onaka,\altaffilmark{\IfA} 61 % P.~A. Price,\altaffilmark{\Princeton}62 % C.~W. Stubbs,\altaffilmark{\CfA}63 % W.~E. Sweeney,\altaffilmark{\IfA}64 63 % J.~L. Tonry, \altaffilmark{\IfA} 65 % R. J. Wainscoat,\altaffilmark{\IfA} and 66 % C. Z. Waters,\altaffilmark{\IfA} 64 R. J. Wainscoat\altaffilmark{\IfA} 67 65 } % this bracket terminates author list 68 66 69 67 % The ordering here should be sequential, matching the sequence in the list of authors: 70 68 \altaffiltext{\IfA}{Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu HI 96822} 71 % \altaffiltext{\CfA}{Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138} 69 \altaffiltext{\LSST}{LSST Project Management Office, Tucson, AZ, U.S.A} 70 \altaffiltext{\Princeton}{Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA} 71 \altaffiltext{\DUR}{Department of Physics, Durham University, South Road, Durham DH1 3LE, UK} 72 \altaffiltext{\CfA}{Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138} 72 73 % \altaffiltext{\Princeton}{Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA} 73 74 % \altaffiltext{\USNO}{US Naval Observatory, Flagstaff Station, Flagstaff, AZ 86001, USA} … … 76 77 \begin{abstract} 77 78 78 Lorem ipsum dolor sit amet, consectetur adipiscing elit. Vestibulum 79 bibendum nisi id tristique posuere. Duis eu mollis nulla. Maecenas est 80 turpis, mattis tempor urna vitae, placerat rhoncus sem. Lorem ipsum 81 dolor sit amet, consectetur adipiscing elit. Sed quis velit 82 nisl. Aliquam erat volutpat. Cras lacinia, nisl tristique auctor 83 molestie, dolor nulla rhoncus purus, ac accumsan nunc nunc ac 84 nibh. Maecenas vitae mollis mauris. Ut sollicitudin pulvinar purus, 85 eget luctus lorem tincidunt vitae. Vestibulum eu mattis neque. Nulla 86 in tortor id urna dapibus gravida a vel leo. 79 The Pan-STARRS Image Processing Pipeline performs the processing 80 needed to downloaded, archive, and process all images obtained by the 81 Pan-STARRS telescopes. This article describes the overall data 82 analysis system. 87 83 88 84 \end{abstract} … … 91 87 \keywords{Surveys:\PSONE } 92 88 93 % \section{INTRODUCTION}\label{sec:intro} 89 \section{INTRODUCTION}\label{sec:intro} 90 91 This is the second in a series of seven papers describing the 92 Pan-STARRS1 Surveys, the data reduction techiques and the resulting 93 data products. This paper (Paper II) describes how the various data 94 processing stages are organised and implemented in the Imaging 95 Processing Pipeline (IPP), including details of the the processing 96 database which is a critical element in the IPP infrastructure . 97 98 %Chambers et al. 2017 (Paper I) 99 %The Pan-STARRS\,1 Surveys 100 \citet[][Paper I]{chambers2017} 101 provides an overview of the Pan-STARRS System, the design and 102 execution of the Surveys, the resulting image and catalog data 103 products, a discussion of the overall data quality and basic 104 characteristics, and a brief summary of important results. 105 106 %Magnier et al. 2017 (Paper II) 107 %Pan-STARRS Data Processing Stages 108 %\citet[][Paper II]{magnier2017c} 109 %describes how the various data processing stages are organised and implemented 110 %in the Imaging Processing Pipeline (IPP), including details of the 111 %the processing database which is a critical element in the IPP infrastructure . 112 113 %Waters et al. 2017 (Paper III) 114 %Pan-STARRS Pixel Processing : Detrending, Warping, Stacking 115 \citet[][Paper III]{waters2017} 116 describes the details of the pixel processing algorithms, including detrending, warping, and adding (to create stacked images) and subtracting (to create difference images) and resulting image products and their properties. 117 118 119 %Magnier et al. 2017 (Paper IV) 120 %Pan-STARRS Pixel Analysis : Source Detection 121 \citet[][Paper IV]{magnier2017a} 122 describes the details of the source detection and photometry, including point-spread-function and extended source fitting models, and the techniques for ``forced" photometry measurements. 123 124 %Magnier et al. 2017 (Paper V) 125 %Pan-STARRS Photometric and Astrometric Calibration 126 \citet[][Paper V]{magnier2017b} 127 describes the final calibration process, and the resulting photometric and astrometric quality. 128 129 130 %Flewelling et al. 2017 (Paper VI) 131 %Pan-STARRS 1 Database and Data Products 132 \citet[][Paper VI]{flewelling2017} 133 describes the details of the resulting catalog data and its organization in the Pan-STARRS database. 134 % 135 % 136 \citet[][Paper VII]{huber2017} 137 %Huber et al. 2017 (Paper VII) 138 describes the Medium Deep Survey in detail, including the unique issues and data products specific to that survey. The Medium Deep Survey is not part of Data Release 1. (DR1) 139 140 % 141 The Pan-STARRS1 filters and photometric system have already been 142 described in detail in \cite{2012ApJ...750...99T}. 143 144 {\color{red} {\em Note: These papers are being placed on arXiv.org to 145 provide crucial support information at the time of the public 146 release of Data Release 1 (DR1). We expect the arXiv versions to 147 be updated prior to submission to the Astrophysical Journal in 148 January 2017. Feedback and suggestions for additional information 149 from early users of the data products are welcome during the 150 submission and refereeing process.}} 94 151 95 152 \section{IPP Software Subsystems} … … 852 909 \subsection{UH Cray Cluster} 853 910 911 \acknowledgments 912 913 The Pan-STARRS1 Surveys (PS1) have been made possible through 914 contributions of the Institute for Astronomy, the University of 915 Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its 916 participating institutes, the Max Planck Institute for Astronomy, 917 Heidelberg and the Max Planck Institute for Extraterrestrial Physics, 918 Garching, The Johns Hopkins University, Durham University, the 919 University of Edinburgh, Queen's University Belfast, the 920 Harvard-Smithsonian Center for Astrophysics, the Las Cumbres 921 Observatory Global Telescope Network Incorporated, the National 922 Central University of Taiwan, the Space Telescope Science Institute, 923 the National Aeronautics and Space Administration under Grant 924 No. NNX08AR22G issued through the Planetary Science Division of the 925 NASA Science Mission Directorate, the National Science Foundation 926 under Grant No. AST-1238877, the University of Maryland, and Eotvos 927 Lorand University (ELTE) and the Los Alamos National Laboratory. 928 929 \bibliographystyle{apj} 930 % \bibliography{lib}{} 931 \input{datasystem.bbl} 932 854 933 \end{document} 855 934
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