Changeset 40599
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- Jan 9, 2019, 4:35:23 PM (8 years ago)
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trunk/doc/release.2015/ps1.datasystem/datasystem.tex
r40593 r40599 127 127 are described by \cite{chambers2017}. 128 128 129 Pan-STARRS produced its first large-scale public data release, Data 130 Release 1 (DR1) on 16 December 2016. DR1 contains the results of the 131 third full reduction of the Pan-STARRS $3\pi$ Survey archival data, 132 identified as PV3. Previous reductions \citep[PV0, PV1, PV2; 133 see][]{magnier2017.datasystem} were used internally for pipeline 134 optimization and the development of the initial photometric and 135 astrometric reference catalog \citep{magnier2017.calibration}. The 136 products from these reductions were not publicly released, but have 137 been used to produce a wide range of scientific papers from the 138 Pan-STARRS 1 Science Consortium members \citep{chambers2017}. DR1 139 contained only average information resulting from the many individual 140 images obtained by the $3\pi$ Survey observations. A second data 141 release, DR2, was made available \note{20 January 2019}. DR2 provides 142 measurements from all of the individual exposures, and include an 143 improved calibration of the PV3 processing of that dataset. 144 129 145 This is the second in a series of seven papers describing the 130 146 Pan-STARRS1 Surveys, the data reduction techiques and the resulting … … 148 164 %The Pan-STARRS\,1 Surveys 149 165 \citet[][Paper I]{chambers2017} 150 provide san overview of the Pan-STARRS System, the design and166 provide an overview of the Pan-STARRS System, the design and 151 167 execution of the Surveys, the resulting image and catalog data 152 168 products, a discussion of the overall data quality and basic … … 162 178 %Waters et al. 2017 (Paper III) 163 179 %Pan-STARRS Pixel Processing : Detrending, Warping, Stacking 164 \citet[][Paper III]{waters2017} 165 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. 166 180 \citet[][Paper III]{waters2017} describe the details of the pixel 181 processing algorithms, including detrending, warping, and adding (to 182 create stacked images) and subtracting (to create difference images) 183 and resulting image products and their properties. 167 184 168 185 %Magnier et al. 2017 (Paper IV) 169 186 %Pan-STARRS Pixel Analysis : Source Detection 170 \citet[][Paper IV]{magnier2017.analysis} 171 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. 187 \citet[][Paper IV]{magnier2017.analysis} describe the details of the 188 source detection and photometry, including point-spread-function and 189 extended source fitting models, and the techniques for ``forced'' 190 photometry measurements. 172 191 173 192 %Magnier et al. 2017 (Paper V) 174 193 %Pan-STARRS Photometric and Astrometric Calibration 175 194 \citet[][Paper V]{magnier2017.calibration} 176 describes the final calibration process, and the resulting photometric and astrometric quality. 177 195 describe the final calibration process, and the resulting photometric and astrometric quality. 178 196 179 197 %Flewelling et al. 2017 (Paper VI) 180 198 %Pan-STARRS 1 Database and Data Products 181 199 \citet[][Paper VI]{flewelling2017} 182 describes the details of the resulting catalog data and its organization in the Pan-STARRS database. 183 % 184 % 185 \citet[][Paper VII]{huber2017} 200 describe the details of the resulting catalog data and its organization in the Pan-STARRS database. 201 186 202 %Huber et al. 2017 (Paper VII) 187 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 or 2. 203 \citet[][Paper VII]{huber2017} describe the Medium Deep Survey in 204 detail, including the unique issues and data products specific to that 205 survey. The Medium Deep Survey is not part of Data Releases 1 or 2 and 206 will be made available in a future data release. 188 207 189 208 Section~\ref{sec:overview} provides an overview of the full data … … 329 348 steps are discussed in detail by 330 349 \citet[][]{magnier2017.analysis}. The data products from the 331 camera, stack photometry, and forced-warp photometry analysis stages350 camera, stack, and forced-warp photometry analysis stages 332 351 are ingested into the internal calibration database (DVO, the Desktop 333 352 Virtual Observatory) and used for photometric and astrometric
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