- Timestamp:
- Dec 14, 2016, 6:10:30 PM (10 years ago)
- Location:
- trunk/doc/release.2015/ps1.detrend
- Files:
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- 2 edited
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arxiv.metadata (modified) (1 diff)
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detrend.tex (modified) (7 diffs)
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trunk/doc/release.2015/ps1.detrend/arxiv.metadata
r39861 r39864 1 1 Pan-Starrs Pixel Processing: Detrending, Warping, Stacking 2 2 3 C. Z. Waters, E. A. Magnier, P. A. Price, K. C. Chambers, H. A. Flewelling, M. E. Huber, R. H. Lupton, A. Rest, W. E. Sweeney, J. L. Tonry, W. M. Wood-Vasey, PS1 Builders3 C. Z. Waters, E. A. Magnier, P. A. Price, K. C. Chambers, H. A. Flewelling, M. E. Huber, R. H. Lupton, A. Rest, W. E. Sweeney, J. L. Tonry, R. J. Wainscoat, W. M. Wood-Vasey, PS1 Builders 4 4 5 5 The Pan-STARRS1 Science Consortium have carried out a set of imaging surveys using the 1.4 giga-pixel GPC1 camera on the PS1 telescope. As this camera is composed of many individual electronic readouts, and covers a very large field of view, great care was taken to ensure that the many instrumental effects were corrected to produce the most uniform detector response possible. We present the image detrending steps used as part of the processing of the data contained within the public release of the Pan-STARRS1 Data Release 1 (DR1). In addition to the single image processing, the methods used to transform the 375,573 individual exposures into a common sky-oriented grid are discussed, as well as those used to produce both the image stack and difference combination products. -
trunk/doc/release.2015/ps1.detrend/detrend.tex
r39862 r39864 70 70 W.~E. Sweeney,\altaffilmark{\IfA} 71 71 J.~L. Tonry, \altaffilmark{\IfA} 72 R.~J. Wainscoat,\altaffilmark{\IfA} 72 73 W.~M. Wood-Vasey,\altaffilmark{\Pitt} 73 74 PS1 Builders … … 88 89 % P. M. Onaka,\altaffilmark{\IfA} 89 90 % C.~W. Stubbs,\altaffilmark{\CfA} 90 % R. J. Wainscoat,\altaffilmark{\IfA} and91 % C. Z. Waters,\altaffilmark{\IfA}92 91 } % this bracket terminates author list 93 92 … … 266 265 and pixel $(1,1)$ to the top right of their position. 267 266 268 % Note taken verbatim from Ken's Paper 1.269 267 \textit{Note: These papers are being placed on the arXiv.org to 270 268 provide crucial support information at the time of the public … … 274 272 users of the data products are welcome during the submission and 275 273 refereeing process.} 276 277 % Discuss 2-phase/3-phase device differnces278 274 279 275 … … 771 767 \subsubsection{Pattern Row} 772 768 %% Statistics so I have them written down somewhere 773 %% chipProcessedImfile.bg/bg_stdev by filter for XY33 (a ``good''chip)769 %% chipProcessedImfile.bg/bg_stdev by filter for XY33 (a good chip) 774 770 %% filter bg_mean stdev median Qsig bg_stdev_mean stdev median Qsig 775 771 %% g 36.37422026669 64.64175104057 32.693 6.10284 14.696938349131 78.80460307171 8.8401 0.5417843 … … 779 775 %% y 371.09019536218 293.57439970375 288.481 133.38769 43.724342221691 135.04286534327 19.9029 7.5396461 780 776 781 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_Bias_Pattern_Study782 777 As discussed above in the dark and noisemap sections, certain 783 778 detectors have significant bias offsets between adjacent rows, caused … … 2170 2165 2171 2166 2172 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_Detrend_Documentation2173 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_Detrend_Documentation#Currentdetrends2174 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/stacking_coverage.201303072175 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/staticsky.20120706_excess_detections2176 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/Stack_Rejection_Discussion2177 % http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/Stack_Algorithm
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