Index: trunk/doc/release.2015/ps1.detrend/Makefile =================================================================== --- trunk/doc/release.2015/ps1.detrend/Makefile (revision 40614) +++ trunk/doc/release.2015/ps1.detrend/Makefile (revision 40615) @@ -14,40 +14,42 @@ quick: detrend.quick.pdf +ALLPICS = \ +images/o5677g0123o_M_OS_NL_XY23_sm.png \ +images/o5677g0123o_to_DARK_XY23_sm.png \ +images/B_profile_v1.pdf \ +images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_sm.png \ +images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_sm.png \ +images/o5220g0025o_nofringe_XY53_sm.png \ +images/o5220g0025o_fringe_XY53_sm.png \ +images/gpc1_mask_indexed.png \ +images/full_fpa_ghosts_sm.png \ +images/full_fpa_glints_sm.png \ +images/o6802g0338o_SATSTAR_XY51_sm.png \ +images/o5677g0123o_nbt_XY11.png \ +images/o5677g0124o_nbt_XY11.png \ +images/o5677g0123o_wbt_XY11.png \ +images/o5677g0124o_wbt_XY11.png \ +images/o5677g0123n4o_XY11_bt_trail.pdf \ +images/pattern_row_edit.png \ +images/o5379g0103o_npt_XY57_sm.png \ +images/o5379g0103o_wpt_XY57_sm.png \ +images/warp_2046019_sci_sm.png \ +images/warp_2046019_var_sm.png \ +images/warp_2046019_mask.png \ +images/stack_3956997_sci_sm.png \ +images/stack_3956997_mask.png \ +images/stack_3956997_var_sm.png \ +images/stack_3956997_num_sm.png \ +images/stack_3956997_exp_sm.png \ +images/stack_3956997_expwt_sm.png + FILES = \ ../inputs/astro.sty \ ../inputs/apj.bst \ -../inputs/lib.bib \ -detrend.tex \ -detrend.bbl \ -images/o5677g0123o_XY11_bt_trail.png \ -images/o5677g0124o_XY11_bt_trail.png \ -images/o5677g0123o_XY11_nobt.png \ -images/o5677g0124o_XY11_nobt.png \ -images/o5677g0123o_XY11_bt.png \ -images/o5677g0124o_XY11_bt.png \ -images/linearity_XY27_xy16.png \ -images/o5677g0123o_M_OS_NL_XY23_b1.jpg \ -images/o5677g0123o_to_DARK_XY23_b1.jpg \ -images/B_profile_ex.png \ -images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_b1.jpg \ -images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_b1.jpg \ -images/pattern_row_edit.png \ -images/o5379g0103o_XY57_nopat.png \ -images/o5379g0103o_XY57_pat.png \ -images/o5220g0025o_XY53_nofringe.png \ -images/o5220g0025o_XY53_fringe.png \ -images/gpc1_mask_indexed.png \ -images/full_fpa_ghosts.jpg \ -images/glint_example_o5379g0103o.jpg \ -images/o6802g0338o_XY51_b1.jpg \ -images/warp_1046511_sci.jpg \ -images/warp_1046511_mask.jpg \ -images/warp_1046511_wt.jpg \ -images/stack_3775944_sci.jpg \ -images/stack_3775944_mask.jpg \ -images/stack_3775944_wt.jpg \ -images/stack_3775944_num.jpg \ -images/stack_3775944_exp.jpg \ -images/stack_3775944_expwt.jpg +$(ALLPICS) \ +detrend.tex + +detrend.pdf: $(FILES) +detrend.tgz: $(FILES) include ../Makefile.Common Index: trunk/doc/release.2015/ps1.detrend/detrend.tex =================================================================== --- trunk/doc/release.2015/ps1.detrend/detrend.tex (revision 40614) +++ trunk/doc/release.2015/ps1.detrend/detrend.tex (revision 40615) @@ -181,5 +181,5 @@ contained only average information resulting from the many individual images obtained by the $3\pi$ Survey observations. A second data -release, DR2, was made available \note{20 January 2019}. DR2 provides +release, DR2, was made available 28 January 2019. DR2 provides measurements from all of the individual exposures, and include an improved calibration of the PV3 processing of that dataset. @@ -415,8 +415,8 @@ \centering \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_M_OS_NL_XY23.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_M_OS_NL_XY23_sm.png} \end{minipage}% \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_to_DARK_XY23.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_to_DARK_XY23_sm.png} \end{minipage} \caption{{\bf Dark Correction:} An example of the dark model application to exposure o5677g0123o, OTA23 (2011-04-26, 43s \gps{} filter). The left panel shows the image data mosaicked to the OTA level, and has had the static mask applied, the overscan subtracted, and the detector non-linearity corrected. The right panel, shows the same exposure with the dark applied in addition to the processing shown on the left, removing the amplifier glows in the cell corners.} @@ -563,8 +563,8 @@ \centering \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_sm.png} \end{minipage}% \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_sm.png} \end{minipage} \caption{{\bf Video Dark:} An example of the video dark model application to exposure o5677g0123o, OTA22 (2011-04-26, 43s \gps{} filter), which has a video cell located in cell xy16. The left panel shows the image data mosaicked to the OTA level, and has had the static mask applied, the overscan subtracted, the detector non-linearity corrected, and a regular dark applied. The right panel, shows the same exposure with a video dark applied instead of the standard dark. The main impact of this change is the improved correction of the corner glows, which are over subtracted with the standard dark.} @@ -704,8 +704,8 @@ \centering \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_nofringe_XY53.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_nofringe_XY53_sm.png} \end{minipage}% \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_fringe_XY53.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_fringe_XY53_sm.png} \end{minipage} \caption{{\bf Fringing:} Example of the \yps{} filter fringe pattern @@ -985,5 +985,5 @@ \centering % \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts.jpg} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts_sm.png} \caption{{\bf Ghosts:} Example of the full GPC1 field of view illustrating the sources and destinations of optical ghosts on exposure o5677g0123o (2011-04-26, 43s \gps{} filter). The bright stars on OTA33 and OTA44 result in nearly circular ghosts on the opposite OTA. In contrast, the trio of stars on OTA11 result in very elongated ghosts on OTA66.} \label{fig:optical ghosts} @@ -1016,5 +1016,5 @@ \centering % \includegraphics[width=0.9\hsize,angle=0,clip]{images/glint_example_o5379g0103o.jpg} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_glints.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_glints_sm.png} \caption{{\bf Glints:} Example of a glint on exposure o5379g0103o (2010-07-02, 45s \ips{} filter). The source star out of the field of view creates a long reflection that extends through OTA73 and OTA63.} \label{fig:optical glints} @@ -1041,5 +1041,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o6802g0338o_SATSTAR_XY51.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o6802g0338o_SATSTAR_XY51_sm.png} \caption{Example of saturated star, with diffraction spikes extending from the core on exposure o6802g0338o, OTA51 (2014-05-25, 45s \gps{} filter).} \label{fig:saturated star} @@ -1480,8 +1480,8 @@ \centering \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57_sm.png} \end{minipage}% \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57_sm.png} \end{minipage} \caption{{\bf Correlated Noise:} Example of the PATTERN.ROW correction on exposure o5379g0103o OTA57 cell xy01 (\ips{} filter 45s). The left panel shows the cell with all appropriate detrending except the PATTERN.ROW, and the right shows the same cell with PATTERN.ROW applied. The correction reduces the correlated noise on the right side, which is most distant from the read out amplifier. There is a slight over subtraction along the rows near the bright star.} @@ -1756,5 +1756,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_sci.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_sci_sm.png} \caption{Example of the warp image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197) for exposure @@ -1769,5 +1769,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_var.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_var_sm.png} \caption{Example of the warp variance image for skycell skycell.1146.095 of exposure o5104g0266o, the same as in Figure @@ -2088,5 +2088,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_sci.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_sci_sm.png} \caption{Example of the stack image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197) in the \rps{} @@ -2117,5 +2117,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_var.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_var_sm.png} \caption{Example of the stack variance image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197) @@ -2131,5 +2131,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_num.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_num_sm.png} \caption{Example of the stack number image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197) @@ -2144,5 +2144,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_exp.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_exp_sm.png} \caption{Example of the stack exposure time image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197) @@ -2156,5 +2156,5 @@ \begin{figure} \centering - \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_expwt.png} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_expwt_sm.png} \caption{Example of the stack weighted exposure image for skycell skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197)