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Changeset 40615


Ignore:
Timestamp:
Jan 27, 2019, 10:28:54 AM (7 years ago)
Author:
eugene
Message:

resize big images down by factor of 2

Location:
trunk/doc/release.2015/ps1.detrend
Files:
18 added
2 edited

Legend:

Unmodified
Added
Removed

  • trunk/doc/release.2015/ps1.detrend/Makefile

    r40564 r40615  
    1414quick: detrend.quick.pdf
    1515
     16ALLPICS = \
     17images/o5677g0123o_M_OS_NL_XY23_sm.png \
     18images/o5677g0123o_to_DARK_XY23_sm.png \
     19images/B_profile_v1.pdf \
     20images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_sm.png \
     21images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_sm.png \
     22images/o5220g0025o_nofringe_XY53_sm.png \
     23images/o5220g0025o_fringe_XY53_sm.png \
     24images/gpc1_mask_indexed.png \
     25images/full_fpa_ghosts_sm.png \
     26images/full_fpa_glints_sm.png \
     27images/o6802g0338o_SATSTAR_XY51_sm.png \
     28images/o5677g0123o_nbt_XY11.png \
     29images/o5677g0124o_nbt_XY11.png \
     30images/o5677g0123o_wbt_XY11.png \
     31images/o5677g0124o_wbt_XY11.png \
     32images/o5677g0123n4o_XY11_bt_trail.pdf \
     33images/pattern_row_edit.png \
     34images/o5379g0103o_npt_XY57_sm.png \
     35images/o5379g0103o_wpt_XY57_sm.png \
     36images/warp_2046019_sci_sm.png \
     37images/warp_2046019_var_sm.png \
     38images/warp_2046019_mask.png \
     39images/stack_3956997_sci_sm.png \
     40images/stack_3956997_mask.png \
     41images/stack_3956997_var_sm.png \
     42images/stack_3956997_num_sm.png \
     43images/stack_3956997_exp_sm.png \
     44images/stack_3956997_expwt_sm.png
     45
    1646FILES = \
    1747../inputs/astro.sty \
    1848../inputs/apj.bst \
    19 ../inputs/lib.bib \
    20 detrend.tex \
    21 detrend.bbl \
    22 images/o5677g0123o_XY11_bt_trail.png \
    23 images/o5677g0124o_XY11_bt_trail.png \
    24 images/o5677g0123o_XY11_nobt.png \
    25 images/o5677g0124o_XY11_nobt.png \
    26 images/o5677g0123o_XY11_bt.png \
    27 images/o5677g0124o_XY11_bt.png \
    28 images/linearity_XY27_xy16.png \
    29 images/o5677g0123o_M_OS_NL_XY23_b1.jpg \
    30 images/o5677g0123o_to_DARK_XY23_b1.jpg \
    31 images/B_profile_ex.png \
    32 images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_b1.jpg \
    33 images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_b1.jpg \
    34 images/pattern_row_edit.png \
    35 images/o5379g0103o_XY57_nopat.png \
    36 images/o5379g0103o_XY57_pat.png \
    37 images/o5220g0025o_XY53_nofringe.png \
    38 images/o5220g0025o_XY53_fringe.png \
    39 images/gpc1_mask_indexed.png \
    40 images/full_fpa_ghosts.jpg \
    41 images/glint_example_o5379g0103o.jpg \
    42 images/o6802g0338o_XY51_b1.jpg \
    43 images/warp_1046511_sci.jpg \
    44 images/warp_1046511_mask.jpg \
    45 images/warp_1046511_wt.jpg \
    46 images/stack_3775944_sci.jpg \
    47 images/stack_3775944_mask.jpg \
    48 images/stack_3775944_wt.jpg \
    49 images/stack_3775944_num.jpg \
    50 images/stack_3775944_exp.jpg \
    51 images/stack_3775944_expwt.jpg
     49$(ALLPICS) \
     50detrend.tex
     51
     52detrend.pdf: $(FILES)
     53detrend.tgz: $(FILES)
    5254
    5355include ../Makefile.Common

  • trunk/doc/release.2015/ps1.detrend/detrend.tex

    r40614 r40615  
    181181contained only average information resulting from the many individual
    182182images obtained by the $3\pi$ Survey observations.  A second data
    183 release, DR2, was made available \note{20 January 2019}.  DR2 provides
     183release, DR2, was made available 28 January 2019.  DR2 provides
    184184measurements from all of the individual exposures, and include an
    185185improved calibration of the PV3 processing of that dataset.
    … …  
    415415  \centering
    416416  \begin{minipage}{0.45\hsize}
    417     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_M_OS_NL_XY23.png}
     417    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_M_OS_NL_XY23_sm.png}
    418418  \end{minipage}%
    419419  \begin{minipage}{0.45\hsize}
    420     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_to_DARK_XY23.png}
     420    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_to_DARK_XY23_sm.png}
    421421  \end{minipage}
    422422  \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.}
    … …  
    563563  \centering
    564564  \begin{minipage}{0.45\hsize}
    565     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22.png}
     565    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_Rdark_XY22_sm.png}
    566566  \end{minipage}%
    567567  \begin{minipage}{0.45\hsize}
    568     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22.png}
     568    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_VIDEODARK_VDim_VDdark_XY22_sm.png}
    569569  \end{minipage}
    570570  \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.}
    … …  
    704704  \centering
    705705  \begin{minipage}{0.45\hsize}
    706     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_nofringe_XY53.png}
     706    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_nofringe_XY53_sm.png}
    707707  \end{minipage}%
    708708  \begin{minipage}{0.45\hsize}
    709     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_fringe_XY53.png}
     709    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5220g0025o_fringe_XY53_sm.png}
    710710  \end{minipage}
    711711  \caption{{\bf Fringing:} Example of the \yps{} filter fringe pattern
    … …  
    985985  \centering
    986986% \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts.jpg}
    987   \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts.png}
     987  \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts_sm.png}
    988988  \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.}
    989989  \label{fig:optical ghosts}
    … …  
    10161016  \centering
    10171017% \includegraphics[width=0.9\hsize,angle=0,clip]{images/glint_example_o5379g0103o.jpg}
    1018   \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_glints.png}
     1018  \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_glints_sm.png}
    10191019  \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.}
    10201020  \label{fig:optical glints}
    … …  
    10411041\begin{figure}
    10421042  \centering
    1043   \includegraphics[width=0.9\hsize,angle=0,clip]{images/o6802g0338o_SATSTAR_XY51.png}
     1043  \includegraphics[width=0.9\hsize,angle=0,clip]{images/o6802g0338o_SATSTAR_XY51_sm.png}
    10441044  \caption{Example of saturated star, with diffraction spikes extending from the core on exposure o6802g0338o, OTA51 (2014-05-25, 45s \gps{} filter).}
    10451045  \label{fig:saturated star}
    … …  
    14801480  \centering
    14811481  \begin{minipage}{0.45\hsize}
    1482     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57.png}
     1482    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57_sm.png}
    14831483  \end{minipage}%
    14841484  \begin{minipage}{0.45\hsize}
    1485     \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57.png}
     1485    \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57_sm.png}
    14861486  \end{minipage}
    14871487  \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.}
    … …  
    17561756\begin{figure}
    17571757  \centering
    1758   \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_sci.png}
     1758  \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_sci_sm.png}
    17591759  \caption{Example of the warp image for skycell skycell.1146.095
    17601760    centered at ($\alpha,\delta$) = (11.934, -4.197) for exposure
    … …  
    17691769\begin{figure}
    17701770  \centering
    1771   \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_var.png}
     1771  \includegraphics[width=0.9\hsize,angle=0,clip]{images/warp_2046019_var_sm.png}
    17721772  \caption{Example of the warp variance image for skycell
    17731773    skycell.1146.095 of exposure o5104g0266o, the same as in Figure
    … …  
    20882088\begin{figure}
    20892089  \centering
    2090   \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_sci.png}
     2090  \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_sci_sm.png}
    20912091  \caption{Example of the stack image for skycell skycell.1146.095
    20922092    centered at ($\alpha,\delta$) = (11.934, -4.197) in the \rps{}
    … …  
    21172117\begin{figure}
    21182118  \centering
    2119   \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_var.png}
     2119  \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_var_sm.png}
    21202120  \caption{Example of the stack variance image for skycell
    21212121    skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197)
    … …  
    21312131\begin{figure}
    21322132  \centering
    2133   \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_num.png}
     2133  \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_num_sm.png}
    21342134  \caption{Example of the stack number image for skycell
    21352135    skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197)
    … …  
    21442144\begin{figure}
    21452145  \centering
    2146   \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_exp.png}
     2146  \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_exp_sm.png}
    21472147  \caption{Example of the stack exposure time image for skycell
    21482148    skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197)
    … …  
    21562156\begin{figure}
    21572157  \centering
    2158   \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_expwt.png}
     2158  \includegraphics[width=0.9\hsize,angle=0,clip]{images/stack_3956997_expwt_sm.png}
    21592159  \caption{Example of the stack weighted exposure image for skycell
    21602160    skycell.1146.095 centered at ($\alpha,\delta$) = (11.934, -4.197)
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