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Changes between Initial Version and Version 1 of MD02.refstack.20130815


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Timestamp:
Aug 19, 2013, 1:39:51 PM (13 years ago)
Author:
Mark Huber
Comment:

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  • MD02.refstack.20130815

    v1 v1  
     1= Summary of MD02.refstack.20130815 (unfinished) =
     2[[PageOutline]]
     3
     4(back to [wiki:MediumDeepFields] summary)
     5
     6Similar to the revised MD02.refstack.20120927 ([wiki:MD02.refstack.20120927]) refstacks for the 2012 season, these include recent improvements for the PV2. Overall fewer inputs to the refstack were done this round and may not be as deep as last season.
     7
     8 * '''PV2 1D convolution now done with MD fields'''
     9 * '''appear to still be psphot problems in poor PSF solution for skycell/regions that may not be realistic (i.e., not in center).
     10
     11MD02 observations:
     12 * planned return to field 8/20/2013 (OC168)
     13 * (some 2008 but pre-survey)
     14{{{
     15| exp_name    | filter  | dateobs             | comment                         |
     16+-------------+---------+---------------------+---------------------------------+
     17| o4740g0323o | g.00000 | 2008-10-01 14:12:56 | md02_2008-09-30 MD02 center     |
     18..
     19| o4803g0125o | i.00000 | 2008-12-03 09:06:03 | md02_2008-12-02_i MD02 center   |
     20----
     21| o5078g0271o | y.00000 | 2009-09-04 14:31:20 | MD02 y MJD55078 MD02 center     |
     22..
     23| o5223g0007o | z.00000 | 2010-01-27 05:11:16 | MD02 z MJD55223 MD02 center     |
     24----
     25| o5439g0579o | z.00000 | 2010-08-31 14:54:22 | MD02 z N5439 MD02 center        |
     26..
     27| o5597g0068o | i.00000 | 2011-02-05 05:26:02 | MD02 i N5597 MD02 center        |
     28----
     29| o5814g0558o | y.00000 | 2011-09-10 14:44:31 | MD02 y N5814 MD02 center        |
     30..
     31| o5985g0031o | z.00000 | 2012-02-28 05:29:41 | MD02 z N5984 MD02 center        |
     32----
     33| o6197g0469o | y.00000 | 2012-09-27 13:16:25 | MD02 y N6197 MD02 center        |
     34..
     35| o6353g0056o | z.00000 | 2013-03-02 05:29:51 | MD02 z N6353 MD02 center        |
     36}}}
     37
     38 
     39
     40
     41|| '''Filter''' || '''N total''' || '''N FWHM<8 pixels''' ||  '''N (FWHM<8 pixels for 2012''' || '''N FWHM<6 pixels''' ||  '''N (FWHM<6 pixels for 2012''' ||
     42|| || || || ||
     43|| 2010--2013 || || || ||
     44|| g || 343 || 320 || 69 || 240 || 52 ||
     45|| r || 363 || 343 || 91 || 270 || 60 ||
     46|| i || 464 || 448 || 137 || 353 || 104 ||
     47|| z || 571 || 554 || 176 || 508 || 155 ||
     48|| y || 565 || 533 || 224 || 487 || 217 ||
     49|| || || || ||
     50|| 2009--2013 || || || ||
     51|| g || 404 || 370 || 69 || 274 || 52 || 
     52|| r || 424 || 393 || 91 || 302 || 60 ||
     53|| i || 567 || 548 || 137 || 432 || 104 ||
     54|| z || 681 || 661 || 176 || 606 || 155 ||
     55|| y || 613 || 575 || 224 || 509 || 217 ||
     56|| || || || ||
     57 * 2012 wasn't a great season for MD01 gr, but better than MD09
     58
     59
     60Status:
     61 * 08/15/2013 selected exposure reprocessing chip->warp for refstack started
     62 * 08/17 exposures finished (processing issues).
     63 * 08/18 reftests started, both ISIS and 1D to test rejections, evaluations made (looks good)
     64 * 08/19 refstack started
     65 * 08/20? refstack finished, checked and working on problem skycells found/fixed if possible.
     66 * 08/20? staticsky single filter only finished and mappings started
     67 * 08/20? mappings finished, field pre-obs exposures setup for diffims and finished, reftest+refstack to distribution
     68 * 08/21? finished updating wiki
     69
     70
     71== MD02.V3  Processing (chip->warp + refstack) ==
     72
     73Exposure reprocessing was done for only a limited number (~150) of the best images from 2010-2012/2013 to provide a balance of N input warps for some depth minimum and assist poor pixel rejection versus best seeing, excluding exposures with large background, low zeropoints and large elongation.
     74
     75Processing chip-warp and the refstack itself has the same label, data_group
     76 * label: MD02.refstack.20130815 --> ''once set as active refstack for diffims, stack label will change to MD02.refstack'', chip/cam/warp label will remain the same
     77 * data_group: MD02.refstack.20130815
     78
     79
     80The ipp-20130712 tag used
     81 * [wiki:GPC1_Detrend_Documentation#Currentdetrends] -- new video darks as started with MD10.refstack.20130731
     82 * dynamic masks now propagating through to warps -- ghost mask is slightly offset or missing at times -- will not be fixed for PV2 and will have ghost/junk clusters still (worse with fewer inputs)
     83 * 1-D convolution PV2 -- has been fixed to just use the max input PSF for target PSF as well as some masking bugs
     84 * changes to psphot, PSF_MAJOR,MINOR root(2) different but appropriate now and 2*root(2) for FWHM; may be stability issue in PSF fitting
     85 * SCL_ keyword fixed back to if rejected the scaling value changed -- now 0 instead of previous value of 1
     86 * new reduction class with clear name MD_REF_STACK, MD_REF_STACK_1DG
     87 * SAFE config now set to false -- has helped to fill in ratty edges
     88
     89
     90Histograms and scatter plots of N exposures and their FWHM major, elongation, zeropoint and background by MJD from the camera stage (i.e., full exposure stats) for the sample of reprocessed exposures (red) and used for refstack.20130731 (top blue) and used for refstack.20120803 (bottom blue) in grizy order.  This replaces the simple histograms of the FWHM major, minor  and elongation.
     91
     92|| [[Image(.g.expfwhmzptbgmjd.png,300px)]] || [[Image(.r.expfwhmzptbgmjd.png,300px)]] || [[Image(.i.expfwhmzptbgmjd.png,300px)]] ||
     93|| [[Image(.z.expfwhmzptbgmjd.png,300px)]] || [[Image(.y.expfwhmzptbgmjd.png,300px)]] ||   ||
     94
     95
     96Test stack (reftest) sample also made again for skycell.055 with different number of input warps.
     97 * label: MD02.reftest.20130815
     98 * data_group:
     99  * MD02.reftest.20130815.c#f<FWHM cut> where #=comparison run, <FWHM cut>=cut  <fwhm_major from camProcessedExp x10>
     100  * MD02.reftest.20130815.all.<FWHM cut> where all means 05/2010+2011+2012/2013 data possible, <FWHM cut>=cut <fwhm_major from camProcessedExp x10>
     101  * MD02.reftest.20130815.2012.<FWHM cut> where 2012 means 2012/2013 data only for season stack example case, <FWHM cut>=cut <fwhm_major from camProcessedExp x10>
     102 * excluding 2009 since usually not very good, or uncharacteristically too good (avoiding problems basically)
     103 * c1 cuts
     104{{{
     105filter: (FWHM set), elongation, zeropoint, background limits
     106y: (3.75, 3.85, 3.95, 4.1), 1.3, 23.0, 4000 --
     107z: (3.75, 3.95, 4.05, 4.2), 1.3, 24.0, 3000 --
     108i: (4.0, 4.2, 4.4, 4.6), 1.25, 24.3, 2000 --
     109r: (4.45, 4.6, 5.0, 5.5), 1.25, 24.3, 700 --
     110g: (5.2, 5.4, 5.6, 5.9max), 1.25, 24.3, 500 --
     111--> refstack starts with  pixels for upper cut in grizy (may go smaller based on MEAN+1.0*STDDEV)
     112}}}
     113
     114Summary comparison table with the approximate FWHM (major) as the PSF FWHM from a center field skycell (V3=055) after running psphot on the stacks.
     115
     116{{{
     117| data_group                        | filter  | stack_id | warps_in | warps_rej |  FWHM_MAJ   IQ_FW1 (pixels)
     118+-----------------------------------+---------+----------+----------+-----------+
     119--> 2013 refstack
     120
     121--> reftest comparisons                                                 
     122
     123
     124--> previous 2012 refstack                                     
     125
     126
     127}}}
     128
     129As before, the FWHM_MAJOR with the central skycell can be variable and more so with largely different input sets. Comparison with the psf_major/minor maps are more useful between refstack versions.
     130
     131== Problems  ==
     132 * as with all past refstacks, generally edge skycells have issues -- now more "bright" chunks but ratty edges filled in now.
     133 * like others, greater % of inputs rejected (~20%) so per pixel input is less, but still of order 30 inputs per pixel minimum across core skycells and base minimum for input images on the outer edges
     134 * skycell notes:
     135  * y:
     136  * z:
     137  * i:
     138  * r:
     139  * g:
     140 * some convolved stacks have poorer FWHM PSF but not significant enough to be likely improved by reprocessing using MD_DEEP_STACK config as in earlier MD fields (input cut <10 rather than <6 and FWHM+100*STDEV rather than FWHM+1.0*STDEV)
     141  * g:
     142  * re-processing tests (have not written this up before and should note):
     143   * data_group -- MD01.refstack.20130731redo
     144   * workdir base -- MD01.refstack.20130731redo
     145  * unused redo processing
     146   * label -- MD01.refstack.20130731skip
     147   * data_group -- MD01.refstack.20130731redo
     148   * workdir base -- MD01.refstack.20130731redo
     149  * replaced original run
     150   * label -- MD01.refstack.20130731poor
     151   * data_group -- MD01.refstack.20130731poor
     152   * workdir base -- original name MD01.refstack.20130731
     153  * redo processing replacing original processing
     154   * label -- normal refstack label
     155   * data_group -- normal refstack data_group
     156   * workdir base -- MD01.refstack.20130731redo
     157
     158
     159Core coverage  -- not a shifted pointing
     160{{{
     161082-087
     162071-078
     163061-068
     164051-058
     165041-048
     166031-038
     167021-028
     168012-017
     169}}}
     170 * skycells with fewer inputs (typical for edges): 012, 017, 021, 028, 071, 078, 082, 087
     171 * skycells with <50% or more of typical input number is filter dependent - usually  028, 078, 082
     172
     173
     174
     175
     176== Refstack Summary ==
     177Stack phomtometry on the refstacks done through the staticsky and skycal stages using the unconvolved images
     178 * single filter mode so basic psphot with deteff measurements that has the zero-point recalculated for the test plots below
     179  * label: MD02.refstack.20130815, MD02.refstack.20130815
     180  * data_group (single filter):  MD02.refstack.20130815.1x20130821, MD02.refstack.20130815.1x20130821.cal20130821
     181 * multi-filter (Nx) not run yet
     182  * label:
     183  * data_group:  (all skycells have 5 filters matched)
     184 * on datastore under ps1-md-staticsky, but only the staticsky version, the skycal product still has no method for distribution
     185
     186
     187Source photometry psf_major,_minor maps (grizy): '''all new plots here scaled by root(2) to match past scaling (plots now labelled accordingly) and so values larger by root(2) to what should actually be'''
     188
     189|| [[Image(md02v2013x1skycal_cmf_g.txt_psfmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_r.txt_psfmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_i.txt_psfmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_z.txt_psfmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_y.txt_psfmap.png,300px)]] ||   
     190
     191
     192
     193Magnitude of sources@5-sigma maps (grizy):
     194
     195|| [[Image(md02v2013x1skycal_cmf_g.txt_mag5sigmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_r.txt_mag5sigmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_i.txt_mag5sigmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_z.txt_mag5sigmap.png,300px)]] ||  [[Image(md02v2013x1skycal_cmf_y.txt_mag5sigmap.png,300px)]] ||
     196
     197
     198
     199Detection efficiency magnitude @50% recovery (500 fakes, grizy): '''0 rej for all now that the SCL_ keyword has its true value other than 1. when rejected in stacking'''
     200
     201|| [[Image(md02v2013x1skycal_cmf_g.txt_mag50gridmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_r.txt_mag50gridmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_i.txt_mag50gridmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_z.txt_mag50gridmap.png,300px)]] || [[Image(md02v2013x1skycal_cmf_y.txt_mag50gridmap.png,300px)]] ||
     202
     203
     204
     205----
     206
     207= 1D convolution mode PV2 =
     208
     209
     210Same naming format as generally above, adding _1dg to the data_group (as will be seen on the datastore)
     211 * label: MD02.reftest.20130815
     212 * data_group:
     213  * MD02.reftest.20130815.c#f<FWHM cut>_1dg where #=comparison run, <FWHM cut>=cut  <fwhm_major from camProcessedExp x10>
     214  * MD02.reftest.20130815.all.<FWHM cut>_1dg where all means 05/2010+2011+2012/2013 data possible, <FWHM cut>=cut <fwhm_major from camProcessedExp x10>
     215  * MD02.reftest.20130815.2012.<FWHM cut>_1dg where 2012 means 2012/2013 data only for season stack example case, <FWHM cut>=cut <fwhm_major from camProcessedExp x10>
     216 * c1 cuts (same as above)
     217
     218Full refstack:
     219 * label: MD02.refstack.20130815_1dg
     220 * data_group: MD02.refstack.20130815_1dg
     221 * workdir basename: MD02.refstack.20130815_1dg
     222
     223Summary comparison table with the approximate FWHM (major) as the PSF FWHM from a center field skycell (V3=055) after running psphot on the stacks.
     224
     225{{{
     226| data_group                        | filter  | stack_id | warps_in | warps_rej |  FWHM_MAJ   IQ_FW1 (pixels)
     227+-----------------------------------+---------+----------+----------+-----------+
     228
     229
     230}}}
     231
     232
     233
     234----