| Version 6 (modified by , 13 years ago) ( diff ) |
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Summary of MD04.pv2_stacktest.20130903
(back to MediumDeepFields summary)
This is a test sample for PV2 and deep stacks using MD04 while it is an inactive field.
PV2: update type reprocessing
Deep stacks:
- for comparison, the last deep stack test using MD09 PV1 (MD09.PV1_deepstack_tests)
Reference stack -- this should be useful for making the MD04 refstack for return to field early November 2013. May move section for refstack to its own page for consistency.
Other stacks:
- in and out of season stacks -- haven't been done yet, need sample for Taiwan meeting
- fewer N input refstack
Status:
- prior 9/3 many issues being worked out for PV2 and MD (MD10.refstack.20130715)
- 9/3 PV2 updates started for MD04 after M31 reprocessing finished
- 9/6 PV2 updates finished
- 10/3 test all-in deep stack skycell run
- 10/10 started full all-in deep stack run
- 11/22 (great amount of updating to do)
PV2 updates
MD04
PV1 camera label -- data_group: mix of processing labels/data_groups, but all of PV1 type (cam_id>=434615)
| label | data_group |
| MD04.pv1.20130322 | MD04.pv1.20130322 |
| MD04.refstack.20121125 | MD04.refstack.20121125 |
| MD04.nightlyscience | MD04.<obsdate 20121129--20130525> |
There have been some test reprocessing that had to be avoided -- czw.MDVDtest%, czw.MDVD.MD04.%
PV2 camera (as well as chip, warp) label MD04.pv2.20130903, data_group left as originally was to be able to track back.
With ipp047 data disk down, have found ~3% of exposures missing a related imfile (~half are the burn.tbl files that can be regenerated) and indicates serious need of fixing the replication of raw data. Also found some replicated but on a host (ipp064X) that no longer exists.. it is also possible some replicated products may be on the same host if push to the stsci nodes with 3 partitions..
Number totals: (not all exposures pass camera stage, FWHM>12 pixels)
| filter | count(cam_id) | count(warp_id) | +---------+---------------+----------------+ | g.00000 | 596 | 577 | | i.00000 | 719 | 713 | | r.00000 | 588 | 571 | | y.00000 | 471 | 465 | | z.00000 | 711 | 710 |
PV2 warps will also be kept available (not cleaned up) for making deep stacks but also will be a accessible via the PSS/PSPS interface more quickly (release name MD04.PV2).
3PI overlap
Unclear what want to do here still, with LAP running, and how useful it will be in the stack.
Deep Stacks
Like with MD09, different versions of stacks will be produced for testing (not all will be full-field?)
- all --
- moderate input cuts --
- best cuts >2010 and moderate input cuts --
All
Basically all warps available with ~FWHM <13 pixels to avoid any badly measured PSF warps.
- label, data_group = MD04.alldeeptest.20131010
Cut
All warps FWHM <10 pixels and input warp cuts
- ZPT > ZPTmean-0.33
g: 24.11 r: 24.32 i: 24.07 z: 23.81 y: 22.79
- elongation <1.5
- background:
g: <400 r: <500 i: <1800 z: <2500 y: <5000
( -- still in progress -- )
- label, data_group = MD04.cutdeeptest.20131103
Best Cut
All warps FWHM <10 pixels and the same input warp cuts, only season years 2-4 (excludes 2009/2010 season)
- label, data_group = MD04.cut2009deeptest.20131103
Reference Stacks
In addition to the normal reference stack for a season, test samples of planned final reference stack types also being made.
| exp_name | filter | dateobs | comment | +-------------+---------+---------------------+---------------------------------+ | o4777g0224o | g.00000 | 2008-11-07 14:56:59 | MD04 g MJD54777 MD04 center | .. | o4803g0354o | r.00000 | 2008-12-03 15:25:16 | MD04 r MJD54803 MD04 center | ---- pre-survey | o5161g0222o | g.00000 | 2009-11-26 13:55:38 | MD04 g,r MJD55161 g MD04 center | .. | o5321g0014o | i.00000 | 2010-05-05 06:20:20 | MD04 i N5321 MD04 center | ---- yr1 -- 11/26/2009 -- 5/5/2010 | o5545g0436o | g.00000 | 2010-12-15 12:12:35 | MD04 g,r N5545 g MD04 center | .. | o5681g0089o | i.00000 | 2011-04-30 07:34:50 | MD04 i N5681 MD04 center | ---- yr2 -- 12/15/2010 -- 4/30/2011 | o5892g0155o | g.00000 | 2011-11-27 14:41:57 | MD04 g,r N5892 g MD04 center | .. | o6056g0114o | z.00000 | 2012-05-09 07:38:31 | MD04 z N6056 MD04 center | ---- yr3 -- 11/27/2011 -- 5/09/2012 | o6260g0448o | y.00000 | 2012-11-29 15:14:41 | MD04 y N6260 MD04 center | .. | o6437g0061o | y.00000 | 2013-05-25 05:50:54 | MD04 y N6437 MD04 center | ---- yr4 -- 11/29/2012 -- 5/25 2013 ---- yr5 -- actively being observed since 2013-11-08
(more details to follow)
Basic Reference Stacks
Default reference stacks for nightly diffims
- reduction MD_REF_STACK_1DG, FWHM <6 pixel and 1D convolution
- best ~60 input warps excluding 2009/2010 year/season
- label, data_group = MD04.refstack.20131018, MD04.refstack.20131018_1dg (_1dg to indicate 1D convolution method, but is now default for all stacks)
IQ Stacks
Basically a best reference stack possible -- used MD_DEEP_STACK_1DG so no extra cuts on FWHM made in order to look for bad warps need to be excluded in future runs
- label, data_group = MD04.iqtest.20131118
Reference Yearly/Seasonal Stacks
Basically a best reference stack possible using the specific year/season data -- used MD_DEEP_STACK_1DG so no extra cuts on FWHM made in order to look for bad warps need to be excluded in future runs
- label, data_group = MD04.yr1.reftest.20131118
- label, data_group = MD04.yr2.reftest.20131118
- label, data_group = MD04.yr3.reftest.20131118
- label, data_group = MD04.yr4.reftest.20131118
Comparison of yr1 and yr2-4 may help show if 2009/2010 season should be excluded from other stack types due to baffle improvements.
Reference Out-of-Season Stack
Two types possible, all exposures before season (default during active observing) and all exposures before/after season (or N seasons)
Not currently possible with current tools unless add warp_id manually for each skycell -- this method may even be necessary for all final stacks to exclude problematic exposure/chips in a warp skycell
