| | 541 | | 16 | MD10.pv2.20130828 | MD10.20121014 | 2012-10-14 07:14:56 | g.00000 | |
| | 542 | | 2 | MD10.pv2.20130828 | MD10.20121211 | 2012-12-11 05:52:58 | i.00000 | |
| | 543 | | 19 | MD10.pv2.20130828 | MD10.20121215 | 2012-12-15 05:47:47 | y.00000 | |
| | 544 | |
| | 545 | | 5 | MD10.pv2.20130828 | MD10.pv1.20130324 | 2010-11-03 08:01:45 | g.00000 | |
| | 546 | | 3 | MD10.pv2.20130828 | MD10.refstack.20120705 | 2010-11-03 08:14:32 | g.00000 | |
| | 547 | |
| | 548 | | 22 | MD10.pv2.20130828 | MD10.20121023 | 2012-10-23 07:07:21 | y.00000 | |
| | 549 | | 18 | MD10.pv2.20130828 | MD10.refstack.20130715 | 2012-10-23 07:28:34 | y.00000 | |
| | 550 | |
| | 551 | | 8 | MD10.pv2.20130828 | MD10.20130714 | 2013-07-14 13:13:17 | i.00000 | -- already PV2 so a normal update process without updating the camera stage |
| | 552 | |
| | 553 | }}} |
| | 554 | |
| | 555 | When doing the update process, have found cases where only a single, valid instance exists for a not insignificant amount of raw data.. this is tracked more in the full MD04 update ([wiki:MD04.pv2_deeptest.20130903]). |
| | 556 | |
| | 557 | |
| | 558 | === PV2 Update Masking Losses in Warp === |
| | 559 | Odd mask lost in PV2 updates -- seems to be limited to |
| | 560 | {{{ |
| | 561 | PM_SOURCE_MODE_CR_LIMIT |
| | 562 | PM_SOURCE_MODE_BLEND |
| | 563 | }}} |
| | 564 | |
| | 565 | Was suggested that possibly from photometry not being run on update -- since masks being remade in PV2 updates then lost, while a normal update uses the already defined mask? Since PV2 is mainly for improved inputs to stacks, should be minor and just rejected? (except for low N..) |
| | 566 | |
| | 567 | |
| | 568 | Example -- one masked CR is lost (full reprocessing retains it while the PV2 update method loses it) and one is gained (as with the full reprocessing and should be) |
| | 569 | {{{ |
| | 570 | exposure.exp_id: o5503g0240o.250240 |
| | 571 | new chip/cam/warp_id = 883673 / 854492 / 835018 |
| | 572 | old/pv1/up chip/cam/warp_id = 810251 / 786993 / 766825 |
| | 573 | skycell.045 |
| | 574 | }}} |
| | 575 | |
| | 576 | * Image panels -- |
| | 577 | |
| | 578 | || full reprocessing || pv1 normal update || pv2 s/ camera update || cleanup and normal update of pv2 || |
| | 579 | |
| | 580 | [[Image(o5503g0240o.s045im_cr_center.jpg,500px)]] |
| | 581 | |
| | 582 | * Mask panels left to right -- (same sequence) |
| | 583 | |
| | 584 | [[Image(o5503g0240o.s045mk_cr_center.jpg,500px)]] |
| | 585 | |
| | 586 | |
| | 587 | === PV2 Update Night Stacks === |
| | 588 | Only focusing on the unconvolved stacks as those are only used for the SSdiff, the convolved stacks will be looked at in more detail when stack photometry is evaluated. |
| | 589 | |
| | 590 | Default/current operations config version with PV2 update warps -- |
| | 591 | * label -- meh_md10nstest20130831 |
| | 592 | * data_group -- meh_md10.<obsdate>ns20130831 (i.e., meh_md10.20101103ns20130831) |
| | 593 | |
| | 594 | Suggested config option version with PV2 update warps -- |
| | 595 | * label -- meh_md10nstest20130830 |
| | 596 | * data_group -- meh_md10.<obsdate>nstest20130830 (i.e. meh_md10.20101103ns20130830) |
| | 597 | |
| | 598 | |
| | 599 | {{{ |
| | 600 | | count(warp_id) | label | data_group | dateobs | filter | |
| | 601 | +----------------+-------------------+------------------------+---------------------+---------+ |
| | 602 | | 4 | MD10.pv2.20130828 | MD10.20120825 | 2012-08-25 13:20:29 | y.00000 | |
| 572 | | When doing the update process, have found cases where only a single, valid instance exists for a not insignificant amount of raw data.. this is tracked more in the full MD04 update ([wiki:MD04.pv2_deeptest.20130903]). |
| 573 | | |
| 574 | | |
| 575 | | === PV2 Update Masking Losses in Warp === |
| 576 | | Odd mask lost in PV2 updates -- seems to be limited to |
| 577 | | {{{ |
| 578 | | PM_SOURCE_MODE_CR_LIMIT |
| 579 | | PM_SOURCE_MODE_BLEND |
| 580 | | }}} |
| 581 | | |
| 582 | | Was suggested that possibly from photometry not being run on update -- since masks being remade in PV2 updates then lost, while a normal update uses the already defined mask? Since PV2 is mainly for improved inputs to stacks, should be minor and just rejected? (except for low N..) |
| 583 | | |
| 584 | | |
| 585 | | Example -- one masked CR is lost (full reprocessing retains it while the PV2 update method loses it) and one is gained (as with the full reprocessing and should be) |
| 586 | | {{{ |
| 587 | | exposure.exp_id: o5503g0240o.250240 |
| 588 | | new chip/cam/warp_id = 883673 / 854492 / 835018 |
| 589 | | old/pv1/up chip/cam/warp_id = 810251 / 786993 / 766825 |
| 590 | | skycell.045 |
| 591 | | }}} |
| 592 | | |
| 593 | | * Image panels -- |
| 594 | | |
| 595 | | || full reprocessing || pv1 normal update || pv2 s/ camera update || cleanup and normal update of pv2 || |
| 596 | | |
| 597 | | [[Image(o5503g0240o.s045im_cr_center.jpg,500px)]] |
| 598 | | |
| 599 | | * Mask panels left to right -- (same sequence) |
| 600 | | |
| 601 | | [[Image(o5503g0240o.s045mk_cr_center.jpg,500px)]] |
| 602 | | |
| 603 | | |
| 604 | | === PV2 Update Night Stacks === |
| 605 | | Only focusing on the unconvolved stacks as those are only used for the SSdiff, the convolved stacks will be looked at in more detail when stack photometry is evaluated. |
| 606 | | |
| 607 | | Default/current operations config version with PV2 update warps -- |
| 608 | | * label -- meh_md10nstest20130831 |
| 609 | | * data_group -- meh_md10.<obsdate>ns20130831 (i.e., meh_md10.20101103ns20130831) |
| 610 | | |
| 611 | | Suggested config option version with PV2 update warps -- |
| 612 | | * label -- meh_md10nstest20130830 |
| 613 | | * data_group -- meh_md10.<obsdate>nstest20130830 (i.e. meh_md10.20101103ns20130830) |
| 614 | | |
| 615 | | |
| 616 | | Rejection comparison -- |
| | 634 | Rejection and detection number comparison -- |