Related documents discussing precursor datasets:

Draft SST Proposal for Test Datasets

Precursor Datasets for AP QA

DMTN-091


Data Set IdSurveyNotesSizeWebsiteUsed in TestsSuggested for testsUse in LSST
HSC-PDR1HSCHSC Public Data Release 1
https://hsc-release.mtk.nao.ac.jp/doc/LVV-T23, LVV-T36, LVV-T37, LVV-T38, LVV-T68, LVV-T76LVV-T24?, LVV-T27, LVV-T49
HSC-RC2HSC

Medium subset of PDR1 (two Wide-layer tract, one UltraDeep tract), selected to sample various features of the full PDR1 dataset; see DM-11345 - Getting issue details... STATUS . This is processed every two weeks using the weekly releases of the DM stack.



LVV-T28, LVV-T67, LVV-T71LVV-T58, LVV-T59, LVV-T69, LVV-T73, LVV-T74, LVV-T75, LVV-T77, LVV-T78, LVV-T79, LVV-T80, LVV-T82, LVV-T132

Useful for verification, but for end-to-end science acceptance testing (validation) we would likely use the full PDR1.

ci_hscHSCSmall HSC dataset.  Not a subset of PDR1; this is engineering data that went public even earlier. `ci_hsc` is run nightly.8.3G
LVV-T2LVV-T24Jenkins CI of ~90% of DRP pipeline steps (not large enough to run Jointcal or FGCM). Not useful for science validation.
HSC-RC1HSCMedium subset of PDR1 (two Wide-layer tract, one UltraDeep tract).  Superseded by RC2.

LVV-T11, LVV-T12, LVV-T13, LVV-T14, LVV-T15, LVV-T16
Won't be used for science validation.
WISEWISE


LVV-T2, LVV-T3, LVV-T4, LVV-T5, LVV-T6
Tables and catalogs for LSP testing.
HiTSHiTS (DECam)

http://astro.cmm.uchile.cl/HiTS/HiTS/LVV-T17, LVV-T18, LVV-T19, LVV-T20, LVV-T21, LVV-T22, LVV-T28, LVV-T35, LVV-T36, LVV-T37, LVV-T38, LVV-T67, LVV-T112, LVV-T113, LVV-T114, LVV-T160LVV-T49, LVV-T50, LVV-T51, LVV-T52, LVV-T53, LVV-T54, LVV-T55, LVV-T56, LVV-T57, LVV-T58Diff imaging and alert generation. From the HiTS data processing, we will also generate an alert stream.
DECam NEODECam NEO surveyPI L. Allen; 320 sq. degrees, 5 epochs/night in a single filter w/ 5 min. cadence. Repeated for 3 nights, 3 seasons of data.


LVV-T53, LVV-T57
DDOSSSDECam KBO surveyPI D. Trilling; KBOs to VR~27
https://www.noao.edu/noaoprop/abstract.mpl?2019A-0337

MOPS
DES-SNDECam DES-SN




Difference imaging, alert production. Benefit over HiTS is multiple filters.

DECam Bulge Survey




Crowded fields.
OpsimLSSTLSST Simulations of various survey strategies
http://astro-lsst-01.astro.washington.edu:8080/


DESC-DC2LSSTDESC DC2




TwinklesLSSTDESC




Stripe82SDSSSDSS Stripe 82 catalog processed with LSST Stack

LVV-T7, LVV-T8, LVV-T9

Gregory Dubois-Felsmann Stripe82 just happened to be convenient at the time of these tests, but doesn't seem essential for them. Is this correct? (i.e., that HSC, WISE, or other datasets could achieve these tests?)

L1TestLSSTL1 Test Stand DAQ; not so much a "data set" as a "data source"

LVV-T29, LVV-T30, LVV-T31, LVV-T32, LVV-T33, LVV-T34, LVV-T45

Verifying LSST headers, formats, and well-formed images.

Eric Bellm

Does LVV-T45 :
(Verify implementation of Prompt Processing Data Quality Report Definition) specifically require test stand data, or would HiTS data be sufficient as for most other AP tests?

photo-zCOSMOS, GAMA (others?)High-quality spectroscopic and photometric redshift catalogs in the HSC-PDR footprint.

LVV-T68
Training of photometric redshifts, but not needed for science validation.








What will be used to create a Prompt Products database that enables tests of MOPS?

Are there any larger sky-area data sets that should be included (e.g., LVV-T76 calls for one)?

Gaia (and possibly a catalog of QSOs) is used in LVV-T80, but only as a catalog for selecting objects in HSC data. The QSO catalog is also re-used in LVV-T160.

LVV-T92 - T95 concern "Special Programs." Are HSC Deep/Ultra-Deep fields appropriate for this? Or HiTS?

LVV-T112 - T114 refer to a "Simulated alert stream" – add this above?

Simulated EFD? (e.g., LVV-T153) – could also wait until single-day operations rehearsal.

A few tests suggest that inserting artificial sources (e.g., variable stars, QSOs, etc.) would be useful. This is more a requirement to write the tools than it is a data set.



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