Changes between Version 2 and Version 3 of PS1_SAS_AstromPhotom_20100310
- Timestamp:
- Mar 11, 2010, 12:39:23 PM (16 years ago)
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PS1_SAS_AstromPhotom_20100310
v2 v3 8 8 the database. Hopefully this will provide more light than smoke... 9 9 10 [[Image(sas.field.png )]]10 [[Image(sas.field.png, 300px)]] 11 11 12 12 The first figure shows the SAS field: black boxes are the outer bounds … … 35 35 which should be must faster (the indexes are still being ignored). 36 36 37 [[Image(sas.test.photom.g.png )]]38 [[Image(sas.test.photom.r.png )]]39 [[Image(sas.test.photom.i.png )]]40 [[Image(sas.test.photom.z.png )]]41 [[Image(sas.test.photom.y.png )]]37 [[Image(sas.test.photom.g.png, 300px)]] 38 [[Image(sas.test.photom.r.png, 300px)]] 39 [[Image(sas.test.photom.i.png, 300px)]] 40 [[Image(sas.test.photom.z.png, 300px)]] 41 [[Image(sas.test.photom.y.png, 300px)]] 42 42 43 43 Aside from those issues, this analysis looks very encouraging. The … … 57 57 (stormy.weather.png), where I show zero point offsets vs time. 58 58 59 [[Image(sas.test.astrom.g.png )]]60 [[Image(sas.test.astrom.r.png )]]61 [[Image(sas.test.astrom.i.png )]]62 [[Image(sas.test.astrom.z.png )]]63 [[Image(sas.test.astrom.y.png )]]59 [[Image(sas.test.astrom.g.png, 300px)]] 60 [[Image(sas.test.astrom.r.png, 300px)]] 61 [[Image(sas.test.astrom.i.png, 300px)]] 62 [[Image(sas.test.astrom.z.png, 300px)]] 63 [[Image(sas.test.astrom.y.png, 300px)]] 64 64 65 65 As for astrometry, the residuals are OK (20-27 mas), but I suspect we
