Changes between Version 20 and Version 21 of MD.GR0

Timestamp:

Sep 27, 2011, 11:40:49 AM (15 years ago)

Author:

Mark Huber

Comment:

--

MD.GR0

@@ -14 +14 @@
 
 Reference stacks -- primarily for difference imaging for transient detection and necessary for magic destreaking.
- * 
+ * Magic destreaking: a fairly clean reference stack (uses convolved version) with as much area coverage as possible to enable release of not-stack data products.
+ * Transient detection: a balance slanted towards best PSF but with some depth (1-1.5 magnitudes over nightly stacks).
  
 Deep stacks -- for deep static sky science.
- *
+ * As deep as possible.. maximum FWHM allowance? minimum exposure time? at least ~10ks has been requested, with best FWHM possible. 
+
+See summary for each MD field reference stack for details on specifics for that field. Due to processing+time constraints/early mistakes, an attempted has been made to merge the similar requests.
 
 = MD.V3 Tessellation =