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--- imagerteleconnotes20180206 [2018/02/07 15:52] – wenxx181
+++ imagerteleconnotes20180206 [2018/02/07 15:54] (current) – wenxx181
@@ Line 1: / Line 1: @@
 ====== Telecon 20180206 ======
-Attending:
+Attending: Brian, Roger, Jacques, Julian, Tom, Toki, Kris, Hannes, Shaul, Karl, Qi
 Notes by : Karl/Qi \\
@@ Line 25: / Line 25: @@
      * Spin rate is dominant over precession, so scan direction is about straight from left to right as shown
      * Shaul: each pixel has both polarizations; we want Q and U pairs, thus the word "detector" may be misleading here
-     * Jaque: arrangement of focal plane, cross scan sampling; shaul: we will take look into Jaques's paper about cross scan sampling in terms of spin, precession etc.
+     * Jacques: arrangement of focal plane, cross scan sampling; shaul: we will take look into Jaques's paper about cross scan sampling in terms of spin, precession etc.
      * Kris: faster precession, if compare 10 days to 10 hrs, gives better sky map coverage; however, if compare 10 hrs to 2 hrs, not sure if it makes a big difference
-     * Jaque: holes on sky map will affect systematics over the focal plane
+     * Jacques: holes on sky map will affect systematics over the focal plane
      * Shaul: fundamental questions have not be addressed, Q and U layout has not been done
      * Q and U alignment is flexible within wafer