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--- imagerteleconnotes20180523 [2018/05/23 16:47] – wenxx181
+++ imagerteleconnotes20180523 [2018/05/23 17:20] (current) – hanany
@@ Line 9: / Line 9: @@
   * Temperature Stability and effects on responsivity variations
     * {{::peter_shirron_adr_stability.pptx|Shirron workshop presentation}}
-  * {{::sensitivity_vs_frequency_may19th_2018.pdf|noise/band Figure}}
+  * {{::sensitivity_vs_frequency_may19th_2018.pdf|noise/band Figure}} and  {{::sensitivity_vs_frequency_may23rd_2018.pdf|Revised noise/band Figure}}
 === Notes ===
@@ Line 69: / Line 69: @@
     * Jacque: Very long time constant, the fluctuation from dilution does not transfer to focal plane; most fluctuations were from cosmic rays
     * Shaul: why was active control still useful if time constant was large? **Check with Brandon (AI)**
+  * The plot is from 4-stage, 4k to low T; 5-stage should outperform with 1K
+    * Shaul: 1K stage would have its own fluctuation
+    * Peter: ASTRO-H lab tests with full space instruments, 3 ADR: 2 upper stage + 1.5 K constant. Fluctuation was within 1mK. Two modes, ADR with liquid helium and without helium. Turned out without was more stable, gave better detector resolution, because of more stability under ADR; with helium, there were drifts.
+      * did not do in-space test due to computation limit on board
+Noise/band Figure
+  * Jacques: this one is mostly wrong, no need to discuss. A lot things have been fixed.
+  * Jacques sends a new figure for Shaul to present. Units are consistent between bands and signals.
+  * Synchrotron not completely clear
+  * BB dominated by lensing
+  * Shaul: six dark blue bands are wrong, should be three
+  * CO lines
+  * Current units are for broader community, who do not understand uK.
+Shaul will be gone for next 3 weeks until June 18th. After Shaul comes back, report writing mode.

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