Difference between revisions of "EGAL02"

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(Proposal)
(Proposal)
Line 11: Line 11:
 
- original criteria to observe Ton 599
 
- original criteria to observe Ton 599
  
  This source is already in a active state, so we request 50 hours of observations
+
  we request 50 hours of observations unless the average integral photon flux (>100 MeV) goes down below 0.5×10−6 cm−2 s−1
unless the average integral photon flux (>100 MeV) goes down below 0.5×10−6 cm−2 s−1
 
  
-  
+
=== Performed observation ===
 +
- 2023-04-19
 +
-- run 12768, 12769, 12770, 12771, 12772, 12774
 +
- 2023-04-23
 +
-- 12832, 12833, 12834, 12835
 +
 
 +
=== Analysis ===
 +
- Summary (google slides)
 
https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing
 
https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing

Revision as of 13:47, 11 May 2023

Proposal

Proposal: EGAL02:Observations of distant bright FSRQs in active states
PI: Seiya Nozaki (nozaki@mpp.mpg.de)

  Source: Ton599 
RA (J2000) 179.88264131
DEC (J2000) 29.24550745

Observational settings/limits

- original criteria to observe Ton 599

we request 50 hours of observations unless the average integral photon flux (>100 MeV) goes down below 0.5×10−6 cm−2 s−1

Performed observation

- 2023-04-19 -- run 12768, 12769, 12770, 12771, 12772, 12774 - 2023-04-23 -- 12832, 12833, 12834, 12835

Analysis

- Summary (google slides) https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing