EGAL02

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Proposal

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

  Source: 3C454.3 

    RA (J2000) 343.49061685 deg 

    DEC (J2000) 16.14821153 deg 


  Source: Ton599 

    RA (J2000) 179.88264131 deg 

    DEC (J2000) 29.24550745 deg

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

It seems the gamma-ray spectrum of Ton 599 is sometimes hard (<2.0) (especially since April) and variable. So even when integral photon flux above 100 MeV is below the original limit (0.5x10-6 cm-2 s-1), there is a possibility to detect this source. When the spectrum is hard enough (e.g. April 23, 2023), it is detectable for a short observation. Thus, we want to request to schedule short exposure observations (1-1.5 hours) for monitoring purposes, rather than longer exposure for less nights, when this source can be scheduled (=no collision with other higher priority tasks/sources).

Past observation

Ton 599
  • 2023-01-13 (ToO)
    • run 11635, 11636, 11637, 11638
    • Zd=40-50, moon (~10 x dark NSB)
    • standard MC (dark)
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-01-13 12:00 to 2023-01-14 12:00)


  • 2023-01-15 (ToO)
    • run 11678
    • Zd~10, moon (3 x dark NSB)
    • standard MC (dark)
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-01-15 12:00 to 2023-01-16 12:00)
  • 2023-01-17 (ToO)
    • run 11704, 11705, 11706, 11707
    • Zd=40-50, dark
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-01-17 12:00 to 2023-01-18 12:00)
  • 2023-01-18 (ToO)
    • run 11718, 11720, 11721
    • Zd=10-20
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-01-18 12:00 to 2023-01-19 12:00)
SED (LST)
SED (LST + Fermi)

Performed observation

Ton 599
  • 2023-04-19 (no detection)
    • run 12768, 12769, 12770, 12771, 12772, 12774
    • Zd=0-30, dark
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-04-19 12:00 to 2023-04-20 12:00)
  • 2023-04-23 (3-5 sigma?)
    • run 12832, 12833, 12834, 12835
    • Zd=0-10, (almost) dark, DAQ PROBLEM (100% busy spikes)
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-04-23 12:00 to 2023-04-24 12:00)
SED (LST)
SED (LST + Fermi)



  • 2023-05-05 (FYI, no LST observation)
Fermi (2023-05-05 12:00 to 2023-05-06 12:00)
  • 2023-05-11 (no detection)
    • run 12941, 12942, 12943, 12944, 12945
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-05-11 12:00 to 2023-05-12 12:00)
  • 2023-05-13 (no detection)
    • run 12988, 12989
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-05-13 12:00 to 2023-05-14 12:00)
  • 2023-05-14
    • run 13013, 13014,13015,13016
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-05-14 12:00 to 2023-05-15 12:00)
  • 2023-05-15
    • run 13034, 13035, 13036, 13037, 13038
    • high cloudiness
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-05-15 12:00 to 2023-05-16 12:00)
  • 2023-05-17 (ToO)
    • run 13070, 13071
intensity>50, gammaness>0.7
intensity>150, gammaness>0.8
Fermi (2023-05-17 12:00 to 2023-05-18 12:00)

Analysis

- Summary (Ton599) https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing

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