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| === Observational settings/limits === | | === Observational settings/limits === |
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− | - original criteria to observe Ton 599 | + | - 3C454.3 |
| | | |
− | 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 | + | The observations should be organized through the ToO form when the integral photon flux (>100 MeV) reaches 1×10−5 cm−2 s−1. |
| + | In this state, LST-1 is expected to detect low-energy gamma-ray signals with ∼30 hours of observations. |
| + | If we detect a significant flare and the integral photon flux is still above the mentioned threshold after the flare, we also request another 30 hours of observations after the flare |
| | | |
− | '''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).'''
| + | - Ton 599 |
| | | |
− | === Past observation ===
| + | 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 |
− | ===== Ton 599 =====
| |
− | * 2023-01-13 (ToO)
| |
− | ** run 11635, 11636, 11637, 11638
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− | ** Zd=40-50, moon (~10 x dark NSB)
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− | {| align='center'
| |
− | | [[File:Ton599_20230113_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
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− | | [[File:Ton599_20230113_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
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− | | [[File:Ton599_fermi_20230113.png|thumb|centre|400px|Fermi (2023-01-13 12:00 to 2023-01-14 12:00)]]
| |
− | |}
| |
| | | |
| + | '''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 (1-2 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). If we detect some signs of active state (e.g. high energy photons), we will contact schedulers.''' |
| | | |
− | * 2023-01-15 (ToO)
| + | == Analysis == |
− | ** run 11678
| |
− | ** Zd~10, moon (3 x dark NSB)
| |
− | {| align='center'
| |
− | | [[File:Ton599_20230115_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
| |
− | | [[File:Ton599_20230115_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
| |
− | | [[File:Ton599_fermi_20230115.png|thumb|centre|400px|Fermi (2023-01-15 12:00 to 2023-01-16 12:00)]]
| |
− | |}
| |
− | | |
− | * 2023-01-17 (ToO)
| |
− | ** run 11704, 11705, 11706, 11707
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− | ** Zd=40-50, dark
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− | {| align='center'
| |
− | | [[File:Ton599_20230117_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
| |
− | | [[File:Ton599_20230117_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
| |
− | | [[File:Ton599_fermi_20230117.png|thumb|centre|400px|Fermi (2023-01-17 12:00 to 2023-01-18 12:00)]]
| |
− | |}
| |
− | | |
− | * 2023-01-18 (ToO)
| |
− | ** run 11718, 11720, 11721
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− | ** Zd=10-20
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− | {| align='center'
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− | | [[File:Ton599_20230118_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
| |
− | | [[File:Ton599_20230118_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
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− | | [[File:Ton599_fermi_20230118.png|thumb|centre|400px|Fermi (2023-01-18 12:00 to 2023-01-19 12:00)]]
| |
− | |}
| |
− | {| align='center'
| |
− | | [[File:Ton599_20230118_srcdep_sed.png|thumb|centre|400px|SED (LST)]]
| |
− | | [[File:Ton599_20230118_srcdep_sed_with_fermi.png|thumb|centre|400px|SED (LST + Fermi)]]
| |
− | | |
− | |}
| |
− | | |
− | === Performed observation ===
| |
− | ===== Ton 599 =====
| |
− | * 2023-04-19 (no detection)
| |
− | ** run 12768, 12769, 12770, 12771, 12772, 12774
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− | ** Zd=0-30, dark
| |
− | {| align='center'
| |
− | | [[File:Ton599_20230419_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
| |
− | | [[File:Ton599_20230419_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
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− | | [[File:Ton599_fermi_20230419.png|thumb|centre|400px|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)
| |
− | {| align='center'
| |
− | | [[File:Ton599_20230423_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
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− | | [[File:Ton599_20230423_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
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− | | [[File:Ton599_fermi_20230423.png|thumb|centre|400px|Fermi (2023-04-23 12:00 to 2023-04-24 12:00)]]
| |
− | |}
| |
− | | |
− | {| align='center'
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− | | [[File:Ton599_20230423_srcdep_sed.png|thumb|centre|400px|SED (LST)]]
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− | | [[File:Ton599_20230423_srcdep_sed_with_fermi.png|thumb|centre|400px|SED (LST + Fermi)]]
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− | | |
− | |}
| |
− | | |
− | | |
− | | |
− | | |
− | | |
− | * 2023-05-05 (FYI, no LST observation)
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− | {| align='center'
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− | | [[File:Ton599_fermi_20230505.png|thumb|centre|400px|Fermi (2023-05-11 12:00 to 2023-05-12 12:00)]]
| |
− | |}
| |
− | | |
− | * 2023-05-11 (no detection)
| |
− | ** run 12941, 12942, 12943, 12944, 12945
| |
− | {| align='center'
| |
− | | [[File:Ton599_20230511_srcdep_g07_i50.png|thumb|centre|400px|intensity>50, gammaness>0.7]]
| |
− | | [[File:Ton599_20230511_srcdep_g08_i150.png|thumb|centre|400px|intensity>150, gammaness>0.8]]
| |
− | | [[File:Ton599_fermi_20230511.png|thumb|centre|400px|Fermi (2023-05-11 12:00 to 2023-05-12 12:00)]]
| |
− | |}
| |
− | | |
− | === Analysis ===
| |
| - Summary (Ton599) | | - Summary (Ton599) |
| https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing | | https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing |
| + | |
| + | - wiki page |
| + | -- https://www.lst1.iac.es/wiki/index.php/TON599 |
| + | -- https://www.lst1.iac.es/wiki/index.php/3C454.3 |
Proposal[edit]
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[edit]
- 3C454.3
The observations should be organized through the ToO form when the integral photon flux (>100 MeV) reaches 1×10−5 cm−2 s−1.
In this state, LST-1 is expected to detect low-energy gamma-ray signals with ∼30 hours of observations.
If we detect a significant flare and the integral photon flux is still above the mentioned threshold after the flare, we also request another 30 hours of observations after the flare
- 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 (1-2 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). If we detect some signs of active state (e.g. high energy photons), we will contact schedulers.
Analysis[edit]
- Summary (Ton599)
https://docs.google.com/presentation/d/1gaDXn9cRdHN7RWg4m9iZqNLSwOAlH4m0W2f5V8CqSI8/edit?usp=sharing
- wiki page
-- https://www.lst1.iac.es/wiki/index.php/TON599
-- https://www.lst1.iac.es/wiki/index.php/3C454.3