Difference between revisions of "GAL04"
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The position is given by Araya by private communication. | The position is given by Araya by private communication. | ||
The assumed shape is the Gaussian with the containment radius of about 0.68 degree. | The assumed shape is the Gaussian with the containment radius of about 0.68 degree. | ||
| − | [[File:Lat_map.png|500px]] | + | [[File:Lat_map.png|500px]] |
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=== Observational settings/limits === | === Observational settings/limits === | ||
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| + | - Wobble observation with a large offset angle | ||
| + | Since this source is largely extended with the diameter of about 1.4 degree, the large Wobble offset angle is required. In the proposal, we set the angle as 0.9 degree. | ||
| + | [[File:Wobble_pos.png|500px]] | ||
Revision as of 03:17, 13 June 2023
Proposal
Proposal: GAL04: Newly discovered GeV-emitting SNR G17.8+16.7
PI: Hideaki Katagiri (hideaki.katagiri.sci@vc.ibaraki.ac.jp)
Source:
RA (J2000) 261.04375 (17h24m10.5s)
DEC (J2000) -5.18125 (-5d10m52.5s)
The corresponding galactic coordinate is (l, b) = (17.85158111, 16.75082053). The position is the best-fit position based on the Fermi-LAT gamma-ray analysis by Araya et al (2022). The Fermi-LAT paper is https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.2920A/abstract . The position is given by Araya by private communication. The assumed shape is the Gaussian with the containment radius of about 0.68 degree.
Observational settings/limits
- Wobble observation with a large offset angle
Since this source is largely extended with the diameter of about 1.4 degree, the large Wobble offset angle is required. In the proposal, we set the angle as 0.9 degree.
