Difference between revisions of "Geminga"
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* Paul K. H. Yeung (pkh91yg@icrr.u-tokyo.ac.jp) | * Paul K. H. Yeung (pkh91yg@icrr.u-tokyo.ac.jp) | ||
| − | == Data | + | == Data-taking information == |
| − | + | Geminga has been observed with standard wobble observations (offset = 0.4 deg), in dark and good weather conditions: | |
| + | * TNG dust < 0.5 ug/m3 | ||
| + | * No clouds both from satellite images and all sky camera | ||
| + | * Rate_LL around 5.5 kHz | ||
| + | * Lidar trans@9km >= 0.85 | ||
| + | |||
| + | |||
| + | == Data analysis == | ||
| + | |||
| + | |||
| + | == Presentations at internal meetings == | ||
| + | |||
| + | |||
| + | == Presentations at external conferences/meetings == | ||
Revision as of 07:20, 16 October 2024
Contents
General information
- Name of the source: Geminga
- Brief description of the source: Radio-quiet middle-aged gamma-ray pulsar
- Object type : Pulsar
- Other relevant information: Third pulsar detected by IACTs
- RA: 06 33 54.15 (hh mm ss), Dec: +17 46 12.9 (dd mm ss)
- RA, Dec in deg (ICRS): 98.48 17.77
- Galactic coordinates: l=195.13 b=+04.27
People involved
- Álvaro Mas-Aguilar (alvmas@ucm.es)
- Marcos López-Moya (marcos@gae.ucm.es)
- Giulia Brunelli (giulia.brunelli@inaf.it)
- Rubén López-Coto (rlopezcoto@iaa.es)
- Giovanni Ceribella (ceribell@mpp.mpg.de)
- Paul K. H. Yeung (pkh91yg@icrr.u-tokyo.ac.jp)
Data-taking information
Geminga has been observed with standard wobble observations (offset = 0.4 deg), in dark and good weather conditions:
- TNG dust < 0.5 ug/m3
- No clouds both from satellite images and all sky camera
- Rate_LL around 5.5 kHz
- Lidar trans@9km >= 0.85
