Action #1855
Add GSkyDir::moon() method
| Status: | Closed | Start date: | 09/28/2016 | |
|---|---|---|---|---|
| Priority: | Normal | Due date: | ||
| Assigned To: |  Knödlseder Jürgen | % Done: | 100% | |
| Category: | - | |||
| Target version: | 1.7.0 | |||
| Duration: |
Description
A moon(const GTime& time) method should be added to the GSkyDir class that returns the position of the moon for a given time with an accuracy sufficient for gamma-ray astronomy (see #1854 for a corresponding method for the Sun position).
Recurrence
No recurrence.
History
#1
Updated by Knödlseder Jürgen over 5 years ago
- Target version set to 1.7.0
#2
Updated by Knödlseder Jürgen about 5 years ago
- File Moon_position_difference.png added
- File test_moon_ephem.py
added - Status changed from New to Pull request
- Assigned To set to Knödlseder Jürgen
- % Done changed from 0 to 100
The method has been implemented inspired by the IDL code moonpos.pro, see https://github.com/awmann/amObserve/blob/master/moonpos.pro. A note on the computation method can be found at https://ntomasse.web.cern.ch/Notes/tomassetti_ams02algorithms.pdf.
I used the script test_moon_ephem.py to compare the Moon position computed using GSkyDir::moon() to the one computed using PyEphem, the results are shown below for the period 2000 - 2050. Overall the accuracy is quite good, but becomes worse at the end of the period. However, it never becomes worse than 1 arcmin, which should be okay for gamma-ray astronomy.
#3
Updated by Knödlseder Jürgen about 5 years ago
- Status changed from Pull request to Closed
Merged into devel.