Closed mperrin closed 6 years ago
Issue by robelgeda Friday Jan 12, 2018 at 17:33 GMT Originally opened as https://github.com/mperrin/webbpsf/pull/184
This is the final draft of WFIRST Cycle 7 updates. The Following changes have been made:
webbpsf:
webbpsf-data-source:
WFI/filters/R062_throughput.fits
WFI/filters.tsv
WFI/wim_zernikes_cycle7.csv
WFIRST_SRR_WFC_Pupil_Mask_Longwave_2048.fits
WFIRST_SRR_WFC_Pupil_Mask_Shortwave_2048.fits
WFI/sources/cycle6/WFI/wim_zernikes_cycle6.csv
_Obsolete/cycle6_pupils/.
WFI/sources/cycle7
Pupil Image explanation:
I was able to obtain the instrument layout in both cycles. Both indicate that the coordinate system is Payload FOV {X, Y}. See axis labels below:
Payload FOV {X, Y}
I was able to figure out that the WSM rotated 90 degrees as follows.
Where purple and orange arrows point to the origin in cycle 6 and 7 respectively.
After that I checked if the pupil files do the same transformation.
I found this to be evidence that the pupil coordinate system conventions are the same.
robelgeda included the following code: https://github.com/mperrin/webbpsf/pull/184/commits
Comment by robelgeda Friday Jan 12, 2018 at 19:19 GMT
Travis fails because it is using Cycle 6 data.
Issue by robelgeda Friday Jan 12, 2018 at 17:33 GMT Originally opened as https://github.com/mperrin/webbpsf/pull/184
This is the final draft of WFIRST Cycle 7 updates. The Following changes have been made:
webbpsf:
webbpsf-data-source:
WFI/filters/R062_throughput.fits
.WFI/filters.tsv
to add R062.WFI/wim_zernikes_cycle7.csv
.WFIRST_SRR_WFC_Pupil_Mask_Longwave_2048.fits
andWFIRST_SRR_WFC_Pupil_Mask_Shortwave_2048.fits
.WFI/sources/cycle6/WFI/wim_zernikes_cycle6.csv
_Obsolete/cycle6_pupils/.
.WFI/sources/cycle7
.Pupil Image explanation:
I was able to obtain the instrument layout in both cycles. Both indicate that the coordinate system is
Payload FOV {X, Y}
. See axis labels below:I was able to figure out that the WSM rotated 90 degrees as follows.
Where purple and orange arrows point to the origin in cycle 6 and 7 respectively.
After that I checked if the pupil files do the same transformation.
I found this to be evidence that the pupil coordinate system conventions are the same.
robelgeda included the following code: https://github.com/mperrin/webbpsf/pull/184/commits