| 1 | = Copilot = |
| 2 | |
| 3 | *copilot.py* is a script that watches for new images, measures them, |
| 4 | and produces a plot, *recent.png* to help observers understand what |
| 5 | the conditions are doing. |
| 6 | |
| 7 | Start it from the `mzls@mayall-idl.kpno.noao.edu` account, |
| 8 | {{{ |
| 9 | python copilot.py & |
| 10 | }}} |
| 11 | |
| 12 | It will monitor the $MOS3_DATA directory, and whenever a new image |
| 13 | comes it, it will measure it, update a little database, and create a |
| 14 | "strip plot" showing the conditions. |
| 15 | |
| 16 | The database is in *~/obsbot/obsdb/obsdb.sqlite3*. |
| 17 | |
| 18 | An example plot is shown here: |
| 19 | |
| 20 | [[Image(copilot-example.png)]] |
| 21 | |
| 22 | The top panel shows the seeing. Any problems with the data we know |
| 23 | how to detect are marked with red vertical bands. These include: |
| 24 | * readtime -- MAY indicate a duplicated image ("md5sum" is a better |
| 25 | indicator). |
| 26 | * md5sum -- this image contains identical pixels as a previous image. |
| 27 | This requires action! Please see the problem description [[https://desi.lbl.gov/trac/wiki/PublicPages/MayallZbandLegacy/NotesforObservers/Problems#a5.Repeatimages HERE]]. |
| 28 | * pixcnt -- the image readout is shifted. Please have a look at this |
| 29 | exposure and note in the logs which CCD has the shift. The shifts |
| 30 | are pretty easily recognized in the *mscexam* IRAF window -- blocks |
| 31 | of one of the images will be shifted to the left or right. Do not |
| 32 | stop observing. |
| 33 | This problem is described [[https://desi.lbl.gov/trac/wiki/PublicPages/MayallZbandLegacy/NotesforObservers/Problems#a4.Shiftedimages here]] |
| 34 | * (unlabelled bar) -- it has been a while since the last image has been seen. Have images stopped being written? See problem description [[https://desi.lbl.gov/trac/wiki/PublicPages/MayallZbandLegacy/NotesforObservers/Problems#a0.Noimagesbeingwritten here]] |
| 35 | |
| 36 | |
| 37 | |