P74-803: Near-Earth-object polarimetry and astrometry for planetary defence
PI: M. Granvik
Imaging polarimetry requiring differential tracking.
This proposal includes 30h Monitoring observations on fixed dates
(see schedule below) for roughly 5 hours per month, as well as
ToO/SoftToO observations triggered on any date (6 hours).
Instrument setup required for ALFOSC linear polarimetry
- Filter: R (#76)
- Aperture wheel: Calcite
- FAPOL: lambda/2
Monitoring schedule P74
Date, Prop-ID, UT-window, Duration, Instrument, Any comment
01-10-2026, 74-803, [ECT]-20:30, 00:25, ALFOSC, Phaethon ph104
01-10-2026, 74-803, 23:30-[SCT], 00:25, ALFOSC, 2001CB21 ph101 + standards
03-10-2026, 74-803, [ECT]-21:20, 00:20, ALFOSC, Phaethon ph95
06-10-2026, 74-803, [ECT]-22:00, 00:20, ALFOSC, Phaethon ph90
06-10-2026, 74-803, [ECT]-[SCT], 00:20, ALFOSC, 2001CB21 ph58
10-10-2026, 74-803, [ECT]-[SCT], 00:20, ALFOSC, 2001CB21 ph45
18-10-2026, 74-803, 03:00-[SAT], 1:15, ALFOSC, Zoozve ph98 + standards
26-10-2026, 74-803, [ENT]-04:30, 00:40, ALFOSC, 2001CB21 ph32
26-10-2026, 74-803, [ENT]-[SNT], 00:40, ALFOSC, Zoozve ph78
30-10-2026, 74-803, [ENT]-[SNT], 00:35, ALFOSC, Zoozve ph65 + standards
02-11-2026, 74-803, [EAT]-04:00, 1:00, ALFOSC, 1999TF211, ph28
04-11-2026, 74-803, [ENT]-03:00, 00:30, ALFOSC, Zoozve ph52
08-11-2026, 74-803, 23:00-[SAT], 1:00, ALFOSC, 1998WZ6 ph28 + standards
26-11-2026, 74-803, 02:30-[SNT], 00:40, ALFOSC, 1998WT24 ph75 + standards
29-11-2026, 74-803, 21:00-[SAT], 00:40, ALFOSC, 1998WZ6 ph17
Daytime domeflat observing instructions:
- Biases are taken as part of
the automatic calibration script alfosc-calibs in the morning
- NB! Afternoon dome-flats with the
full polarimetry setup as follows (set off
some afternoon time for this):
- power-on the telescope, place it and open mirror covers with the TCS
commands alt 45 and o-m-c
- tcs.setup-tel-alfosc
- Place the halogen "FF lamp" under the telescope and plug in
- alfosc.propid 74-803 (puts the files in the right directory)
- alfosc.carriage in
- alfosc.wheels -s Calcite -f 76
- alfosc.focus-offset
- alfosc.resetxy; alfosc.polwin; alfosc.bin 2
- Take a test exposure to determine the exptime t that gives between 300-400kADUs
- In order to make 3 cycles of 16 angles each with exptime t, do:
alfosc.linpolexpose 16 domeflat t 3 -nowindow; astrowakeup
- When finished, do alfosc.carriage out, alfosc.resetxy, and
alfosc.allopen
- When setup is ready, reset focus: alfosc.focus-offset
- Close mirror covers and park the telescope with the TCS commands c-m-c
and zenith
- In the dome disconnect the "FF lamp" and store it (NB! it can be hot!)
- If it takes more than about 1 hour before your evening observations start, do
power-off on the TCS.
Observing instructions:
- If you are not already using ALFOSC, go to the desktop where the ALFOSC
Sequencer is running, and change the telescope settings with the command:
tcs.setup-tel-alfosc
- Go to the directory
cd ~/scripts/74-803
List the available scripts
ls -lrt
All OBs to be observed will have tonight's date (i.e. start of the night)
in their name.
Note that in addition to the target there can also be standard star polarimetry OBs
- Start the target OB script, when it tells you to do the pointing, go to
another sequencer window to run the ASTEPH tool
- The different target speeds may require 3 different observing modes:
- For rates < [70 ("/h) x OB-execution (h)], typically this command is used (auto-guiding):
tcs.asteph -n targetname
- For rates > [70 ("/h) x OB-execution (h)] either of the following two are used (auto-guiding & repositioning):
tcs.asteph -m optimal-ll -n targetname
tcs.asteph -m optimal-lr -n targetname
- For rates >> 800 ("/h) blind tracking with update of rates may be requested:
tcs.asteph_new -g update -n targetname
ASTEPH connects to JPL Horizon to get the actual position and rates. See examples in green color below.
In the case of using the optimal modes you also get the
best setting of the field-rotation to optimize guide star area for repositioning.
FOR EXPERTS: You can check both optimal-ll and optimal-lr (ASTEPH only outputs information on the screen)
To optimize slewing time select the case that involves less turning of the rotator
(the flag -f xx.xx gives field-rotation in the guide-object command).
> tcs.asteph -n 68548
...
These tasks should be given to the TCS:
***************************
tcs.append-object 68548_2001_XR31-1 17 06 18.91 +78 39 35.7 2000.0 0.0 0.0 17.314
tcs.ag-off
tcs.guide-object 68548_2001_XR31-1
tcs.reposition-guide-probe 193.864 41.25260
> tcs.asteph -m optimal-lr -n K07S06Q
...
These tasks should be given to the TCS:
***************************
tcs.append-object 2007_SQ6-1010 03 20 02.18 +09 15 10.5 2000.0 0.0 0.0 17.709
tcs.ag-off
tcs.tcs-command "instrument-name ALFOSC ALFOSC-LR"; tcs.guide-object -f 57.173 2007_SQ6-1010
tcs.reposition-guide-probe 241.628 -374.546
> tcs.asteph_new -g update -n 2023 SZ3
...
These tasks should be given to the TCS:
***************************
### IN THE FIRST SEQUENCER WINDOW ###
tcs.append-object 2023_SZ3-1737 01 15 47.49 -31 28 29.2 2000.0 0.0 0.0 18.615
tcs.ag-off
tcs.guide-object
#### IN THE SECOND SEQUENCER WINDOW ####
hitandrun 2023_SZ3-1737 hitandrun.input '2026-Sep-22 17:38:01.000' 10 3600 ima
- The next step is to point the telescope to the target in question.
- For the first two cases, cut and paste the 4 TCS commands into
the sequencer window.
The 4th command starts the differential
tracking and autoguiding.
- for the 3rd case (-g update) you need to do as follows:
- open a third sequencer terminal and cd scripts/74-803
- ignore the 3 first TCS commands
- run hitandrun as output by ASTEPH,
BUT make sure the UT time is set 2-3 min into the future
- when guiding is OK, press RETURN (it is only used for pointing correction)
- now wait until the script does ag-off and starts updating rates
- For all cases, you are now ready press return where the OB script is
running to start taking data.
NB! When differential guiding is used,
you need to reposition before the guide star reaches the opposite edge of the guide TV screen!
This is done by repeating the 4th command, tcs.reposition-guide-probe ....
before the edge is reached!
TCS warning beeps are given when there is 120, 90, and 60 seconds left.
Ideally, the telescope is not moved while the guide probe is repositioned, but if
many short exposures are used, it is wise to do this while the CCD is reading out.
For more general information on how this works, see the section "Moving Targets" in the ALFOSC Cookbook.
At the end of the night:
- When all OBs are done (check also for standard
star OBs with today's date ), please, close them.
- Please, fill in the
Mon tracking log.
- Remember to run alfosc-calibs ALF*** in the morning, where the input parameter
is the file prefix.
Thank you for your help!
| Program Tracking |
| Proposal |
74-803 |
| Semester |
P74: 20261001 - 20270401 |
| Principal Investigator |
Mikael Granvik |
| Programme |
Near-Earth-object polarimetry and astrometry for planetary defence |
| Instrument |
ALFOSC |
| Time Allocation |
30 hours Monitoring as 5 hours/month; 2 hours ToO and 4 hours SoftToO |
| Total Nights |
36h |
| Type |
ToO/SoftToO/Monitoring |
| Notes |
Fixed dates to be scheduled |
| Total Time Spent |
00:53 (hh:mm)
|
| Proposal |
Date |
Time |
Type |
Targets |
Files |
Comments |
Status |
|
| 74-803 |
2026-10-01 |
00:53 |
Monitoring |
Phaethon, BDp32_3739, VICyg12, 2001CB21 |
ALJj010056 - ALJj010071, ALJj010092 - ALJj010095, ALJj010096 - ALJj010099, ALJj010142 - ALJj010161 |
Targets observed successfully with clear skies and good seeing. |
Observed |
|
The above information is collected from the ToO/Mon reports that have been created by the observer.
Should any of the observations have been carried out using the OB system, you will find additional information
HERE
|