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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):

    1. power-on the telescope, place it and open mirror covers with the TCS commands alt 45 and o-m-c

    2. tcs.setup-tel-alfosc

    3. Place the halogen "FF lamp" under the telescope and plug in

    4. alfosc.propid 74-803 (puts the files in the right directory)

    5. alfosc.carriage in

    6. alfosc.wheels -s Calcite -f 76

    7. alfosc.focus-offset

    8. alfosc.resetxy; alfosc.polwin; alfosc.bin 2

    9. Take a test exposure to determine the exptime t that gives between 300-400kADUs

    10. In order to make 3 cycles of 16 angles each with exptime t, do:
      alfosc.linpolexpose 16 domeflat t 3 -nowindow; astrowakeup

    11. When finished, do alfosc.carriage out, alfosc.resetxy, and alfosc.allopen

    12. When setup is ready, reset focus: alfosc.focus-offset

    13. Close mirror covers and park the telescope with the TCS commands c-m-c and zenith

    14. In the dome disconnect the "FF lamp" and store it (NB! it can be hot!)

    15. If it takes more than about 1 hour before your evening observations start, do power-off on the TCS.

Observing instructions:

  1. 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

  2. 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

  3. Start the target OB script, when it tells you to do the pointing, go to another sequencer window to run the ASTEPH tool

  4. 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
    
  5. 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:
      1. open a third sequencer terminal and cd scripts/74-803
      2. ignore the 3 first TCS commands
      3. run hitandrun as output by ASTEPH, BUT make sure the UT time is set 2-3 min into the future
      4. when guiding is OK, press RETURN (it is only used for pointing correction)
      5. now wait until the script does ag-off and starts updating rates

  6. 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

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