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Instructions from the PI

Dear NOT observer and staff.

This is a set of instructions for NOT monitoring programme P70-502 (PI:HÃ¥kon Dahle), scheduled for service observations. The purpose is to monitor three of the five currently known gravitationally lensed quasars where the lens is a galaxy cluster. The main purpose of the observations is to use the light curves to make time delay measurements between multiple lensed quasar images in order to estimate the value of the Hubble constant. We will also determine the level of microlensing in each lens system. The target information and the observing strategy are reported below.

Please let us know whether you carried out these observations.

Thank you!

Best regards,
Håkon Dahle

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For the "monitoring" observations use the script indicated by the OB.

Calibrations:

For calibration we request:

- A set of three twilight flats for the SDSS g' filter
- alfosc-calibs


Available scripts

Go to the directory
  cd ~/scripts/71-510

For these observations use the appropriate script for the date, complie the OB if needed.


Observations

CJ0335-1927 20 minutes 15 epochs

CJ0542-2125 20 minutes 17 epochs

J0909+44, 20 minutes 6 epochs

CJ1153+0756 35 minutes 15 epochs

J1326+48 13 minutes 15 epochs

J2222+2745 20 minutes 4 epochs


Date Time (UT) Duration Comments
14-10-2025 (EAT-15m)-01:35 00:20 epoch1 SDSSJ2222+2745
15-10-2025 00:35-02:40 00:20 epoch1 COOLJ0335-1927
18-10-2025 02:45-(SAT+15m) 00:20 epoch1 COOLJ0542-2125
18-10-2025 03:50-(SAT+15m) 00:50 epoch1 SDSSJ0909+4449
19-10-2025 00:25-05:15 00:20 epoch2 COOLJ0335-1927
19-10-2025 04:50-(SAT+15m) 00:35 epoch1 SDSSJ1004+4112
25-10-2025 02:20-(SAT+15m) 00:20 epoch2 COOLJ0542-2125
28-10-2025 23:50-04:40 00:20 epoch3 COOLJ0335-1927
28-10-2025 02:10-(SAT+15m) 00:20 epoch3 COOLJ0542-2125
29-10-2025 03:20-(SAT+15m) 00:50 epoch2 SDSSJ0909+4449
30-10-2025 04:15-(SAT+15m) 00:35 epoch2 SDSSJ1004+4112
13-11-2025 (EAT-15m)-00:35 00:20 epoch2 SDSSJ2222+2745
13-11-2025 22:50-02:25 00:20 epoch4 COOLJ0335-1927
16-11-2025 00:55-05:10 00:20 epoch4 COOLJ0542-2125
16-11-2025 05:20-(SAT+15m) 00:35 epoch1 COOLJ1153+0756
16-11-2025 05:45-(SAT+15m) 00:13 epoch1 SDSSJ1326+4806
17-11-2025 03:00-(SAT+15m) 00:35 epoch3 SDSSJ1004+4112
18-11-2025 02:00-(SAT+15m) 00:50 epoch3 SDSSJ0909+4449
19-11-2025 22:20-03:10 00:20 epoch5 COOLJ0335-1927
19-11-2025 05:30-(SAT+15m) 00:13 epoch2 SDSSJ1326+4806
23-11-2025 00:20-04:55 00:20 epoch5 COOLJ0542-2125
24-11-2025 04:45-(SAT+15m) 00:35 epoch2 COOLJ1153+0756
25-11-2025 01:30-(SAT+15m) 00:50 epoch4 SDSSJ0909+4449
25-11-2025 05:15-(SAT+15m) 00:13 epoch3 SDSSJ1326+4806
26-11-2025 23:40-02:45 00:20 epoch6 COOLJ0335-1927
26-11-2025 02:25-(SAT+15m) 00:35 epoch4 SDSSJ1004+4112
27-11-2025 00:35-04:35 00:20 epoch6 COOLJ0542-2125
27-11-2025 04:35-(SAT+15m) 00:35 epoch3 COOLJ1153+0756

Program Tracking
Proposal 72-510
Semester P72: 20251001 - 20260401
Principal Investigator Hakon Dahle
Programme A novel pathway to solving the Hubble tension
Instrument ALFOSC
Time Allocation g-band monitoring
Total Nights 36.6h
Type Monitoring
Notes Fixed dates to be scheduled
Total Time Spent 02:24 (hh:mm)
Proposal Date Time Type Targets Files Comments Status
72-510 2025-10-14 00:19 Monitoring SDSSJ2222 ALIj140076 - ALIj140078 Clear skies, and the seeing was around 1.0". Observed
72-510 2025-10-15 00:00 Monitoring Could not be observed due to bad weather. Failed
72-510 2025-10-18 00:19 Monitoring COOLJ0542-2125 ALIj180169 - ALIj180171 observed through thin clouds and approx. 0.8 arcsec. seeing. Observed
72-510 2025-10-19 00:00 Monitoring None None All targets missed due to weather. Failed
72-510 2025-10-25 00:22 Monitoring COOLJ0542-2125 ALIj250068 - ALIj250070 Observed under partial light cloud cover and seeing 1.1". Observed
72-510 2025-10-28 00:00 Monitoring Could not observe any targets due to 100% humidity Failed
72-510 2025-10-29 00:50 Monitoring SDSSJ0909 ALIj290104 - ALIj290106 Observed with good conditions and dark, clear skies. Observed
72-510 2025-10-30 00:34 Monitoring SDSSJ1004 ALIj300129 - ALIj300131 Good seeing and clear sky 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

Back to top Last modified: October 28 2025