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P69-101: Photometry and spectroscopy of FUor-type eruptive young stars

PI: Z. Nagy

This program is a Monitoring program using NOTCam J-, H-, and K-band imaging and spectroscopy. For NOTCam spectroscopy, see How to run NOTCam spectroscopy OBs manually.

Instrument setup:

  • NOTCam: WF-camera, Grism #1, 0.6'' slit, filters J (#201), H (#203), and K (#208).

Daytime calibrations:

  • NOTCam differential skyflats WF-camera and filters J (#201) , H (#207), and K (#208).
  • notcam.notcam-calibs NC**** in the morning after the observations.

Monitoring schedule

Date           UT-window     Duration

22-04-2024   03:00 - SNT     01:40
25-04-2024   03:00 - SNT     01:40
15-05-2024   02:30 - SNT     01:20
12-08-2024   00:00 - SNT     01:30 

The OB generator will be used to request all observations.

For the observer:

Go to the directory
  cd ~/scripts/69-101
List the available scripts
  ls -lrt
and execute the OB generated script for the appropriate date as requested.

See observer's Guide to NOTCam Spectroscopy OBs

Remember to fill in the tracking report Mon
Program Tracking
Proposal 69-101
Semester P69: 20240401 - 20241001
Principal Investigator dr. Zsofia Nagy
Programme Photometry and spectroscopy of FUor-type eruptive young stars
Instrument NOTCam
Time Allocation Ima+spec of 4 targets
Total Nights 1.0
Type Mon
Notes Fixed dates to be scheduled
Total Time Spent 05:38 (hh:mm)
Proposal Date Time Type Targets Files Comments Status
69-101 2024-04-22 01:53 Mon Gaia18dvy, HD192538 NCHd220814 - NCHd220877 Observed with thin clouds and seeing better than 1 arcsec. Observed
69-101 2024-04-25 01:55 Mon Parsamian21, HIP95002 NCHd250464 - NCHd250525 There were thin clouds and good seeing Observed
69-101 2024-05-15 01:50 Mon HD199217, HBC722 NCHe150807 - NCHe150870 Clear skies, seeing of less than one. Did telluric first, then spec then phot. Did easy-calib at the end of telluric. Phot observation went into nautical twilight (05:38, nautical at 05:23). 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: May 29 2024