INAF queue observing, 2019 April 28-29

Observer: F. Cusano, A. Gargiulo
Telescope Operator: D. Gonzalez-Huerta
Support Astronomer: O. Kuhn
Instrument:

At the sunset the sky is clear

Summary

Night duration (12 degree el twilight) 3:00 - 11:35 UT = 8 h 35m

Observing time: 5*h* 48*min* 68(%)

Weather time loss: 1*h* 59*min* 23(%)

technical time loss 0*h 47*min* 9(%)

Data Summary

Project_RUN Objects Instrument Configuration ExpTime /Time_tot Images Notes
Calibrations Bias Annibali LBC        
Calibrations Skyflat Annibali LBC g,r      
Annibali R24 LBC g,r 1/1h in both band   Completed
Annibali R22 LBC g,r 1/1h in both band   Completed
Annibali R29 LBC g,r 0.66/0.6h in both band   Completed with images from last year
Annibali R36 LBC g,r 1/1h in both band   Completed
Calibrations Dark Bianchi sci (2MASJ13 MRK695) LUCI2     luci2.0006-0010  
Calibrations Dark Bianchi tell (2MASJ13 MRK695) LUCI2     luci2.0011-0015  
Calibrations Dark Severgnini tell and sci LUCI2     luci2.0016-0020  

Details

Calibrations
  • Bias Annibali LBC
  • Skyflat g,r Annibali

02:03 The sky is clear, we decide to use LBC

02:43 Slew to Annibali R24
  • 02:57 seeing on dimm 1.1"
  • 02:57 we run again dohybrid
  • the difference in temperature between the primary mirror and the ambient is > 1.5 degrees and this causes problem with convergence.
  • 03:05 seeing on dimm 0.95"
  • 03:07 we reach the convergence
  • 03:08 copointing
  • 03:10 lbcrangebal
  • 03:12 dofpia
  • 03:16 we start science executing NGC3741_1
  • 03:21 we stop integration, guide star on red side was lost. Image acquired on the blue side (g band, lbcb.20190429.031753.fits) is good!
  • 03:24 dohybrid again
  • 03:26 seeing on dimm 1.1"
  • 03:36 we run again the script NGC3741_1
  • 03:44 seeing on g-band image 0.66"
  • 04:01 OB finished. We run dopia
  • 04:04 we run the script NGC3741_2
  • 04:06 seeing on dimm 1.0"
  • 04:29 dofpia
  • 04:30 seeing on dimm 1.0", on images 0.7"
  • 04:34 we run the script NGC3741_3

04:58 slew to Annibali R22
  • 05:03 we run the script UGC6541_1
  • 05:05 seeing on dimm 0.86"
  • 05:09 fwhm on blue image 0.8"
  • 05:30 dofpia
  • 05:47 clear active optic on the blue side, because blue is not converging
  • 05:50 blue is converged
  • 05:50 we run the script UGC6541_2
  • 05:50 seeing on dimm 0.98"
  • 06:10 seeing on dimm 0.73", on images 0.7"
  • 06:18 we run the script UGC6541_3

06:47 slew to Annibali R29
  • 06:50 seeing on dimm 0.96"
  • 07:00 red and blue channel converged
  • 07:01 we run the script UGC7408_1, 7:15 fwhm on image 0.8"
  • 07:26 dofpia
  • 07:31 we run the script UGC7408_2, dimm seeing 0.9"
  • 07:49 seeing on dimm 0.83

07:56 slew to Annibali R36
  • 07:58 dofpia
  • 08:02 we run the script NGC5238_1
  • 08:04 seeing on dimm 0.88"
  • 08:29 dofpia
  • 08:34 we run the script NGC5238_2
  • 08:40 seeing on dimm 0.86", on image 0.8"
  • 09:01 dofpia
  • 09:10 we run the script NGC5238_3
  • 09:26 seeing on dimm 0.9"

09:34 slew to Annibali R42
  • 09:40 no pupil found, maybe for clouds.
  • we move to R44 since in R42 there are too clouds.

09:44 slew to Annibali R44
  • 10:00 clouds, data no good.

10:10 we close for clouds

Calibrations
  • Dark for Bianchi's science (2MASJ13 MRX695 luci2.0006-0010
  • Dark for Bianchi's tell (2MASJ13 MRX695) luci2.0011-0015
  • Dark for Severgnini's science and tell luci2.0016-0020
Topic revision: r5 - 02 May 2019, FeliceCusano
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