Search
Text Size:
Smaller Text Normal Text Larger Text

Facebook page

Twitter profile

YouTube channel

First night NOTCam goes on telescope

The following tests are to be made on the first afternoon/night after NOTCam has been mounted on the telescope. These tests are supposed to be carried out and analysed by staff, and the tables on this webpage should be updated.

List of content in this document:

Check reset level
Optical alignment of wheels
Measure pinhole positions
NOTCam Quality Control (detector monitoring)
Rotation centre measured on the sky
Instrument alignment (measured on the sky)


During daytime


  • Start up the software according the instructions in the NOTCam Cookbok, and make sure you have valid entries in the optical path (status on the UIF being green, not red). Note that the setup script notcam.setup-ima crashes if you have the optical elements initially set to "Initialized" or "Not-initialized". Set the wheels manually by clicking on the menus in the UIF and then on the item of your choice. As soon as these positions are valid (green), the setup script notcam.setup-ima can be run.

  • Check reset level. This is being done automatically by the QC script since November 2010, and strictly speaking you don't have to go through this test.

    If you want to do it manually, it simply consists of finding the count level on the reset readout in each of the four quadrants. Take a simple exposure or a dark with the command dark 0. Open up an IRAF session with a DS9 on Florence, and display the reset image

    • displ /data/notcam/"filename"[2]
    • use imexamin and m to find the median value

    For the new Science Array the reset image level should be 6000 ± 1000 ADU in the centre of each quadrant. If the median is less than 3000 or more than 9000 ADU, the dc-offset voltages for the corresponding quadrant should be adjusted. You have to login as staff on the instrument computer and edit a script in the NOTCam directory of instrument scripts /home/softremote/inst-scripts/NOTCAM/ that is called "notcam.volt_newpcb_max". Note that there are three different type of voltages and you should only adjust the ones called "dc-offset" that are set with the commands:

    notcam.sendcamcmd @VBLB00+03566
    notcam.sendcamcmd @VBLB01+03532
    notcam.sendcamcmd @VBLB02+03410
    notcam.sendcamcmd @VBLB03+03524
    
    for the 4 quadrants numbered from 0 to 3. Comment out the old values and try adjusting the level by changing the 4 digit number at the end of each command . Start by changing only 10 units. Run the script, take a new test exposure, measure the new reset level, and iterate.

    Fig 1: A reset image obtained on the commissioning day of the new science array (SWIR3, 13/12-2007).



  • Optical alignment of wheels. This is not necessary every time NOTCam is mounted, typically after every opening of NOTCam only.

    Check, using the pupil imager, that filters and stops seem aligned with the pupil. If the 15mm stop or any filter is not aligned, then update the stepper motor units using edit-setup.

    TBD: Write proper instructions for how to do this.


  • Pinhole position. Monitoring the pinhole position.

    The idea is to check the internal stability of the instrument and the position of the detector whenever the 50 micron pinhole has not been moved during the opening, or the repositioning of the aperture wheel if it has. Note that from the 26/10-2005 until April 2006 the first science array was in.

    This task is done by running the interactive SEQUENCER script notcam.pinholePosition. Turn on/off the lamp when you are asked, and use imexam to measure and note down the X,Y values for each camera. Play around with the scale on the DS9 to actually see the pinholes. NB! Note that the Argon lamp may come on very slowly. The sequencer commands to switch on the argon lamp is tcs.baffle-lamp-2-on, and to switch it off tcs.baffle-lamp-2-off. The lamp status (i.e. commanded status) can be seen on the TCS status page 31. Update the table below. NB! some minor changes to be made to the script with the new 'common DS9 display' needed (remark 7/6-09).

    Date         X (WF)    Y (WF)     X(HR)     Y(HR)     Comment
    --------------------------------------------------------------
    2003-12-10   577.3     554.3                          SWIR1       
    2003-12-11   576.0     554.0
    2004-04-27   556.2     538.9
    2004-06-03   554.3     539.0
    2004-07-02   551.4     539.4
    2005-01-21   555.1     538.9
    2005-03-25   553.4     539.5
    2005-04-15   551.5     540.8
    2005-05-18   559.8     539.2
    2005-06-15   550.1     538.6     560.1    520.8
    2005-08-18   555.0     535.5     561.3    511.3
    2005-10-26   575.0     538.5     582.3    514.4    SWIR2 installed 2005-10-20
    2006-02-07   572.1     539.2
    2006-03-15   573.6     539.3     576.0    517.4
    2006-05-11   482.5     542.3     481.7    523.6    SWIR1 reinstalled 2006-05-02
    2006-07-05   489.8     538.3     474.8    524.8
    2007-02-24   485.7     541.8     483.9    522.5
    2007-03-29   487.1     541.7     481.1    522.3
    2007-04-29   483.5     541.9     476.3    521.9
    2007-05-27   483.88    541.85    481.40   522.10
    2007-08-28   484.02    543.05    475.75   524.23
    2008-04-16   471.9     524.2     464.9    512.4    SWIR3 installed 2007-12-07
    2008-05-21   470.0     525.0     460.7    508.8
    2008-06-09   471.7     525.6     465.6    508.4
    2008-06-12   472.4     524.9     465.7    509.4
    2008-07-07   470.6     524.1     461.8    506.1
    2008-07-16   470.5     523.5     459.6    506.4
    2008-09-14   471.0     523.2     462.4    514.6
    2009-01-07   473.4     519.0     469.6    514.4
    2009-03-07   475.5     523.9     462.4    508.6
    2009-04-04   469.8     523.0     459.2    514.5
    2009-05-10   456.8     532.8     457.6    515.5    Opening 2009-04-20, SWIR3 touched
    2009-06-07   468.1     533.8     462.5    517.7
    2009-07-10   463.5     532.2     457.5    514.4
    2009-09-30   467.1     531.9     466.5    515.3
    2010-02-06   466.5     532.8     463.8    514.5
    2010-10-28   466.5     531.7     461.1    515.1
    2010-11-18   468.9     530.8     457.0    513.3
    2010-12-10   468.5     530.4     466.2    513.6
    2011-02-12   465.6     531.7     459.1    539.6    Opening 2011-01-10, detector plate dismounted
    2011-06-10   468.1     520.6     463.7    520.2    Opening 2011-05-26, detector plate dismounted
    2011-08-11   464.9     521.4     450.1    520.0
    2011-10-12   462.6     521.3     442.7    519.6
    2012-01-07   469.4     521.3     463.0    517.1
    2012-03-01   463.7     520.8     446.6    518.9
    2012-04-01   467.8     528.9     462.9    522.3    Opening 2012-03-15, aperture unit dismounted  
    2012-05-01   468.0     527.7     465.8    518.9
    2012-06-09   466.1     528.8     456.7    521.4
    2012-09-06   461.4     529.0     443.7    520.2
    2012-10-01   460.8     529.0     444.7    521.0
    2012-12-17   461.98    529.83    445.34   523.67
    2013-01-22   464.47    529.64    449.46   521.55
    2013-02-19   461.57    530.36    447.36   518.73
    2013-03-21   463.24    530.36    450.38   520.47
    2013-04-25   458.68    530.42    438.80   521.98
    2013-05-25   463.2     530.9     449.4    522.3
    2013-06-22   464.0     530.0     452.1    521.2
    2013-08-29   459.4     530.0     439.9    519.9
    2013-09-14   459.2     529.1     442.5    518.6     
    2013-12-15   460.04    529.36    445.03   519.28    Opening 2013-10-25, aperture unit dismounted 
    2014-01-16   460.42    528.36    442.81   514.73
    2014-02-13   458.34    529.58    439.02   519.52
    2014-03-13   459.12    529.11 	 443.06   519.42
    2014-04-04   460.09    529.27 	 444.27   518.52 	
    2014-04-14   458.5     528.7 	 436.8    519.1 
    2014-05-19   459.1     529.1 	 438.7 	  519.3 	
    2014-06-09   462.4     529.1   	 448.4 	  519.6
    2014-07-09   457.9     528.9 	 435.2 	  519.0 	
    2014-08-08   463.4     529.2 	 448.8 	  518.8
    2014-08-22   461.9     528.7 	 445.4 	  516.0
    2014-09-03   462.9     528.8 	 449.3 	  518.8 	
    2014-10-05   460.2     529.2 	 437.8 	  519.0 
    2014-10-29   461.2     530.0 	 442.6 	  521.5 	
    2014-11-07   463.0 	529.4 	449.7 	 519.8 	
    2014-11-29   457.6 	529.1 	433.0 	 519.8 
    2015-01-05   460.4 	530.3 	442.5 	 521.5 	
    2015-02-04   462.2 	529.7 	449.4 	 521.6 
    2015-03-05   461.6 	529.9 	445.6 	 522.2
    2015-04-04   463.1 	528.6 	447.4 	 514.8
    2015-05-01   464.8 	529.0 	452.1 	 519.5 	
    2015-05-29   461.7 	529.0 	441.2 	 520.4 
    2015-07-03   463.4 	528.9 	448.0 	 520.5  
    2015-08-02   459.1 	529.5 	436.7 	 521.8 	
    2015-09-02   459.0 	529.2 	437.5 	 520.1 	
    2015-09-26   462.0 	529.1 	443.7 	 520.8 
    2015-10-27   461.4 	529.8 	441.7 	 521.4 
    2015-11-23   463.7 	529.0 	445.2 	 520.2 	
    2015-12-22   465.4 	530.0 	450.9 	 522.4 
    2016-01-23   465.6 	521.4 	457.3 	 500.8 
    2016-02-22   460.8 	522.0 	447.5 	 500.1 	
    2016-03-23   465.1 	528.2 	453.2 	 519.0 
    2016-04-20   463.8 	528.1 	450.9 	 518.3 	
    2016-04-29   459.6 	528.3 	440.1 	 517.9 
    2016-05-21   464.8 	529.0 	453.7 	 519.7 	
    2016-06-11   453.4 	528.3 	422.5 	 520.5
    2016-07-14   462.6 	527.8 	445.7 	 516.8 
    2016-07-27   467.3 	528.5 	465.0 	 515.9 
    2016-08-11   469.2 	528.5 	466.9 	 518.9 
    2016-09-15   459.9 	528.3 	443.6 	 518.9
    2016-10-12   463.5 	528.4 	451.0 	 517.7
    2016-10-25   458.5 	528.2 	437.9 	 516.3 
    2016-11-10   459.0 	528.3 	437.7 	 517.5 	
    2016-11-30   468.9 	528.8 	469.6 	 519.8 	
    2017-01-09   464.9 	527.9 	456.7 	 514.9 	
    2017-02-07   464.2 	528.5 	452.8 	 519.6 
    2017-02-19   463.7 	529.2 	451.2 	 520.3 
    2017-05-01   463.9 	528.2 	449.5 	 518.1 	
    2017-05-24   466.2 	528.3 	457.7 	 517.4 
    2017-06-20   463.7 	528.3 	447.0 	 518.1 	
    2017-09-02   461.4 	528.7 	443.8 	 518.7 
    2017-10-26   463.3 	528.1 	446.5 	 518.2 	
    2017-11-02   464.3 	527.8 	446.2 	 518.9 	
    2017-12-07   470.4 	528.6 	464.6 	 518.9 
    2018-01-03   467.5 	528.4 	461.5 	 518.2 
    2018-02-16   466.1 	528.9 	456.8 	 520.0
    2018-03-11   465.9 	528.0 	455.1 	 519.1
    2018-04-17   465.0 	529.6 	447.6 	 521.4
    2018-05-11   470.0 	528.7 	462.3 	 518.7
    2018-05-26   464.9      528.4   448.1    519.3
    2018-06-10   467.8      528.2   458.8    518.0
    2018-06-27   464.2      526.2   449.7    514.3  Opening 15-6. Aperture unit dismounted.
    2018-07-13   465.4      526.1   456.3    513.0
    2018-07-30   466.1	526.7	460.3	 514.5
    2018-08-19   464.0      527.5   455.8    515.5
    2018-08-28   465.0      526.7   454.6    514.1	
    2018-09-23   465.1      526.6   454.6    513.7
    2018-11-02   463.6      526.3   445.7    513.1
    2019-01-29   467.7      526.5   460.1    514.1
    2019-02-15   470.2      526.9   466.8    515.1
    2019-03-04   471.7      526.2   468.3    513.1
    2019-03-17   471.2      526.1   469.8    512.8
    2019-04-09   467.8      526.5   459.0    513.0
    2019-04-30   467.1      527.4   457.8    516.0
    2019-05-17   464.8      526.7   451.2    513.7
    2019-07-21   466.6      526.7   454.1    514.7
    2019-08-17   460.2      525.2   436.0    514.0
    2019-08-22   462.4      526.1   443.3    514.4
    2019-09-13   465.8      524.9   456.7    510.3
    2019-12-16   466.5      526.0   457.7    513.7
    2020-02-05   465.6      526.4   453.0    514.6
    2020-03-02   469.0      526.1   459.8    514.3
    2020-03-26   467.8      526.4   456.1    514.9
    2020-05-30   465.5      527.1   451.5    515.4
    2020-07-08   469.5      527.3   464.2    516.3
    2020-08-06   467.8      526.5   459.8    513.8
    2020-09-09   469.0      527.0   466.0    517.3
    2020-11-20   470.4      527.7   466.7    517.6
    2021-01-25   468.32     528.47  462.36   518.15
    2021-03-01   467.2      528.34  458.97   517.8
    2021-03-16   464.6      528.4   452.0    518.2
    2021-03-29   468.9      528.41  460.81   519.13
    2021-04-23   455.5 !    528.51  423.82!  518    large shift in X
    2021-04-25   451.6 !    528.36  407.45!  518.29 large shift in X
    2021-04-26   464.12     528.38  449.43   518.07
    2021-05-05   467.27     528.34  455.36   517.88
                 467.41     528.37  456.15   517.71 turned aperture wheel
                 466.37     528.38  452.71   518.42 turned aperture wheel
                 466.54     528.39  452.21   517.41 turned aperture wheel
                 468.89     528.31  458.83   518.24 + having moved to alt=20 and back to alt=90
                 470.29     528.32  463.66   518.21 having turned aperture wheel
    2021-05-20   466.59     528.34  454.97   517.95 
    2021-06-18   466.01     528.40  455.02   517.66 
    2021-07-14   467.09	525.97  464.07   515.83
    2021-08-09   466.33	525.72  461.46   514.16
    2021-08-23   468.45	525.73  464.79   514.55
    2021-09-13   470.68	525.75	470.05	 514.32
    2021-10-12   471.35     525.50  470.73   514.01
    2021-12-08   468.36     527.12  464.66   517.25
    2021-12-12   464.63     526.46  455.5    516.12
    2022-01-05   467.8      526.29  463.7    514.9
    2022-02-04   469.60     526.87  468.5    515.01
    2022-02-06   469.91	527.99	470.73	 518.66
    2022-02-24   467.67	526.68	466.92   514.96
    2022-03-17   460.61     527.85  466.82   518.28 
    2022-04-12   466.71     527.18  465.8    516.43
    2022-05-06   468.32     527.11  465.93   515.25
    2022-05-31   471.24	527.69	473.60   517.97
    2022-06-08   468.74     526.93  464.28   516.39
    2022-06-15   466.95     522.69  461.32   517.47
    2022-07-08   468.25	528.38	466.38   519.25
    2022-07-25   468.4	528.16	464.88   519.26
    2022-08-16   471.39     528.00  471.21   517.73
    2022-09-13   470.75     528.43  468.88   520.14 
    2022-10-09   470.30     528.05  470.77   518.76
    2022-10-28   466.67	528.81	466.58   521.54
    2022-11-22   467.25	528.46	465.61   518.76
    2022-12-05   467.21     529.28  466.53   520.88
    2022-12-11   467.69     529.27  465.55   521.60
    2023-01-04   468.52	529.10	465.04   520.77
    2023-02-01   469.71	529.31	468.64   521.40
    2023-02-21   470.50     529.35  467.41   521.32
    2023-04-03   469.79     529.43  469.99   521.61
    2023-04-25   468.37     528.67  460.95   521.41
    2023-05-01   467.81     529.12  465.36   521.67
    2023-05-18   469.41     528.77  469.31   521.75
    2023-06-13   468.71     528.46  465.51   518.99
    2023-07-11   468.49     528.96  467.31   518.61
    2023-08-02   469.04     528.56  465.69   515.86
    2023-08-29   468.57     529.07  466.38   519.18
    2023-10-05   467.92     528.94  468.03   519.69
    2023-10-26   469.54     529.05  467.71   519.58
    2023-10-28   469.33     529.18  456.70   520.82
    2023-11-20   468.48     529.19  464.50   520.55
    2023-12-05   470.14     528.96  467.51   519.86
    2024-01-09   471.00     528.75  
    2024-01-20   468.66     528.09  466.95   520.07
    2024-02-13   467.51     529.00  463.70   520.63
    2024-03-02   469.30     527.53  466.10   519.55
    2024-04-22   471.85     528.92  469.90   520.74
    2024-05-15   470.05     528.47  466.73   521.10
    2024-05-15   470.54     528.98  467.10   521.70
    2024-06-26   465.57     526.43  460.34   520.32
    2024-07-15   466.87     527.37  463.70   518.54
    2024-09-03   469.74     527.16  464.81   514.81
    2024-10-25   468.91     528.50  468.15   519.75
    


  • Detector monitoring. This should be done once every time NOTCam is mounted on the telescope, preferrably on the first day. Do as follows:

    1. Switch on the NOTCam QC lamp from the panel on the wall in the control room. Make sure all other dome-lights are off.

    2. Power-on the telescope.

    3. Run the setup script for notcam: tcs.setup-tel-notcam.

    4. Lower telescope and open mirror covers: alt 45 and o-m-c on the TCS UIF.

    5. Run the setup script notcam.setup-ima wf 201 which sets up the instrument to WF-camera and J-band filter.

    6. Test that exp 4.2 gives around 5000 adu per pixel in the brightest areas. If needed, adjust the lamp intensity using the large knob labelled "intensity level", default is around 56.

    7. Close the staircase entrance to make sure nobody enters the dome.

    8. In the NOTCam Sequencer start the QC script (either the first one, or the two readout modes individually) as follows:

      • notcam.lintest (both modes, takes about 90 min and produces 168 files)
      • notcam.lintest-rrr (r-r-r mode, takes about 60 min and produces 138 files)
      • notcam.lintest-rs (r-s mode, takes about 30 min and produces 30 files)

    9. Don't forget to switch off the lamp when finished!

    10. Close mirror cover c-m-c and put telescope to zenith zenith .

    11. when the telescope stops moving power off the unless you are starting observations within 1 hour from now.

    12. The above sets of data provide readout noise, gain, bad pixels, dark level and non-linearity for each readout mode. To analyse the data, type:

      • notcam.lintest-analyse rrr filename1 (for the reset-read-read dataset)
      • notcam.lintest-analyse rs filename1 (for the ramp-sampling dataset)

      where filename1 is the first file in each dataset. For the rrr dataset this is the first image with OBJECT name "Lintest drk 0s". For the rs dataset, the first file has OBJECT name "mdark 0 5", and if the data is taken in one go with the command notcam.lintest, then this file has a running number of 138 + the above file number.

      Check that the NOTCam detector behaviour is OK by looking at the QC result plots on the web pages: Ramp-sampling mode detector monitoring and Reset-read-read mode detector monitoring.

    The instrument setup is checked and set in the lintest scripts, but for your reference it is:

    Wheel Position Content
    Aperture #4 OPEN large
    Filter 1 #15 OPEN
    Filter 2 #13 J
    Stop #12 15mm ring
    Grism #2 empty
    Lens #1 WF
    Camera focus 5650 5650


On the sky


  • Rotation centre This should be done every time NOTCam is re-mounted on the telescope. Update the table below.

    Script: Make sure you have field-r -90 and go to a suitable star (e.g. focus or standard star) high in the sky. Then run the script:

    notcam.rotation-centre <exptime>

    This takes images for both WF and HR camera. You must manually find the positions of stars (use imexam) and calculate the rotation centre (can be done later). This will be improved in a future version.

    Or manually: Use the same setting as for detector monitoring above and point the telescope to a focus star close to zenith. and foc-del -75 for J-band is good enough to safely measure star centers. --> Use first the default sky orientation for NOTCam: field-r -90 and take an exposure with exp 15. If this leads to overexposure, then use a fainter star. Save the image. Then set field-r 90 and take another exposure. Go back to field-r -90 and take a new exposure. This should be sufficient to determine the XY values of the rotation centre on the array and to have an idea of the accuracy. Do the same for the HR camera.



    Date WF X WF Y HR X HR Y note
    5-Sep-2001 451.9 555.4


    27 Apr 2004 527 549

    Hband, short exposures, daytime
    2 Jul 2004 533.8 549.7


    21 Jan 2005 529.9 550.8


    25 Mar 2005 531.0 543.2


    18 May 2005 538.5 546.0

    2 stars, 1 measurement
    15 Jun 2005 531 546 499 546 1 star, 1 measurement
    14 Jan 2006 473.4+-0.1 554.5+-0.07 507.6 562.9 5 stars (WF), new array! X-flip
    15 Mar 2006 472.8 550.3 511.0 557.8 2 stars (WF), 1 star (HR) X-flip
    11 May 2006 518.1+-0.2 558.7+-0.1
     
     
    3 stars (WF), old array! X-flip
    29 Jan 2007 501.0+-0.1 548.8+-0.1 530.1+-0.4 550.5+-0.04 2 stars, old array! X-flip
    24 Feb 2007 501.4+-0.1 551.2+-0.1 - - old array! X-flip
    29 Apr 2007 500.4+-0.1 552.3+-0.1 523.3+-0.3 554.9+-0.3 old array! X-flip
    2 Sep 2007 500.8 556.18 - - old array! X-flip
    30 Sep 2007 498.0 552.2 508.8 558.5 2 stars, old array! X-flip
    16 Nov 2007 501.8 550.4 531.9 551.2 old array! X-flip
    13 Dec 2007 502.2 537.8 549.6 549.9 New Science array! X-flip
    16 Apr 2008 497.6 536.2 543.9 541.6 New Science array! X-flip
    21 May 2008 498.8 533.7 - - New Science array! X-flip
    11 Jan 2009 501.2 535.5 - - New Science array! X-flip
    07 Mar 2009 501.8 534.1 - - New Science array! X-flip
    03 Aug 2009 496.7 533.9 554.4 518.2 New Science array! X-flip
    09 Sep 2009 483.7 541.5 511.4 538.1 New Science array! X-flip
    15 Oct 2009 483.0 541.5 508.5 540.0 New Science array! X-flip
    26 Nov 2009 484.1 540.0 509.7 543.0 New Science array! X-flip
    19 May 2010 488.8 540.8 518.9 538.7 New Science array! X-flip
    20 Jun 2010 484.2 540.5 - - New Science array! X-flip
    18 Nov 2010 486.4 541.9 521.5 546.6 New Science array! X-flip
    10 Dec 2010 491.0 541.3 529.7 549.0 New Science array! X-flip
    12 Feb 2011 495.2 548.8 545.4 585.8 New Science array! X-flip
    19 Feb 2011 495.8 544.7 548.1 585.6 New Science array! X-flip
    10 Jun 2011 500.2 529.4 551.4 549.8 New Science array! X-flip
    13 Aug 2011 496.0 532.9 542.8 554.9 New Science array! X-flip
    12 Oct 2011 500.2 531.7 547.8 554.8 New Science array! X-flip
    07 Jan 2012 497.7 531.2 554.6 546.4 New Science array! X-flip
    01 Apr 2012 500.8 544.5 549.3 573.0 New Science array! X-flip
    01 May 2012 500.0 544.0 554.5 564.0 New Science array! X-flip!
    09 Jun 2012 488.0 543.9 522.7 569.8 New Science array! X-flip!
    01 Oct 2012 491.6 540.8 525.9 561.2 New Science array! X-flip!
    17 Feb 2013 499.5 547.8 556.9 576.8 New Science array! X-flip!
    22 Mar 2013 501.7 547.0 561.3 572.8 New Science array! X-flip!
    25 Apr 2013 498.4 548.9 556.0 577.4 New Science array! X-flip!
    22 Jun 2013 499.5 530.6 549.7 573.1 New Science array! X-flip!
    29 Aug 2013 New Science array! X-flip!
    20 Oct 2013 502.3 548.9 541.1 565.1 New Science array! X-flip!
    15 Dec 2013 497.6 540.9 547.5 559.7 New Science array! X-flip!
    13 Mar 2014 499.3 541.1 554.7 547.1 New Science array! X-flip!
    04 Apr 2014 493.5 540.6 553.6 563.7 New Science array! X-flip!
    19 May 2014 496.6 540.0 544.1 557.2 New Science array! X-flip!
    9 Jun 2014 495.3 542.1 550.9 559.9 New Science array! X-flip!
    8 Aug 2014 497.3 540.0 544.6 548.4 New Science array! X-flip!
    3 Sep 2014 502.7 540.2 552.0 557.4 New Science array! X-flip!
    5 Oct 2014 501.5 541.5 545.5 557.0 New Science array! X-flip!
    29 Oct 2014 499.9 539.2 560.3 565.6 New Science array! X-flip!
    7 Nov 2014 506.7 538.3 580.8(?) 539.5(?) New Science array! X-flip!
    Script crashed after first HR exp
    4 Feb 2015 488.9 541.7 538.6 563.7 New Science array! X-flip!
    5 Mar 2015 498.3 539.8 555.0 559.1 New Science array! X-flip!
    2 May 2015 493.1 543.5 536.0 563.0 New Science array! X-flip!
    29 May 2015 497.7 541.0 552.3 558.8 New Science array! X-flip!
    2 Aug 2015 495.8 542.0 537.8 561.5 New Science array! X-flip!
    2 Sep 2015 498.2 541.9 538.8 555.5 New Science array! X-flip!
    26 Sep 2015 497.6 540.5 541.2 557.0 New Science array! X-flip!
    27 Oct 2015 495.1 543.0 535.8 563.1 New Science array! X-flip!
    23 Jan 2016 499.6 537.9 559.3 554.3 New Science array! X-flip!
    20 Apr 2016 498.4 539.5 550.1 550.9 New Science array! X-flip!
    29 Apr 2016 497.5 540.5 537.4 550.1 New Science array! X-flip!
    22 May 2016 494.6 539.9 549.3 554.8 New Science array! X-flip!
    11 June 2016 498.7 538.3 549.4 550.8 New Science array! X-flip!
    14 July 2016 496.4 539.5 541.1 556.0 New Science array! X-flip!
    27 July 2016 496.4 538.1 550.5 551.9 New Science array! X-flip!
    11 Aug 2016 509.1 527.1 547.1 559.1 New Science array! X-flip!
    15 Sept 2016 494.5 539.9 520.3 555.8 New Science array! X-flip!
    13 Oct 2016 498.9 537.3 555.9 549.1 New Science array! X-flip!
    10 Nov 2016 493.5 542.2 536.8 563.6 New Science array! X-flip!
    30 Nov 2016 493.6 539.7 530.2 558.1 New Science array! X-flip!
    15 Dec 2016 493.5 538.2 541.5 552.5 New Science array! X-flip!
    09 Jan 2017 488.3 540.1 535.8 552.7 New Science array! X-flip!
    07 Feb 2017 494.3 535.9 539.8 537.4 New Science array! X-flip!
    19 Feb 2017 494.3 535.9 539.8 537.4 New Science array! X-flip!
    01 Mar 2017 494.2 539.5 541.2 554.2 New Science array! X-flip!
    24 May 2017 496.0 535.8 539.8 545.6 New Science array! X-flip!
    20 June 2017 495.7 537.8 528.9 546.9 New Science array! X-flip!
    26 Oct 2017 497.6 537.6 535.5 549.1 New Science array! X-flip!
    11 May 2018 491.9 537.5 531.5 555.5 New Science array! X-flip!
    10 Jun 2018 494.2 541.2 541.5 552.2 New Science array! X-flip!
    30 Jun 2018 498.1 538.3 544.2 550.8 New Science array! X-flip!
    19 Aug 2018 493.0 540.0 544.0 551.5 New Science array! X-flip!
    23 Sep 2018 497.5 541.0 545.6 553.8 New Science array! X-flip!
    10 Dec 2018 496.6 540.0 550.0 556.7 New Science array! X-flip!
    29 Jan 2019 499.1 540.2 547.5 554.7 New Science array! X-flip!
    09 Apr 2019 493.1 541.5 551.2 518.3 New Science array! X-flip!
    30 Apr 2019 495.8 538.7 556.2 557.9.3 New Science array! X-flip!
    13 Sep 2019 499.3 535.6 -- -- New Science array! X-flip!
    16 Nov 2019 502.2 536.5 554 550 New Science array! X-flip!
    05 Feb 2020 496.3 539.9 538.6 554.0 2 stars (WF, HR)
    03 Mar 2020 493.6 541.5 567.6 560.9 1 star (WF, HR)
    09 Sep 2020 496.4 540.3 532.6 555.3 1 star (WF, HR)
    30 Oct 2020 494.2 541.7 535.1 559.35 2 stars, poor seeing (WF, HR)
    20 Nov 2020 492.5 541.1 527.0 568.3 1 star (WF, HR)
    25 Jan 2021 493.88 541.09 533.77 599.05 1 star (WF, HR)
    26 Apr 2021 495.2 541.9 537.4 563.4 2 stars (WF, HR)
    20 May 2021 493.2 542.2 ... ... 1 star (WF)
    15 Jul 2021 495.4 535.8 536.9 548.4 1 star (WF)
    24 Aug 2021 497.1 534.4 549.3 539.8 3, 1 stars in WF, HR
    12 Oct 2021 495.6 535.2 552.8 544.4 3 stars (WF, HR)
    15 Jun 2022 495.9 538.1 552.3 545.9
    05 Dec 2022 490.0 536.6 538.7 545.7
    01 Feb 2023 490.6 537.2 537.4 554.9
    25 Apr 2023 491.8 537.2 528.2 547.0
    18 May 2023 499.0 532.8 - - MOXA box broke after WF images
    14 Jun 2023 493.8 538.3 535.9 548.6 1 star (WF,HR)
    2 Aug 2023 490.9 538.2 530.4 555.3 5 star (WF,HR)
    20 Nov 2023 495.9 536.9 537.2 551.7 3,2 stars in WF, HR
    27 Dec 2023 492.8 541.0 527.5 550.6 1 star WF, HR
    15 Jul 2024 487.8 538.0 533.1 555.1 1 star WF, HR


  • Instrument alignment This should be done every time NOTCam is mounted on the telescope. Update the table below.

    Use the same setting as for detector monitoring above and point the telescope to a focus or standard star close to zenith. and foc-del -75 for J-band is good enough to safely measure star centers.-->

    In order to determine the alignment, make sure the field orientation is set to field -90, and put the star on position X=200, Y=600. Do this by using the sequencer command slitoff 200 600, where you follow the instructions and iterate once. Make an exp 15 integration, and use imexam (and the 'a' key) to measure the X,Y position of the star. Then move the star to X ~ 800 by using the command teloffset 140 0. Take another exp 15 and move back by teloffset -140 0 to take a third exposure. Now you have the two positions X1,Y1 and X2,Y2 of the star, of which the first one is measured twice such that you have an indication of the error.

    The line connecting the two observed positions of the star will make a small angle with the detector rows. This angle can be determined as offset_angle = arctan(dY/dX), where dY = Y2-Y1, and dX = X2-X1. Add this small number to the field-r value (-90) in table below. If it is very different from the previously measured values, the slits must be realigned. (The slits should be aligned to follow this slight tilt.) See instructions on How to align NOTCam slits.



    Date Field angle needed
    to align RA with X (deg)
    Comment
    Aug-2003 -90.3 Eng. Grade Array
    Jul-2004 -90.5 Eng. Grade Array
    Mar-2005 -90.7 Eng. Grade Array
    May-2005 -90.8 Eng. Grade Array
    Jun-2005 -90.8 Eng. Grade Array
    Jan-2006 -90.8 First Science Array (X-flipped image)
    Mar-2006 -90.5 First Science Array (X-flipped image)
    May-2006 -89.1 Eng. Grade Array back (X-flipped image)
    Jan-2007 -89.4 Eng. Grade Array back (X-flipped image)
    Feb-2007 -89.2 Eng. Grade Array back (X-flipped image)
    Apr-2007 -89.0 Eng. Grade Array back (X-flipped image)
    Sep-2007 -89.3 Eng. Grade Array back (X-flipped image)
    Dec-2007 -90.1 New Science Array (X-flipped image)
    Apr-2008 -90.2 New Science Array (X-flipped image)
    May-2008 -90.1 New Science Array (X-flipped image)
    Sep-2008 -90.1 New Science Array (X-flipped image)
    Jan-2009 -90.1 New Science Array (X-flipped image)
    Mar-2009 -90.1 New Science Array (X-flipped image)
    Apr-2009 -90.2 New Science Array (X-flipped image)
    Aug-2009 -90.2 New Science Array (X-flipped image)
    Dec-2010 -90.1 New Science Array (X-flipped image)
    Feb-2011 -90.1 New Science Array (X-flipped image)
    13 Aug 2011 -90.1 New Science Array (X-flipped image)
    12 Oct 2011 -90.1 New Science Array (X-flipped image)
    07 Jan 2012 -90.1 New Science Array (X-flipped image)
    05 Feb 2012 -90.0 New Science Array (X-flipped image)
    01 May 2012 -89.86 New Science Array (X-flipped image)
    09 Jun 2012 -90.1 New Science Array (X-flipped image)
    19 Feb 2013 -90.1 New Science Array (X-flipped image)
    22 Mar 2013 -90.0 New Science Array (X-flipped image)
    25 Apr 2013 -90.1 New Science Array (X-flipped image)
    20 Oct 2013 -90.2 New Science Array (X-flipped image)
    15 Dec 2013 -89.9 New Science Array (X-flipped image)
    13 Mar 2014 -90.1 New Science Array (X-flipped image)
    04 Apr 2014 -89.9 New Science Array (X-flipped image)
    14 Apr 2014 -89.9 New Science Array (X-flipped image)
    19 May 2014 -89.9 New Science Array (X-flipped image)
    8 Aug 2014 -90.05 New Science Array (X-flipped image)
    22 Aug 2014 -89.96 New Science Array (X-flipped image)
    3 Sep 2014 -89.88 New Science Array (X-flipped image)
    5 Oct 2014 -90.02 New Science Array (X-flipped image)
    29 Oct 2014 -90.02 New Science Array (X-flipped image)
    5 Mar 2015 -90.00 New Science Array (X-flipped image)
    4 Apr 2015 -89.90 New Science Array (X-flipped image)
    2 may 2015 -90.0 New Science Array (X-flipped image)
    29 May 2015 -90.00 New Science Array (X-flipped image)
    3 Jul 2015 -90.00 New Science Array (X-flipped image)
    2 Aug 2015 -90.00 New Science Array (X-flipped image)
    2 Sep 2015 -90.00 New Science Array (X-flipped image)
    26 Sep 2015 -90.06 New Science Array (X-flipped image)
    23 Jan 2016 -89.84 New Science Array (X-flipped image)
    20 Apr 2016 -90.06 New Science Array (X-flipped image)
    29 Apr 2016 -89.96 New Science Array (X-flipped image)
    22 May 2016 -89.90 New Science Array (X-flipped image)
    11 June 2016 -89.86 New Science Array (X-flipped image)
    14 July 2016 -89.96 New Science Array (X-flipped image)
    11 Aug 2016 -90.00 New Science Array (X-flipped image)
    15 Sept 2016 -90.06 New Science Array (X-flipped image)
    13 Oct 2016 -90.02 New Science Array (X-flipped image)
    30 Nov 2016 -89.88 New Science Array (X-flipped image)
    15 Dec 2016 -89.81 New Science Array (X-flipped image)
    09 Jan 2017 -90.04 New Science Array (X-flipped image)
    07 Feb 2017 -89.98 New Science Array (X-flipped image)
    01 Mar 2017 -89.83 New Science Array (X-flipped image)
    24 May 2017 -89.90 New Science Array (X-flipped image)
    20 June 2017 -89.91 New Science Array (X-flipped image)
    26 May 2018 -89.87 New Science Array (X-flipped image)
    10 Jun 2018 -90.08 New Science Array (X-flipped image)
    13 Jul 2018 -89.63 New Science Array (X-flipped image)
    30 Jul 2018 -89.85 New Science Array (X-flipped image)
    19 Aug 2018 -89.87 New Science Array (X-flipped image)
    23 Sep 2018 -89.91 New Science Array (X-flipped image)
    03 Nov 2018 -89.87 New Science Array (X-flipped image)
    10 Dec 2018 -89.96 New Science Array (X-flipped image)
    05 Feb 2020 -89.99 New Science Array (X-flipped image)
    02 Mar 2020 -90.08 New Science Array (X-flipped image)
    09 Sep 2020 -89.83 New Science Array (X-flipped image)
    30 Oct 2020 -90.16 New Science Array (X-flipped image)
    20 Nov 2020 -88.99 New Science Array (X-flipped image)
    25 Jan 2021 -89.74 New Science Array (X-flipped image)
    20 May 2021 -89.73 New Science Array (X-flipped image)
    15 Jul 2021 -89.77 New Science Array (X-flipped image)
    12 Oct 2021 -89.83 New Science Array (X-flipped image)
    15 Jun 2022 -89.77 New Science Array (X-flipped image)
    05 Dec 2022 -90.11 New Science Array (X-flipped image)
    17 Jul 2024 -90.03 New Science Array (X-flipped image)


    Since beginning of 2004 we have attached alignment devices to secure a repeatable position of NOTCam with respect to its blue adapter flange. Thus, the placement of NOTCam with respect to the telescope should be more stable. From the above values the precision seems to be +- 0.1 degrees. The 3 different arrays clearly have a slightly different orientation in the socket.

    To check what field-r value is needed to get RA and DEC perfectly aligned along the detector XY, set the rotator to the required field angle (current field angle plus the above derived offset angle) and move the telescope using the TCS ('alt' plus 'arrow' keys one step) having first set o-s 140 140 on the TCS. Do not use teloffset because it will account for the change to the new field angle and the stars will still move tilted wrt the rows of the detector.

    If the rotational offset that you have determined is different from the previous determination (see table above), then the slits have to be realigned! See instructions.


Comments to Amanda

Back to top Last modified: October 25 2024