IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Changes between Version 7 and Version 8 of QUB_SV_21012010_templates


Ignore:
Timestamp:
Jan 21, 2010, 10:10:09 AM (16 years ago)
Author:
kpat.uk
Comment:

--

Legend:

Unmodified
Added
Removed
Modified
  • QUB_SV_21012010_templates

    v7 v8  
    44'''STEP 1'''[[BR]]
    55
    6 
    76'''Stack for testing on skycell with good target already selected ''' [[BR]]
     7Before produce all the difference stack-stack it would be probably useful to test the ppsub on a small number of stacks.
     8On MD03 skycel 043 the Harvard/JHU PS1 Group found some SN candidates. Using good images for this skycel, we could test
     9ppsub and the photometry of psphot.
    810
    911'''MD03''' [[BR]]
     
    1315'''r skycell.043 stack.39693'''[[BR]]
    1416
    15 '''i skycell.043 stack.'''[[BR]]
     17'''i skycell.043 stack.36944'''[[BR]]
    1618
    17 
     19'''z skycell.043 stack.'''[[BR]]
    1820
    1921'''STEP 2'''[[BR]]
    2022
    2123I'm selecting good stacks looking the following 4 parameters in the unconvolved stacks:
    22 average fhwm Minimum;   average fhwm Major;   average moment along xx;  average momentum along yy
     24average fhwm Minimum;   average fhwm Major;   average moment along xx;  average momentum along yy.[[BR]]
     25
    2326Once a good night is selected in each filter, I checked 3-4 skycells by eyes and run ppSub using these images as template.
    24 The good stacks I suggest as teplate are reported below, followed by a summary of all the steps I did.[[BR]]
     27(any suggestion how to improve the selection of the templates is welcomed). [[BR]]
     28
     29
     30Here are all the steps I'm doing:  [[BR]]
     31
     32* Download all new stacks in the archive[[BR]]
     33
     34* Run psphot on unconvolved images [[BR]]
     35
     36* Compare the following parameters from cmf files: [[BR]]
     37
     38   PSF magnitudes vs aperture magntude [[BR]]
     39
     40   moment along x vs moment along y [[BR]]
     41 
     42   minimum fwhm vs major fwhm [[BR]]
     43
     44[[Image(MD04.skycell.044.stk.41186.cmf_1.png, 400px)]][[BR]]
     45[[Image(MD04.skycell.099.stk.38684.cmf_1.png, 400px)]][[BR]]
     46
     47 '''COMMENTS:'''
     48the unconvolved images have more detections (but probably several of them are not real)
     49the FWHM of the objects is degraded in the convolved image (probably too much in some skycells)
     50To investigate the quality of stacks and select good templates, I used the fwhm and moments values of the unconvnolved images.[[BR]]
     51
     52The choice of the unconvolved images to investigate the fwhm and moment variation is because in the convolved images the fwhm and moments are all degraded at similar values.
     53 
     54 The average values for each skycell is computed rejecting at 3 sigma (5 iterations) [[BR]]
     55
     56* I'm comparing the values of these parameters in each filters and each field  [[BR]]
     57
     58* taking a look by eyes some of the skycells of the best epochs, I choose the best templates  [[BR]]
     59
     60 some epochs with small fwhm and moments (in principle good templates) seem to be masked too much  [[BR]]
     61
     62[[Image(MD02.skycell.066.stk.36184.unconv.jpg, 400px)]][[BR]]
     63Good nights from which we can probably take the template stacks are reported below: [[BR]]
    2564
    2665'''MD02'''[[BR]]
     
    73112[[Image(MD04.png, 800px)]][[BR]]
    74113
    75 Here is all the step I'm doing what I'm doing:  [[BR]]
    76114
    77 * Download all new stacks in the archive[[BR]]
    78 
    79 * Run psphot on unconvolved images [[BR]]
    80 
    81 * Compare the following parameters from cmf files: [[BR]]
    82 
    83    PSF magnitudes vs aperture magntude [[BR]]
    84 
    85    moment along x vs moment along y [[BR]]
    86  
    87    minimum fwhm vs major fwhm [[BR]]
    88 
    89 [[Image(MD04.skycell.044.stk.41186.cmf_1.png, 400px)]][[BR]]
    90 [[Image(MD04.skycell.099.stk.38684.cmf_1.png, 400px)]][[BR]]
    91 
    92  '''COMMENTS:'''
    93 
    94 the unconvolved images have more detections (but probably several of them are not real)
    95 the FWHM of the objects is degradated in the convolved image (probably too much in some skycells)
    96 To investigate the quality of stacks and select good templates, I used the fwhm and moments values of the unconvnolved images.
    97 
    98 
    99 
    100  The average values for each skycell is computed rejecting at 3 sigma (5 iterations) [[BR]]
    101 
    102 * I'm comparing the values of these parameters in each filters and each field  [[BR]]
    103 
    104 * taking a look by eyes some of the skycells of the best epochs, I choose the best templates  [[BR]]
    105 
    106  some epochs with small fwhm and moments (in principle good templates) seem to be masked too much  [[BR]]
    107 
    108 [[Image(MD02.skycell.066.stk.36184.unconv.jpg, 400px)]][[BR]]
    109115
    110116* Finally, I'm testing ppSub with the templates selected [[BR]]