| 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 | |
| | 30 | Here 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:''' |
| | 48 | the unconvolved images have more detections (but probably several of them are not real) |
| | 49 | the FWHM of the objects is degraded in the convolved image (probably too much in some skycells) |
| | 50 | To investigate the quality of stacks and select good templates, I used the fwhm and moments values of the unconvnolved images.[[BR]] |
| | 51 | |
| | 52 | The 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]] |
| | 63 | Good nights from which we can probably take the template stacks are reported below: [[BR]] |
| 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]] |