Changes between Version 43 and Version 44 of Durham_MDS_Testing
- Timestamp:
- Aug 19, 2009, 12:19:19 AM (17 years ago)
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Durham_MDS_Testing
v43 v44 72 72 Here is a comparison of the PSFmags from the cmf files of four adjacent (arbitrarily chosen) MD07 stacks with SDSS model mags (r,g,i and z, as labelled). Blue indicates an object flagged as a star by SDSS. I haven't rejected any images flagged as defective in any way, so this probably explains the blue points offset by 2 mags. UPDATE: looks like these offset points are stars with masked centres - note that there are brighter stars which are not masked. Is this the 'removing intermediate brightness stars as cosmic rays' problem again? It appears particularly bad on r cells 40 and 52. 73 73 74 Clearly the zero-point varies from cell to cell (do we expected this? after all, no calibration has been done as far as I can tell ). The r-band stellar locus also appears tighter in cell 41 than in the other r-band cells. As the are no extended source magnitudes in the cmf files, all the galaxies (black open circles) are offset.74 Clearly the zero-point varies from cell to cell (do we expected this? after all, no calibration has been done as far as I can tell - '''YES''' ''the zero point depends on the number of warps which went into the stack''). The r-band stellar locus also appears tighter in cell 41 than in the other r-band cells. As the are no extended source magnitudes in the cmf files, all the galaxies (black open circles) are offset. 75 75 76 76 [[Image(MD07_rband_sdss_v2.jpg, 600px)]] [[Image(MD07_gband_sdss.jpg, 600px)]] … … 78 78 [[Image(MD07_iband_sdss.jpg, 600px)]] [[Image(MD07_zband_sdss.jpg, 600px)]] 79 79 80 Update: I have now done the SDSS comparisons for all the MD0 7 stacked skycells. Here are the histograms of the zero-point distributions. Outliers havebeen clipped before determining the mean and rms.80 Update: I have now done the SDSS comparisons for all the MD08 stacked skycells. Here are the histograms of the instrumental zero-point distributions, corrected for the number of warps which went into each skycell. In z, one outlier has been clipped before determining the mean and rms. 81 81 82 [[Image(md0 7_r_zp.jpg,400px)]] [[Image(md07_g_zp.jpg,400px)]]82 [[Image(md08_r_zp.jpg,400px)]] [[Image(md08_g_zp.jpg,400px)]] 83 83 84 [[Image(md0 7_i_zp.jpg,400px)]] [[Image(md07_z_zp.jpg,400px)]]84 [[Image(md08_i_zp.jpg,400px)]] [[Image(md08_z_zp.jpg,400px)]] 85 85 86 I have now done MD08. The (clipped) means of all skycells are: 86 g 33.63 +/- 0.05 87 87 88 g 33.61 +/- 0.06 88 r 34.16 +/- 0.04 89 89 90 r 34.13 +/- 0.07 90 i 33.93 +/- 0.06 91 91 92 i 33.90 +/- 0.05 92 z 33.59 +/- 0.06 (cell 074 with a zp of 35.2 has been excluded) 93 93 94 z 33.58 +/- 0.04 95 96 The file attachment:md07_stack_zeropoints lists the zero points for each skycell in g,r,i and z. attachment:md08_stack_zeropoints is the version for MD08. 94 The file attachment:md08_stack_zeropoints lists the zero points for each skycell in g,r,i and z, both before and after correction for the number of warps. 97 95 98 96 == zeropoints in stacked frames == #zeropoints-stacked 99 97 100 I have measured the zeropoints from the MD07/08 stacks, from comparing IPP cmf uncalibrated PSF mags with SDSS 98 Using the data above, I have measured the zeropoints per second from the MD07/08 stacks, presuming 19, 25, 20 & 24 warps went into the g,r,i & z stacks respectively (these numbers came from the dbinfo files for each stack). 101 99 102 100 ||filter||MD07||MD08|| 103 ||g|| 24.46||24.42||104 ||r|| 24.68||24.71||105 ||i|| 24.70||24.70||106 ||z|| 24.18||24.23||101 ||g|| ||24.48|| 102 ||r|| ||24.71|| 103 ||i|| ||24.73|| 104 ||z|| ||24.19|| 107 105 108 These are all slightly brighter (0.05-0.1) than [wiki:GPC_Zero_Points_July09 Eddie Schlafly's values]. There will be correction (of the right sign) for light missing outside the IPP PSF though.106 Apart from the i-band, these are all slightly brighter (0.05-0.1) than [wiki:GPC_Zero_Points_July09 Eddie Schlafly's values]. There will be correction (of the right sign) for light missing outside the IPP PSF though (''Eugene says this should affect both sets of measurements''). 109 107 110 108 --Nigel
