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Images are all of the same scale. | Images are all of the same scale. | ||
- | First row: (1) original image of saturated star centered | + | First row: (1,2,3) original image of saturated star centered |
Second row: (1) PSF bmodel subtracted from saturated star; (2) PSF bmodel normalized to the maximum flux value of saturated star and then subtracted; (3) PSF bmodel normalized to the flux above 60000ADU that is limiting (black area is a consequence of over subtraction but spikes clearly appear) | Second row: (1) PSF bmodel subtracted from saturated star; (2) PSF bmodel normalized to the maximum flux value of saturated star and then subtracted; (3) PSF bmodel normalized to the flux above 60000ADU that is limiting (black area is a consequence of over subtraction but spikes clearly appear) | ||
- | [[Image:original.png|330px]] | + | [[Image:original.png|330px]][[Image:original.png|330px]][[Image:original.png|330px]] |
[[Image:psf_sub.png|330px]][[Image:psf_sub_norm_max.png|330px]][[Image:psf_sub_norm_105000.png|330px]] | [[Image:psf_sub.png|330px]][[Image:psf_sub_norm_max.png|330px]][[Image:psf_sub_norm_105000.png|330px]] |
Revision as of 19:21, 11 January 2021
Contents |
Stars
# Faint stars (19<=g<22): 41 in total. Median combined. Inner profile R[pix]<9, outer profile R[pix]< 200 and curve-of-growth up to 250 pix
# Bright stars (16<=g<19): 52 in total. Median combined. Inner profile R[pix]<9, outer profile R[pix]< 200 and curve-of-growth up to 250 pix
# Saturated stars (g<16): 29 in total.Median combined. Inner profile R[pix]<9, outer profile R[pix]< 200 and curve-of-growth up to 250 pix
# PSF created by average combining and scaling to the median bright, faint and saturated star: inner profile R[pix]<9, outer profile R[pix]< 200 and curve-of-growth up to 250 pix
Images in the 1st row: faint, bright and saturated star
Each image is 501 x 501 pix large ~ 200 arcsec x 200 arcsec (radius ~ 100 arcsec). Radial profiles and curve-of-growths given above.
Final PSF by average combining previous three images and scaled to median
Central part of the saturated star masked during combining.
Joining stars
Points from SMA>10 & SMA < 20 are used to create an overlap region for fitting: (1) inner region of saturated star is replaced by bright, unsaturated star; (2) full extent of the PSF
Testing PSF
Images are all of the same scale.
First row: (1,2,3) original image of saturated star centered
Second row: (1) PSF bmodel subtracted from saturated star; (2) PSF bmodel normalized to the maximum flux value of saturated star and then subtracted; (3) PSF bmodel normalized to the flux above 60000ADU that is limiting (black area is a consequence of over subtraction but spikes clearly appear)