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From: | Mohammad Akhlaghi |
Subject: | Re: Regarding astsegment clump detection |
Date: | Thu, 19 Oct 2023 15:42:17 +0200 |
User-agent: | Mozilla Thunderbird |
Hi Chandan,The Segment program doesn't provide semi-major and semi-minor axis measurements, do you mean MakeCatalog's output catalog of Segement's clumps?
The semi-major and semi-minor axises are calculated differently from the FWHM; you can see how they are calculated here:
https://www.gnu.org/software/gnuastro/manual/html_node/Measuring-elliptical-parameters.htmlBut with MakeCatalog, you can also measure the FWHM of clumps using the '--fwhm' option. But be careful with very faint clumps: because even a star that is too close to the noise its "Maximum" (for the half-max of FWHM) can be very noisy; and thus your FWHM measurements will be very noisy in the faint-end.
Regarding your question on the "realistic"-ness of the clumps, a signal-to-noise of 3 sounds pretty non-noisy. But the best way is to use the '--upperlimit-sigma' column/option of MakeCatalog, which will take the clump/object footprint and place it randomly over un-detected parts of the image for a large number of times (you can set the number of random positions to test with the '--upnum' option); it is described more fully in these sections of the manual:
https://www.gnu.org/software/gnuastro/manual/html_node/Upper-limit-magnitude-of-each-detection.html https://www.gnu.org/software/gnuastro/manual/html_node/Brightness-measurements.html Cheers, Mohammad On 10/19/23 14:44, chandan watts wrote:
Hi, Thanks for your reply. Regarding PSF size, this refers to the FWHM of the PSF image of the target. Clump size is determined by the semimajor and semiminor axes provided by the astsegment output. To compare the sizes, I check the diameter of clumps by measuring twice the semiminor axis or semimajor axis and comparing it with the FWHM of the PSF image. The objective is to ensure that the clumps detected should have a diameter greater than the FWHM of the PSF image for the photometric calculations. However, astsegment is detecting most of the clumps with diameters less than FWHM. Also, I want to mention that I detected these clumps for very faint signals, and astsegment signal-to-noise output varies for these from ~3 - 8. Can these clumps be considered as realistic or not? Regards, Chandan
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