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Photometric catalogs with bagpipes output used to compute SMFs in 
https://ui.adsabs.harvard.edu/abs/2024arXiv240308872W/abstract

Please cite this paper when using the catalogs.

The catalog contains the following columns, where <fil> stands for the respective filter keys in lowercase letters (e.g. f444w):

id                          n/a                 identification number from the original SExtractor run
ra                          deg                 right ascension (J2000)
dec                         deg                 declination (J2000)
x_image                     pixel               centroid x-position of the object (SExtractor)
y_image                     pixel               centroid y-position of the object (SExtractor)
a_image                     pixel               isophotal image major axis (SExtractor)
b_image                     pixel               isophotal image minor axis (SExtractor)
theta_image                 deg                 isophotal image position angle (SExtractor)
kron_radius                 n/a                 Kron radius in units of A or B (SExtractor)
sn_lw_det_img	    	    n/a			S/N in the LW detection image (inverse variance weighted F277W+F356W+F444W stack)
aper_corr                   n/a                 aperture correction factor derived from F444W and applied to all bands (see above)
enclosed_flux_fraction      n/a			fraction of energy encircled by the Kron-ellipse in the F444W PSF. To get the total 
                                                correction applied to the aperture fluxes, use aper_corr / enclosed_flux_fraction

class_star_<fil>	    n/a	                CLASS_STAR parameter (SExtractor) in <fil> (only for NIRCam wide filters), 
						value between 0 and 1 specifying the probability that the object is a star 
					        (use with caution)
faper_<fil>		    nJy			flux in <fil> measured in a circular aperture of radius 0.16"
eaper_<fil>		    nJy		        error in the aperture flux
f_<fil>		            nJy		        aperture-corrected, psf-matched flux in <fil>
e_<fil>			    nJy			error in the aperture-corrected, psf-matched flux in <fil>, with a 5% error floor
sn_<fil>		    n/a			signal-to-noise ratio in <fil> before applying the 5% error floor
r50_<fil>		    pixel		radius containing 50% of the flux in <fil> (SExtractor)

sn_flag			    binary		1, if the corresponding source has S/N < 3 in ALL the NIRCam wide filters F115W, F150W, 
					        F200W, F277W, F356W and F444W

flag_<fil>		    binary		1, if the corresponding source is flagged in <fil>, in this case f_<fil> = e_<fil> = -99		
c_<fil>			    n/a			compactness parameter f(D=0.4") / f(D=0.2") for LRD selection

z_phot_eazy                 n/a                 best-fit photometric redshift from eazy (peak of the PDF)
z_phot_160_eazy             n/a                 16th percentile of the redshift PDF (eazy)
z_phot_840_eazy             n/a                 84th percentile of the redshift PDF (eazy)
z_phot_chi2_eazy            n/a                 chi^2 of the best-fit photometric redshift (eazy)
f_restU_eazy                nJy                 restframe U-flux (eazy)
e_restU_eazy                nJy                 error in the restframe U-flux (eazy)
f_restB_eazy                nJy                 restframe B-flux (eazy)
e_restB_eazy                nJy                 error in the restframe B-flux (eazy)
f_restV_eazy                nJy                 restframe V-flux (eazy)
e_restV_eazy                nJy                 error in the restframe V-flux (eazy)
f_restJ_eazy                nJy                 restframe J-flux (eazy)
e_restJ_eazy                nJy                 error in the restframe J-flux (eazy)
Lv_eazy			    L_sun	        V-band luminosity (eazy)
Av_eazy			    mag		        extinction in V-band (eazy)
m_star_eazy		    M_sun		stellar mass (eazy)
m_star_160_eazy	            M_sun		16th percentile of the stellar mass (eazy)
m_star_840_eazy		    M_sun		84th percentile of the stellar mass (eazy)
sfr_eazy	            M_sun/yr		star formation rate (eazy)
sfr_160_eazy	            M_sun/yr		16th percentile of the star formation rate (eazy)
sfr_840_eazy	            M_sun/yr		84th percentile of the star formation rate (eazy)
chi2_eazy_phoenix_stars	    n/a			Chi^2 of the eazy fit using phoenix star templates
stellar_flag		    binary		if 1, the source is likely a star, diffraction spike or contaminated by stellar light
hugekron_flag		    binary		if 1, R50(F444W) > 50 pix or r_kron,red > 150 pix
nofit_flag		    binary		if 1, eazy did not return a reasonable fit for this source (best-fit redshift -1 or 19.9)
junk_flag		    binary		if 1, R_50(F444W) < 1.2 and mag(F444W) < 28.5
use_phot		    binary		if 1, the source is likely a galaxy with reliable photometry (see above)

Additional columns are direct output from bagpipes which we run with the settings described in Section 2.4 of the paper.

See the bagpipes documentation for more information: https://bagpipes.readthedocs.io/en/latest/

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