Strong lensing of tidal disruption events: Detection rates in imaging surveys
	K. Szekerczes, T. Ryu, S. H. Suyu, S. Huber, M. Oguri, L. Dai

arXiv:2402.03443

Summary: The unlensed and strongly lensed tidal disruption event (TDE) catalogs 
at the fiducial temperature of T = 20,000 K for the L1 and L2 luminosity models 
separately. The L1 luminosity model is an observationally driven upper limit 
defined by 1% of stellar fallback material turning into radiation. The L2 
luminosity model is defined by self-crossing shocks of stellar debris. Each line of 
a file represents a TDE (unlensed or lensed), so to compute the TDE detection rate
one would need to iterate through the entire file, sum over the TDE weighting 
factors, apply magnitude cuts according to the desired survey limit and then 
normalize by any oversampling factors (only relevant for lensed catalogs). These 
catalogs assume a survey area of 20,000 deg^2; no magnitude cuts have been 
applied, so one can choose a limiting survey magnitude. 

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Notes for all files: the weighting of each TDE needs to be accounted for post-
processing, and 'band' in the file name can be either u, g, r, or i.


Description of file: unlensed_L1_band_weighted.txt
Explanation: The catalog of unlensed TDEs at a temperature of T = 20,000 K 
following the L1 luminosity model assuming a survey area of 20,000 deg^2 and one 
year of observation.
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Column		Units			Description
1.		mag			Unlensed TDE magnitude
2. 		--			TDE redshift
3. 		erg/s			TDE model L1 luminosity 
4. 		K			TDE temperature
5. 		solar masses		Black hole mass
6. 		mag			Eddington limited magnitude (adjusted 
					magnitude calculated if L1 > L_edd)
7. 		erg/s			Eddington limited luminosity (L_new = L_edd 
					if L_new > L_edd, L_new = L1 if 
					L_new <= L_edd)
8. 		erg/s			Eddington luminosity
9.		--			TDE post-processing weighting factor


Description of file: unlensed_L2_band_weighting.txt
Explanation: The catalog of unlensed TDEs at a temperature of T = 20,000 K 
following the L2 luminosity model assuming a survey area of 20,000 deg^2 and one 
year of observation. 
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Column		Units			Description
1.		mag			Unlensed TDE magnitude
2. 		--			TDE redshift
3.		erg/s			TDE model L2 luminosity
4. 		K			TDE temperature
5. 		solar masses		Black hole mass
6.		--			TDE post-processing weighting factor


Description of file: lensed_L1_band_catalog.txt
Explanation: The catalog of strongly lensed TDEs at a temperature of T = 20,000 K 
following the L1 luminosity model assuming a survey area of 20,000 deg^2 and one 
year of observation. This catalog has been oversampled by a factor of 1,000.
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Column		Units			Description
1. 		--			Number of images
2.		--			Lens redshift
3.		km/s			Velocity dispersion
4.		--			TDE redshift
5.		mag			Unlensed TDE magnitude
6. 		mag			Lensed TDE magnitude
7. 		arcsec			Image Separation
8. 		erg/s			TDE model L1 luminosity
9. 		solar masses		Black hole mass
10. 		--			Magnification
11.		days			Time delays for all images
12. 		mag			Eddington limited unlensed magnitude 
					(adjusted unlensed magnitude calculated 
					if L1 > L_edd)
13. 		mag			Eddington limited lensed magnitude 
					(adjusted lensed magnitude calculated if 
					L1 > L_edd)
14. 		erg/s			Eddington limited luminosity (L_new = L_edd 
					if L1 > L_edd, L_new = L1 if L1 <= L_edd)
15. 		erg/s			Eddington luminosity
16. 		--			TDE post-processing weighting factor		


Description of file: lensed_L2_band_catalog.txt
Explanation: The catalog of strongly lensed TDEs at a temperature of T = 20,000 K 
following the L2 luminosity model assuming a survey area of 20,000 deg^2 and one 
year of observation. This catalog has been oversampled by a factor of 1,000.
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Column		Units			Description
1. 		--			Number of images
2.		--			Lens redshift
3.		km/s			Velocity dispersion
4.		--			TDE redshift
5.		mag			Unlensed TDE magnitude
6. 		mag			Lensed TDE magnitude
7. 		arcsec			Image Separation
8. 		erg/s			TDE model L2 luminosity
9. 		solar masses		Black hole mass
10. 		--			Magnification
11.		days			Time delays for all images
12. 		--			TDE post-processing weighting factor








