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. ----------------------------------------------------------------------------------- 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. ----------------------------------------------------------------------------------- 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. ----------------------------------------------------------------------------------- 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. ----------------------------------------------------------------------------------- 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. ----------------------------------------------------------------------------------- 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