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=== Catalogs as input for the eROSITA catalog tool ===

|| '''OBJECT CLASS''' || '''Science''' || '''Catalogs''' || '''comment''' ||
|| CVs || ADS, IT, VB, RSC, AR || ADS(AIP) || known CVs and candidates with and without orbital periods [[attachment:cv_master_2019jul.fits]]||
|| pre-CVs || || ADS (AIP) || all known non-resolved WD/dM pairs ||
|| SSS || ||MPE || ||
|| Novae || FWH, WNP ||MPE? || ||
|| AM CVns, UCBs ||AR || AR ||||
|| Symbiotics || || ADS(AIP)|| ||
|| LMXBs || ASa, SP, LD, TT ||VD ||version by VD: [[attachment:lmxbcat.fits]] based on Liu et al 2007, and Ritter&Kolb v 7.17||
|| HMXBs || DK, IK, LD, ASa, FWH ||VD ||version by VD: [[attachment:hmxbcat.fits]] based on Liu et al, 2006||
|| BHCs  || JW, WNP, FWH, AR ||AR ||||
|| White Dwarfs || KW, VB, ADS ||IAAT - TR || ||
|| NSs - Pulsars || ||VD ||version by VD: [[attachment:atnf.fits]] based on ATNF catalogue. Includes also PWN pulsars and isolated NSs (most). X-ray fluxes are only estimates (based spin/dot as done in Vink et al, 2011). NS classes are quoted according to HEASARC (limited), so difficult to select subsets of NSs ||
|| NSs - PWN || || WB|| ||
|| NSs - isolated || WB, FWH, MS, GP, ASa, VD, AP, ADS, TP, TT || AP,VD,DK || XDINs, AXPs, SGRs, CCOs, RRATs ||
|| ULX || ||VD ||version by VD: [[attachment:ulxcat.fits]] based on Swartz et al 2011 ||