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|| '''OBJECT CLASS''' || '''WHO''' || '''comment''' || || CVs || ADS(AIP) || known CVs and candidates with and without orbital periods || || SSS || || || || Novae || || || || pre-CVs || ADS (AIP) || all known non-resolved WD/dM pairs || || AM CVns, UCBs || AR |||| || Symbiotics || || || || LMXBs ||AR,VD ||version by VD: [[attachment:lmxbcat.fits]] based on Liu et al 2007, and Ritter&Kolb v 7.17|| || HMXBs ||VD ||version by VD: [[attachment:hmxbcat.fits]] based on Liu et al, 2006|| || BHCs ||AR |||| || White Dwarfs || || || || 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 || || || || NSs - isolated || AP,VD || XDINs, AXPs, SGRs, CCOs, RRATs || || ULX ||VD ||version by VD: [[attachment:ulxcat.fits]] based on Swartz et al 2011 || |
|| '''OBJECT CLASS''' || '''Science''' || '''Catalogs''' || '''comment''' || || CVs || ADS, IT, VB, RSC, AR || ADS(AIP) || known CVs and candidates with and without orbital periods || || SSS || || || || || Novae || FWH, WNP || || || || pre-CVs || || ADS (AIP) || all known non-resolved WD/dM pairs || || AM CVns, UCBs || || AR |||| || Symbiotics || || || || || LMXBs || ASa, SP, LD, TT ||AR,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 || || || || 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 || || || || || NSs - isolated || WB, FWH, MS, GP, ASa, VD, AP, ADS, TP, TT || AP,VD || XDINs, AXPs, SGRs, CCOs, RRATs || || ULX || ||VD ||version by VD: [[attachment:ulxcat.fits]] based on Swartz et al 2011 || |
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 |
SSS |
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|
|
Novae |
FWH, WNP |
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|
pre-CVs |
|
ADS (AIP) |
all known non-resolved WD/dM pairs |
AM CVns, UCBs |
|
AR |
|
Symbiotics |
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|
LMXBs |
ASa, SP, LD, TT |
AR,VD |
version by VD: lmxbcat.fits based on Liu et al 2007, and Ritter&Kolb v 7.17 |
HMXBs |
DK, IK, LD, ASa, FWH |
VD |
version by VD: hmxbcat.fits based on Liu et al, 2006 |
BHCs |
JW, WNP, FWH, AR |
AR |
|
White Dwarfs |
KW, VB, ADS |
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|
NSs - Pulsars |
|
VD |
version by VD: 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 |
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|
|
NSs - isolated |
WB, FWH, MS, GP, ASa, VD, AP, ADS, TP, TT |
AP,VD |
XDINs, AXPs, SGRs, CCOs, RRATs |
ULX |
|
VD |
version by VD: ulxcat.fits based on Swartz et al 2011 |