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Revision 5 as of 2012-06-22 12:39:16
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|| LMXBs ||AR,VD ||||
|| HMXBs ||VD ||||
|| 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||
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|| NSs - Pulsars||VD || || || 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 ||
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|| ULX ||VD || || || ULX ||VD ||version by VD: [[attachment:ulxcat.fits]] based on Swartz et al 2011 ||

Catalogs as input for the eROSITA catalog tool

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: lmxbcat.fits based on Liu et al 2007, and Ritter&Kolb v 7.17

HMXBs

VD

version by VD: hmxbcat.fits based on Liu et al, 2006

BHCs

AR

White Dwarfs

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

NSs - isolated

AP,VD

XDINs, AXPs, SGRs, CCOs, RRATs

ULX

VD

version by VD: ulxcat.fits based on Swartz et al 2011

EROSITAwiki: erocom_catalogs (last edited 2019-08-28 11:55:30 by AxelSchwope)