Differences between revisions 12 and 13
Revision 12 as of 2013-07-01 08:13:44
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Editor: AxelSchwope
Comment:
Revision 13 as of 2014-09-08 13:58:10
Size: 1346
Editor: ArneRau
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Deletions are marked like this. Additions are marked like this.
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|| AM CVns, UCBs || || AR |||| || AM CVns, UCBs ||AR || AR ||||
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|| 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|| || LMXBs || ASa, SP, LD, TT ||VD ||version by VD: [[attachment:lmxbcat.fits]] based on Liu et al 2007, and Ritter&Kolb v 7.17||

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

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: 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

IAAT - TR

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

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: ulxcat.fits based on Swartz et al 2011

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