Differences between revisions 8 and 9
Revision 8 as of 2012-08-08 19:42:06
Size: 1321
Comment:
Revision 9 as of 2013-07-01 08:04:31
Size: 1347
Editor: AxelSchwope
Comment:
Deletions are marked like this. Additions are marked like this.
Line 7: Line 7:
|| SSS || || || ||
|| Novae || FWH, WNP || || ||
|| SSS || ||MPE || ||
|| Novae || FWH, WNP ||MPE? || ||
Line 11: Line 11:
|| Symbiotics || || || || || Symbiotics || || ADS(AIP)|| ||
Line 15: Line 15:
|| White Dwarfs || KW, VB, ADS || || || || White Dwarfs || KW, VB, ADS ||IAAT - TR || ||
Line 17: Line 17:
|| NSs - PWN || || || || || NSs - PWN || || WB|| ||

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

MPE

Novae

FWH, WNP

MPE?

pre-CVs

ADS (AIP)

all known non-resolved WD/dM pairs

AM CVns, UCBs

AR

Symbiotics

ADS(AIP)

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

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)