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HEASARC: Calibration Database

High Energy Cross-Calibration Information


Targets

Astrophysical objects which have been used for instrument calibration include the following:

ROSAT Calibration Targets

  • N132D, HZ 43, Crab Nebula, AR Lac, the "Meaty" Source (aka RE 1629+781, a white dwarf discovered by the ROSAT WFC, see Pye, 1996, MPE Report 263,627 & Cooke et al., 1992, Nature 355, 61), Vela SNR, Cyg X-2, Cyg X-3, A 2256, LMC X-1, LMC X-2, Cas A, MKN 421, Beta Car, Beta Leo, Vega, GD695, BPM97895, and EG 187, Delta Dor, BETA Aur, EPS Lyr

ASCA Calibration Targets

ASCA has used the following targets for the following purposes:

Swift Calibration Targets for the XRT

These targets are taken from "The in-flight spectroscopic performance of the Swift XRT CCD camera", J. Osborne et al.,
Object Type Mode Purpose Exposure (ks)
RXJ 0720.4-3125 Pulsar PC Low energy response 19.6
RXJ 1856.5-3754 Neutron Star PC Low energy response 5.4
PKS 0745-19 Cluster of galaxies PC Low energy shelf and effective area 29.7
2E 0102-7217 SNR PC
WT
LrPD
Effective area and gain 24.3
25.4
6.0
Cas A SNR PC
WT
Effective area and gain 5.8
45.7
3C 273 Quasar WT Effective area and cross-calibration 10.0
Crab SNR WT
LrPD
Effective area and gain 5.8
25.0
PSR 0540-69 Pulsar PC Effective area 33.9

Suzaku Calibration Targets

Suzaku calibration targets are listed in Table B.1.1 of the Suzaku Technical Description, which is reproduced here: B.1.1 Calibration

Target RA Dec Stat Exp. #obs Remarks
E0102-72 01 04 02.4 -72 01 60.0 Obs 75 2 XIS window open
E0102-72 01 04 02.4 -72 01 60.0   20 1 XIS
N132D 05 25 03.3 -69 38 27.2 Obs 105 6 HXD HV ON
Crab 05 34 32.0 +22 00 52.2 Obs 170 31  
Eta Carina 10 45 03.6 -59 41 04.3   20 1 XIS
Lockman Hole 10 52 00.0 +57 18 00.0   100 1 HXD
North Ecliptic Pole 18 11 12.0 +66 00 0.0 Obs 70 1  
Vega 18 36 56.3 +38 47 01.3 Obs 10 1 Optical light leak check
PKS2155-304 21 58 52.1 -30 13 32.1   60 1 XIS; coordinated obs.
            with XMM-Newton
Cas A 23 23 24.0 +58 48 54.0   10 1 XIS


Documents

Attempts at intercomparison of instrumental performance between 2 (or among 3 or more) observatories, or between multiple instruments on a single observatory.

ASCA

Chandra

XMM-Newton

INTEGRAL


Other Links


Questions/Comments/Problems with the CALDB to: caldbhelp@athena.gsfc.nasa.gov

Page Author: Michael F. Corcoran 1-301-286-5576
Last Update: Wednesday, 11-Feb-2009 14:59:47 EST

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