IACHEC CROSS-CALIBRATION OF CHANDRA, NuSTAR, SWIFT, SUZAKU, XMM-NEWTON WITH 3C 273 ANDPKS 2155-304

被引：107

作者：

Madsen, Kristin K. ^{[1
]}

Beardmore, Andrew P. ^{[2
]}

Forster, Karl ^{[1
]}

Guainazzi, Matteo ^{[3
,5
]}

Marshall, Herman L. ^{[4
]}

Miller, Eric D. ^{[4
]}

Page, Kim L. ^{[2
]}

Stuhlinger, Martin ^{[5
]}

机构：

[1] CALTECH, Cahill Ctr Astron & Astrophys, Pasadena, CA 91125 USA

[2] Univ Leicester, Dept Phys & Astron, Xray & Observat Astron Grp, Leicester LE1 7RH, Leics, England

[3] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525201, Japan

[4] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA

[5] ESAC, POB 78, E-28691 Madrid, Spain

来源：

ASTRONOMICAL JOURNAL | 2017年 / 153卷 / 01期

基金：

美国国家航空航天局;

关键词：

space vehicles: instruments; OBJECT PKS 2155-304; X-RAY TELESCOPE; GALAXY CLUSTERS; VARIABILITY; 3C-273; EMISSION; JET; ABSORPTION; ABUNDANCES; SECTIONS;

D O I：

10.3847/1538-3881/153/1/2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

On behalf of the International Astronomical Consortium for High Energy Calibration, we present results from the cross-calibration campaigns in 2012 on 3C 273 and in 2013 on PKS 2155-304 between the then active X-ray observatories Chandra, NuSTAR, Suzaku, Swift, and XMM-Newton. We compare measured fluxes between instrument pairs in two energy bands, 1-5 keV and 3-7 keV, and calculate an average cross-normalization constant for each energy range. We review known cross-calibration features and provide a series of tables and figures to be used for evaluating cross-normalization constants obtained from other observations with the above mentioned observatories.

引用

页数：17

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