The cosmic X-ray background level at its emission peak

被引:0
作者
Frontera, F. [1 ,2 ]
Orlandini, M. [2 ]
机构
[1] Univ Ferrara, Dipartimento Fis, I-44100 Ferrara, Italy
[2] INAF IASF Bologna, I-40129 Bologna, Italy
来源
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS | 2007年 / 122卷 / 12期
关键词
D O I
10.1393/ncb/i2008-10480-3
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We discuss an accurate measurement of the CXB in the 15-50 keV range performed with the Phoswich Detection System. (PDS) instrument aboard the BeppoSAX satellite, whose results have already been recently reported elsewhere (Frontera F. et al., Astrophys. J., 666 (2007) 86). Unlike the recently reported 2-10keV CXB measurements obtained with the imaging instruments aboard the X-ray satellites BeppoSAX, XMM-Newton, and Chandra that give CXB intensities systematically higher than those obtained with HEAO-I, using the BeppoSAX PDS pointings at high galactic latitude (vertical bar b vertical bar > 15 degrees) we measure a CXB spectrum and intensity level in the 15-50 keV energy band, which are consistent with those obtained with HEAO-1. Astrophysical consequences are discussed.
引用
收藏
页码:1365 / 1369
页数:5
相关论文
共 16 条
  • [1] BeppoSAX, the wide band mission for X-ray astronomy
    Boella, G
    Butler, RC
    Perola, GC
    Piro, L
    Scarsi, L
    Bleeker, JAM
    [J]. ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (02): : 299 - 307
  • [2] COMASTRI A, 1995, ASTRON ASTROPHYS, V296, P1
  • [3] COMASTRI A, 2007, 07111356 ARXIV
  • [4] COMASTRI A, 2006, ASTRO NACHR, V711, P789
  • [5] The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton
    De Luca, A
    Molendi, S
    [J]. ASTRONOMY & ASTROPHYSICS, 2004, 419 (03): : 837 - 848
  • [6] The cosmic X-ray background and the population of the most heavily obscured agns
    Frontera, Filippo
    Orlandini, Mauro
    Landi, Raffaella
    Comastri, Andrea
    Fiore, Fabrizio
    Setti, Giancarlo
    Amati, Lorenzo
    Costa, Enrico
    Masetti, Nicola
    Palazzi, Eliana
    [J]. ASTROPHYSICAL JOURNAL, 2007, 666 (01) : 86 - 95
  • [7] The X-ray background and the deep X-ray surveys
    Gilli, R
    [J]. NEW X-RAY RESULTS, THE NEXT GENERATION OF X-RAY OBSERVATORIES AND GAMMA RAY BURST AFTERGLOW PHYSICS, 2004, 34 (12): : 2470 - 2477
  • [8] The spectrum of diffuse cosmic hard X-rays measured with HEAO 1
    Gruber, DE
    Matteson, JL
    Peterson, LE
    Jung, GV
    [J]. ASTROPHYSICAL JOURNAL, 1999, 520 (01) : 124 - 129
  • [9] Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 kev band with Chandra
    Hickox, Ryan C.
    Markevitch, Maxim
    [J]. ASTROPHYSICAL JOURNAL, 2006, 645 (01) : 95 - 114
  • [10] Horstman H. M., 1975, Rivista del Nuovo Cimento, V5, P255, DOI 10.1007/BF02747042