메뉴 건너뛰기




Volumn 546, Issue , 2012, Pages

Constraining the fraction of Compton-thick AGN in the Universe by modelling the diffuse X-ray background spectrum

Author keywords

X rays: diffuse background; X rays: general

Indexed keywords

ACTIVE GALACTIC NUCLEI; CONFIDENCE LEVELS; DENSE MEDIUM; DIRECT DETECTION; HIGH ENERGY; INPUT PARAMETER; MONTE CARLO SIMULATION; NUMBER DENSITY; POWER LAW INDEX; RED SHIFT; REFLECTION COMPONENTS; SYNTHESIS CODE; X RAY PHOTONS; X-RAY BACKGROUND; X-RAY MISSION; X-RAY SPECTRA; X-RAYS: DIFFUSE BACKGROUND; X-RAYS: GENERAL;

EID: 84867386523     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219387     Document Type: Article
Times cited : (153)

References (74)
  • 23
    • 46649116298 scopus 로고    scopus 로고
    • Dadina, M. 2008, A&A, 485, 417
    • (2008) A&A , vol.485 , pp. 417
    • Dadina, M.1
  • 41
    • 84867363844 scopus 로고    scopus 로고
    • AAS/High Energy Astrophysics Division #11
    • Harrison, F., Boggs, S., Christensen, F., et al. 2010, in AAS/High Energy Astrophysics Division #11, BAAS, 42, 737
    • (2010) BAAS , vol.42 , pp. 737
    • Harrison, F.1    Boggs, S.2    Christensen, F.3
  • 42
    • 54949121440 scopus 로고    scopus 로고
    • Hasinger, G. 2008, A&A, 490, 905
    • (2008) A&A , vol.490 , pp. 905
    • Hasinger, G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.