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Volumn 58, Issue 6, 1998, Pages

Data analysis of gravitational-wave signals from spinning neutron stars: The signal and its detection

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Indexed keywords


EID: 0542418905     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.063001     Document Type: Article
Times cited : (791)

References (44)
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    • Our functions (Formula presented) and (Formula presented) from Eqs. (12) and (13) are connected with the functions (Formula presented) and (Formula presented) from Eqs. (9) and (10) of 19 is made (assuming (Formula presented) The last identification means that the angle ψ is measured clockwise from the first interferometer’s arm to north.
    • Our functions (Formula presented) and (Formula presented) from Eqs. (12) and (13) are connected with the functions (Formula presented) and (Formula presented) from Eqs. (9) and (10) of 19 is made (assuming (Formula presented) The last identification means that the angle ψ is measured clockwise from the first interferometer’s arm to north.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.