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  1. 010 学術雑誌論文
  2. 池内, 了 / IKEUCHI, Satoru

Galaxy structures and external perturbations in gravitational lenses

https://ir.soken.ac.jp/records/3293
https://ir.soken.ac.jp/records/3293
581ddf0e-2cdd-42b2-a80c-9261429010cb
名前 / ファイル ライセンス アクション
56022559.pdf 56022559 (119.9 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2012-12-13
タイトル
タイトル Galaxy structures and external perturbations in gravitational lenses
タイトル
言語 en
タイトル Galaxy structures and external perturbations in gravitational lenses
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
著者 KAWANO, Yozo

× KAWANO, Yozo

WEKO 740

KAWANO, Yozo

Search repository
OGURI, Masamune

× OGURI, Masamune

WEKO 741

OGURI, Masamune

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MATSUBARA, Takahiko

× MATSUBARA, Takahiko

WEKO 742

MATSUBARA, Takahiko

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IKEUCHI, Satoru

× IKEUCHI, Satoru

WEKO 734

IKEUCHI, Satoru

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著者別名 池内, 了

× 池内, 了

WEKO 738
NRID 1000090025461
e-Rad 90025461

池内, 了

Search repository
抄録
内容記述タイプ Abstract
内容記述 In modeling strong gravitational lens systems, one often adopts simple models, such as singular isothermal elliptical density plus lowest-order external perturbation. However, such simple models may mislead us if the real mass distribution is more complicated than that in the assumed models. In particular, assumptions on mass models are crucial in studying flux ratio anomalies that have been suggested as evidence for a cold dark-matter substructure. We reinvestigated four quadruple lens systems using power-law Fourier models, which have advantages of clear physical meanings and the applicability of a linear method, as well as a simple singular isothermal elliptical density model. We also investigated the effect of external perturbations, including a singular isothermal sphere, lowest-order expansion, and next-order expansion. We have found that the $\cos3\theta$ terms of the primary galaxy and/or of external perturbation significantly reduce the \chi^2 in PG 1115+080 and B1422+231. In particular, we could reproduce the flux ratios of B1422+231 with next-order external perturbation assuming 5% flux uncertainties, suggesting that external perturbation cannot be described by a simple singular isothermal sphere approximation. On the other hand, we could not fit B0712+472 and B2045+265 very well even with our models, although the \chi^2 were reduced compared with the case of using simple models. Our results clearly demonstrate that both the primary lens galaxy and the external perturbation are often more complicated than we usually assume.
書誌情報 Publications of the Astronomical Society of Japan
en : Publications of the Astronomical Society of Japan

巻 56, 号 2, p. 253-260, 発行日 2004
ISSN
収録物識別子タイプ ISSN
収録物識別子 00046264
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1093/pasj/56.2.253
関連名称 10.1093/pasj/56.2.253
権利
権利情報 © Y. Kawano et al.
関連サイト
識別子タイプ URI
関連識別子 http://arxiv.org/help/general
関連名称 Copyright
フォーマット
内容記述タイプ Other
内容記述 application/pdf
著者版フラグ
出版タイプ AM
出版タイプResource http://purl.org/coar/version/c_ab4af688f83e57aa
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