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  1. 学術雑誌論文
  2. 4 自然科学

Inferred Measurements of the Zodiacal Light Absolute Intensity through Fraunhofer Absorption Line Spectroscopy with CIBER

http://hdl.handle.net/10228/00009071
http://hdl.handle.net/10228/00009071
1e6cedf8-4bc1-488d-9e4e-b75733325d33
名前 / ファイル ライセンス アクション
LaSEINE-2021_039.pdf LaSEINE-2021_039.pdf (2.5 MB)
アイテムタイプ 学術雑誌論文 = Journal Article(1)
公開日 2023-02-03
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
タイトル
タイトル Inferred Measurements of the Zodiacal Light Absolute Intensity through Fraunhofer Absorption Line Spectroscopy with CIBER
言語 en
言語
言語 eng
著者 Korngut, P. M.

× Korngut, P. M.

WEKO 34616

en Korngut, P. M.

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Kim, M. G.

× Kim, M. G.

WEKO 34617

en Kim, M. G.

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Arai, T.

× Arai, T.

WEKO 34618

en Arai, T.

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Bangale, P.

× Bangale, P.

WEKO 34619

en Bangale, P.

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Bock, J.

× Bock, J.

WEKO 34620

en Bock, J.

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Cooray, A.

× Cooray, A.

WEKO 34621

en Cooray, A.

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Cheng, Y. T.

× Cheng, Y. T.

WEKO 34622

en Cheng, Y. T.

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Feder, R.

× Feder, R.

WEKO 34623

en Feder, R.

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Hristov, V.

× Hristov, V.

WEKO 34624

en Hristov, V.

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Lanz, A.

× Lanz, A.

WEKO 34625

en Lanz, A.

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Lee, D. H.

× Lee, D. H.

WEKO 34626

en Lee, D. H.

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Levenson, L.

× Levenson, L.

WEKO 34627

en Levenson, L.

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Matsumoto, T.

× Matsumoto, T.

WEKO 34628

en Matsumoto, T.

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Matsuura, S.

× Matsuura, S.

WEKO 34629

en Matsuura, S.

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Nguyen, C.

× Nguyen, C.

WEKO 34630

en Nguyen, C.

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佐野, 圭

× 佐野, 圭

WEKO 31407
e-Rad 70802908
Scopus著者ID 56708069700
ORCiD 0000-0002-6468-8532
九工大研究者情報 100001400

en Sano, Kei

ja 佐野, 圭

ja-Kana サノ, ケイ


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Tsumura, K.

× Tsumura, K.

WEKO 34632

en Tsumura, K.

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Zemcov, M.

× Zemcov, M.

WEKO 34633

en Zemcov, M.

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抄録
内容記述タイプ Abstract
内容記述 Scattered sunlight from the interplanetary dust (IPD) cloud in our solar system presents a serious foreground challenge for spectrophotometric measurements of the extragalactic background light (EBL). In this work, we report on inferred measurements of the absolute intensity of the zodiacal light (ZL) using the novel technique of Fraunhofer line spectroscopy on the deepest 8542 Å line of the near-infrared Ca ii absorption triplet. The measurements are performed with the narrow band spectrometer (NBS) on board the Cosmic Infrared Background Experiment sounding rocket instrument. We use the NBS data to test the accuracy of two ZL models widely cited in the literature, the Kelsall and Wright models, which have been used in foreground removal analyses that produce high and low EBL results respectively. We find a mean reduced χ2 = 3.5 for the Kelsall model and χ2 = 2.0 for the Wright model. The best description of our data is provided by a simple modification to the Kelsall model, which includes a free ZL offset parameter. This adjusted model describes the data with a reduced χ2 = 1.5 and yields an inferred offset amplitude of 46 ± 19 nW m−2 sr−1 extrapolated to 12500 Å. These measurements elude to the potential existence of a dust cloud component in the inner solar system whose intensity does not strongly modulate with the Earth's motion around the Sun.
言語 en
書誌情報 en : Astrophysical Journal

巻 926, 号 2, p. 133-1-133-15, 発行日 2022-02-18
出版社
出版者 IOP Publishing
言語 en
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/1538-4357/ac44ff
日本十進分類法
主題Scheme NDC
主題 440
ISSN
収録物識別子タイプ EISSN
収録物識別子 1538-4357
ISSN
収録物識別子タイプ PISSN
収録物識別子 0004-637X
著作権関連情報
権利情報Resource http://creativecommons.org/licenses/by/4.0/
権利情報 Copyright (c) 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
査読の有無
値 yes
連携ID
値 10866
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