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    GALACTIC EXTINCTION AND REDDENING FROM THE SOUTH GALACTIC CAP u -BAND SKY SURVEY: u -BAND GALAXY NUMBER COUNTS AND u − r COLOR DISTRIBUTION

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    Author
    Li, Linlin cc
    Shen, Shiyin cc
    Hou, Jinliang
    Yuan, Fangting
    Zhong, Jing cc
    Zou, Hu cc
    Zhou, Xu
    Jiang, Zhaoji
    Peng, Xiyan
    Fan, Dongwei
    Fan, Xiaohui cc
    Fan, Zhou cc
    He, Boliang
    Jing, Yipeng
    Lesser, Michael
    Li, Cheng cc
    Ma, Jun cc
    Nie, Jundan
    Wang, Jiali
    Wu, Zhenyu
    Zhang, Tianmeng
    Zhou, Zhimin
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Issue Date
    2017-01-30
    Keywords
    dust
    extinction
    methods: statistical
    techniques: photometric
    
    Metadata
    Show full item record
    Publisher
    IOP PUBLISHING LTD
    Citation
    GALACTIC EXTINCTION AND REDDENING FROM THE SOUTH GALACTIC CAP u -BAND SKY SURVEY: u -BAND GALAXY NUMBER COUNTS AND u − r COLOR DISTRIBUTION 2017, 153 (2):88 The Astronomical Journal
    Journal
    The Astronomical Journal
    Rights
    © 2017. The American Astronomical Society. All rights reserved.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    We study the integral Galactic extinction and reddening based on the galaxy catalog of the South Galactic Cap u-band Sky Survey (SCUSS), where u-band galaxy number counts and u - r color distribution are used to derive the Galactic extinction and reddening respectively. We compare these independent statistical measurements with the reddening map of Schlegel et al. (SFD) and find that both the extinction and reddening from the number counts and color distribution are in good agreement with the SFD results at low extinction regions (E(B - V)(SFD) < 0.12 mag). However, for high extinction regions (E(B - V)(SFD) > 0.12 mag), the SFD map overestimates the Galactic reddening systematically, which can be approximated by a linear relation Delta E(B - V)= 0.43[ E(B - V)(SFD) - 0.12]. By combining the results from galaxy number counts and color distribution, we find that the shape of the Galactic extinction curve is in good agreement with the standard R-V = 3.1 extinction law of O'Donnell.
    ISSN
    1538-3881
    DOI
    10.3847/1538-3881/153/2/88
    Version
    Final published version
    Sponsors
    National Natural Science Foundation of China (NSFC) [11573050, 11433003, 11433005]; 973 Program [CB845705]; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences (CAS) [XDB09030200]; NSFC [11303070]
    Additional Links
    http://stacks.iop.org/1538-3881/153/i=2/a=88?key=crossref.45c097698e1646aa7f9229093f1841b9
    ae974a485f413a2113503eed53cd6c53
    10.3847/1538-3881/153/2/88
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    UA Faculty Publications

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