Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory

Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory
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附近超新星工厂 SN 2011fe 的分光光度时间序列

DOI:
10.1051/0004-6361/201221008
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发表时间:
2013-02
期刊:
Astronomy & Astrophysics
影响因子:
--
通讯作者:
Wu, C.
Wu, C.
中科院分区:
其他
文献类型:
--
作者:
Tao, C.;Taubenberger, S.;Tilquin, A.;Wu, C.

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我们用光学方法(3300-9700 A)对M101星系中最典型的Ia型超新星(SNIa)SN2011Fe进行了32个历元的光学(3300-9700 A)分光光度观测,相对于B带极大值的范围从15天延长到+97天
We present 32 epochs of optical (3300‐9700 A) spectrophotometric observations of the nearby quintessential “normal” type Ia supernova (SN Ia) SN 2011fe in the galaxy M101, extending from 15 to + 97 d with respect to B-band maximum, obtained by the Nearby
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