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Type II-P supernovae as standardized candles: Improvements using near-infrared data

Abstract:
We present the first near-infrared Hubble diagram for Type II-P supernovae (SNe), to further explore their value as distance indicators. We use a modified version of the standardized candle method, which relies on the tight correlation between the absolute magnitudes of Type II-P SNe and their expansion velocities during the plateau phase. Although our sample contains only 12 II-P SNe and they are necessarily local (z < 0.02), we demonstrate using near-infrared JHK photometry that it may be possible to reduce the scatter in the Hubble diagram to 0.1-0.15 mag. While this is potentially similar to the dispersion seen for Type Ia SNe, we caution that this needs to be confirmed with a larger sample of II-P SNe in the Hubble flow. © 2010 The Authors. Journal compilation © 2010 RAS.

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Publisher copy:
10.1111/j.1745-3933.2009.00804.x

Authors


Journal:
Monthly Notices of the Royal Astronomical Society: Letters More from this journal
Volume:
403
Issue:
1
Pages:
L11-L15
Publication date:
2010-03-01
DOI:
EISSN:
1745-3933
ISSN:
1745-3933


Language:
English
Keywords:
Pubs id:
pubs:187611
UUID:
uuid:e99108bf-c9c3-4530-b4b8-f5b4d29a61b3
Local pid:
pubs:187611
Source identifiers:
187611
Deposit date:
2012-12-19
ARK identifier:

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