posted on 2019-08-05, 14:40authored byRAJ Eyles, PT O'Brien, K Wiersema, RLC Starling, BP Gompertz, GP Lamb, JD Lyman, AJ Levan, S Rosswog, NR Tanvir
We present X-ray and optical observations of the short duration gamma-ray burst GRB
071227 and its host at z = 0.381, obtained using Swift, Gemini South and the Very
Large Telescope. We identify a short-lived and moderately bright optical transient,
with flux significantly in excess of that expected from a simple extrapolation of the Xray spectrum at 0.2-0.3 days after burst. We fit the SED with afterglow models allowing
for high extinction and thermal emission models that approximate a kilonova to assess
the excess’ origins. While some kilonova contribution is plausible, it is not favoured due
to the low temperature and high luminosity required, implying superluminal expansion
and a large ejecta mass of ∼ 0.1 M . We find, instead, that the transient is broadly
consistent with power-law spectra with additional dust extinction of E(B − V) ∼ 0.4
mag, although a possibly thermal excess remains in the z -band. We investigate the
host, a spiral galaxy with an edge-on orientation, resolving its spectrum along its
major axis to construct the galaxy rotation curve and analyse the star formation and
chemical properties. The integrated host emission shows evidence for high extinction,
consistent with the afterglow findings. The metallicity and extinction are consistent
with previous studies of this host and indicate the galaxy is a typical, but dusty,
late-type SGRB host.
Funding
Based on observations obtained at the Gemini Observatory,
which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement
with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de
Ciencia, Tecnolog´ıa e Innovaci´on Productiva (Argentina),
and Minist´erio da Ciˆencia, Tecnologia e Inova¸c˜ao (Brazil)
(acquired through the Gemini Observatory Archive and processed using the Gemini IRAF package).
This research has made use of the services of the ESO
Science Archive Facility. Based on observations collected at
the European Southern Observatory under ESO programme
080.D-0906(G).
This work made use of data supplied by the UK Swift
Science Data Centre at the University of Leicester.
The national facility capability for SkyMapper has been
funded through ARC LIEF grant LE130100104 from the
Australian Research Council, awarded to the University of
Sydney, the Australian National University, Swinburne University of Technology, the University of Queensland, the University of Western Australia, the University of Melbourne,
Curtin University of Technology, Monash University and the
Australian Astronomical Observatory. SkyMapper is owned
and operated by The Australian National University’s Research School of Astronomy and Astrophysics. The survey
data were processed and provided by the SkyMapper Team
at ANU. The SkyMapper node of the All-Sky Virtual Observatory (ASVO) is hosted at the National Computational Infrastructure (NCI). Development and support the SkyMapper node of the ASVO has been funded in part by Astronomy Australia Limited (AAL) and the Australian Government through the Commonwealth’s Education Investment
Fund (EIF) and National Collaborative Research Infrastructure Strategy (NCRIS), particularly the National eResearch
Collaboration Tools and Resources (NeCTAR) and the Australian Natio
History
Citation
Monthly Notices of the Royal Astronomical Society, Volume 489, Issue 1, October 2019, Pages 13–27, https://doi.org/10.1093/mnras/stz2040
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
AM (Accepted Manuscript)
Published in
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP), Royal Astronomical Society