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First Results of the SkyMapper Transient Survey

Published online by Cambridge University Press:  29 August 2019

A. Möller ,
B. E. Tucker ,
P. Armstrong ,
S.-W. Chang ,
N. Lowson ,
C. A. Onken ,
F. Panther ,
R. Ridden-Harper ,
A. J. Ruiter  and
R. Scalzo
...Show all authors
A. Möller
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
B. E. Tucker
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
P. Armstrong
Affiliation:
Australian National University, Canberra, Australia
S.-W. Chang
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
N. Lowson
Affiliation:
Australian National University, Canberra, Australia
C. A. Onken
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
F. Panther
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
R. Ridden-Harper
Affiliation:
Australian National University, Canberra, Australia
A. J. Ruiter
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia UNSW and Australian Defense Force Academy, Canberra, Australia
R. Scalzo
Affiliation:
Centre for Translational Data Science, University of Sydney, Australia email: anais.moller@anu.edu.au
B. P. Schmidt
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
I. R. Seitenzahl
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia UNSW and Australian Defense Force Academy, Canberra, Australia
N. E. Sommer
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
C. Wolf
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
F. Yuan
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
B. Zhang
Affiliation:
Australian National University, Canberra, Australia ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia
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Abstract

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The SkyMapper Transient survey (SMT) is exploring variability in the southern sky by performing (a) a rolling search to discover and study supernovæ, and (b) a Target of Opportunity programme that uses the robotic SkyMapper Telescope at Siding Spring Observatory. The supernova survey is obtaining a non-targeted sample of Type Ia supernovæ (SNe Ia) at low redshifts, z < 0.1, and studying other interesting transients found with the search strategy. We have a Target of Opportunity programme with an automatic response mechanism to search for optical counterparts to gravitational-wave and fast radio-burst events; it benefits from SkyMapper’s large field of view of 5.7 sq. deg. and a rapid data reduction pipeline.

We present first results of the SMT survey. The SMT pipeline can process and obtain potential candidates within 12 hours of observation. It disentangles real transients from processing artefacts using a machine-learning algorithm. To date, SMT has discovered over 60 spectroscopically confirmed supernovæ, several peculiar objects, and over 40 SNe Ia including one (SNIa 2016hhd) which was found within the first few days of explosion. We have also participated in searches for optical counterparts of gravitational waves, fast radio bursts and other transients, and have published observations of the optical counterpart of the gravitational-wave event GW170817. We also participate in coordinated observations with the Deeper Wider Faster programme, and the Kepler K2 cosmology project.

Keywords

Supernovæ: generalsurveysgravitational wavescosmology: observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S339: Southern Horizons in Time-Domain Astronomy , November 2017 , pp. 3 - 6
Copyright
© International Astronomical Union 2019 

References

Andreoni, I., Ackley, K., Cooke, J., et al. 2017, PASA, 34, 69Google Scholar
Arcavi, I., Wolf, W. M., Howell, D. A., et al. 2016, ApJ, 819, 35CrossRefGoogle Scholar
Bertin, E., Mellier, Y., Radovich, M., et al. 2002, in: Bohlender, D. A., Durand, D., & Handley, T. H. (eds.), ADASS XI, (ASPCS, 281), p. 228Google Scholar
Bessell, M., Bloxham, G., Schmidt, B., et al. 2011, PASP, 123, 789CrossRefGoogle Scholar
Farah, W., Bailes, M., Jameson, A., et al. 2018, MNRAS, 478, 1209CrossRefGoogle Scholar
Keller, S. C., Schmidt, B. P., Bessell, M. S., et al. 2007, PASA, 24, 110.1071/AS07001CrossRefGoogle Scholar
LIGO-Virgo collaborations, Abbott, B. P., et al. 2017, ApJ, 848, L12CrossRefGoogle Scholar
Möller, A., Chang, S., Wolf, C., et al. 2017, GCN Circular #21542Google Scholar
Pedregosa, F., Varoquaux, G., Gramfort, A., et al. 2011, J. Mach. Learning Res., 12, 2825Google Scholar
Rest, A., Garnavich, P. M., Khatami, P., et al. Nature Astronomy, 2, 307, 2018.CrossRefGoogle Scholar
Scalzo, R. A., Yuan, F., Childress, M. J., et al. 2017, PASA, 34, 30CrossRefGoogle Scholar
Scolnic, D., Kessler, R., Brout, D., et al. 2017, ApJ, 852, L3CrossRefGoogle Scholar
Tucker, B. E., Moller, A., Armstrong, P., et al. 2017, ATel, 10426Google Scholar
Wolf, C., et al. 2018, PASA, 35, 10Google Scholar