2018ApJS..236....9N


Query : 2018ApJS..236....9N

2018ApJS..236....9N - Astrophys. J., Suppl. Ser., 236, 9-9 (2018/May-0)

Machine-learning-based brokers for real-time classification of the LSST alert stream.

NARAYAN G., ZAIDI T., SORAISAM M.D., WANG Z., LOCHNER M., MATHESON T., SAHA A., YANG S., ZHAO Z., KECECIOGLU J., SCHEIDEGGER C., SNODGRASS R.T., AXELROD T., JENNESS T., MAIER R.S., RIDGWAY S.T., SEAMAN R.L., EVANS E.M., SINGH N., TAYLOR C., TOENISKOETTER J., WELCH E., ZHU S. (The ANTARES Collaboration)

Abstract (from CDS):

The unprecedented volume and rate of transient events that will be discovered by the Large Synoptic Survey Telescope (LSST) demand that the astronomical community update its follow-up paradigm. Alert-brokers-automated software system to sift through, characterize, annotate, and prioritize events for follow-up-will be critical tools for managing alert streams in the LSST era. The Arizona-NOAO Temporal Analysis and Response to Events System (ANTARES) is one such broker. In this work, we develop a machine learning pipeline to characterize and classify variable and transient sources only using the available multiband optical photometry. We describe three illustrative stages of the pipeline, serving the three goals of early, intermediate, and retrospective classification of alerts. The first takes the form of variable versus transient categorization, the second a multiclass typing of the combined variable and transient data set, and the third a purity-driven subtyping of a transient class. Although several similar algorithms have proven themselves in simulations, we validate their performance on real observations for the first time. We quantitatively evaluate our pipeline on sparse, unevenly sampled, heteroskedastic data from various existing observational campaigns, and demonstrate very competitive classification performance. We describe our progress toward adapting the pipeline developed in this work into a real-time broker working on live alert streams from time-domain surveys.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): methods: data analysis - methods: statistical - stars: variables: general - supernovae: general - surveys - virtual observatory tools

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 OGLE BLG-RRLYR-11078 RR* 18 01 33.9164367864 -29 07 14.575651032     17.688   16.172 ~ 15 0

Query : 2018ApJS..236....9N

Basic data :
OGLE BLG-RRLYR-11078 -- RR Lyrae Variable
Other object types:
otypes_help
RR* (2014AcA,OGLE), * (OGLE,Gaia)
ICRS coord. (ep=J2000) :
18 01 33.9164367864 -29 07 14.575651032 (Optical) [ 0.1415 0.1174 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
17 58 22.9045693355 -29 07 14.350266870 [ 0.1415 0.1174 90 ]
Gal coord. (ep=J2000) :
001.6080346053870 -03.0981889312628 [ 0.1415 0.1174 90 ]
Proper motions mas/yr :
1.540 -1.658 [0.177 0.124 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.8540 [0.2043] A 2018yCat.1345....0G
Fluxes (3) :
V 17.688 [~] D 2011AcA....61....1S
G 17.247244 [0.012649] C 2020yCat.1350....0G
I 16.172 [~] V3 D 2011AcA....61....1S
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Identifiers (6) :
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OGLE BLG-RRLYR-11078 OGLE BLG512.6 126404 Gaia DR2 4062312216146792704
OGLE BUL-SC30 432698 OGLE BLG207.8 76684 Gaia DR3 4062312216146792704

References (15 between 1850 and 2026) (Total 15)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Var : 9    Plx : 1    PM : 2   

   


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OGLE BUL-SC30 432698 Gaia DR2 4062312216146792704 Gaia DR3 4062312216146792704

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