2020MNRAS.499..524G


Query : 2020MNRAS.499..524G

2020MNRAS.499..524G - Mon. Not. R. Astron. Soc., 499, 524-542 (2020/November-3)

Density-based outlier scoring on Kepler data.

GILES D.K. and WALKOWICZ L.

Abstract (from CDS):

In the present era of large-scale surveys, big data present new challenges to the discovery process for anomalous data. Such data can be indicative of systematic errors, extreme (or rare) forms of known phenomena, or most interestingly, truly novel phenomena that exhibit as-of-yet unobserved behaviours. In this work, we present an outlier scoring methodology to identify and characterize the most promising unusual sources to facilitate discoveries of such anomalous data. We have developed a data mining method based on k-nearest neighbour distance in feature space to efficiently identify the most anomalous light curves. We test variations of this method including using principal components of the feature space, removing select features, the effect of the choice of k, and scoring to subset samples. We evaluate the performance of our scoring on known object classes and find that our scoring consistently scores rare (<1000) object classes higher than common classes. We have applied scoring to all long cadence light curves of Quarters 1-17 of Kepler's prime mission and present outlier scores for all 2.8 million light curves for the roughly 200k objects.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - surveys - stars: general

VizieR on-line data: <Available at CDS (J/MNRAS/499/524): table1.dat table3.dat table3.txt tableb1.dat tablec1.dat>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 24

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Number of rows : 24
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 IRAS F18481+4834 LP* 18 49 28.4075593224 +48 38 13.366318524           M6III 10 0
2 2MASS J18523168+4702137 LM* 18 52 31.7248077713 +47 02 14.033097618           ~ 6 0
3 2MASS J18543173+4003367 * 18 54 31.7303285952 +40 03 36.837539460           ~ 10 0
4 V* V447 Lyr CV* 19 00 19.91 +44 27 45.0           ~ 24 0
5 2MASS J19043327+4116297 V* 19 04 33.2767981992 +41 16 29.669850480           K1V 4 0
6 ZTF J190609.08+502748.5 EB* 19 06 09.131448 +50 27 49.99428   17.484 15.774 15.549   ~ 20 0
7 V* V450 Lyr RR* 19 09 36.6322966296 +43 21 49.964734332   14.3       ~ 32 0
8 UCAC4 653-070979 * 19 11 18.7965371904 +40 27 02.912370192       15.60   ~ 1 0
9 2MASS J19133855+4342269 EB* 19 13 38.4697500408 +43 42 26.766126612           ~ 12 0
10 V* V1104 Cyg RR* 19 18 00.4918937064 +50 45 17.809657164       14.84   ~ 35 0
11 ASAS J191840+4325.7 LP* 19 18 40.4400705072 +43 25 39.226241820   13.45 11.39   9.105 K5III 11 0
12 IRAS 19195+4128 LP* 19 21 08.4804925344 +41 34 33.968720640     12.599   8.716 M4e 7 0
13 2MASS J19252521+3712347 * 19 25 25.2148953600 +37 12 34.681989924           K7V 5 0
14 UCAC4 664-074567 Er* 19 25 31.1449382304 +42 46 11.648498592   15.651 14.873 14.776   ~ 7 0
15 KOI-1346 EB* 19 26 26.4146564376 +42 45 35.106094404           ~ 28 0
16 V* V1504 Cyg CV* 19 28 56.4508657536 +43 05 37.081595940           ~ 122 0
17 2MASS J19402000+4510143 Ro* 19 40 20.0031643968 +45 10 14.343850380           ~ 10 0
18 UCAC4 695-069503 * 19 43 53.9249005848 +48 48 13.044099960       15.94   ~ 1 0
19 V* V1580 Cyg EB* 19 44 00.3758939424 +45 26 53.243356668           ~ 38 0
20 2MASS J19453822+4451174 AB? 19 45 38.2207034520 +44 51 17.387829504           M3.0III 10 0
21 ASAS J194626+4736.7 LP* 19 46 26.2545577608 +47 36 44.079667632   14.853 13.455 12.866 9.636 M6.0III 6 0
22 TYC 3561-1088-1 dS* 19 50 28.7824663536 +48 15 41.041038204   11.83 11.49     ~ 3 0
23 Kepler-1647 EB* 19 52 36.0203935200 +40 39 22.342749552           F5 84 0
24 GSC 03162-00665 Er* 20 06 15.4526521026 +44 27 24.790869158   12.82 12.01 11.75   F3V 159 0

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