Right Ascension: Declination: Radius (arcmin):

Mean Mag: Min Max

Amplitude: Min Max

Period: Min Max Show non-periodic variables

LKSL Statistic: Min Max

Class Probability: Min Max Show variables without ASAS-SN classifications

RF Regression Score: Min Max

Variable Type ROT (Spotted stars showing rotational modulation) DSCT (δ Scuti type variables) HADS (High amplitude δ Scuti type variables) CWA ( W Virginis type variables with P > 8d) CWB ( W Virginis type variables with P < 8d) DCEP ( δ Cephei-type/classical Cepheid variables) DCEPS (δ Cephei-type variables with almost symmetrical light curves) RVA (RV Tauri variables) M (Mira variables) EA (Detached Algol-type binaries) EB (Beta Lyrae type binaries) EW (W Ursae Majoris type binaries) YSO (Young Stellar Objects) L (Red irregular variables) GCAS (Rapidly rotating early type stars with mass outflow) SR (Long period semi-regular variables) SRD ('yellow' semi-regular variables) GCAS: (Suspected GCAS variables) ROT: (Suspected rotational variables) SR: (Suspected semi-regular variables) VAR (Variable star of unspecified type) RRAB: (Suspected RRAB variables) DSCT: (Suspected DSCT: variables) M: (Suspected Mira variables) RRAB (RR Lyrae variables with asymmetric light curves) RRC (RR Lyrae variables with nearly symmetric light curves) RRD (Double Mode RR Lyrae variables) RCB RCB: DYPer CV CV+E CV: UG UGER UGSS UGSU UGSU+E UGSU: UGWZ UGZ AM AM+E AM: DQ DQ: UV UV: SXARI SXARI: ELL HB R SXPHE PPN PVTELI V1093HER V361HYA V838MON WR ZAND SDOR SDOR: HMXB LMXB ZZ ZZ: ZZA ZZB ZZLep ZZO

References The ASAS-SN Catalog of Variable Stars: II The ASAS-SN Catalog of Variable Stars: I

Sort By LCID RAJ2000 DEJ2000 Mean VMag Amplitude Period Distance (pc) LKSL Statistic Classification Probability RF Regression Score BP-RP J-K W1-W2 W3-W4 Ascending Descending

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Total Light Curves found: 415915

When using ASAS-SN light curves in publications, cite Shappee et al. (2014) and either (i) The ASAS-SN Catalog of Variable Stars I: Jayasinghe et al. (2018a), or (ii) The ASAS-SN Catalog of Variable Stars II: Jayasinghe et al. (2018b)