D3CS — Interactive Curve Shifting

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Help us finding the time delays !
All the COSMOGRAIL light curves are listed below.
Click on a curve pair (e.g. "AB") to visualize the data and add your time-delay estimate.
For each pair, the median of the time delays found by the users is shown, together with the median of the uncertainties. Time delays are in day.
For a description of this curve-shifting tool, please see the COSMOGRAIL XV paper.
All light curves will be released after publication of the COSMOGRAIL XIX and TDCOSMO II papers.
Download all available light curves

2M1134WFI
A, B, C, D
AB-30.5 ± 2.2TDCOSMO2: -30.5 +/- 2.2
AC+8.6 ± 1.4TDCOSMO2: 8.6 +/- 1.4
AD-71.9 ± 6.7TDCOSMO2: -71.9 +/- 6.7
BC+38.9 ± 2.2TDCOSMO2: 38.9 +/- 2.2
BD-41.5 ± 7.6TDCOSMO2: -41.5 +/- 7.6
CD-80.5 ± 6.8TDCOSMO2: -80.5 +/- 6.8
 Millon et al. (2020b)
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DES0407WFI
A, B
AB-128.4 ± 3.6TDCOSMO2: -128.4 +/- 3.6
 Millon et al. (2020b)
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DES0408ECAM
A, B, D
AB-115.8 ± 14.9mtewes: -119.5 +/- 27.6
CosmograilXVI: -112.2 +/- 2.1
AD-155.5 ± 12.8CosmograilXVI: -155.5 +/- 12.8
BD-42.4 ± 17.6CosmograilXVI: -42.4 +/- 17.6
 Courbin et al. (2018)
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DES0408WFI
A, B, C, D
AB-112.8 ± 3.8remy.joseph: -113.5 +/- 5.6
CosmograilXVI: -112.1 +/- 2.1
AC-122.4 ± 15.3M.Millon: -122.4 +/- 15.3
AD-155.5 ± 12.8CosmograilXVI: -155.5 +/- 12.8
BC-11.9 ± 11.2M.Millon: -11.9 +/- 11.2
BD-42.4 ± 17.6CosmograilXVI: -42.4 +/- 17.6
CD
 Courbin et al. (2018)
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DES2325WFI
A, B
AB+43.9 ± 4.2TDCOSMO2: 43.9 +/- 4.2
 Millon et al. (2020b)
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HE0047Euler
A, B
AB-10.4 ± 3.5CosmograilXIX: -10.4 +/- 3.5
 Millon et al. (2020a)
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HE0047WFI
A, B
AB-10.8 ± 1.0TDCOSMO2: -10.8 +/- 1.0
 Millon et al. (2020b)
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HE0230ECAM
A, C, D
AC+15.7 ± 3.9CosmograilXIX: 15.7 +/- 3.9
AD
CD
 Millon et al. (2020a)
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HE0435Courbin2011
A, B, C, D
AB-8.4 ± 2.1CosmograilIX: -8.4 +/- 2.1
AC-0.6 ± 2.3CosmograilIX: -0.6 +/- 2.3
AD-14.9 ± 2.1CosmograilIX: -14.9 +/- 2.1
BC+7.8 ± 0.8CosmograilIX: 7.8 +/- 0.8
BD-6.5 ± 0.7CosmograilIX: -6.5 +/- 0.7
CD-14.3 ± 0.8CosmograilIX: -14.3 +/- 0.8
 Courbin et al. (2011)
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HE0435Millon2020
A, B, C, D
AB-9.0 ± 0.8CosmograilXIX: -9.0 +/- 0.8
AC-0.8 ± 0.7CosmograilXIX: -0.8 +/- 0.7
AD-13.8 ± 0.8CosmograilXIX: -13.8 +/- 0.8
BC+7.8 ± 0.9CosmograilXIX: 7.8 +/- 0.9
BD-5.4 ± 0.8CosmograilXIX: -5.4 +/- 0.8
CD-13.2 ± 0.8CosmograilXIX: -13.2 +/- 0.8
 Millon et al. (2020a)
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HE2149Euler
A, B
AB-39.0 ± 15.8CosmograilXIX: -39.0 +/- 15.8
 Millon et al. (2020a)
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HS0818Euler
A, B
AB-153.8 ± 13.9CosmograilXIX: -153.8 +/- 13.9
 Millon et al. (2020a)
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HS2209Eulaers2013
A, B
AB+20.0 ± 5.0CosmograilXII: 20.0 +/- 5.0
 Eulaers et al. (2013)
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J0158Euler-microlensing
M
 Millon et al. (2022)
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J0158Euler
A, B
AB-22.7 ± 3.6CosmograilXIX: -22.7 +/- 3.6
 Millon et al. (2020a)
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J0246Euler
A, B
AB+0.8 ± 5.1CosmograilXIX: 0.8 +/- 5.1
 Millon et al. (2020a)
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J0832ECAM
A, B
AB-125.3 ± 18.1CosmograilXIX: -125.3 +/- 18.1
 Millon et al. (2020a)
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J0924Euler-SMARTS
A, B, C
AB+2.4 ± 3.8CosmograilXIX: 2.4 +/- 3.8
AC
BC
 Millon et al. (2020a)
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J0924Euler
A, B, C
AB+2.4 ± 3.8CosmograilXIX: 2.4 +/- 3.8
AC
BC
 Millon et al. (2020a)
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J1001Rathna2013
A, B
AB-119.3 ± 3.3CosmograilXIV: -119.3 +/- 3.3
 Rathna Kumar et al. (2013)
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J1206Eulaers2013
A, B
AB-111.3 ± 3.0CosmograilXII: -111.3 +/- 3.0
 Eulaers et al. (2013)
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J1226Euler
A, B
AB+33.7 ± 2.7CosmograilXIX: 33.7 +/- 2.7
 Millon et al. (2020a)
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J1320ECAM
A, B
AB
 Millon et al. (2020a)
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J1322ECAM
A, B
AB
 Millon et al. (2020a)
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J1335Euler
A, B
AB-56.0 ± 5.9CosmograilXIX: -56.0 +/- 5.9
 Millon et al. (2020a)
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J1349ECAM
A, B
AB
 Millon et al. (2020a)
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J1405ECAM
A, B
AB
 Millon et al. (2020a)
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J1455ECAM
A, B
AB-47.2 ± 7.6CosmograilXIX: -47.2 +/- 7.6
 Millon et al. (2020a)
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J1515ECAM-Liverpool
A, B
AB-210.2 ± 5.6CosmograilXIX: -210.2 +/- 5.6
 Millon et al. (2020a)
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J1515ECAM
A, B
AB-210.2 ± 5.6CosmograilXIX: -210.2 +/- 5.6
 Millon et al. (2020a)
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J1620Euler
A, B
AB-171.5 ± 8.7CosmograilXIX: -171.5 +/- 8.7
 Millon et al. (2020a)
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PG1115WFI
A, B, C
AB-8.3 ± 1.5CosmograilXVII: -8.3 +/- 1.5
AC+9.9 ± 1.1CosmograilXVII: 9.9 +/- 1.1
BC+18.8 ± 1.6CosmograilXVII: 18.8 +/- 1.6
 Bonvin et al. (2018)
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PS1606WFI
A, B, C, D
AB-10.4 ± 2.2TDCOSMO2: -10.4 +/- 2.2
AC-29.2 ± 4.7TDCOSMO2: -29.2 +/- 4.7
AD-45.7 ± 10.9TDCOSMO2: -45.7 +/- 10.9
BC-19.3 ± 4.5TDCOSMO2: -19.3 +/- 4.5
BD-36.2 ± 10.4TDCOSMO2: -36.2 +/- 10.4
CD-13.8 ± 8.4TDCOSMO2: -13.8 +/- 8.4
 Millon et al. (2020b)
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Q1355Euler
A, B
AB-81.5 ± 11.4CosmograilXIX: -81.5 +/- 11.4
 Millon et al. (2020a)
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Q2237ECAM
A, B
AB
 Millon et al. (2020a)
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RXJ1131Millon2020
A, B, C, D
AB+1.6 ± 0.7CosmograilXIX: 1.6 +/- 0.7
AC-1.0 ± 1.2CosmograilXIX: -1.0 +/- 1.2
AD-92.5 ± 1.8CosmograilXIX: -92.5 +/- 1.8
BC-2.0 ± 1.4CosmograilXIX: -2.0 +/- 1.4
BD-93.7 ± 2.0CosmograilXIX: -93.7 +/- 2.0
CD-91.8 ± 2.2CosmograilXIX: -91.8 +/- 2.2
 Millon et al. (2020a)
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RXJ1131Tewes2013
A, B, C, D
AB-0.7 ± 1.0CosmograilXIII: -0.7 +/- 1.0
AC+0.0 ± 1.3CosmograilXIII: 0.0 +/- 1.3
AD-93.8 ± 1.5CosmograilXIII: -93.8 +/- 1.5
BC+0.7 ± 1.5CosmograilXIII: 0.7 +/- 1.5
BD-93.2 ± 1.5CosmograilXIII: -93.2 +/- 1.5
CD-93.8 ± 2.0CosmograilXIII: -93.8 +/- 2.0
 Tewes et al. (2013)
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UM673Euler
A, B
AB-97.7 ± 15.8CosmograilXIX: -97.7 +/- 15.8
 Millon et al. (2020a)
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WFI2026Euler
A, B, C
AB+18.0 ± 4.8CosmograilXIX: 18.0 +/- 4.8
AC-8.0 ± 45.8M.Millon: -8.0 +/- 45.8
BC
 Millon et al. (2020a)
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WFI2033Euler-SMARTS
A, B, C
AB+36.2 ± 0.7CosmograilXVIII: 36.2 +/- 0.7
AC-23.3 ± 1.3CosmograilXVIII: -23.3 +/- 1.3
BC-59.4 ± 1.3CosmograilXVIII: -59.4 +/- 1.3
 Bonvin et al. (2019)
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WFI2033Euler
A, B, C
AB+36.2 ± 0.7CosmograilXVIII: 36.2 +/- 0.7
AC-23.3 ± 1.3CosmograilXVIII: -23.3 +/- 1.3
BC-59.4 ± 1.3CosmograilXVIII: -59.4 +/- 1.3
 Bonvin et al. (2019)
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WFI2033WFI
A1, A2, B, C
A1A2-1.0 ± 2.9CosmograilXVIII: -1.0 +/- 2.9
A1B+36.2 ± 1.9CosmograilXVIII: 36.2 +/- 1.9
A1C-20.5 ± 3.3CosmograilXVIII: -20.5 +/- 3.3
A2B+37.3 ± 2.8CosmograilXVIII: 37.3 +/- 2.8
A2C-19.5 ± 3.4CosmograilXVIII: -19.5 +/- 3.4
BC-57.1 ± 3.1CosmograilXVIII: -57.1 +/- 3.1
 Bonvin et al. (2019)
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WG0214WFI
A, B, C, D
AB+7.5 ± 2.8TDCOSMO2: 7.5 +/- 2.8
AC-6.7 ± 3.6TDCOSMO2: -6.7 +/- 3.6
AD-14.1 ± 4.9TDCOSMO2: -14.1 +/- 4.9
BC-14.2 ± 2.6TDCOSMO2: -14.2 +/- 2.6
BD-21.6 ± 4.6TDCOSMO2: -21.6 +/- 4.6
CD-7.5 ± 4.7TDCOSMO2: -7.5 +/- 4.7
 Millon et al. (2020b)
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