Table 3
All image pairs of multiply lensed background galaxies with spectroscopic redshift and a predicted time delay shorter than five years.
| Images | z spec | Δta | Δm1 | Δm2b | rCC × 102 | rIa × 103c | Detectable SN typesd | ||||||
| (d) | (mag) | (yr-1) | Ia | IIP | IIL | IILb | IIn | Ib/c | HN | ||||
|
|
|||||||||||||
| 1.1 + 1.2 | 3.04 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 1.3 + 1.6 | 3.04 |
|
|
|
... | ... | y | y | |||||
| 1.4 + 1.5 | 3.04 |
|
|
|
... | ... | y | y | y | y | |||
| 2.2 + 2.3 | 2.53 |
|
|
|
|
|
y | y | y | y | y | y | |
| 2.4 + 2.5 | 2.53 |
|
|
|
... | ... | y | y | y | y | |||
| 4.1 + 4.2 | 1.16 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 5.1 + 5.2 | 2.64 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 6.1 + 6.2 | 1.15 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 6.1 + 6.3 | 1.15 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 6.1 + 6.4 | 1.15 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 6.2 + 6.3 | 1.15 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 6.2 + 6.4 | 1.15 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 6.3 + 6.4 | 1.15 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 7.2 + 7.3 | 4.87 |
|
|
|
|
|
|||||||
| 10.2 + 10.3 | 1.83 |
|
|
|
|
|
y | y | y | y | |||
| 12.2 + 12.3 | 1.83 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 14.1 + 14.2 | 3.40 |
|
|
|
... | ... | y | y | y | y | |||
| 15.1 + 15.3 | 1.82 |
|
|
|
|
|
y | y | y | y | |||
| 17.1 + 17.2 | 2.66 |
|
|
|
|
|
y | y | y | y | |||
| 19.1 + 19.5 | 2.60 |
|
|
|
|
|
y | y | y | y | |||
| 19.3 + 19.4 | 2.60 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 22.1 + 22.2 | 1.70 |
|
|
|
|
|
y | y | y | y | |||
| 24.2 + 24.3 | 2.63 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 24.2 + 24.4 | 2.63 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 24.3 + 24.4 | 2.63 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 29.2 + 29.3 | 2.57 |
|
|
|
|
|
y | y | y | y | y | y | y |
| 29.2 + 29.4 | 2.57 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 29.3 + 29.4 | 2.57 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 30.1 + 30.2 | 3.05 |
|
|
|
|
|
y | y | y | y | |||
| 30.1 + 30.3 | 3.05 |
|
|
|
... | ... | y | y | y | y | |||
| 30.2 + 30.3 | 3.05 |
|
|
|
... | ... | y | y | y | y | y | y | y |
| 32.1 + 32.2 | 3.00 |
|
|
|
|
|
y | y | y | y | |||
| 32.3 + 32.4 | 3.00 |
|
|
|
... | ... | y | y | y | ||||
| 35.1 + 35.3 | 1.91 |
|
|
|
|
|
y | y | y | y | |||
| 36.1 + 36.2 | 3.01 |
|
|
|
|
|
y | y | y | y | y | y | y |
Notes. Errors are given as 1σ confidence intervals.
Predicted time delay between the images. A negative time delay indicates that image 2 will occur before image 1.
Detectability of a lensed SN for the different SN types assuming a limiting magnitude of 25.25 mag (Vega) in F140W, e.g. in a survey using one-third of an orbit with the HST/WFC3 instrument (compare with Fig. 2).
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