Table A.1
Parameters for lensed compact regions of star formation compiled from the literature.
Name | log L(Hβ) | logσ | μ | References |
erg s-1 | km s-1 | |||
|
||||
ID11 | 40.15 | 1.36 | 16.7 | Vanzella et al. (2016) |
Cl0024* | 42.28 | 1.84 | 1.4 | Jones et al. (2010) (1) |
MACSJ0451 | 41.70 | 1.90 | 49. | Jones et al. (2010) (1) |
MACSJ0712 | 41.55 | 1.91 | 28. | Jones et al. (2010) (1) |
Cl0949* | 42.15 | 1.82 | 7.3 | Jones et al. (2010) (1) |
Cl0949(NE) | 41.96 | 1.85 | 7.3 | Jones et al. (2010) (1) |
Cl0949(SW) | 41.70 | 1.76 | 7.3 | Jones et al. (2010) (1) |
MACSJ2135 | 42.45 | 1.73 | 28. | Jones et al. (2010) (1) |
A4.1 | 40.18 | 1.23 | 23.0 | Christensen et al. (2012) (2) |
M0304 | 42.08 | 1.75 | 42.0 | Christensen et al. (2012) (2) |
M0359 | 41.06 | 1.72 | 18.0 | Christensen et al. (2012) (2) |
M2031 | 42.04 | 1.63 | 4.2 | Christensen et al. (2012) (2) |
RCSGA032727b | 40.73 | 1.54 | — | Wuyts et al. (2014) (3) |
RCSGA032727d | 40.70 | 1.62 | — | Wuyts et al. (2014) (3) |
RCSGA032727e | 41.10 | 1.67 | — | Wuyts et al. (2014) (3) |
RCSGA032727f | 40.45 | 1.55 | — | Wuyts et al. (2014) (3) |
RCSGA032727g | 41.65 | 1.83 | — | Wuyts et al. (2014) (3) |
MS1512-cB58 | 41.90 | 1.91 | 30.0 | Teplitz et al. (2000) |
RXJ0848 | 42.50 | 1.52 | 10. | Fosbury et al. (2003) (4) |
RXJ0848 | 42.50 | 1.90 | 10. | Fosbury et al. (2003) (5) |
A68-C1 | 40.68 | 1.85 | 2.52 | Richard et al. (2011) (6) |
CEYE | 41.98 | 1.73 | 3.69 | Richard et al. (2011) (6) |
MACS0744 | 41.77 | 1.90 | 3.01 | Richard et al. (2011) (6) |
Cl0024* | 41.68 | 1.84 | 1.38 | Richard et al. (2011) (6) |
MACS0451 | 41.86 | 1.90 | 4.22 | Richard et al. (2011) (6) |
RXJ1053 | 41.87 | 1.83 | 4.03 | Richard et al. (2011) (6) |
A2218-Flank. | 41.35 | 1.91 | 3.60 | Richard et al. (2011) (6) |
Cl0949* | 41.42 | 1.91 | 2.16 | Richard et al. (2011) (6) |
A773 | 41.56 | 1.81 | 2.69 | Richard et al. (2011) (6,7) |
A2218-Mult | 42.28 | 1.76 | 3.39 | Richard et al. (2011) (6) |
A2218-Smm | 42.01 | 1.91 | 3.01 | Richard et al. (2011) (6) |
8OCLOCKA2 | 42.95 | 1.95 | 6.3 | Shirazi et al. (2014) |
8OCLOCKA3 | 42.93 | 1.95 | 4.9 | Shirazi et al. (2014) |
Notes. Names are those listed in the corresponding reference. Luminosities are de-lensed. μ is the published magnification. Luminosities recalculated from the observed fluxes for a flat universe with H0 = 74.3km s-1 Mpc-1 ; Ωλ = 0.70. (1) Velocity dispersion from either Hα or [OIII]λ5007 Å. (2) Velocity dispersion is the weighted average of all lines from UV to optical excluding only Lyα. (3) Provides de-lensed luminosities but do not list the magnifications. (4) Velocity dispersion from OIII]λ1666 Å and CIII]λλ1907,1909 Å. (5) Velocity dispersion from CIVλ1550 Å. (6) Velocity dispersion from either [OII]λ3727 Å, Hα or [OIII]λ5007 Å; undefined. (7) Used Hβ flux.
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