Name . | |$M_{\rm FUV}^{\rm a}$| . | log |$M_\star ^{\rm b}$| . | log L(H β)c . | |$t_b^{\rm d}$| . | SFRe . | |$\alpha ^{\rm f}$| . | |$r_{50}^{\rm g}$| . | |$\Sigma \, _1^{\rm h}$| . | |$\Sigma \, _2^{\rm i}$| . |
---|---|---|---|---|---|---|---|---|---|
J0130−0014 | −18.24 | 8.63 | 41.22 | 0.4 | 3.7 | 0.20 | 0.10 | 27 | 118 |
J0141−0304 | −19.47 | 9.99 | 42.23 | 2.0 | 36.0 | 0.63 | 0.21 | 30 | 269 |
J0844+5312 | −20.79 | 8.18 | 42.07 | 3.8 | 25.3 | 0.54 | 0.19 | 28 | 228 |
J1014+5501 | −19.32 | 7.48 | 41.60 | 3.0 | 8.6 | ...j | ...j | ...j | ...j |
J1137+3605 | −18.46 | 9.17 | 41.99 | 0.3 | 21.1 | 0.46 | 0.19 | 33 | 191 |
J1157+5801 | −18.49 | 9.28 | 41.77 | 3.0 | 13.0 | 0.21 | 0.16 | 95 | 163 |
J1352+5617 | −19.48 | 9.40 | 41.76 | 2.7 | 12.6 | ...j | ...j | ...j | ...j |
Name . | |$M_{\rm FUV}^{\rm a}$| . | log |$M_\star ^{\rm b}$| . | log L(H β)c . | |$t_b^{\rm d}$| . | SFRe . | |$\alpha ^{\rm f}$| . | |$r_{50}^{\rm g}$| . | |$\Sigma \, _1^{\rm h}$| . | |$\Sigma \, _2^{\rm i}$| . |
---|---|---|---|---|---|---|---|---|---|
J0130−0014 | −18.24 | 8.63 | 41.22 | 0.4 | 3.7 | 0.20 | 0.10 | 27 | 118 |
J0141−0304 | −19.47 | 9.99 | 42.23 | 2.0 | 36.0 | 0.63 | 0.21 | 30 | 269 |
J0844+5312 | −20.79 | 8.18 | 42.07 | 3.8 | 25.3 | 0.54 | 0.19 | 28 | 228 |
J1014+5501 | −19.32 | 7.48 | 41.60 | 3.0 | 8.6 | ...j | ...j | ...j | ...j |
J1137+3605 | −18.46 | 9.17 | 41.99 | 0.3 | 21.1 | 0.46 | 0.19 | 33 | 191 |
J1157+5801 | −18.49 | 9.28 | 41.77 | 3.0 | 13.0 | 0.21 | 0.16 | 95 | 163 |
J1352+5617 | −19.48 | 9.40 | 41.76 | 2.7 | 12.6 | ...j | ...j | ...j | ...j |
aAbsolute FUV magnitude derived from the intrinsic rest-frame SED in mag.
|$^{\rm b}M_\star$| = |$M_{\rm y}\, +\, M_{\rm o}$| is the total stellar mass in M⊙, where My and Mo are masses of the young and old stellar population, respectively.
|$^{\rm c}\, L$|(H β) is the H β luminosity corrected for the Milky Way and internal extinction in erg s−1.
|$^{\rm d}\, t_b$| is the starburst age in Myr.
eStar-formation rate in M⊙ yr−1 corrected for the Milky Way and internal extinction, and escaping LyC radiation.
fExponential disc scale length in kpc.
gGalaxy radius, at which NUV intensity is equal to half of maximal intensity, in kpc.
hStar formation rate surface density assuming galaxy radius is equal to α in M⊙ yr−1 kpc−2.
iStar formation rate surface density assuming galaxy radius is equal to r50 in M⊙ yr−1 kpc−2.
jAcquisition image not obtained.
Name . | |$M_{\rm FUV}^{\rm a}$| . | log |$M_\star ^{\rm b}$| . | log L(H β)c . | |$t_b^{\rm d}$| . | SFRe . | |$\alpha ^{\rm f}$| . | |$r_{50}^{\rm g}$| . | |$\Sigma \, _1^{\rm h}$| . | |$\Sigma \, _2^{\rm i}$| . |
---|---|---|---|---|---|---|---|---|---|
J0130−0014 | −18.24 | 8.63 | 41.22 | 0.4 | 3.7 | 0.20 | 0.10 | 27 | 118 |
J0141−0304 | −19.47 | 9.99 | 42.23 | 2.0 | 36.0 | 0.63 | 0.21 | 30 | 269 |
J0844+5312 | −20.79 | 8.18 | 42.07 | 3.8 | 25.3 | 0.54 | 0.19 | 28 | 228 |
J1014+5501 | −19.32 | 7.48 | 41.60 | 3.0 | 8.6 | ...j | ...j | ...j | ...j |
J1137+3605 | −18.46 | 9.17 | 41.99 | 0.3 | 21.1 | 0.46 | 0.19 | 33 | 191 |
J1157+5801 | −18.49 | 9.28 | 41.77 | 3.0 | 13.0 | 0.21 | 0.16 | 95 | 163 |
J1352+5617 | −19.48 | 9.40 | 41.76 | 2.7 | 12.6 | ...j | ...j | ...j | ...j |
Name . | |$M_{\rm FUV}^{\rm a}$| . | log |$M_\star ^{\rm b}$| . | log L(H β)c . | |$t_b^{\rm d}$| . | SFRe . | |$\alpha ^{\rm f}$| . | |$r_{50}^{\rm g}$| . | |$\Sigma \, _1^{\rm h}$| . | |$\Sigma \, _2^{\rm i}$| . |
---|---|---|---|---|---|---|---|---|---|
J0130−0014 | −18.24 | 8.63 | 41.22 | 0.4 | 3.7 | 0.20 | 0.10 | 27 | 118 |
J0141−0304 | −19.47 | 9.99 | 42.23 | 2.0 | 36.0 | 0.63 | 0.21 | 30 | 269 |
J0844+5312 | −20.79 | 8.18 | 42.07 | 3.8 | 25.3 | 0.54 | 0.19 | 28 | 228 |
J1014+5501 | −19.32 | 7.48 | 41.60 | 3.0 | 8.6 | ...j | ...j | ...j | ...j |
J1137+3605 | −18.46 | 9.17 | 41.99 | 0.3 | 21.1 | 0.46 | 0.19 | 33 | 191 |
J1157+5801 | −18.49 | 9.28 | 41.77 | 3.0 | 13.0 | 0.21 | 0.16 | 95 | 163 |
J1352+5617 | −19.48 | 9.40 | 41.76 | 2.7 | 12.6 | ...j | ...j | ...j | ...j |
aAbsolute FUV magnitude derived from the intrinsic rest-frame SED in mag.
|$^{\rm b}M_\star$| = |$M_{\rm y}\, +\, M_{\rm o}$| is the total stellar mass in M⊙, where My and Mo are masses of the young and old stellar population, respectively.
|$^{\rm c}\, L$|(H β) is the H β luminosity corrected for the Milky Way and internal extinction in erg s−1.
|$^{\rm d}\, t_b$| is the starburst age in Myr.
eStar-formation rate in M⊙ yr−1 corrected for the Milky Way and internal extinction, and escaping LyC radiation.
fExponential disc scale length in kpc.
gGalaxy radius, at which NUV intensity is equal to half of maximal intensity, in kpc.
hStar formation rate surface density assuming galaxy radius is equal to α in M⊙ yr−1 kpc−2.
iStar formation rate surface density assuming galaxy radius is equal to r50 in M⊙ yr−1 kpc−2.
jAcquisition image not obtained.
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