Table 1.
Open in new tab

Properties of the z ≳ 12 JWST targets explored in this work.

SectionIDzMUVlog10 (M*/M⊙)|$\mathrm{SFR}(\mathrm{M}_{\odot}\mathrm{yr}^{-1})^{\mathrm{a}}$|ReferencesbCommentsc
4.1JADES-GS-z13|$13.20^{+0.04}_{-0.07}$|−18.5 ± 0.2|$7.8^{+0.4}_{-0.5}$||$1.0_{-0.5}^{+1.0}$|CL23, R22, D23b, H23a
4.1JADES-GS-z12|$12.63^{+0.24}_{-0.08}$|−18.8 ± 0.1|$8.4^{+0.4}_{-0.7}$||$1.3_{-0.9}^{+1.9}$|CL23, R22, H23aConsistent with fiducial
4.2S5-z12 − 1|$12.58^{+1.23}_{-0.46}$|−20.2 ± 0.1|$8.53^{+0.61}_{-0.69}$||$5.5^{+4.7}_{-4.4}$|H23b
4.3GLz12|$12.2^{+0.1}_{-0.2}$|−21.0 ± 0.1|$9.1^{+0.3}_{-0.4}$||$6^{+5}_{-2}$|N22, B23, D23a, H23b, O22, P23, S23Consistent with fiducial but challenging
4.4Maisie’s Galaxy|$11.44^{+0.09}_{-0.08}$||$-20.32^{+0.08}_{-0.06}$||$8.50^{+0.29}_{-0.44}$||$2.1^{+4.8}_{-2.0}$|FI22, AH23, D23a, H23ab, O22, Z23
4.5SMACS_z16a|$15.92^{+0.17}_{-0.15}$|−20.59 ± 0.15|$8.79^{+0.32}_{-0.33}$||$16.6^{+2.9}_{-16.4}$|AT23, AD23, FU23, H23bInconsistent with fiducial, requiring maxSF
4.5SMACS_z16b|$15.32^{+0.16}_{-0.13}$|−20.96 ± 0.14|$8.80^{+0.44}_{-0.25}$||$57.5^{+38.0}_{-29.4}$|
4.6S5-z16 − 1|$16.41^{+0.66}_{-0.55}$|−21.6 ± 0.3|$8.59^{+1.23}_{-0.31}$||$5.1^{+21.7}_{-1.8}$|H23b, O22Inconsistent with fiducial, even challenging to maxSF
SectionIDzMUVlog10 (M*/M⊙)|$\mathrm{SFR}(\mathrm{M}_{\odot}\mathrm{yr}^{-1})^{\mathrm{a}}$|ReferencesbCommentsc
4.1JADES-GS-z13|$13.20^{+0.04}_{-0.07}$|−18.5 ± 0.2|$7.8^{+0.4}_{-0.5}$||$1.0_{-0.5}^{+1.0}$|CL23, R22, D23b, H23a
4.1JADES-GS-z12|$12.63^{+0.24}_{-0.08}$|−18.8 ± 0.1|$8.4^{+0.4}_{-0.7}$||$1.3_{-0.9}^{+1.9}$|CL23, R22, H23aConsistent with fiducial
4.2S5-z12 − 1|$12.58^{+1.23}_{-0.46}$|−20.2 ± 0.1|$8.53^{+0.61}_{-0.69}$||$5.5^{+4.7}_{-4.4}$|H23b
4.3GLz12|$12.2^{+0.1}_{-0.2}$|−21.0 ± 0.1|$9.1^{+0.3}_{-0.4}$||$6^{+5}_{-2}$|N22, B23, D23a, H23b, O22, P23, S23Consistent with fiducial but challenging
4.4Maisie’s Galaxy|$11.44^{+0.09}_{-0.08}$||$-20.32^{+0.08}_{-0.06}$||$8.50^{+0.29}_{-0.44}$||$2.1^{+4.8}_{-2.0}$|FI22, AH23, D23a, H23ab, O22, Z23
4.5SMACS_z16a|$15.92^{+0.17}_{-0.15}$|−20.59 ± 0.15|$8.79^{+0.32}_{-0.33}$||$16.6^{+2.9}_{-16.4}$|AT23, AD23, FU23, H23bInconsistent with fiducial, requiring maxSF
4.5SMACS_z16b|$15.32^{+0.16}_{-0.13}$|−20.96 ± 0.14|$8.80^{+0.44}_{-0.25}$||$57.5^{+38.0}_{-29.4}$|
4.6S5-z16 − 1|$16.41^{+0.66}_{-0.55}$|−21.6 ± 0.3|$8.59^{+1.23}_{-0.31}$||$5.1^{+21.7}_{-1.8}$|H23b, O22Inconsistent with fiducial, even challenging to maxSF

aSFR is averaged over 50 Myr except for JADES-GS-z12, JADES-GS-z13, and Maisie’s Galaxy in which 30, 30, and 10 Myr are considered, respectively.

bReferences are Adams et al. (2023b, AD23), Arrabal Haro et al. (2023, AH23), Atek et al. (2023, AT23), Bakx et al. (2023, B23), Curtis-Lake et al. (2023, CL23), Donnan et al. (2023a, D23a), Donnan et al. (2023b, D23b), Finkelstein et al. (2022, FI22), Furtak et al. (2023, FU23), Harikane et al. (2023a, b, H23ab), Naidu et al. (2022b, N22), Ono et al. (2022, O22), Popping (2023, P23), Robertson et al. (2023, R22), Santini et al. (2023, S23), and Zavala et al. (2023, Z23). cThis last column states whether the galaxy is consistent with our galaxy-formation models.

Table 1.
Open in new tab

Properties of the z ≳ 12 JWST targets explored in this work.

SectionIDzMUVlog10 (M*/M⊙)|$\mathrm{SFR}(\mathrm{M}_{\odot}\mathrm{yr}^{-1})^{\mathrm{a}}$|ReferencesbCommentsc
4.1JADES-GS-z13|$13.20^{+0.04}_{-0.07}$|−18.5 ± 0.2|$7.8^{+0.4}_{-0.5}$||$1.0_{-0.5}^{+1.0}$|CL23, R22, D23b, H23a
4.1JADES-GS-z12|$12.63^{+0.24}_{-0.08}$|−18.8 ± 0.1|$8.4^{+0.4}_{-0.7}$||$1.3_{-0.9}^{+1.9}$|CL23, R22, H23aConsistent with fiducial
4.2S5-z12 − 1|$12.58^{+1.23}_{-0.46}$|−20.2 ± 0.1|$8.53^{+0.61}_{-0.69}$||$5.5^{+4.7}_{-4.4}$|H23b
4.3GLz12|$12.2^{+0.1}_{-0.2}$|−21.0 ± 0.1|$9.1^{+0.3}_{-0.4}$||$6^{+5}_{-2}$|N22, B23, D23a, H23b, O22, P23, S23Consistent with fiducial but challenging
4.4Maisie’s Galaxy|$11.44^{+0.09}_{-0.08}$||$-20.32^{+0.08}_{-0.06}$||$8.50^{+0.29}_{-0.44}$||$2.1^{+4.8}_{-2.0}$|FI22, AH23, D23a, H23ab, O22, Z23
4.5SMACS_z16a|$15.92^{+0.17}_{-0.15}$|−20.59 ± 0.15|$8.79^{+0.32}_{-0.33}$||$16.6^{+2.9}_{-16.4}$|AT23, AD23, FU23, H23bInconsistent with fiducial, requiring maxSF
4.5SMACS_z16b|$15.32^{+0.16}_{-0.13}$|−20.96 ± 0.14|$8.80^{+0.44}_{-0.25}$||$57.5^{+38.0}_{-29.4}$|
4.6S5-z16 − 1|$16.41^{+0.66}_{-0.55}$|−21.6 ± 0.3|$8.59^{+1.23}_{-0.31}$||$5.1^{+21.7}_{-1.8}$|H23b, O22Inconsistent with fiducial, even challenging to maxSF
SectionIDzMUVlog10 (M*/M⊙)|$\mathrm{SFR}(\mathrm{M}_{\odot}\mathrm{yr}^{-1})^{\mathrm{a}}$|ReferencesbCommentsc
4.1JADES-GS-z13|$13.20^{+0.04}_{-0.07}$|−18.5 ± 0.2|$7.8^{+0.4}_{-0.5}$||$1.0_{-0.5}^{+1.0}$|CL23, R22, D23b, H23a
4.1JADES-GS-z12|$12.63^{+0.24}_{-0.08}$|−18.8 ± 0.1|$8.4^{+0.4}_{-0.7}$||$1.3_{-0.9}^{+1.9}$|CL23, R22, H23aConsistent with fiducial
4.2S5-z12 − 1|$12.58^{+1.23}_{-0.46}$|−20.2 ± 0.1|$8.53^{+0.61}_{-0.69}$||$5.5^{+4.7}_{-4.4}$|H23b
4.3GLz12|$12.2^{+0.1}_{-0.2}$|−21.0 ± 0.1|$9.1^{+0.3}_{-0.4}$||$6^{+5}_{-2}$|N22, B23, D23a, H23b, O22, P23, S23Consistent with fiducial but challenging
4.4Maisie’s Galaxy|$11.44^{+0.09}_{-0.08}$||$-20.32^{+0.08}_{-0.06}$||$8.50^{+0.29}_{-0.44}$||$2.1^{+4.8}_{-2.0}$|FI22, AH23, D23a, H23ab, O22, Z23
4.5SMACS_z16a|$15.92^{+0.17}_{-0.15}$|−20.59 ± 0.15|$8.79^{+0.32}_{-0.33}$||$16.6^{+2.9}_{-16.4}$|AT23, AD23, FU23, H23bInconsistent with fiducial, requiring maxSF
4.5SMACS_z16b|$15.32^{+0.16}_{-0.13}$|−20.96 ± 0.14|$8.80^{+0.44}_{-0.25}$||$57.5^{+38.0}_{-29.4}$|
4.6S5-z16 − 1|$16.41^{+0.66}_{-0.55}$|−21.6 ± 0.3|$8.59^{+1.23}_{-0.31}$||$5.1^{+21.7}_{-1.8}$|H23b, O22Inconsistent with fiducial, even challenging to maxSF

aSFR is averaged over 50 Myr except for JADES-GS-z12, JADES-GS-z13, and Maisie’s Galaxy in which 30, 30, and 10 Myr are considered, respectively.

bReferences are Adams et al. (2023b, AD23), Arrabal Haro et al. (2023, AH23), Atek et al. (2023, AT23), Bakx et al. (2023, B23), Curtis-Lake et al. (2023, CL23), Donnan et al. (2023a, D23a), Donnan et al. (2023b, D23b), Finkelstein et al. (2022, FI22), Furtak et al. (2023, FU23), Harikane et al. (2023a, b, H23ab), Naidu et al. (2022b, N22), Ono et al. (2022, O22), Popping (2023, P23), Robertson et al. (2023, R22), Santini et al. (2023, S23), and Zavala et al. (2023, Z23). cThis last column states whether the galaxy is consistent with our galaxy-formation models.

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