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Action Items Related to LAE Full Paper †
- SED fits for low-z emitters
- necessary to evaluate the efficiency of our photo-z determination to LAEs (i.e., to see the number of low-z emitter candidates with z_spec consistent with high-z LAEs)
- revising Tab. 5: number of LAEs in Step 3 and 4 and of the LAEs with EW0 >= 100 A
- revising Fig. 2: color-magnitude diagram
- revising Fig. 3: Donley+12 criteria
- revising Fig. 4: photo-z vs. spec-z
- revising Fig. 5: spatial distribution of LAEs
- revising Fig. 6: spatial distribution of LAEs at z=4.86 and 5.70
- revising Fig. 7: EWobs distribution
- revising Fig. 8: EW0 distribution
- revising Fig. 9: L(Lya) distribution
- revising Fig. 10: EW0--L(Lya) distribution
- revising Fig. 11: EW0--Mstar distribution w/ histogram
- revising Fig. 12: SFR(UV)--Mstar distribution
- revising Fig. 13: sSFR distribution separated into 3 groups according to Mstar
- revising Fig. 14: average SED normalized at lam = 1350 A separated into 3 panels
- revising Fig. A3: flowchart for the Step 3
- revising Fig. B1: observed SED of the strong LAEs w/ EW0 >= 100 A
Manuscript †
Fixed Action Items †
as of xxx †
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ms_LAE_COSMOS20.pdf 
