MAESTLO のバックアップ(No.4) - PukiWiki

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Action Items Related to MAESTLO †

evaluating SFR(UV) instead of SFR(SED)
- to make the error-bar of SFR smaller
- L_lam @ lambda = 1500 +/- 150 A and E(B-V) of the best-fit model SED --[Kennicutt98 relation]--> SFR(UV)

making the Figure and Table for AGN-MAESTLO in the same format with Fig. 1 and Tab. 1 of the MAESTLO paper

revising Fig. 3 (SFR vs. Mstar): grayscale for the galaxies @ z = 2.5--3.5 (redshift range of the old MAESTLO samples) --> z = 2.5--3.1 (redshift range of the new MAESTLO samples)

Manuscript †

ApJL submitted version (2015/05/25): ms.pdf ms.tex

Figures †

ApJL submitted version (2015/05/25):
- Fig. 1: f1.eps
- Fig. 2: f2.eps
- Fig. 3: f3.eps
- Fig. 4: f4.eps

Fixed Action Items †

as of xxx †