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Energy balance SED modelling can be effective at high redsh..:
Haskell, P
;
Smith, D J B
;
Cochrane, R K
..
Monthly Notices of the Royal Astronomical Society. 525 (2023) 1 - p. 1535-1552 , 2023
Link:
https://doi.org/10.1093/mnras/stad2315
RT Journal T1 <Title>Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets</Title> UL https://suche.suub.uni-bremen.de/peid=cr-10.1093_mnras_stad2315&Exemplar=1&LAN=DE A1 Haskell, P A1 Smith, D J B A1 Cochrane, R K A1 Hayward, C C A1 Anglés-Alcázar, D PB Oxford University Press (OUP) YR 2023 SN 0035-8711 SN 1365-2966 JF Monthly Notices of the Royal Astronomical Society VO 525 IS 1 SP 1535 OP 1552 LK http://dx.doi.org/https://doi.org/10.1093/mnras/stad2315 DO https://doi.org/10.1093/mnras/stad2315 SF ELIB - SuUB Bremen
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