Autor: |
Riffel, Rogério, Mallmann, Nicolas D, Ilha, Gabriele S, Storchi-Bergmann, Thaisa, Riffel, Rogemar A, Rembold, Sandro B, Bizyaev, Dmitry, do Nascimento, Janaina C, Schimoia, Jaderson S, da Costa, Luiz N, Boardman, Nicholas Fraser, Boquien, Médéric, Couto, Guilherme S |
Předmět: |
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Zdroj: |
Monthly Notices of the Royal Astronomical Society; Aug2024, Vol. 532 Issue 2, p2485-2489, 5p |
Abstrakt: |
This document is a correction to a paper titled "Determining star-formation rates in active galactic nuclei hosts via stellar population synthesis." The correction addresses an inconsistency in the value of |$H_0$| used in the analysis. The authors have now adopted a uniform value of |$H_0=73.0$| km s|$^{-1}$| Mpc|$^{-1}$| for both star-formation rates (SFR|$_\\star$| and SFR|$_{Gas}$|). As a result, some figures and the transformation equation have been updated. The conclusions of the paper remain unchanged. The document provides the corrected equations and figures for reference. [Extracted from the article] |
Databáze: |
Complementary Index |
Externí odkaz: |
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