Early Growth of the Star Formation Rate Function in the Epoch of Reionization: An Approach with Rest-frame Optical Emissions
Abstract
We present a star formation rate function (SFRF) at z ~ 6 based on star formation rates (SFRs) derived by spectral energy distribution fitting on data from rest-frame UV to optical wavelengths of galaxies in the CANDELS GOODS-South and North fields. The resulting SFRF shows an excess compared to the previous estimations by using rest-frame UV luminosity functions (LFs) corrected for the dust attenuation and is comparable to that estimated from a far-infrared LF. This suggests that the number density of dust-obscured intensively star-forming galaxies at z ~ 6 has been underestimated in the previous approach based only on rest-frame UV observations. We parameterize the SFRF using the Schechter function and obtain the best-fit parameter of the characteristic SFR (SFR*) when the faint-end slope and characteristic number density are fixed. The best-fit SFR* at z ~ 6 is comparable to that at z ~ 2, when the cosmic star formation activity reaches its peak. Together with SFRF estimations with a similar approach using rest-frame UV to optical data, the SFR* is roughly constant from z ~ 2 to ~6 and may decrease above z ~ 6. Since the SFR* is sensitive to the high-SFR end of the SFRF, this evolution of SFR* suggests that the high-SFR end of the SFRF grows rapidly during the epoch of reionization and reaches a similar level observed at z ~ 2.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- February 2024
- DOI:
- 10.3847/1538-4357/ad0e67
- arXiv:
- arXiv:2208.00749
- Bibcode:
- 2024ApJ...961..152A
- Keywords:
-
- Galaxy evolution;
- Galaxy formation;
- High-redshift galaxies;
- 594;
- 595;
- 734;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 24 pages, 14 figures, and 3 tables. Accepted for publication in ApJ