Joint analysis constraints on the physics of the first galaxies with low-frequency radio astronomy data

• Published in: Monthly notices of the Royal Astronomical Society 2024-01, Vol.527 (1), p.813-827
• Main Authors: Bevins, Harry T J, Heimersheim, Stefan, Abril-Cabezas, Irene, Fialkov, Anastasia, de Lera Acedo, Eloy, Handley, William, Singh, Saurabh, Barkana, Rennan
• Format: Article
• Language: English
• Subjects: Antenna arrays; Big bang cosmology; Constraints; Data analysis; Datasets; Emission spectra; Emitters; Galaxies; Hydrogen; Ionization; LF radio; Luminosity; Machine learning; Power spectra; Radio astronomy; Radio emission; Radio signals; Radio spectra; Red shift; Spectral emittance; Spectrum allocation; Star & galaxy formation; Star formation; X-ray astronomy
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stad3194

ABSTRACT The first billion years of cosmic history remains largely unobserved. We demonstrate, using a novel machine learning technique, how combining upper limits on the spatial fluctuations in the 21-cm signal with observations of the sky-averaged 21-cm signal from neutral hydrogen can improve our understanding of this epoch. By jointly analysing data from the Shaped Antenna measurement of the background RAdio Spectrum (SARAS3, redshift z ≈ 15−25) and limits from the Hydrogen Epoch of Reionization Array (HERA, z ≈ 8 and 10), we show that such a synergetic analysis provides tighter constraints on the astrophysics of galaxies 200 million years after the big bang than can be achieved with the individual data sets. Although our constraints are weak, this is the first time data from a sky-averaged 21-cm experiment and power spectrum experiment have been analysed together. In synergy, the two experiments leave only $64.9^{+0.3}_{-0.1}$ per cent of the explored broad theoretical parameter space to be consistent with the joint data set, in comparison to $92.3^{+0.3}_{-0.1}$ per cent for SARAS3 and $79.0^{+0.5}_{-0.2}$ per cent for HERA alone. We use the joint analysis to constrain star formation efficiency, minimum halo mass for star formation, X-ray luminosity of early emitters, and the radio luminosity of early galaxies. The joint analysis disfavours at 68 per cent confidence a combination of galaxies with X-ray emission that is ≲33 and radio emission that is ≳32 times as efficient as present day galaxies. We disfavour at 95 per cent confidence scenarios in which power spectra are ≥126 mK2 at z = 25 and the sky-averaged signals are ≤−277 mK.