Science1 publisherNot yet confirmed elsewhere3 min readPublished
Astronomers confirm a redshift-4.946 radio galaxy that may be the most powerful known
INAF-led astronomers place radio galaxy TXS 2354+015 at redshift 4.946 and, in a preprint, rank it the most powerful radio galaxy known. Most radio searches use a steep-spectrum filter that misses it, so early radio-galaxy counts built on that filter likely run short.
The Scientist · Science desk

What happened
- A team led by Barbara Balmaverde of INAF's Turin observatory matched Subaru Hyper Suprime-Cam imaging with TGSS and VLASS radio catalogs to find optical dropouts at redshift 4.5 to 5.3.
- Spectroscopy showed a strong Lyman-alpha line, checked against a second, fainter line, making TXS 2354+015 the second-most-distant radio galaxy known.
- The team ruled out a chance alignment using the precise radio-optical position match, the rarity of the radio brightness and the expected radio-to-optical ratio.
Compiled by The ScientistSomething wrong?How this is made
Why it matters
- decision Groups building samples of the earliest radio galaxies now have grounds to run optical-dropout selection alongside steep-spectrum cuts, since the current power record holder fails those cuts.
- constraint Dropout selection still needs visible optical light, so the up-to-90% of early sources a 2024 study says may be dark in that band remain hard to find and confirm by this route.
- capability Feedback simulations gain an extreme jet source from under 1.2 billion years after the Big Bang to check against, though the host-mass estimate is too uncertain for a firm jet-to-host comparison.
Jets like this one matter to galaxy models because of feedback. The energy they carry can influence star formation in the host and heat its surrounding gas, and simulations build in this AGN feedback to predict the right number of galaxies in the universe [13]. Powerful radio galaxies in the early universe also tend to sit where the most massive, earliest-forming galaxies and clusters are [14]. TXS 2354+015 adds an extreme example from when the universe was less than 1.2 billion years old [5]. Testing feedback with it would take a further measurement: what the jets have done to the host's stars and gas.
The host mass is the shakiest number in the paper. The team estimates around 2 trillion solar masses, putting the galaxy among the brightest known [10]. Any comparison of jet power against the galaxy hosting it inherits the problem the authors flag. "This estimate is clearly plagued by several large uncertainties, in particular by the age of the stellar population," they wrote [11].
The power ranking comes from the team's own comparison with the literature. According to the preprint, its estimated radio power at 500 MHz exceeds that of the previous record-holder from a 2008 census, and no other known high-redshift radio galaxy matches it [1]. "TXS 2354+015, thus, appears to be the most powerful radio galaxy known to date," the team wrote [2].
I think the more durable result is how it was found. The dominant way to hunt distant radio galaxies flags sources with unusually steep radio spectra, and that approach appears to miss a large portion of the true population [4]. TXS 2354+015 does not meet the ultra-steep-spectrum criteria [3]. It surfaced through the Lyman-break technique instead. Intervening clouds of neutral hydrogen absorb ultraviolet light, so a very distant galaxy's optical spectrum drops off abruptly [16]. The search window, redshift 4.5 to 5.3, covers the era when the universe was 1.1 billion to 1.3 billion years old [7]. That is about 200 million years of cosmic time [17]. So the most powerful radio galaxy on record is one the standard filter would have passed over [3].
One object does not measure how incomplete the standard method is. The report does not say how many dropout candidates the search returned or how many were confirmed. Dropout selection has its own limit, too: it works only on radio sources with a detectable optical counterpart [7]. In most powerful early radio galaxies, dusty gas hides the black hole and its surroundings, and only the radio jet escapes to be seen directly [15]. A 2024 study suggests as many as 90% of these sources beyond redshift 3.5 might be hidden in the ultraviolet and optical bands [12]. If that figure holds, an optical search reaches as few as one in ten of them [18]. The obscured remainder would show no optical dropout at all, and such sources are hard to find and confirm spectroscopically by any route [12].
What to watch
- Peer review of the Sept. 23 preprint, and whether independent radio measurements uphold the 500 MHz power ranking against the 2008 record-holder.
- Observations that pin down the host's stellar population age, which the team names as the main uncertainty in its 2-trillion-solar-mass estimate.
- Further confirmations from the same Subaru-plus-radio dropout search that also fail steep-spectrum criteria, which would turn one case into a measure of how much the standard method misses.