A luminous fast radio burst that probes the Universe at redshift 1.

Fast radio bursts (FRBs) are millisecond-duration pulses of radio emission originating from extragalactic distances. Radio dispersion is imparted on each burst by intervening plasma, mostly located in the intergalactic medium. In this work, we observe the burst FRB 20220610A and localize it to a morphologically complex host galaxy system at redshift 1.016 ± 0.002. The burst redshift and dispersion measure are consistent with passage through a substantial column of plasma in the intergalactic medium and extend the relationship between those quantities measured at lower redshift. The burst shows evidence for passage through additional turbulent magnetized plasma, potentially associated with the host galaxy. We use the burst energy of 2 × 1042 erg to revise the empirical maximum energy of an FRB.

A single fast radio burst localized to a massive galaxy at cosmological distance.

Fast radio bursts (FRBs) are brief radio emissions from distant astronomical sources. Some are known to repeat, but most are single bursts. Nonrepeating FRB observations have had insufficient positional accuracy to localize them to an individual host galaxy. We report the interferometric localization of the single-pulse FRB 180924 to a position 4 kiloparsecs from the center of a luminous galaxy at redshift 0.3214. The burst has not been observed to repeat. The properties of the burst and its host are markedly different from those of the only other accurately localized FRB source. The integrated electron column density along the line of sight closely matches models of the intergalactic medium, indicating that some FRBs are clean probes of the baryonic component of the cosmic web.

The dispersion-brightness relation for fast radio bursts from a wide-field survey.

Despite considerable efforts over the past decade, only 34 fast radio bursts-intense bursts of radio emission from beyond our Galaxy-have been reported1,2. Attempts to understand the population as a whole have been hindered by the highly heterogeneous nature of the searches, which have been conducted with telescopes of different sensitivities, at a range of radio frequencies, and in environments corrupted by different levels of radio-frequency interference from human activity. Searches have been further complicated by uncertain burst positions and brightnesses-a consequence of the transient nature of the sources and the poor angular resolution of the detecting instruments. The discovery of repeating bursts from one source3, and its subsequent localization4 to a dwarf galaxy at a distance of 3.7 billion light years, confirmed that the population of fast radio bursts is located at cosmological distances. However, the nature of the emission remains elusive. Here we report a well controlled, wide-field radio survey for these bursts. We found 20, none of which repeated during follow-up observations between 185-1,097 hours after the initial detections. The sample includes both the nearest and the most energetic bursts detected so far. The survey demonstrates that there is a relationship between burst dispersion and brightness and that the high-fluence bursts are the nearby analogues of the more distant events found in higher-sensitivity, narrower-field surveys5.

A radio counterpart to a neutron star merger.

Gravitational waves have been detected from a binary neutron star merger event, GW170817. The detection of electromagnetic radiation from the same source has shown that the merger occurred in the outskirts of the galaxy NGC 4993, at a distance of 40 megaparsecs from Earth. We report the detection of a counterpart radio source that appears 16 days after the event, allowing us to diagnose the energetics and environment of the merger. The observed radio emission can be explained by either a collimated ultrarelativistic jet, viewed off-axis, or a cocoon of mildly relativistic ejecta. Within 100 days of the merger, the radio light curves will enable observers to distinguish between these models, and the angular velocity and geometry of the debris will be directly measurable by very long baseline interferometry.

Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.

The largest galaxies in the universe reside in galaxy clusters. Using sensitive observations of carbon monoxide, we show that the Spiderweb galaxy-a massive galaxy in a distant protocluster-is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched intergalactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift.

Increased rat testicular heme oxygenase activity associated with depressed microsomal heme and cytochrome P-450 levels after repeated administration of human chorionic gonadotropin.

Repeated administration of human chorionic gonadotropin to rats results in a maximal depression of testicular microsomal heme and cytochrome P-450 levels at 24 h, followed by increases that plateau at pretreatment levels by day six. Associated with the depressed levels of microsomal heme and cytochrome P-450 is an increase of testicular microsomal heme oxygenase activity at 12-24 h. Testicular mitochondrial delta-aminolevulinic acid synthase activity was increased at 24 h, and remained elevated throughout the 9-day treatment period. Pretreatment with 1,4,6-androstatrien-3,17-dione, an aromatase inhibitor, failed to prevent the depression of testicular microsomal heme or cytochrome P-450 or increased heme oxygenase activity caused by repeated administration of human chorionic gonadotropin, and administration of estradiol benzoate failed to alter testicular microsomal heme oxygenase activity suggesting that these parameters were not related to altered testicular estrogen content caused by increased aromatase activity. These results suggest that increased testicular heme oxygenase activity is associated with decreased microsomal heme and cytochrome P-450 content during human chorionic gonadotropin-induced desensitization.

Inhibition of the biosynthesis of uroporphyrinogen and heme in rat liver during obstructive jaundice produced by bile duct ligation.

Altered hepatic microsomal drug metabolism has been reported to occur in afflicted with hyperbilirubinemia. Similarities of the chemical structures of hydroxymethylbilane, an intermediate in the biosynthesis of uroporphyrinogen, to bilirubin prompted investigations of the effect of bilirubin on the activity of uroporphyrinogen I synthase (porphobilinogen deaminase, EC 4.3.1.8) and the biosynthesis of heme. Bilirubin was found to be a reversible, noncompetitive inhibitor of uroporphyrinogen I synthase. The inhibition constant (Ki) for bilirubin was 1.5 microM. Bile acids had no effect on rat hepatic uroporphyrinogen I synthase activity. Hyperbilirubinemia was achieved in rats by biliary ligation in order to investigate whether elevated levels of bilirubin impair the biosynthesis of hepatic heme in vivo. The relative rate of heme biosynthesis, as measured by the rate of incorporation of delta-[4-14C]aminolevulinic acid into heme, was decreased 59% 24 h after biliary obstruction. The levels of hepatic microsomal heme and cytochrome P-450 were decreased by 43 and 40%, respectively, 72 h after biliary obstruction. The activities of hepatic delta-aminolevulinic acid synthase and uroporphyrinogen I synthase were increased by 39 and 46%, respectively, 72 h after biliary obstruction. During the 48- to 72-h period following biliary obstruction, the urinary excretion of porphobilinogen and uroporphyrin was increased 3.0- and 3.5-fold, respectively, whereas, the urinary excretion of delta-aminolevulinic acid was not altered. During this 48-to 72-h time interval following biliary obstruction, 100% of the uroporphyrin was excreted as isomer I. These results indicate that bilirubin is capable of depressing the biosynthesis of rat hepatic heme and thus cytochrome P-450-mediated drug metabolism by inhibition of the formation of uroporphyrinogen. These findings are a plausible mechanism for reports of impaired clearance of various drugs in patients afflicted with hyperbilirubinemic disease states.

Activation of liver tryptophan oxygenase by hydrocortisone, hematin and tryptophan in streptozotocin-diabetic rats.

This study compared changes in liver tryptophan oxygenase (TPO) activity in response to hydrocortisone, hematin and tryptophan administration to non-diabetic and diabetic (streptozotocin) rats. Hydrocortisone caused similar increases in apoenzyme (inactive), holoenzyme (heme-saturated) and total (holoenzyme + apoenzyme) TPO activities in non-diabetic and diabetic rats. The ability of hematin to increase total TPO activity was significantly less in diabetic rats. The largest differences between diabetic and non-diabetic rats were found with tryptophan which increased total TPO and holoenzyme activities 300% and 650% respectively in non-diabetic rats. However, tryptophan increased both apoenzyme (unchanged in non-diabetic rats) and holoenzyme activities by 300% in diabetic rats. These results indicate that in the diabetic state, the TPO-heme conjugation process is impaired, especially substrate mediated TPO-heme saturation.