The weaning process negatively affects the haematological parameters and innate immune response of dairy calves, even when managed under an intensive milk program. Here we describe haematological and innate immunity changes in 47 Holstein calves aged 69-85 days subjected to a gradual weaning process. Blood samples were collected at six (D-6), four (D-4), and two (D-2) days before and on the weaning day (D0) for the phagocytosis assay and to measure the production of reactive oxygen species (ROS) after stimulation with Staphylococcus aureus, Escherichia coli, and Mannhemia haemolytica, in addition to total protein (TP), haptoglobin (Hp), and iron concentration. The highest mean neutrophil number was recorded at D-2. The absolute number of monocytes was initially high on D-6 and D-4 but declined as the calf progressed to weaning. The number of basophils decreased rapidly, reaching a low value on D-4, and remained low for the remainder of the study period. The TP, Hp, and Fe concentrations decreased. Overall, polymorphonuclear leukocyte phagocytosis activity induced by S. aureus and E. coli decreased from D-6 to D-2, indicating persistence of the low phagocytosis rate for S. aureus. ROS production was constant for all bacterial stimulations from D-6 to D-2, followed by an increase on D0. Phagocytosis and ROS production indicate that the weaning process dampens the innate immune response relative to exposure to these common pathogenic bacteria in dairy calves. Phagocytosis and the corresponding indicators of intracellular killing activities (ROS production and myeloperoxidase index) represent the most accepted core mechanisms for the early elimination of pathogenic microorganisms in calves. Despite a slow gradual weaning management system, the study concluded that intensive milk production programs contribute to innate immune response suppression during weaning.

Distinguishing early domesticates from their wild progenitors presents a significant obstacle for understanding human-mediated effects in the past. The origin of dogs is particularly controversial because potential early dog remains often lack corroborating evidence that can provide secure links between proposed dog remains and human activity. The Tumat Puppies, two permafrost-preserved Late Pleistocene canids, have been hypothesized to have been littermates and early domesticates due to a physical association with putatively butchered mammoth bones. Through a combination of osteometry, stable isotope analysis, plant macrofossil analysis, and genomic and metagenomic analyses, this study exploits the unique properties of the naturally mummified Tumat Puppies to examine their familial relationship and to determine whether dietary information links them to human activities. The multifaceted analysis reveals that the 14,965–14,046 cal yr BP Tumat Puppies were littermates who inhabited a dry and relatively mild environment with heterogeneous vegetation and consumed a diverse diet, including woolly rhinoceros in their final days. However, because there is no evidence of mammoth consumption, these data do not establish a link between the canids and ancient humans.

The First Large Absorption Survey in H i (FLASH) is a large-area radio survey for neutral hydrogen in and around galaxies in the intermediate redshift range $0.4\lt z\lt1.0$, using the 21-cm H i absorption line as a probe of cold neutral gas. The survey uses the ASKAP radio telescope and will cover 24,000 deg$^2$ of sky over the next five years. FLASH breaks new ground in two ways – it is the first large H i absorption survey to be carried out without any optical preselection of targets, and we use an automated Bayesian line-finding tool to search through large datasets and assign a statistical significance to potential line detections. Two Pilot Surveys, covering around 3000 deg$^2$ of sky, were carried out in 2019-22 to test and verify the strategy for the full FLASH survey. The processed data products from these Pilot Surveys (spectral-line cubes, continuum images, and catalogues) are public and available online. In this paper, we describe the FLASH spectral-line and continuum data products and discuss the quality of the H i spectra and the completeness of our automated line search. Finally, we present a set of 30 new H i absorption lines that were robustly detected in the Pilot Surveys, almost doubling the number of known H i absorption systems at $0.4\lt z\lt1$. The detected lines span a wide range in H i optical depth, including three lines with a peak optical depth $\tau\gt1$, and appear to be a mixture of intervening and associated systems. Interestingly, around two-thirds of the lines found in this untargeted sample are detected against sources with a peaked-spectrum radio continuum, which are only a minor (5–20%) fraction of the overall radio-source population. The detection rate for H i absorption lines in the Pilot Surveys (0.3 to 0.5 lines per 40 deg$^2$ ASKAP field) is a factor of two below the expected value. One possible reason for this is the presence of a range of spectral-line artefacts in the Pilot Survey data that have now been mitigated and are not expected to recur in the full FLASH survey. A future paper in this series will discuss the host galaxies of the H i absorption systems identified here.