Aims The COVID-19 pandemic has caused strain on hospital systems and potential delay in diagnosis of type 1 diabetes (T1D). Outpatient diagnosis and treatment of metabolically stable young persons with new-onset T1D have been shown to be equivalent to inpatient. We describe an approach to outpatient management of newly diagnosed T1D during the COVID-19 pandemic using an interdisciplinary team, telemedicine, and diabetes technologies including rapid implementation of continuous glucose monitoring (CGM). Methods Following the onset of the COVID-19 pandemic, new-onset cases of T1D were tracked. After laboratory confirmation of diagnosis and metabolic stability, patients and families were referred for ambulatory initiation of insulin therapy and diabetes education. These cases were reviewed using data extracted from the electronic health record, comments from multidisciplinary team members, and cloud-based glucose data. Results We report on seven young people with new-onset T1D without diabetic ketoacidosis from April to June 2020, during the COVID-19 pandemic. https://www.selleckchem.com/products/hada-hydrochloride.html Ages ranged 9-23 years with presenting hemoglobin A1c (HbA1c) values 10-14.5%. Initial evaluation was generally face-to-face, followed by frequent telemedicine visits. Five patients had a family history of T1D. Two patients had access to at-home HbA1c kits prompting evaluation in the absence of symptoms. Four patients required emergency department evaluation. Five patients presented with ketosis. All patients were prescribed CGM at the first visit, most starting within 1 month. Conclusions Technology is extraordinarily useful for the care of young persons with new-onset T1D in the ambulatory setting during the COVID-19 pandemic. Large observational studies are needed to better understand outcomes of an outpatient, technology-focused approach.The aim of this study was to examine if the peripheral antinociception of α-bisabolol involve the participation of nitric oxide (NO) and cyclic guanosine monophosphate (cGMP) synthesis followed by K+ channel opening in the formalin test. Wistar rats were injected in the dorsal surface of the right hind paw with formalin (1%). Rats received a subcutaneous injection into the dorsal surface of the paw of vehicles or increasing doses of α-bisabolol (100-300 µg/paw). To determine whether the peripheral antinociception induced by α-bisabolol was mediated by either the opioid receptors or the NO-cGMP-K+ channels pathway, the effect of pretreatment (10 min before formalin injection) with the appropriate vehicles, naloxone, naltrexone, L-NAME, ODQ, glibenclamide, glipizide, apamin, charybdotoxin, tetraethylammonium or 4-aminopyridine on the antinociceptive effects induced by local peripheral α-bisabolol (300 µg/paw) were assessed. α-bisabolol produced antinociception during both phases of the formalin test. α-bisabolol antinociception was blocked by L-NAME, ODQ, and all the K+ channels blockers. The peripheral antinociceptive effect produced by α-bisabolol was not blocked by the opioid receptor inhibitors. α-bisabolol was able to active the NO-cGMP-K+ channels pathway in order to produce its antinoceptive effect. The participation of opioid receptors in the peripheral local antinociception induced by α-bisabolol is excluded.The emergence of West Nile Virus lineage 2 (WNV-2) has contributed to multiple major human outbreaks in Greece since 2010. Studies to date investigating biological and environmental factors that contribute to West Nile Virus (WNV) transmission have resulted in complex statistical models. We sought to examine open publicly available data to ascertain if a predictive risk assessment could be employed for WNV-2 in Greece. Based on accessible data, factors such as precipitation, temperature, and range of avian host species did not yield conclusive outcomes. However, by measuring the average rate of temperature change leading up to peak caseloads, we found a predictive characteristic to the timing of outbreaks. Detailed evolutionary studies revealed possible multiple introductions of WNV-2 in Europe, and that Greece acts through a source-sink inversion model, thereby allowing continued reseeding of WNV transmission each year by overwintering the Culex pipiens mosquito vector. Greece has proven an excellent model in WNV surveillance and has demonstrated the importance of rapid reporting for proper preparedness and response to vector-borne diseases.The martian meteorite ALH 84001 formed before ∼4.0 Ga, so it could have preserved information about habitability on early Mars and habitability since then. ALH 84001 is particularly important as it contains carbonate (and other) minerals that were deposited by liquid water, raising the chance that they may have formed in a habitable environment. Despite vigorous efforts from the scientific community, there is no accepted evidence that ALH 84001 contains traces or markers of ancient martian life-all the purported signs have been shown to be incorrect or ambiguous. However, the meteorite provides evidence for three distinct episodes of potentially habitable environments on early Mars. First is evidence that the meteorite's precursors interacted with clay-rich material, formed approximately at 4.2 Ga. Second is that igneous olivine crystals in ALH 84001 were partially dissolved and removed, presumably by liquid water. Third is, of course, the deposition of the carbonate globules, which occurred at ∼15-25°C and involved near-neutral to alkaline waters. The environments of olivine dissolution and carbonate deposition are not known precisely; hydrothermal and soil environments are current possibilities. By analogies with similar alteration minerals and sequences in the nakhlite martian meteorites and volcanic rocks from Spitzbergen (Norway), a hydrothermal environment is favored. As with the nakhlite alterations, those in ALH 84001 likely formed in a hydrothermal system related to a meteoroid impact event. Following deposition of the carbonates (at 3.95 Ga), ALH 84001 preserves no evidence of habitable environments, that is, interaction with water. The meteorite contains several materials (formed by impact shock at ∼3.9 Ga) that should have reacted readily with water to form hydrous silicates, but there is no evidence any formed.