Approach offers greener route to amide-containing drugs via aldehydes
Intraductal papillary mucinous neoplasm and pancreatic cancer: opportunity knocks twice hamada, et al.
📕 doi.org/10.14309/ajg.
L, the wide variation in cancer risk necessitates prolonged surveillance for most patients. There is an unmet need to optimize surveillance strategies for patients with IPMNs to address the rising global mortality associated with pancreatic cancer and to balance early cancer detection against healthcare resource allocation. While published guidelines outline common risk factors of carcinoma derived from IPMN, the resource-intensive nature of surveillance underscores the need for more granular management strategies—a need not yet reflected in current recommendations. Moreover, it is important to appreciate that patients with IPMNs also face an elevated risk of developing pancreatic carcinoma arising concomitantly with IPMN. This type of carcinoma presents unique challenges for surveillance but also offers novel opportunities for the timely identification of incident pancreatic cancer.
An international team of astronomers has discovered a distant planetary system that challenges long-standing theories of how planets form. Across our galaxy, astronomers routinely observe a characteristic pattern in planetary systems: rocky planets orbiting close to their host star with gas giants farther away. Our own solar system follows this rule, with the inner planets: Mercury, Venus, Earth and Mars, composed of rock and iron, and the outer planets: Jupiter, Saturn, Uranus and Neptune being predominantly gaseous.
This pattern stems from a well-established theory of planet formation: intense radiation from the host star strips away gas accumulated by close-in planets, leaving behind bare rocky bodies. While further from the star, cooler conditions allow thick atmospheres to build, forming gaseous planets.
But a newly discovered planetary system orbiting the star LHS 1903 breaks this rule. The findings are published in Science.
Researchers have developed a solar cell system that uses mirrors to concentrate solar energy. In addition to electricity, it produces heat for a plant that will capture carbon from industrial emissions. The solar cells in the large pilot plant are a full 5 meters high and consist of many mirrors that are angled toward the solar cells to concentrate sunlight. They make it possible to collect the sun’s rays into concentrated solar energy, as well as heat that supports a plant designed to capture CO2.
“The system has been tested and validated. It is quite innovative and unique and stands out by storing heat in addition to the electrical current,” says SINTEF research scientist Alfredo Sanchez Garcia.
The energy from the plant will be used to capture carbon from industrial emissions.
Researchers at the Ribeirao Preto Blood Center and the Center for Cell-Based Therapy (CTC) conducted a study using the NK-92 cell line to test new models of chimeric antigen receptors (CARs) with specific costimulatory domains, such as 2B4 and DAP12. The tests showed that these components helped make the cells “ready to attack,” thereby increasing their ability to destroy tumors. The results were published in the journal Frontiers in Immunology.
The CTC is one of the Research, Innovation, and Dissemination Centers (RIDCs) supported by FAPESP. It is based at the Ribeirao Preto Blood Center and is linked to the general and teaching hospital (“Hospital das Clínicas”) of the Ribeirao Preto Medical School of the University of São Paulo (FMRP-USP).
CAR-based cell therapies are revolutionizing cancer treatment, especially for hematological tumors. However, although it is already known which components work best in CAR-T cells, many questions remain about which intracellular signals make CAR-NK cells more effective.
An enjoyable article exploring the science of reproduction in space. I appreciate the genuine curiosity and hopeful outlook here!
The annual SXSW conference in Austin, Texas, can be a bit overwhelming. What started as a fairly modest four-day music festival in 1987, drawing some 700 attendees, has become a ten-day extravaganza of panel presentations featuring celebrities and business leaders, film screenings, technology showcases, and—yes—music. These days hundreds of thousands of people converge on downtown Austin for “South By,” as it’s called by those in the know. When I was a graduate student at the University of Texas in the early 2000s, I always avoided the festival and its inevitable crowds, which was relatively easy to do since it tended to be held the same week as the university’s Spring Break.
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But when I received an invitation in 2023 to attend a SXSW panel presentation with the title “Sex in Space: Sex and Reproduction Beyond Earth,” I knew I had to go. After all, any plans to create a permanent settlement on Mars or elsewhere in space wouldn’t last long if we can’t have kids there.
A thorough study exploring how astrocytes affect fear conditioning and fear extinction in the basolateral amygdala of mice. Subpopulations of astrocytes were found to interact with neurons in such a way as to help encode representations of fear. [ https://www.nature.com/articles/s41586-025-10068-0](https://www.nature.com/articles/s41586-025-10068-0)
Gq G-protein-coupled receptor (GPCR) signalling increases astrocyte Ca2+ activity through IP3-mediated release of intracellular Ca2+ stores42,43 and hM3Dq actuation causes a Ca2+ surge preceded by prolonged quiescence, possibly due to intracellular Ca2+ depletion24,44,45. Replicating these effects in the BLA, we expressed hM3Dq in BLA astrocytes and used in vivo cyto-GCaMP6f photometry and observed that clozapine–N-oxide (CNO) injection markedly increased Ca2+ activity within around 10 min but, thereafter, decreased and remained low for at least 2 h (Fig. 2c and Extended Data Figs. 6a–e and 8e, f). A lower hM3Dq virus concentration or lower CNO dose had modest or negligible effects on Ca2+ activity and behaviour (Extended Data Fig. 6h–p). On the basis of these data, we posited that BLA astrocyte Ca2+ dynamics would be constrained by hM3Dq actuation at timepoints relevant to behavioural testing. Consistent with this supposition, hM3Dq-actuation essentially abolished Ca2+ responses to a potent stimulus (footshock) given 30 min after CNO injection (Extended Data Fig. 6f, g).
We leveraged these effects of hM3Dq actuation to test how constraining astrocyte Ca2+ dynamics affected memory acquisition, retrieval, consolidation and extinction by injecting separate groups of animals with 3 mg per kg CNO either before or immediately after F-Con, or before fear retrieval/extinction training. We found that CNO given before extinction training reduced CS-related freezing during E-Ext—consistent with impaired memory retrieval—in hM3Dq-expressing mice compared with viral controls (Fig. 2d, e). In vivo fibre photometry confirmed that this behavioural effect was accompanied by loss of CS-related astrocyte Ca2+ responses (Fig. 2f and Extended Data Fig. 7a–c). In contrast to these memory-retrieval-impairing effects, CNO had no behavioural effect when injected before or after F-Con26,27 and did not alter uncued freezing, shock-induced flinching or various measures of anxiety-like behaviour (Extended Data Fig. 7d–i). Behavioural effects were also absent when CNO was injected in mice not expressing hM3Dq or when vehicle was injected in hM3Dq-expressing animals, excluding potential non-specific CNO and hM3Dq-virus effects, respectively (Extended Data Fig. 7j–n).
We next compared these effects with those of another DREADD, hM4Di, that produces effects on cortical, striatal and (as we show here; Fig. 2g–i) BLA astrocyte Ca2+ activity that mirror those of hM3Dq, that is, increase Ca2+ transients24,46,47. Accordingly, we found that hM4Di actuation produced effects on memory retrieval that were opposite to hM3Dq: pre-Ext CNO injection produced increases in CS-related freezing and astrocyte Ca2+ responses during E-Ext in hM4Di-expressing mice compared with viral controls (Fig. 2j–l and Extended Data Fig. 8a–f). Pre-Ext hM4Di actuation also increased freezing during (CNO-free) E-Ret, indicative of a deficit in extinction memory formation, and attenuated CS-related Ca2+ activity during this test stage. This latter effect is notable given that hM3Dq actuation produced a similar extinction deficit and blunted the CS-related Ca2+ response on E-Ret (Fig. 2e and Extended Data Fig. 7b), despite the two manipulations having opposite effects on fear retrieval and neither affecting extinction memory when CNO was given before E-Ret (Extended Data Fig. 8g, h). This convergence of extinction-impairing effects suggests that extinction is sensitive to perturbations—whether increases or decreases—in astrocyte Ca2+ activity and, by extension, implies an important role for BLA astrocytes in the plastic adaptations underlying extinction memory formation.
ROS derived from NADPH oxidase, particularly NOX2, are central to antimicrobial defense, coupling direct pathogen killing with redox signaling that shapes inflammation. This narrative review integrates recent advances on NOX2 structure, assembly, and spatiotemporal control in phagocytes, and outlines how ROS interact with NF-κB, MAPK, and Nrf2 networks to coordinate microbicidal activity and immune modulation. We summarize evidence that both ROS deficiency, as in chronic granulomatous disease, and uncontrolled excess, as in sepsis and severe COVID-19, drive clinically significant pathology, emphasizing the need for precise redox balance.