Multi-chamber cardioids unravel human heart development and cardiac defects.

The number one cause of human fetal death are defects in heart development. Because the human embryonic heart is inaccessible and the impacts of mutations, drugs, and environmental factors on the specialized functions of different heart compartments are not captured by in vitro models, determining the underlying causes is difficult. Here, we established a human cardioid platform that recapitulates the development of all major embryonic heart compartments, including right and left ventricles, atria, outflow tract, and atrioventricular canal. By leveraging 2D and 3D differentiation, we efficiently generated progenitor subsets with distinct first, anterior, and posterior second heart field identities. This advance enabled the reproducible generation of cardioids with compartment-specific in vivo-like gene expression profiles, morphologies, and functions. We used this platform to unravel the ontogeny of signal and contraction propagation between interacting heart chambers and dissect how mutations, teratogens, and drugs cause compartment-specific defects in the developing human heart.

The Transcriptomic Landscape of Pediatric Astrocytoma.

Central nervous system tumors are the most common solid neoplasia during childhood and represent one of the leading causes of cancer-related mortality. Tumors arising from astrocytic cells (astrocytomas) are the most frequently diagnosed, and according to their histological and pathological characteristics, they are classified into four categories. However, an additional layer of molecular classification considering the DNA sequence of the tumorigenesis-associated genes IDH1/2 and H3F3A has recently been incorporated into the classification guidelines. Although mutations in H3F3A are found exclusively in a subtype of grade IV pediatric astrocytoma, mutations in IDH1/2 genes are very rare in children under 14 years of age. The transcriptomic profiles of astrocytoma in adults and children have been extensively studied. However, there is scarce information on these profiles in pediatric populations considering the status of tumorigenesis-associated genes. Therefore, here we report the transcriptomic landscape of the four grades of pediatric astrocytoma by RNA sequencing. We found several well-documented biological functions associated with the misregulated genes in the four grades of astrocytoma, as well as additional biological pathways. Among the four grades of astrocytoma, we found shared misregulated genes that could have implications in tumorigenesis. Finally, we identified a transcriptional signature for almost all grades of astrocytoma that could be used as a transcription-based identification method.

Evaluation of the melting temperature of TaqMan probes as a genotyping method for IDH1, IDH2, and H3F3A in pediatric astrocytomas.

Background: Astrocytomas are cancer tumors of the central nervous system and represent the most common type of solid tumors during human childhood. In 2016, the World Health Organization established a molecular classification system to regroup tumor entities to achieve a more accurate diagnosis and a better clinical decision-making and selection of treatment in patients with these types of tumors. Methods: We evaluated a genotyping assay for rapid and cost-effective mutation detection in astrocytomas using TaqMan probes in an asymmetric polymerase chain reaction (PCR) assay. Results: Four diffuse astrocytomas (Grade II), three anaplastic astrocytomas (Grade III), and four glioblastomas (Grade IV) were sequenced, and all of them displayed the wild-type (WT) sequence. We tried to set up this melting analysis for the genotyping of pediatric astrocytomas by identifying the specific melting temperatures of the TaqMan probes due to the presence of the WT sequences in the isocitrate dehydrogenase 1 and 2 (IDH1 and IDH2) and H3.3 histone A genes (H3F3A). We used an IDH1-TaqMan probe to identify the WT status of IDH1 in two different WT deoxyribonucleic acid (DNA) templates (pilocytic and diffuse astrocytoma) and obtained four melting temperature values ranged from 65.6 to 92.2°C. Furthermore, only four out of 29 reactions displayed amplification of the DNA template. Sanger sequencing was faster and more reliable to detect the gene status in all the sequenced samples. Conclusions: We conclude that conventional Sanger sequencing remains the gold standard for the genotyping of pediatric astrocytomas.

Introducción: Los astrocitomas son un tipo de cáncer que afecta al sistema nervioso central y representan el tumor sólido más común durante la infancia. En el año 2016, la Organización Mundial de la Salud estableció un sistema de clasificación molecular para reagrupar tumores con identidades genéticas similares y lograr un diagnóstico más preciso, lo que lleva a tomar las decisiones clínicas idóneas al elegir el tratamiento de pacientes con este tipo de tumores. Métodos: Se evaluó un protocolo que involucra el uso de sondas TaqMan en un ensayo de reacción en cadena de la polimerasa asimétrica para la detección de mutaciones en astrocitomas. Se secuenciaron cuatro astrocitomas difusos (Grado II), tres astrocitomas anaplásicos (Grado III) y cuatro glioblastomas (Grado IV). Se intentó establecer las condiciones del análisis para la genotipificación de los astrocitomas pediátricos mediante la identificación de las temperaturas de disociación específicas de las sondas TaqMan producidas por la prescencia de las secuancias WT en los genes isocitrato deshidrogenasa 1 y 2 (IDH1, IDH2) y H3.3 histona A (H3F3A). Resultados: Los astrocitomas mostraron la secuencia wild type (WT) (silvestre) de los genes. Se utilizó una sonda TaqMan IDH1 para identificar el estado de este gen en dos templados WT de DNA (astrocitoma pilocítico y difuso) y se obtuvieron cuatro valores de temperatura de disociación (65.6-92.2 °C). Solo cuatro de las 29 reacciones mostraron amplificación de DNA. La secuenciación de Sanger fue más rápida y confiable para detectar el estado de los genes en todas las muestras. Conclusiones: La secuenciación de Sanger sigue siendo la técnica más práctica para la genotipificación de astrocitomas pediátricos.

Evaluation of the melting temperature of TaqMan probes as a genotyping method for IDH1, IDH2, and H3F3A in pediatric astrocytomas / Evaluación del método de temperatura de disociación de sondas TaqMan para la genotipificación de IDH1, IDH2 y H3F3A en astrocitomas pediátricos

Abstract Background: Astrocytomas are cancer tumors of the central nervous system and represent the most common type of solid tumors during human childhood. In 2016, the World Health Organization established a molecular classification system to regroup tumor entities to achieve a more accurate diagnosis and a better clinical decision-making and selection of treatment in patients with these types of tumors. Methods: We evaluated a genotyping assay for rapid and cost-effective mutation detection in astrocytomas using TaqMan probes in an asymmetric polymerase chain reaction (PCR) assay. Results: Four diffuse astrocytomas (Grade II), three anaplastic astrocytomas (Grade III), and four glioblastomas (Grade IV) were sequenced, and all of them displayed the wild-type (WT) sequence. We tried to set up this melting analysis for the genotyping of pediatric astrocytomas by identifying the specific melting temperatures of the TaqMan probes due to the presence of the WT sequences in the isocitrate dehydrogenase 1 and 2 (IDH1 and IDH2) and H3.3 histone A genes (H3F3A). We used an IDH1-TaqMan probe to identify the WT status of IDH1 in two different WT deoxyribonucleic acid (DNA) templates (pilocytic and diffuse astrocytoma) and obtained four melting temperature values ranged from 65.6 to 92.2°C. Furthermore, only four out of 29 reactions displayed amplification of the DNA template. Sanger sequencing was faster and more reliable to detect the gene status in all the sequenced samples. Conclusions: We conclude that conventional Sanger sequencing remains the gold standard for the genotyping of pediatric astrocytomas.

Resumen Introducción: Los astrocitomas son un tipo de cáncer que afecta al sistema nervioso central y representan el tumor sólido más común durante la infancia. En el año 2016, la Organización Mundial de la Salud estableció un sistema de clasificación molecular para reagrupar tumores con identidades genéticas similares y lograr un diagnóstico más preciso, lo que lleva a tomar las decisiones clínicas idóneas al elegir el tratamiento de pacientes con este tipo de tumores. Métodos: Se evaluó un protocolo que involucra el uso de sondas TaqMan en un ensayo de reacción en cadena de la polimerasa asimétrica para la detección de mutaciones en astrocitomas. Se secuenciaron cuatro astrocitomas difusos (Grado II), tres astrocitomas anaplásicos (Grado III) y cuatro glioblastomas (Grado IV). Se intentó establecer las condiciones del análisis para la genotipificación de los astrocitomas pediátricos mediante la identificación de las temperaturas de disociación específicas de las sondas TaqMan producidas por la prescencia de las secuancias WT en los genes isocitrato deshidrogenasa 1 y 2 (IDH1, IDH2) y H3.3 histona A (H3F3A). Resultados: Los astrocitomas mostraron la secuencia wild type (WT) (silvestre) de los genes. Se utilizó una sonda TaqMan IDH1 para identificar el estado de este gen en dos templados WT de DNA (astrocitoma pilocítico y difuso) y se obtuvieron cuatro valores de temperatura de disociación (65.6-92.2 °C). Solo cuatro de las 29 reacciones mostraron amplificación de DNA. La secuenciación de Sanger fue más rápida y confiable para detectar el estado de los genes en todas las muestras. Conclusiones: La secuenciación de Sanger sigue siendo la técnica más práctica para la genotipificación de astrocitomas pediátricos.