Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages

HOXA1 drives melanoma tumor growth and metastasis and elicits an invasion gene expression signature that prognosticates clinical outcome

Dermatology-oncolog

Proinvasion Metastasis Drivers in Early-Stage Melanoma Are Oncogenes

Dermatology-oncolog

In Vivo Genetic Screens of Patient-Derived Tumors Revealed Unexpected Frailty of the Transformed Phenotype

The identification of genes maintaining cancer growth is critical to our understanding of tumorigenesis. We report the first in vivo genetic screen of patient-derived tumors, using metastatic melanomas and targeting 236 chromatin genes by expression of specific shRNA libraries. Our screens revealed unprecedented numerosity of genes indispensable for tumor growth ( 3c50% of tested genes) and unexpected functional heterogeneity among patients (<15% in common). Notably, these genes were not activated by somatic mutations in the same patients and are therefore distinguished from mutated cancer driver genes. We analyzed underlying molecular mechanisms of one of the identified genes, the Histone-lysine N-methyltransferase KMT2D, and showed that it promotes tumorigenesis by dysregulating a subset of transcriptional enhancers and target genes involved in cell migration. The assembly of enhancer genomic patterns by activated KMT2D was highly patient-specific, regardless of the identity of transcriptional targets, suggesting that KMT2D might be activated by distinct upstream signaling pathways

Immigration and the metropolis: Reflections on urban history

This article presents an outline of the relationship between migration and the city in its evolution over time. I sketch the central aspects of this historical relation as a prelude to examining three aspects of the contemporary scene: the various determinants of contemporary labour flows; the political sources of resistance to international migration; and the renewed protagonist role of metropolitan areas as strategic nodes of the international system. As part of the latter process, I sketch the rise of transnationalism as a novel form of adaptation to immigration and as a potential response to the overriding logic of global capitalism. Implications of a migration-centred approach to cities for theory and policy are dismissed

Transepidermal UV radiation of scalp skin ex vivo induces hair follicle damage that is alleviated by the topical treatment with caffeine

Objectives Although the effect of ultraviolet radiation (UVR) on human skin has been extensively studied, very little is known on how UVR impacts on hair follicle (HF) homeostasis. Here, we investigated how solar spectrum UVR that hits the human skin surface impacts on HF biology, and whether any detrimental effects can be mitigated by a widely used cosmetic and nutraceutical ingredient, caffeine. Methods Human scalp skin with terminal HFs was irradiated transepidermally ex vivo using either 10 J/cm2 UVA (340–440 nm) + 20 mJ/cm2 UVB (290–320 nm) (low dose) or 50 J/cm2 UVA + 50 mJ/cm2 UVB (high dose) and organ‐cultured under serum‐free conditions for 1 or 3 days. 0.1% caffeine (5.15 mmol/L) was topically applied for 3 days prior to UV exposure with 40 J/cm2 UVA + 40 mJ/cm2 UVB and for 3 days after UVR. The effects on various toxicity and vitality read‐out parameters were measured in defined skin and HF compartments. Results Consistent with previous results, transepidermal UVR exerted skin cytotoxicity and epidermal damage. Treatment with high and/or low UVA+UVB doses also induced oxidative DNA damage and cytotoxicity in human HFs. In addition, it decreased proliferation and promoted apoptosis of HF outer root sheath (ORS) and hair matrix (HM) keratinocytes, stimulated catagen development, differentially regulated the expression of HF growth factors, and induced perifollicular mast cell degranulation. UVR‐mediated HF damage was more severe after irradiation with high UVR dose and reached also proximal HF compartments. The topical application of 0.1% caffeine did not induce skin or HF cytotoxicity and stimulated the expression of IGF‐1 in the proximal HF ORS. However, it promoted keratinocyte apoptosis in selected HF compartments. Moreover, caffeine provided protection towards UVR‐mediated HF cytotoxicity and dystrophy, keratinocyte apoptosis, and tendential up‐regulation of the catagen‐promoting growth factor. Conclusion Our study highlights the clinical relevance of our scalp UV irradiation ex vivo assay and provides the first evidence that transepidermal UV radiation negatively affects important human HF functions. This suggests that it is a sensible prophylactic strategy to integrate agents such as caffeine that can act as HF photoprotectants into sun‐protective cosmeceutical and nutraceutical formulations. We show here that solar UVA+UVB radiation impacting on the skin surface negatively affects HF functions, namely it triggers HF cytotoxicity, dystrophy, oxidative DNA damage, decrease in keratinocyte proliferation and increase in their apoptosis, stimulation of the production of transforming growth factor (TGF)‐β2 and decrease in insulin growth factor (IGF)‐1 expression in ORS keratinocytes, premature catagen development, and perifollicular mast cell degranulation. UV‐mediated damage is present throughout the HF length, but is more prominent in the upper layers of the skin (distal HF), as compared to the lower HF (central and proximal). Our study also shows that the topical application of 0.1% caffeine protects HFs from UVR‐mediated damaged, namely it alleviated UV‐mediated HF cytotoxicity and dystrophy, keratinocyte apoptosis in the distal and central ORS, and increased expression of TGF‐β2 in the proximal ORS. Résumé Objectifs Alors que l'effet de rayons ultraviolets (RUV) sur la peau humaine a été largement étudié, on sait très peu de choses de l'impact des UV sur l'homéostasie du follicule pileux (FP). Ici, nous avons étudié l'effet du spectre des RUV solaires qui atteignent la surface de la peau humaine sur la biologie du FP, et si tout effet nocif peut être atténué par de la caféine, un ingrédient cosmétique et neutraceutique largement utilisé. MÉthodes Une peau de cuir chevelu humain avec ses FP terminaux a été irradiée ex vivo via l’épiderme soit par 10 J/cm2 d’UVA (340–440 nm) + 20 mJ/cm2 d’UVB (290–320 nm) (dose faible) soit par 50 J/cm2 d’UVA + 50 mJ/cm2 d’UVB (dose élevée) et placée en culture sans sérum pendant 1 ou 3 jours. 0,1% (5,15 mM) de caféine a été appliquée par voie topique pendant 3 jours avant l'exposition aux UV à raison de 40 J/cm2 d’UVA + 40 mJ/cm2 UVB et pendant 3 jours après l'exposition aux RUV. Les effets sur divers paramètres de toxicité et de vitalité ont été mesurés au niveau de compartiments définis de la peau et des FP. RÉsultats Cohérent avec les résultats précédents, les RUV transépidermique ont exercé une cytotoxicité au niveau de la peau et des lésions épidermiques. Le traitement par des doses élevées et/ou faibles d’UVA+UVB a également induit des lésions oxydatives de l’ADN et une cytotoxicité au niveau des FP humains. En outre, il a diminué la prolifération et favorisé l'apoptose de la gaine externe de la racine (ORS) du FP et des kératinocytes de la matrice des cheveux (MC), a stimulé le développement de la phase catagène, a régulé de manière différentielle l'expression des facteurs de croissance des FP, et induit une dégranulation périfolliculaire des mastocytes. Les lésions du FP médiées par les RUV étaient plus graves après une irradiation par dose élevée de RUV et atteignaient également les compartiments proximaux du FP. L'application topique de 0,1 % de caféine n'a pas induit de cytotoxicité de la peau ou du FP et a stimulé l'expression d’IGF‐1 dans la partie proximale de l’ORS du FP. Cependant, elle a promu l'apoptose des kératinocytes dans certains compartiments de FP. En outre, la caféine a fourni une protection des FP contre la cytotoxicité et la dystrophie médiées par les RUV, l'apoptose des kératinocytes et une régulation à tendance positive de l'effet catagène induit par le facteur de croissance. Conclusion Notre étude souligne la pertinence clinique de notre dosage d'irradiation UV ex vivo du cuir chevelu et fournit la première preuve que le rayonnement UV transépidermique affecte négativement d'importantes fonctions du FP chez l'homme. Cela suggère que l'intégration d'agents photoprotecteurs des FP tels que la caféine dans les formulations cosmétiques et nutraceutiques des écrans solaires pourrait constituer une stratégie prophylactique sensée

Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo

International audienceDespite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass $M>70$$M_\odot$) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities $0 < e \leq 0.3$ at $0.33$ Gpc$^{-3}$ yr$^{-1}$ at 90% confidence level

Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo

International audienceDespite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass $M>70$$M_\odot$) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities $0 < e \leq 0.3$ at $0.33$ Gpc$^{-3}$ yr$^{-1}$ at 90% confidence level