The role of ACKR3 in breast, lung, and brain cancer

Recent reports regarding the significance of chemokine receptors in disease have put a spotlight on atypical chemokine receptor 3 (ACKR3). This atypical chemokine receptor is overexpressed in numerous cancer types and has been involved in the modulation of tumor cell proliferation and migration, tumor angiogenesis, or resistance to drugs, thus contributing to cancer progression and metastasis occurrence. Here, we focus on the clinical significance and potential mechanisms underlying the pathologic role of ACKR3 in breast, lung, and brain cancer and discuss its possible relevance as a prognostic factor and potential therapeutic target in these contexts.European Union H2020-MSCA Program [Grant Agreement 64183], ONCORNET to P.M., M.J.S., and F.M.; Ministerio de Economía, Industria y Competitividad of Spain [Grant SAF2017-84125-R] to F.M.; CIBERCV-Instituto de Salud Carlos III, Spain [Grant CB16/11/00278] to F.M.; cofunded with European FEDER contribution, Comunidad de Madrid [B2017/BMD-3671-INFLAMUNE] to F.M.; Fundación Ramón Areces to F.M.; Portuguese Foundation for Science and Technology [Grant SFRH/BD/136574/2018] to M.N.; Netherlands Organization for Scientific Research NWO: Vici [Grant 016.140.657] to M.J.S.; and grants from CNRS, INSERM, Université de Montpellier and Fondation pour la Recherche Médical

Quasar Sightline and Galaxy Evolution (QSAGE) - III. The mass-metallicity and fundamental metallicity relation of z ≈ 2.2 galaxies

We present analysis of the mass-metallicity relation (MZR) for a sample of 67 [O iii]-selected star-forming (SF) galaxies at a redshift range of z = 1.99-2.32 (zmed = 2.16) using Hubble Space Telescope Wide Field Camera 3 grism spectroscopy from the Quasar Sightline and Galaxy Evolution survey. Metallicities were determined using empirical gas-phase metallicity calibrations based on the strong emission lines [O ii]3727, 3729, [O iii]4959, 5007 and Hβ. SF galaxies were identified, and distinguished from active-galactic nuclei, via Mass-Excitation diagrams. Using z ∼0 metallicity calibrations, we observe a negative offset in the z = 2.2 MZR of ≈-0.51 dex in metallicity when compared to locally derived relationships, in agreement with previous literature analysis. A similar offset of ≈-0.46 dex in metallicity is found when using empirical metallicity calibrations that are suitable out to z ∼5, though our z = 2.2 MZR, in this case, has a shallower slope. We find agreement between our MZR and those predicted from various galaxy evolution models and simulations. Additionally, we explore the extended fundamental metallicity relation (FMR) which includes an additional dependence on star formation rate. Our results consistently support the existence of the FMR, as well as revealing an offset of 0.28 ± 0.04 dex in metallicity compared to locally derived relationships, consistent with previous studies at similar redshifts. We interpret the negative correlation with SFR at fixed mass, inferred from an FMR existing for our sample, as being caused by the efficient accretion of metal-poor gas fuelling SFR at cosmic noon

The wide-field, multiplexed, spectroscopic facility WEAVE : survey design, overview, and simulated implementation

Funding for the WEAVE facility has been provided by UKRI STFC, the University of Oxford, NOVA, NWO, Instituto de Astrofísica de Canarias (IAC), the Isaac Newton Group partners (STFC, NWO, and Spain, led by the IAC), INAF, CNRS-INSU, the Observatoire de Paris, Région Île-de-France, CONCYT through INAOE, Konkoly Observatory (CSFK), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Lund University, the Leibniz Institute for Astrophysics Potsdam (AIP), the Swedish Research Council, the European Commission, and the University of Pennsylvania.WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366-959 nm at R ∼ 5000, or two shorter ranges at R ∼ 20,000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for ∼ 3 million stars and detailed abundances for ∼ 1.5 million brighter field and open-cluster stars; (ii) survey ∼ 0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey  ∼ 400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z 1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.PostprintPeer reviewe

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z<0.5$ cluster galaxies; (vi) survey stellar populations and kinematics in $\sim25\,000$ field galaxies at $0.3\lesssim z \lesssim 0.7$; (vii) study the cosmic evolution of accretion and star formation using $>1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.Comment: 41 pages, 27 figures, accepted for publication by MNRA

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366−959\,nm at R∼5000, or two shorter ranges at R∼20000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for ∼3 million stars and detailed abundances for ∼1.5 million brighter field and open-cluster stars; (ii) survey ∼0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey ∼400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z>2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator

Le déchiffrage de l'interactome de CXCR4 et ACKR3 révèle la régulation par ACKR3 de l'activité des jonctions Gap

The Atypical Chemokine Receptor 3 (ACKR3) and CXCR4 are two G protein-coupled receptors (GPCR) belonging to the CXC chemokine receptor family. Both receptors are activated upon CXCL12 binding and are over-expressed in various tumours, including glioma, where they have been found to promote proliferation and invasive behaviours. Upon CXCL12 binding, CXCR4 activates canonical GPCR signalling pathways involving Gαi protein and β-arrestins. In addition, CXCR4 was found to interact with several proteins able to modify its signalling, trafficking and localization. In contrast, the cellular pathways underlying ACKR3-dependent effects remain poorly characterized. Several reports show that ACKR3 engages β-arrestin-dependent signalling pathways, but its coupling to G proteins is restricted to either specific cellular populations, including astrocytes, or occurs indirectly via its interaction with CXCR4. ACKR3 also associates with the epidermal growth factor receptor to promote proliferation of tumour cells in an agonist-independent manner. These examples suggest that the extensive characterization of ACKR3 and CXCR4 interactomes might be a key step in understanding or clarifying their roles in physiological and pathological contexts. This thesis addressed this issue employing an affinity purification coupled to high-resolution mass spectrometry proteomic strategy that identified 19 and 151 potential protein partners of CXCR4 and ACKR3 transiently expressed in HEK-293T cells, respectively. Amongst ACKR3 interacting proteins identified, we paid particular attention on the gap junction protein Connexin-43 (Cx43), in line with its overlapping roles with the receptor in the control of leukocyte entry into the brain, interneuron migration and glioma progression. Western blotting and BRET confirmed the specific association of Cx43 with ACKR3 compared to CXCR4. Likewise, Cx43 is co-localized with ACKR3 but not CXCR4 in glioma initiating cell lines, and ACKR3 and Cx43 are co-expressed in astrocytes of the sub-ventricular zone and surrounding blood vessels in adult mouse brain, suggesting that both proteins form a complex in authentic cell or tissue contexts. Further functional studies showed that ACKR3 influences Cx43 trafficking and functionality at multiple levels. Transient expression of ACKR3 in HEK-293T cells to mimic ACKR3 overexpression detected in several cancer types, induces Gap Junctional Intercellular Communication (GJIC) inhibition in an agonist-independent manner. In addition, agonist stimulation of endogenously expressed ACKR3 in primary cultured astrocytes inhibits Cx43-mediated GJIC through a mechanism that requires activation of Gαi protein, and dynamin- and β-arrestin2-dependent Cx43 internalisation. Therefore, this thesis work provides the first functional link between the CXCL11/CXCL12/ACKR3 axis and gap junctions that might underlie their critical role in glioma progression.Le récepteur atypique ACKR3 et le récepteur CXCR4 sont des récepteurs couplés aux protéines G appartenant à la famille des récepteurs CXC des chimiokines. Ces deux récepteurs sont activés par la chimiokine CXCL12 et sont surexprimés dans de nombreux cancers comme les gliomes, dont ils favorisent la prolifération et le caractère invasif. Le récepteur CXCR4 active des voies de signalisation qui dépendent de la protéine Gi et des β-arrestines et s’associe à plusieurs protéines impliquées dans la transduction du signal, le trafic et la localisation cellulaire du récepteur. Par contre, les mécanismes de signalisation impliqués dans les effets d’ACKR3 restent mal connus. Le récepteur déclenche une signalisation dépendant des β-arrestines, mais son couplage aux protéines G dépend du type cellulaire ou se fait par un mécanisme indirect via son association au récepteur CXCR4. Le récepteur ACKR3 s’associe également au récepteur de l’EGF pour induire la prolifération cellulaire par un mécanisme indépendant de sa stimulation par un agoniste. Ces données illustrent l’intérêt de caractériser de façon systématique l’interactome de ces récepteurs pour comprendre leurs rôles physiologiques et pathologiques. Cette thèse a poursuivi cet objectif grâce à la mise en œuvre d’une approche protéomique combinant la purification des partenaires des deux récepteurs par affinité suivie de leur identification par spectrométrie de masse. J’ai ainsi identifié respectivement 19 et 151 partenaires protéiques potentiels des récepteurs CXCR4 et ACKR3 exprimés dans les cellules HEK-293T. Parmi les protéines recrutées par ACKR3, nous nous sommes focalisés sur la connexine 43 (Cx43, une des protéines constituant les jonctions Gap) du fait de la similitude des effets du récepteur et de la Cx43 dans la pénétration des leucocytes dans le parenchyme cérébral, la migration des interneurones et la progression des gliomes. J’ai confirmé par Western blot et par BRET l’association spécifique de la Cx43 à l’ACKR3 et non pas au CXCR4. De la même façon, j’ai montré une co-localisation de la Cx43 et de l’ACKR3 dans des cellules de gliome humain, ainsi que dans les astrocytes de la zone sous-ventriculaire et les pieds astrocytaires entourant les capillaires cérébraux chez la souris, suggérant que les deux protéines forment un complexe protéique dans un contexte biologique authentique. Des études fonctionnelles ont révélé que l’ACKR3 module les fonctions de la Cx43 par différents mécanismes. L’expression de l’ACKR3 dans les cellules HEK-293T (mimant la surexpression du récepteur dans les tumeurs), induit par elle-même une inhibition de l’activité jonctionnelle de la Cx43. De même, la stimulation du récepteur par un agoniste réduit l’activité jonctionnelle de la Cx43 par un mécanisme impliquant l’activation d’une protéine Gi, la β-arrestine2 et l’internalisation de la Cx43. Cette thèse établit donc pour la première fois un lien fonctionnel entre le système constitué par les chimiokines CXCL11, CXCL12 et leur récepteur ACKR3 d’une part et les jonctions Gap d’autre part qui pourrait jouer un rôle critique dans la progression des gliomes

Molecular mechanisms of non-genetic aberrant peptide production in cancer

The cancer peptidome has long been known to be altered by genetic mutations. However, more recently, non-genetic polypeptide mutations have also been related to cancer cells. These non-genetic mutations occur post-t30ranscriptionally, leading to the modification of the peptide primary structure, while the corresponding genes remain unchanged. Three main processes participate in the production of these aberrant proteins: mRNA alternative splicing, mRNA editing, and mRNA aberrant translation. In this review, we summarize the molecular mechanisms underlying these processes and the recent findings on the functions of the aberrant proteins, as well as their exploitability as new therapeutic targets due to their specific enrichment in cancer cells. These non-genetic aberrant polypeptides represent a source of novel cancer cell targets independent from their level of mutational burden, still to be exhaustively explored.</p

CXCR4/AckR3 phosphorylation and recruitment of interacting proteins: Key mechanisms regulating their functional status

The C-X-C motif chemokine receptor type 4 (CXCR4) and the atypical chemokine receptor 3 (ACKR3/CXCR7) are class A G protein-coupled receptors (GPCRs). Accumulating evidence indicates that GPCR subcellular localization, trafficking, transduction properties, and ultimately their pathophysiological functions are regulated by both interacting proteins and post-translational modifications. This has encouraged the development of novel techniques to characterize the GPCR interactome and to identify residues subjected to post-translational modifications, with a special focus on phosphorylation. This review first describes state-of-the-art methods for the identification of GPCR-interacting proteins and GPCR phosphorylated sites. In addition, we provide an overview of the current knowledge of CXCR4 and ACKR3 post-translational modifications and an exhaustive list of previously identified CXCR4- or ACKR3-interacting proteins. We then describe studies highlighting the importance of the reciprocal influence of CXCR4/ACKR3 interactomes and phosphorylation states. We also discuss their impact on the functional status of each receptor. These studies suggest that deeper knowledge of the CXCR4/ACKR3 interactomes along with their phosphorylation and ubiquitination status would shed new light on their regulation and pathophysiological functions.European Union’s Horizon2020 MSCA European Union’s Horizon2020 MSCA Program [Grant agreement 641833 (ONCORNET)]; A.F. and P.M. are also supported by CNRS, INSERM, Université de Montpellier and Fondation pour la Recherche Médicale (FRM); F.M. laboratory is also supported by grants from Ministerio de Economía; Industria y Competitividad (MINECO) of Spain [Grant SAF2017-84125-R]; CIBERCV-Instituto de Salud Carlos III, Spain [Grant CB16/11/00278] to F.M., cofunded with European FEDER contribution); Comunidad de Madrid-B2017/BMD-3671-INFLAMUNE; and Fundación Ramón Areces. Program [Grant agreement 641833 (ONCORNET)]; A.F. and P.M. are also supported by CNRS, INSERM, Université de Montpellier and Fondation pour la Recherche Médicale (FRM); F.M. laboratory is also supported by grants from Ministerio de Economía; Industria y Competitividad (MINECO) of Spain [Grant SAF2017-84125-R]; CIBERCV-Instituto de Salud Carlos III, Spain [Grant CB16/11/00278] to F.M., cofunded with European FEDER contribution); Comunidad de Madrid-B2017/BMD-3671-INFLAMUNE; and Fundación Ramón Areces

The role of ACKR3 in breast, lung, and brain cancer

Recent reports regarding the significance of chemokine receptors in disease have put a spotlight on atypical chemokine receptor 3 (ACKR3). This atypical chemokine receptor is overexpressed in numerous cancer types and has been involved in the modulation of tumor cell proliferation and migration, tumor angiogenesis, or resistance to drugs, thus contributing to cancer progression and metastasis occurrence. Here, we focus on the clinical significance and potential mechanisms underlying the pathologic role of ACKR3 in breast, lung, and brain cancer and discuss its possible relevance as a prognostic factor and potential therapeutic target in these contexts