4.6 Editorial Material

Organs-on-chip: The way forward

Journal

STEM CELL REPORTS
Volume 16, Issue 9, Pages 2037-2043

Publisher

CELL PRESS
DOI: 10.1016/j.stemcr.2021.06.015

Keywords

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Funding

  1. Netherlands Organ-on-Chip Initiative, an NWO gravitation project - Ministry of Education, Cul-ture and Science of the government of the Netherlands [024.003.001]
  2. Moore4Medical project - ECSEL Joint Undertaking [H2020-ECSEL-2019-IA-876190]

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Organ-on-chip (OoC) technology is thriving due to the availability of stem cells and international OoC programs. Coordinated standardization, qualification, and independent testing of devices are needed to further develop OoC technology and maximize its potential in drug development, disease modeling, and personalized medicine. The OoC roadmap can guide the way forward.
Organ-on-chip (OoC) technology is thriving thanks to stem cells availability and international OoC programs. Concerted standardization, qualification, and independent testing of devices are needed to coherently develop OoC technology further and fulfill its potential in drug development, disease modeling, and personalized medicine. The OoC roadmap can lead the way forward.

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E. Merlin, M. Castellano, H. Bretonniere, M. Huertas-Company, U. Kuchner, D. Tuccillo, F. Buitrago, J. R. Peterson, C. J. Conselice, F. Caro, P. Dimauro, L. Nemani, A. Fontana, M. Kuemmel, B. Haussler, W. G. Hartley, A. Alvarez Ayllon, E. Bertin, P. Dubath, F. Ferrari, L. Ferreira, R. Gavazzi, D. Hernandez-Lang, G. Lucatelli, A. S. G. Robotham, M. Schefer, C. Tortora, N. Aghanim, A. Amara, L. Amendola, N. Auricchio, M. Baldi, R. Bender, C. Bodendorf, E. Branchini, M. Brescia, S. Camera, V. Capobianco, C. Carbone, J. Carretero, F. J. Castander, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, F. Courbin, M. Cropper, A. Da Silva, H. Degaudenzi, J. Dinis, M. Douspis, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, P. Franzetti, S. Galeotta, B. Garilli, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, H. Hoekstra, W. Holmes, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnke, S. Kermiche, A. Kiessling, T. Kitching, R. Kohley, M. Kunz, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, H. J. McCracken, E. Medinaceli, M. Melchior, M. Meneghetti, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, J. Skottfelt, J. -L. Starck, P. Tallada-Crespi, A. N. Taylor, I. Tereno, R. Toledo-Moreo, I. Tutusaus, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, A. Zacchei, G. Zamorani, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, C. Colodro-Conde, D. Di Ferdinando, J. Gracia-Carpio, V. Lindholm, N. Mauri, S. Mei, C. Neissner, V. Scottez, A. Tramacere, E. Zucca, C. Baccigalupi, A. Balaguera-Antolinez, M. Ballardini, F. Bernardeau, A. Biviano, S. Borgani, A. S. Borlaff, C. Burigana, R. Cabanac, A. Cappi, C. S. Carvalho, S. Casas, G. Castignani, A. R. Cooray, J. Coupon, H. M. Courtois, O. Cucciati, S. Davini, G. De Lucia, G. Desprez, J. A. Escartin, S. Escoffier, M. Farina, K. Ganga, J. Garcia-Bellido, K. George, G. Gozaliasl, H. Hildebrandt, I. Hook, O. Ilbert, S. Ilic, B. Joachimi, V. Kansal, E. Keihanen, C. C. Kirkpatrick, A. Loureiro, J. Macias-Perez, M. Magliocchetti, G. Mainetti, R. Maoli, S. Marcin, M. Martinelli, N. Martinet, S. Matthew, M. Maturi, R. B. Metcalf, P. Monaco, G. Morgante, S. Nadathur, A. A. Nucita, L. Patrizii, V. Popa, C. Porciani, D. Potter, A. Pourtsidou, M. Pontinen, P. Reimberg, A. G. Sanchez, Z. Sakr, M. Schirmer, M. Sereno, J. Stadel, R. Teyssier, C. Valieri, J. Valiviita, S. E. van Mierlo, A. Veropalumbo, M. Viel, J. R. Weaver, D. Scott

Summary: The Euclid mission of the European Space Agency aims to provide high-quality imaging for 1.5 billion galaxies. A software pipeline is being developed to process and analyze the massive amount of data in real time, including a model-fitting algorithm for important photometric and morphological estimates. The Euclid Morphology Challenge compares five model-fitting software packages on simulated data to identify the best algorithm for implementation.

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Article Astronomy & Astrophysics

Euclid: Testing the Copernican principle with next-generation surveys

D. Camarena, V. Marra, Z. Sakr, S. Nesseris, A. Da Silva., J. Garcia-Bellido., P. Fleury., L. Lombriser, M. Martinelli, C. J. A. P. Martins, J. Mimoso, D. Sapone, C. Clarkson, S. Camera, C. Carbone, S. Casas, S. Ilic, V. Pettorino, I. Tutusaus, N. Aghanim, B. Altieri, A. Amara, N. Auricchio, M. Baldi, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, G. P. Candini, V. Capobianco, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, F. Courbin, M. Cropper, H. Degaudenzi, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, A. Ealet, S. Farrens, P. Fosalba, M. Frailis, E. Franceschi, M. Fumana, B. Garilli, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, A. Kiessling, R. Kohley, M. Kunz, H. Kurki-Suonio, P. B. Lilje, I. Lloro, O. Mansutti, O. Marggraf, F. Marulli, R. Massey, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rebolo, J. Rhodes, G. Riccio, H. -w. Rix, E. Rossetti, R. Saglia, B. Sartoris, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, L. Stanco, C. Surace, P. Tallada-Crespi, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, E. A. Valentijn, L. Valenziano, Y. Wang, G. Zamorani, J. Zoubian, S. Andreon, V. Scottez, M. Tenti

Summary: This paper investigates the precision and ability of future surveys to test the Copernican principle and detect possible violations. The results show that next-generation surveys, such as Euclid, will thoroughly test homogeneity at large scales and tighten the constraints on possible violations of the Copernican principle.

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Summary: The Euclid space telescope will survey cosmic voids using galaxy samples and estimate its performance in utilizing photometric void clustering, galaxy weak lensing, and their cross-correlation. The study finds that the inclusion of the void-lensing cross-correlation signal enhances parameter constraints and improves the joint void clustering and galaxy lensing figure of merit. When combined with spectroscopic galaxy clustering, the study shows that the FoM increases significantly. The conclusion suggests that photometric void clustering and its cross-correlation with galaxy lensing should be utilized in the data analysis of the Euclid galaxy survey to improve its constraining power.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

The PAU Survey and Euclid: Improving broadband photometric redshifts with multi-task learning☆

L. Cabayol, M. Eriksen, J. Carretero, R. Casas, F. J. Castander, E. Fernandez, J. Garcia-Bellido, E. Gaztanaga, H. Hildebrandt, H. Hoekstra, B. Joachimi, R. Miquel, C. Padilla, A. Pocino, E. Sanchez, S. Serrano, I. Sevilla, M. Siudek, P. Tallada-Crespi, N. Aghanim, A. Amara, N. Auricchio, M. Baldi, R. Bender, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, C. J. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, M. Cropper, A. Da Silva, H. Degaudenzi, M. Douspis, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, S. Farrens, P. Fosalba, M. Frailis, E. Franceschi, P. Franzetti, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnke, M. Kuemmel, S. Kermiche, A. Kiessling, M. Kilbinger, R. Kohley, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, S. Mei, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, S. M. Niemi, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rebolo, J. Rhodes, G. Riccio, C. Rosset, E. Rossetti, R. Saglia, B. Sartoris, P. Schneider, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, L. Stanco, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. Valentijn, L. Valenziano, Y. Wang, J. Weller, G. Zamorani, J. Zoubian, S. Andreon, V. Scottez, A. Tramacere

Summary: Current and future imaging surveys require accurate estimation of photometric redshifts (photo-zs) for millions of galaxies. This paper investigates the improvement of broadband photo-z estimates by leveraging the synergies between narrow-band photometric data and large imaging surveys. A multi-task learning (MTL) network is applied to simultaneously predict broadband photo-z and narrow-band photometry from broadband photometry, resulting in a 13% increase in precision and a 40% reduction in outlier rate for photo-z predictions. MTL also reduces the bias for high-redshift galaxies and improves the redshift distributions. The application of this technique to deeper samples is crucial for future surveys such as Euclid or LSST.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

Euclid: Calibrating photometric redshifts with spectroscopic cross-correlations

K. Naidoo, H. Johnston, B. Joachimi, J. L. van den Busch, H. Hildebrandt, O. Ilbert, O. Lahav, N. Aghanim, B. Altieri, A. Amara, M. Baldi, R. Bender, C. Bodendorf, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, F. J. Castander, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, C. J. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, M. Cropper, A. Da Silva, H. Degaudenzi, J. Dinis, F. Dubath, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, S. Galeotta, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, M. Kuemmel, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, S. Maurogordato, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, C. Rosset, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, J. -l. Starck, C. Surace, P. Tallada-Crespi, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. A. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, M. Wetzstein, A. Zacchei, G. Zamorani, J. Zoubian, S. Andreon, D. Maino, V. Scottez, A. H. Wright

Summary: Cosmological constraints from the Euclid imaging survey rely on accurate determination of tomographic redshift bins' true redshift distributions, n(z). We investigate the calibration of mean redshift, < z >, of ten Euclid tomographic redshift bins using cross-correlation with spectroscopic samples. Our results show that clustering redshifts can attain uncertainties exceeding the Euclid requirement by at least a factor of three, but systematic biases limit the accuracy. Future work includes extending the method to higher redshifts with quasar reference samples.

ASTRONOMY & ASTROPHYSICS (2023)

Correction Astronomy & Astrophysics

On the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates (vol 919, 85, 2021)

V. F. Braga, J. Crestani, M. Fabrizio, G. Bono, C. Sneden, G. W. Preston, J. Storm, S. Kamann, M. Latour, H. Lala, B. Lemasle, Z. Prudil, G. Altavilla, B. Chaboyer, M. Dall'Ora, I. Ferraro, C. K. Gilligan, G. Fiorentino, G. Iannicola, L. Inno, S. Kwak, M. Marengo, S. Marinoni, P. M. Marrese, C. E. Martinez-Vazquez, M. Monelli, J. P. Mullen, N. Matsunaga, J. Neeley, P. B. Stetson, E. Valenti, M. Zoccali

ASTROPHYSICAL JOURNAL (2023)

Article Engineering, Biomedical

Comparison and Integration of Voltage and Charge Amplifiers for Capacitive ECG Measurements

Yijing Zhang, Lin Xu, Myrthe van der Ven, Sotir Ouzounov, Mohammed Meftah, Massimo Mischi, Eugenio Cantatore, Pieter Harpe

Summary: This paper introduces a VA-CA switchable amplifier that can adapt to different situations and passively estimate the body-to-electrode capacitance (C-e). The study found that VAs are less affected by C-e variation artifacts, while CAs recover faster from triboelectricity artifacts. The results show that this structure has the potential for optimal amplifier selection and provides additional information on the body-to-electrode interface quality (C-e estimation).

IEEE TRANSACTIONS ON BIOMEDICAL ENGINEERING (2023)

Article Computer Science, Interdisciplinary Applications

Automated detection and classification of patient-ventilator asynchrony by means of machine learning and simulated data

Tom Bakkes, Anouk van Diepen, Ashley De Bie, Leon Montenij, Francesco Mojoli, Arthur Bouwman, Massimo Mischi, Pierre Woerlee, Simona Turco

Summary: An automatic detection and classification algorithm for patient-ventilator asynchrony (PVA) was developed using a neural network and simulated data. The algorithm achieved over 90% accuracy in detecting and classifying PVAs, providing a tool to optimize mechanical ventilation and monitor ventilation strategies.

COMPUTER METHODS AND PROGRAMS IN BIOMEDICINE (2023)

Article Astronomy & Astrophysics

Properties and observables of massive galaxies in self-interacting dark matter cosmologies

Claudio Mastromarino, Giulia Despali, Lauro Moscardini, Andrew Robertson, Massimo Meneghetti, Matteo Maturi

Summary: We tested the differences between cold dark matter (CDM) and self-interacting dark matter (SIDM) models in the mass range of massive galaxies using hydrodynamic cosmological simulations. The inclusion of baryons erased the differences between SIDM and CDM density profiles observed in the dark-matter-only case. We also found that the distributions of strong lensing Einstein radii derived from CDM and SIDM simulations were comparable to observational samples. The discrimination between CDM and SIDM models is challenging at this mass scale, but the deviations of SIDM from CDM can still be found by considering the dark matter/baryonic fractions separately.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

A Bayesian chemical evolution model of the DustPedia galaxy M74

Francesco Calura, Marco Palla, Laura Morselli, Emanuele Spitoni, Viviana Casasola, Kuldeep Verma, Andrea Enia, Massimo Meneghetti, Simone Bianchi, Francesca Pozzi, Carlotta Gruppioni

Summary: In this study, a new multizone chemical evolution model was introduced for the DustPedia galaxy M74, calibrated using Markov Chain Monte Carlo methods. The observed stellar and gas density profiles were taken into account, and Bayesian analysis was used to constrain two fundamental parameters characterizing the gas accretion and star formation time-scale. The results support an 'Inside-Out' formation for M74, with an infall time-scale increasing with galactocentric radius and a star formation efficiency decreasing with radius. The dust content of M74 was also investigated, and two models with different balances between destruction and accretion were found to reproduce the observed dust profile equally well.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters

Massimo Meneghetti, Weiguang Cui, Elena Rasia, Gustavo Yepes, Ana Acebron, Giuseppe Angora, Pietro Bergamini, Stefano Borgani, Francesco Calura, Giulia Despali, Carlo Giocoli, Giovanni Granata, Claudio Grillo, Alexander Knebe, Andrea V. Maccio, Amata Mercurio, Lauro Moscardini, Priyamvada Natarajan, Antonio Ragagnin, Piero Rosati, Eros Vanzella

Summary: Previous studies have found an excess in the estimated probability of galaxy-galaxy strong lensing in observed galaxy clusters compared to the theoretical predictions. In this study, the researchers analyzed a larger set of simulated galaxy clusters and investigated how different implementations of star formation and feedback in simulations affect the theoretical expectations. The results show that the probability for galaxy-galaxy strong lensing is higher in simulations with denser stellar cores, but the discrepancy with observations still persists.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

The GLASS-JWST Early Release Science Program. III. Strong-lensing Model of Abell 2744 and Its Infalling Regions

Pietro Bergamini, Ana Acebron, Claudio Grillo, Piero Rosati, Gabriel Bartosch Caminha, Amata Mercurio, Eros Vanzella, Charlotte Mason, Tommaso Treu, Giuseppe Angora, Gabriel B. Brammer, Massimo Meneghetti, Mario Nonino, Kristan Boyett, Marusa Bradac, Marco Castellano, Adriano Fontana, Takahiro Morishita, Diego Paris, Gonzalo Prieto-Lyon, Guido Roberts-Borsani, Namrata Roy, Paola Santini, Benedetta Vulcani, Xin Wang, Lilan Yang

Summary: We propose a new high-precision strong-lensing model for the galaxy cluster Abell 2744 at z = 0.3072, based on JWST observations, MUSE data, and spectroscopic confirmation. The improved lens model covers an extended redshift range and shows a remarkably low scatter between predicted and observed positions of multiple images. This precise model provides a reliable magnification map critical for understanding the intrinsic properties of highly magnified, high-z sources. The model and MUSE redshift catalog are released with this publication.

ASTROPHYSICAL JOURNAL (2023)

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