cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Delete or merge regressors for linear model selection
Creators: name: Maj-Kańska, Aleksandra
name: Pokarowski, Piotr
name: Prochenka, Agnieszka
Publisher: name: arXiv
Year: 2015
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: We consider a problem of linear model selection in the presence of both continuous and categorical predictors. Feasible models consist of subsets of numerical variables and partitions of levels of factors. A new algorithm called delete or merge regressors (DMR) is presented which is a stepwise backward procedure involving ranking the predictors according to squared t-statistics and choosing the final model minimizing BIC. In the article we prove consistency of DMR when the number of predictors tends to infinity with the sample size and describe a simulation study using a pertaining R package. The results indicate significant advantage in time complexity and selection accuracy of our algorithm over Lasso-based methods described in the literature. Moreover, a version of DMR for generalized linear models is proposed.
Evolved Eclipsing Binaries and the Age of the Open Cluster NGC 752
Creators: name: Sandquist, Eric L.
name: Buckner, Andrew J.
name: Shetrone, Matthew D.
name: Barden, Samuel C.
name: Pilachowski, Catherine A.
name: Deliyannis, Constantine P.
name: Harmer, Dianne
name: Mathieu, Robert
name: Meibom, Søren
name: Frandsen, Søren
name: Orosz, Jerome A.
Publisher: name: London : Institute of Physics Publ.
Year: 2022
Subjects: subject: intermediate-age
subject: ds andromedae
subject: red giants
subject: spectroscopic binary
subject: chemical-composition
subject: absolute dimensions
subject: model atmospheres
subject: radial-velocities
subject: stellar tracks
subject: light-curve
subject: 520

description: We present analyses of improved photometric and spectroscopic observations for two detached eclipsing binaries at the turnoff of the open cluster NGC 752: the 1.01 days binary DS And and the 15.53 days BD +37 410. For DS And, we find M1 = 1.692 ± 0.004 ± 0.010M⊙, R1 = 2.185 ± 0.004 ± 0.008R⊙, M2 = 1.184 ± 0.001 ± 0.003M⊙, and R2 = 1.200 ± 0.003 ± 0.005R⊙. We either confirm or newly identify unusual characteristics of both stars in the binary: the primary star is found to be slightly hotter than the main-sequence turnoff and there is a more substantial discrepancy in its luminosity compared to models (model luminosities are too large by about 40%), while the secondary star is oversized and cooler compared to other main-sequence stars in the same cluster. The evidence points to nonstandard evolution for both stars, but most plausible paths cannot explain the low luminosity of the primary star. BD +37 410 only has one eclipse per cycle, but extensive spectroscopic observations and the Transiting Exoplanet Survey Satellite light curve constrain the stellar masses well: M1 = 1.717 ± 0.011M⊙ and M2 = 1.175 ± 0.005M⊙. The radius of the main-sequence primary star near 2.9R⊙ definitively requires large convective core overshooting (>0.2 pressure scale heights) in models for its mass, and multiple lines of evidence point toward an age of 1.61 ± 0.03 ± 0.05 Gyr (statistical and systematic uncertainties). Because NGC 752 is currently undergoing the transition from nondegenerate to degenerate He ignition of its red clump stars, BD +37 410 A directly constrains the star mass where this transition occurs.
title: Ψηφιακός μετασχηματισμός Δήμου Αθηναίων
title: Digital transformation of the Municipality of Athens
titleType: AlternativeTitle
Creators: name: Καθρέπτης, Μιχαήλ
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2023
Subjects: subject: Δήμος Αθηναίων
subject: Έξυπνες πόλεις
subject: Καλές πρακτικές
subject: Ψηφιακός μετασχηματισμός
subject: Ψηφιακή στρατηγική

description: Η παρούσα Διπλωματική Εργασία εξετάζει τον Ψηφιακό Μετασχηματισμό του Δήμου Αθηναίων. Αρχικά μελετώνται γενικές έννοιες όπως ο ψηφιακός μετασχηματισμός, η έξυπνη διακυβέρνηση, οι έξυπνες πόλεις, ενώ ακολούθως παρουσιάζονται καλές πρακτικές ψηφιακού μετασχηματισμού από την Ευρώπη, αλλά και από την Ελλάδα. Έμφαση δίνεται στον τρόπο υλοποίησης του μετασχηματισμού αυτού, όπου εξετάζονται τα διαθέσιμα χρηματοδοτικά εργαλεία, η συνέργεια με άλλες πολιτικές, καθώς και οι προκλήσεις που καλούνται να αντιμετωπίσουν οι πόλεις αυτές. Ειδικότερα, όσον αφορά την Αθήνα, παρουσιάζονται οι υφιστάμενες δράσεις που έχουν υλοποιηθεί και γίνεται μια εκτενής ανάλυση της ψηφιακής στρατηγικής που έχει εκπονηθεί από τον Δήμο Αθηναίων και βρίσκεται σε διαδικασία υλοποίησης. Από την εργασία αυτή διαπιστώνεται ότι η Αθήνα είναι ήδη αρκετά ώριμη σε ζητήματα ψηφιακού μετασχηματισμού, αλλά θα πρέπει να εφαρμόσει τον σχεδιασμό της, αξιοποιώντας τους διαθέσιμους πόρους που προέρχονται από διάφορες χρηματοδοτικές πηγές, με τον βέλτιστο δυνατό τρόπο. Κρίσιμος είναι ο ρόλος των πολιτών, καθώς και ο ρόλος της καινοτομίας, ενώ θα πρέπει να αξιοποιήσει καλές πρακτικές και να αντιμετωπίσει απειλές και κινδύνους, όπως είναι η κυβερνοασφάλεια. Σχετικά με την μεθοδολογία που χρησιμοποιείται, πρόκειται για εκτενή βιβλιογραφική αναζήτηση, η οποία λαμβάνει χώρα σε επιστημονικά περιοδικά και άλλα συγγράμματα, τα οποία αναφέρονται σε ζητήματα ψηφιακού μετασχηματισμού και έξυπνων πόλεων. Ακόμη, χρησιμοποιούνται σχετικές μελέτες, που έχουν δημοσιευθεί τόσο στην αγγλική, όσο και στην ελληνική γλώσσα, ενώ αξιοποιούνται και πηγές από το διαδίκτυο, έτσι ώστε η προσέγγιση του υπό μελέτη ζητήματος να είναι όσο το δυνατόν πιο επικαιροποιημένη. Για την εκτενέστερη μελέτη του ψηφιακού μετασχηματισμού του Δήμου Αθηναίων, αντλήθηκε υλικό από την δημοσιευμένη Ψηφιακή Στρατηγική του Δήμου Αθηναίων, όπως επίσης και από σχετικές μελέτες, αλλά και ιστοσελίδες που αφορούν τον Δήμο Αθηναίων.
Revisiting the Space Weather Environment of Proxima Centauri b
Creators: name: Garraffo, Cecilia
name: Alvarado-Gómez, Julián D.
name: Cohen, Ofer
name: Drake, Jeremy J.
Publisher: name: London : Institute of Physics Publ.
Year: 2022
Subjects: subject: stellar rotation
subject: magnetic-fields
subject: large-scale
subject: emission
subject: mass
subject: dependence
subject: evolution
subject: einstein
subject: radio
subject: stars
subject: 520

description: Close-in planets orbiting around low-mass stars are exposed to intense energetic photon and particle radiation and harsh space weather. We have modeled such conditions for Proxima Centauri b, a rocky planet orbiting in the habitable zone of our closest neighboring star, finding a stellar wind pressure 3 orders of magnitude higher than the solar wind pressure on Earth. At that time, no Zeeman-Doppler observations of the surface magnetic field distribution of Proxima Cen were available and a proxy from a star with a similar Rossby number to Proxima was used to drive the MHD model. Recently, the first Zeeman-Doppler imaging (ZDI) observation of Proxima Cen became available. We have modeled Proxima b’s space weather using this map and compared it with the results from the proxy magnetogram. We also computed models for a high-resolution synthetic magnetogram for Proxima b generated by a state-of-the-art dynamo model. The resulting space weather conditions for these three scenarios are similar with only small differences found between the models based on the ZDI observed magnetogram and the proxy. We conclude that our proxy magnetogram prescription based on the Rossby number is valid, and provides a simple way to estimate stellar magnetic flux distributions when no direct observations are available. Comparisons with models based on the synthetic magnetogram show that the exact magnetogram details are not important for predicting global space weather conditions of planets, reinforcing earlier conclusions that the large-scale (low-order) field dominates, and that the small-scale field does not have much influence on the ambient stellar wind.
Burden of Gastrointestinal Disease in the United States: 2012 Update
Creators: name: Thiny, Michelle T.
name: McGowan, Christopher E.
name: Dellon, Evan S.
name: Gangarosa, Lisa M.
name: Morgan, Douglas R.
name: Bulsiewicz, William J.
name: Allen, Jeffery K.
name: Lund, Jennifer
name: Kappelman, Michael D.
name: Carroll, Charlotte F.
name: Shaheen, Nicholas J.
name: Kim, Hannah P.
name: Ringel, Yehuda
name: Sandler, Robert S.
name: Crockett, Seth D.
name: Stizenberg, Karyn
name: Dibonaventura, Marco Dacosta
name: Peery, Anne F.
name: Cook, Suzanne F.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Gastrointestinal (GI) diseases account for substantial morbidity, mortality and cost. Statistical analyses of the most recent data are necessary to guide GI research, education and clinical practice. We estimate the burden of GI disease in the US.
Interpretation of Radio Wave Scintillation Observed through LOFAR Radio Telescopes
Creators: name: Forte, Biagio
name: Fallows, Richard A.
name: Bisi, Mario M.
name: Zhang, Jinge
name: Krankowski, Andrzej
name: Dabrowski, Bartosz
name: Rothkaehl, Hanna
name: Vocks, Christian
Publisher: name: London : Institute of Physics Publ.
Year: 2022
Subjects: subject: interplanetary scintillation
subject: ionospheric scintillation
subject: solar-wind
subject: parabolic arcs
subject: scattering
subject: turbulence
subject: pulsars
subject: diffraction
subject: frequency
subject: receiver
subject: 520

description: Radio waves propagating through a medium containing irregularities in the spatial distribution of the electron density develop fluctuations in their intensities and phases. In the case of radio waves emitted from astronomical objects, they propagate through electron density irregularities in the interstellar medium, the interplanetary medium, and Earth’s ionosphere. The LOFAR radio telescope, with stations across Europe, can measure intensity across the VHF radio band and thus intensity scintillation on the signals received from compact astronomical objects. Modeling intensity scintillation allows the estimate of various parameters of the propagation medium, for example, its drift velocity and its turbulent power spectrum. However, these estimates are based on the assumptions of ergodicity of the observed intensity fluctuations and, typically, of weak scattering. A case study of single-station LOFAR observations of the strong astronomical source Cassiopeia A in the VHF range is utilized to illustrate deviations from ergodicity, as well as the presence of both weak and strong scattering. Here it is demonstrated how these aspects can lead to misleading estimates of the propagation medium properties, for example, in the solar wind. This analysis provides a method to model errors in these estimates, which can be used in the characterization of both the interplanetary medium and Earth’s ionosphere. Although the discussion is limited to the case of the interplanetary medium and Earth’s ionosphere, its ideas are also applicable to the case of the interstellar medium.
Additional file 1 of Improved fed-batch processes with Wickerhamomyces anomalus WC 1501 for the production of d-arabitol from pure glycerol
Creators: name: Raimondi, Stefano
name: Foca, Giorgia
name: Ulrici, Alessandro
name: Destro, Lorenza
name: Leonardi, Alan
name: Buzzi, Raissa
name: Candeliere, Francesco
name: Rossi, Maddalena
name: Amaretti, Alberto
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Space Science
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry

description: Additional file 1: Figure S1. 1H NMR (400 MHz, DMSO-d6) of the lyophilized supernatant of W.anomalus WC 1501 fed batch culture. δ 3.27 – 3.49 (m, 5H, 1-5), 3.59 (d, J = 10.9 Hz, 1H, 6 or 7),3.66 (d, J = 6.9 Hz, 1H 6 or 7), 4.12 (d, J = 7.2 Hz, 1H 8), 4.19 (bs, J = 5.8 Hz, 1H, 9 or 10), 4.30 (bs,J = 6.6 Hz, 1H, 9 or 10), 4.43 (bs, J = 6.1, 6.7 Hz, 2H, 11, 12).
Porting the Plasma Simulation PIConGPU to Heterogeneous Architectures with Alpaka
Creators: name: Widera, Rene
name: Zenker, Erik
name: Juckeland, Guido
name: Worpitz, Benjamin
name: Huebl, Axel
name: Knuepfer, Andreas
name: Nagel, Wolfgang E
name: Bussmann, Michael
Publisher: name: Zenodo
Year: 2016
Subjects: GPU
performance-portability
Alpaka
PIConGPU
C++

description: Our presentation on Alpaka and PIConGPU at GTC 2016.
title: Γεωργία ακριβείας και οι εφαρμογές της στα εσπεριδοειδή
title: Precision agriculture and its applications to citrus
titleType: AlternativeTitle
Creators: name: Καπόγιαννης, Γιάννος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2023
Subjects: subject: Γεωργία ακριβείας
subject: Εσπεριδοειδή

description: Η διπλωματική εργασία επικεντρώνεται στη Γεωργία Ακρίβειας και τις εφαρμογές της στα εσπεριδοειδή. Η Γεωργία Ακρίβειας αναφέρεται στη χρήση προηγμένης τεχνολογίας, όπως οι καταμετρήσεις χώρου με χρήση δορυφόρων (GPS) και αισθητήρων, για τη βελτίωση της αποδοτικότητας και της ακρίβειας στη γεωργική παραγωγή. Στη διπλωματική εξετάζεται η εφαρμογή της Γεωργίας Ακρίβειας στην παραγωγή εσπεριδοειδών, μιας από τις σημαντικότερες γεωργικές καλλιέργειες στην Ελλάδα. Πιο συγκεκριμένα, η διπλωματική εργασία περιγράφει τη καλλιέργεια των εσπεριδοειδών, συμπεριλαμβανομένων των ειδικών απαιτήσεων τους σε ό,τι αφορά την ύδρευση, την προμήθεια θρεπτικών στοιχείων και την παρακολούθηση της υγείας των δέντρων και στην συνέχεια περιγράφεται μια εισαγωγή στη Γεωργία Ακρίβειας, συμπεριλαμβανομένων των τεχνολογιών που χρησιμοποιούνται και των πλεονεκτημάτων της.
Covering dimension of C*-algebras and 2-coloured classification
Creators: name: Bosa, Joan
name: Brown, Nathanial P.
name: Sato, Yasuhiko
name: Tikuisis, Aaron
name: White, Stuart
name: Winter, Wilhelm
Publisher: name: arXiv
Year: 2015
Subjects: subject: Operator Algebras (math.OA)
subject: FOS: Mathematics
subject: 46L05, 46L35

description: We introduce the concept of finitely coloured equivalence for unital *-homomorphisms between C*-algebras, for which unitary equivalence is the 1-coloured case. We use this notion to classify *-homomorphisms from separable, unital, nuclear C*-algebras into ultrapowers of simple, unital, nuclear, Z-stable C*-algebras with compact extremal trace space up to 2-coloured equivalence by their behaviour on traces; this is based on a 1-coloured classification theorem for certain order zero maps, also in terms of tracial data. As an application we calculate the nuclear dimension of non-AF, simple, separable, unital, nuclear, Z-stable C*-algebras with compact extremal trace space: it is 1. In the case that the extremal trace space also has finite topological covering dimension, this confirms the remaining open implication of the Toms-Winter conjecture. Inspired by homotopy-rigidity theorems in geometry and topology, we derive a "homotopy equivalence implies isomorphism" result for large classes of C*-algebras with finite nuclear dimension.
description: 93 Pages. Final accepted version. Mem. Amer. Math. Soc., to appear
Campylobacter jejuni Induces Colitis Through Activation of Mammalian Target of Rapamycin Signaling
Creators: name: Threadgill, Deborah
name: Jobin, Christian
name: Sun, Xiaolun
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Campylobacter jejuni is the worldwide leading cause of bacterial-induced enteritis. The molecular and cellular events that lead to campylobacteriosis are poorly understood. We identify mammalian target of rapamycin (mTOR) as a signaling pathway that leads to C jejuni-induced intestinal inflammation.
The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX). III. A Red Quasar with Extremely High Equivalent Widths Showing Powerful Outflows
Creators: name: Liu, Chenxu
name: Gebhardt, Karl
name: Kollatschny, Wolfram
name: Ciardullo, Robin
name: Mentuch Cooper, Erin
name: Davis, Dustin
name: Farrow, Daniel J.
name: Finkelstein, Steven L.
name: Gawiser, Eric
name: Gronwall, Caryl
name: Hill, Gary J.
name: House, Lindsay
name: Schneider, Donald P.
name: Urrutia, Tanya
name: Zeimann, Gregory R.
Publisher: name: London : Institute of Physics Publ.
Year: 2022
Subjects: subject: images
subject: galaxy
subject: sky
subject: 520

description: We report an active galactic nucleus (AGN) with an extremely high equivalent width (EW), EWLyα+N V,rest ≳921 Å, in the rest frame, at z ∼ 2.24 in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX), as a representative case of the high-EW AGN population. The continuum level is a nondetection in the HETDEX spectrum; thus the measured EW is a lower limit. The source is detected with significant emission lines (>7σ) at Lyα + N v λ1241, C iv λ1549, and a moderate emission line (∼4σ) at He ii λ1640 within the wavelength coverage of HETDEX (3500-5500 Å). The r-band magnitude is 24.57 from the Hyper Suprime-Cam-HETDEX joint survey with a detection limit of r = 25.12 at 5σ. The Lyα emission line spans a clearly resolved region of ∼10″ (85 kpc) in diameter. The Lyα line profile is strongly double peaked. The spectral decomposed blue gas and red gas Lyα emission are separated by ∼1.″2 (10.1 kpc) with a line-of-sight velocity offset of ∼1100 km s−1. This source is probably an obscured AGN with powerful winds.
Chiral d-wave superfluid in periodically driven lattices
Creators: name: Zhang, Shao-Liang
name: Lang, Li-Jun
name: Zhou, Qi
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Chiral d-wave superfluid is a preliminary example of topological matters that intrinsically encodes interaction effects. It exhibits fascinating properties including a finite Chern number in the bulk and topologically protected edge states, which have been invoking physicists for decades. However, unlike s-wave superfluids prevalent in nature, its existence requires a strong interaction in the d-wave channel, a criterion that is difficult to access in ordinary systems. So far, such an unconventional superfluid has not been discovered in experiments. Here, we present a new principle for creating a two-dimensional chiral d-wave superfluid using periodically driven lattices. Due to an imprinted two-dimensional pseudospin-orbit coupling, where the sublattice index serves as the pseudospin, s-wave interaction between two hyperfine spin states naturally creates a chiral d-wave superfluid. This scheme also allows physicists to study the phase transition between the topologically distinct s- and d-wave superfluids by controlling the driving field or the particle density.
description: 10pages, 7figures
KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap
Creators: name: Gatto, M.
name: Ripepi, V.
name: Bellazzini, M.
name: Tosi, M.
name: Tortora, C.
name: Cignoni, M.
name: Dall’Ora, M.
name: Cioni, M.-R.L.
name: Cusano, F.
name: Longo, G.
name: Marconi, M.
name: Musella, I.
name: Schipani, P.
name: Spavone, M.
Publisher: name: Les Ulis : EDP Sciences
Year: 2022
Subjects: subject: dynamics
subject: galaxies: star clusters: general
subject: galaxies: star clusters: individual: KMHK 1762
subject: Hertzsprung-Russell and C-M diagrams
subject: Magellanic Clouds
subject: stars: kinematics
subject: 520

description: Context. The star cluster (SC) age distribution of the Large Magellanic Cloud (LMC) exhibits a gap from ∼4 to 10 Gyr ago, with an almost total absence of SCs. Within this age gap, only two confirmed SCs have been identified hitherto. Nonetheless, the star field counterpart does not show the same characteristics, making the LMC a peculiar galaxy where the star formation history and cluster formation history appear to differ significantly. Aims. We re-analysed the colour-magnitude diagram (CMD) of the KMHK 1762 SC by using the deep optical photometry provided by the ‘Yes, Magellanic Clouds Again’ survey, so as to robustly assess its age. Methods. First, we partially removed foreground and/or field stars by means of parallaxes and proper motions obtained from the Gaia Early Data Release 3. Then, we applied the Automated Stellar Cluster Analysis package to the cleaned photometric catalogue to identify the isochrone that best matches the CMD of KMHK 1762. Results. The estimated age of KMHK 1762 is log(t) = 9.74 ± 0.15 dex (∼5.5 Gyr), which is more than 2 Gyr older than the previous estimation which was obtained with shallower photometry. This value makes KMHK 1762 the third confirmed age-gap SC of the LMC. Conclusions. The physical existence of a quiescent period of the LMC SC formation is questioned. We suggest it can be the result of an observational bias, originating from the combination of shallow photometry and limited investigation of the LMC periphery.
Additional file 3 of Accumulation of copy number alterations and clinical progression across advanced prostate cancer
Creators: name: Grist, Emily
name: Friedrich, Stefanie
name: Brawley, Christopher
name: Mendes, Larissa
name: Parry, Marina
name: Ali, Adnan
name: Haran, Aine
name: Hoyle, Alex
name: Gilson, Claire
name: Lall, Sharanpreet
name: Zakka, Leila
name: Bautista, Carla
name: Landless, Alex
name: Nowakowska, Karolina
name: Wingate, Anna
name: Wetterskog, Daniel
name: Hasan, A. M. Mahedi
name: Akato, Nafisah B.
name: Richmond, Malissa
name: Ishaq, Sofeya
name: Matthews, Nik
name: Hamid, Anis A.
name: Sweeney, Christopher J.
name: Sydes, Matthew R.
name: Berney, Daniel M.
name: Lise, Stefano
name: Parmar, Mahesh K. B.
name: Clarke, Noel W.
name: James, Nicholas D.
name: Cremaschi, Paolo
name: Brown, Louise C.
name: Attard, Gerhardt
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 3. Contains supplemental methods-full list of STAMPEDE trial eligibility criteria and criteria for inclusion in the CN-300 cohort.
Cigarette Smoking Increases Risk of Barrett's Esophagus: An Analysis of the Barrett's and Esophageal Adenocarcinoma Consortium
Creators: name: Giffen, Carol
name: Corley, Douglas A.
name: Chow, Wong Ho
name: Whiteman, David C.
name: Anderson, Lesley A.
name: Cook, Michael B.
name: Vaughan, Thomas L.
name: Shaheen, Nicholas J.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Cigarette smoking has been implicated in the etiology of esophageal adenocarcinoma, but it is not clear if smoking is a risk factor for Barrett’s esophagus (BE). We investigated whether tobacco smoking and other factors increase risk for BE.
Additional proofs and code for "Data-flow analyses as effects and graded monads"
Creators: name: Ivaskovic, Andrej
name: Mycroft, Alan
name: Orchard, Dominic
Publisher: name: Zenodo
Year: 2020
Subjects: data-flow analysis
effect systems
graded monads
correctness

description: This deposit provides code and additional proofs associated to the paper "Data-flow analyses as effects and graded monads" appearing at FSCD 2020 (5th International Conference On Formal Structures for Computation and Deduction). extra-proofs.pdf provides additional proofs not included in the appendix of the published paper for space reasons. GradedMonad.agda provides further mechanised proofs, referred to from extra-proofs.pdf dataflow-effects-as-grades-fscd2020.zip provides the source code corresponding to Section 4.4 and Appendix B The code is hosted on GitHub as well: https://github.com/dorchard/dataflow-effects-as-grades This .zip corresponds to this release https://github.com/dorchard/dataflow-effects-as-grades/releases/tag/fscd2020 Unzip and see README.md for details on how to build and interact with this code
Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE
Creators: name: Cairós, L. M.
name: González-Pérez, J.N.
name: Weilbacher, P.M.
name: Manso Sainz, R.
Publisher: name: Les Ulis : EDP Sciences
Year: 2022
Subjects: subject: galaxies: abundances
subject: galaxies: dwarf
subject: galaxies: individual: Haro14
subject: galaxies: ISM
subject: galaxies: star formation
subject: galaxies: starburst
subject: 520

description: We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral field spectroscopic observations taken with the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope. The large field of view of MUSE and its unprecedented sensitivity enable observations of the galaxy nebular emission up to large galactocentric distances, even in the important but very faint [O i] λ6300 diagnostic line. This allowed us to trace the ionized gas morphology and ionization structure of Haro 14 up to kiloparsec scales and, for the first time, to accurately investigate the excitation mechanism operating in the outskirts of a typical BCG. The intensity and diagnostic maps reveal at least two highly distinct components of ionized gas: the bright central regions, mostly made of individual clumps, and a faint component which extends up to kiloparsec scales and consists of widespread diffuse emission, well-delineated filamentary structures, and faint knots. Noteworthy are the two curvilinear filaments extending up to 2 and 2.3 kpc southwest, which likely trace the edges of supergiant expanding bubbles driven by galactic outflows. We find that while the central clumps in Haro 14 are Hii-region complexes, the morphology and line ratios of the whole low-surface-brightness component are not compatible with star formation photoionization. In the spatially resolved emission-line-ratio diagnostic diagrams, spaxels above the maximum starburst line form the majority (∼75% and ∼50% in the diagnostic diagrams involving [O i] and [S ii] respectively). Moreover, our findings suggest that more than one alternative mechanism is ionizing the outer galaxy regions. The properties of the diffiuse component are consistent with ionization by diluted radiation and the large filaments and shells are most probably shocked areas at the edge of bubbles. The mechanism responsible for the ionization of the faint individual clumps observed in the galaxy periphery is more difficult to assess. These clumps could be the shocked debris of fragmented shells or regions where star formation is proceeding under extreme conditions.
Fast quantum non-demolition readout from longitudinal qubit-oscillator interaction
Creators: name: Didier, Nicolas
name: Bourassa, Jérôme
name: Blais, Alexandre
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show how to realize high-fidelity quantum non-demolition qubit readout using longitudinal qubit-oscillator interaction. This is realized by modulating the longitudinal coupling at the cavity frequency. The qubit-oscillator interaction then acts as a qubit-state dependent drive on the cavity, a situation that is fundamentally different from the standard dispersive case. Single-mode squeezing can be exploited to exponentially increase the signal-to-noise ratio of this readout protocol. We present an implementation of this idea in circuit quantum electrodynamics and a possible multi-qubit architecture.
description: 5 pages, 3 figures, Supplemental Material
A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. III. Discrete Multicomponent Population-dynamical Models Based on the Jeans Equations
Creators: name: Kacharov, Nikolay
name: Alfaro-Cuello, Mayte
name: Neumayer, Nadine
name: Lützgendorf, Nora
name: Watkins, Laura L.
name: Mastrobuono-Battisti, Alessandra
name: Kamann, Sebastian
name: Van De Ven, Glenn
name: Seth, Anil C.
name: Voggel, Karina T.
name: Georgiev, Iskren Y.
name: Leaman, Ryan
name: Bianchini, Paolo
name: Böker, Torsten
name: Mieske, Steffen
Publisher: name: London : Institute of Physics Publ.
Year: 2022
Subjects: subject: Stellar kinematics
subject: Globular star clusters
subject: Galaxy dynamics
subject: Ultracompact dwarf galaxies
subject: Stellar populations
subject: Galaxy nuclei
subject: 520

description: We present comprehensive multicomponent dynamical models of M54 (NGC 6715), the nuclear star cluster of the Sagittarius (Sgr) dwarf galaxy, which is undergoing a tidal disruption in the Milky Way halo. Previous papers in this series used a large MUSE mosaic data set to identify multiple stellar populations in the system and study their kinematic differences. Here, we use Jeans-based dynamical models that fit the population properties (mean age and metallicity), spatial distributions, and kinematics simultaneously. They provide a solid physical explanation for our previous findings. Population-dynamical models deliver a comprehensive view of the whole system, and allow us to disentangle the different stellar populations. We explore their dynamical interplay and confirm our previous findings about the build-up of Sgr’s nuclear cluster via contributions from globular cluster stars, Sgr inner field stars, and in situ star formation. We explore various parameterizations of the gravitational potential and show the importance of a radially varying mass-to-light ratio for the proper treatment of the mass profile. We find a total dynamical mass within M54's tidal radius (∼75 pc) of 1.60 ± 0.07 × 106 M ⊙ in excellent agreement with N-body simulations. Metal-poor globular cluster stars contribute about 65% of the total mass or 1.04 ± 0.05 × 106 M ⊙. Metal-rich stars can be further divided into young and intermediate-age populations, which contribute 0.32 ± 0.02 × 106 M ⊙ (20%) and 0.24 ± 0.02 × 106 M ⊙ (15%), respectively. Our population-dynamical models successfully distinguish the different stellar populations in Sgr’s nucleus because of their different spatial distributions, ages, metallicities, and kinematic features.
Οι ελληνοαλβανικές σχέσεις στο διάστημα 1971-1991 και ο ρόλος της ελληνικής εθνικής μειονότητας
Creators: name: Ζύκα, Αλέξανδρος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2023
Subjects: subject: Ελλάδα
subject: Αλβανία
subject: Ελληνική εθνική μειονότητα
subject: Ελληνο-αλβανικές σχέσεις

description: Στόχος της παρούσας διπλωματικής εργασίας είναι η παρουσίαση των ελληνοαλβανικών σχέσεων στο διάστημα 1971(επανέναρξη των διπλωματικών επαφών των 2 χωρών)-1991(κατάρρευση του κομμουνιστικού καθεστώτος στην Αλβανία) και η συνεισφορά της ελληνικής εθνικής μειονότητας. Ο κύριος λόγος που επιλέχθηκε το συγκεκριμένο θέμα είναι η έλλειψη επαρκών στοιχείων εκατέρωθεν μέχρι το τέλος του Ψυχρού Πολέμου. Η πραγματικότητα μεταξύ τους όμως δεν ξεκινά με τον Ψυχρό Πόλεμο αλλά πριν. Είχαν πολεμήσει μεταξύ τους στον Δεύτερο Παγκόσμιο Πόλεμο αφού η Αλβανία επιτέθηκε στην Ελλάδα μαζί με την Ιταλία ως προτεκτοράτο της, ενώ είχαν επίσης προστριβές με την ελληνική μειονότητα και με τις αλβανικές διεκδικήσεις για τους Τσάμηδες. Οπότε το ενδιαφέρον για τον λόγο αυτό επικεντρώνεται στη μετά το 1971 περίοδο που αποκαταστάθηκαν σιγά σιγά οι επαφές. Σε ένα πρώτο επίπεδο, θεωρείται σκόπιμη η συνοπτική παρουσίαση της ελληνικής μειονότητας στην Αλβανία, με αναφορά στις περιοχές όπου βρισκόταν, τη δημογραφική της κατάσταση και τη θέση της στην Αλβανία από την ανεξαρτησία της χώρας το 1912 ως την δημιουργία της Λαϊκής Δημοκρατίας της Αλβανίας το 1946. Στη συνέχεια, ακολουθεί η περιγραφή των ελληνοαλβανικών σχέσεων με τη διάκρισή τους σε δύο χρονικές περιόδους: η πρώτη είναι από το 1946 ως το 1971-η οποία λειτουργεί ως υπόβαθρο για τη βασική χρονική περίοδο-και η δεύτερη που είναι και το αντικείμενο της εργασίας. Για την ευκολότερη παρουσίασή του, κρίνεται σκόπιμη η διάκρισή της σε δύο υποπεριόδους: από το 1971 ως το 1985 και από το 1985 ως το 1991, έχοντας ως «ορόσημο» το έτος 1985, όταν και πέθανε ο Αλβανός ηγέτης Ενβέρ Χότζα. Επομένως, αυτή η διάκριση γίνεται για να εντοπιστούν οι διαφορές της αλβανικής εξωτερικής πολιτικής πριν και μετά τον θάνατο του Χότζα. Τέλος, θα γίνει λόγος για τον ρόλο που άσκησε η μειονότητα στις σχέσεις των 2 χωρών. Και στις 2 αυτές υποπεριόδους, γίνεται αναφορά σε επιμέρους γεγονότα τα οποία διαδραμάτισαν σημαντικό ρόλο στις ελληνοαλβανικές σχέσεις, όπως είναι για παράδειγμα ο ελληνικός εμφύλιος πόλεμος, η επιχείρηση Valuable με σκοπό την ανατροπή του Χότζα, η γεωστρατηγική επιλογή της Αλβανίας μετά το 1961 να στραφεί αρχικά στη Λαϊκή Δημοκρατία της Κίνας κι ύστερα από τον θάνατο του Μάο Τσε-τούνγκ το 1976 να στραφεί στην εσωστρέφεια. Στο τελευταίο μέρος, θα επιχειρηθεί η ανάλυση για το πώς η μειονότητα επηρέασε κι επηρεάστηκε από τις εξελίξεις στις σχέσεις των δύο χωρών στη περίοδο που απασχολεί τη παρούσα εργασία.
Nucleosome positioning: resources and tools online
Creators: name: Teif, Vladimir B.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Genomics (q-bio.GN)
subject: Biological Physics (physics.bio-ph)
subject: Biomolecules (q-bio.BM)
subject: Machine Learning (stat.ML)
subject: FOS: Biological sciences
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Nucleosome positioning is an important process required for proper genome packing and its accessibility to execute the genetic program in a cell-specific, timely manner. In the recent years hundreds of papers have been devoted to the bioinformatics, physics and biology of nucleosome positioning. The purpose of this review is to cover a practical aspect of this field, namely to provide a guide to the multitude of nucleosome positioning resources available online. These include almost 300 experimental datasets of genome-wide nucleosome occupancy profiles determined in different cell types and more than 40 computational tools for the analysis of experimental nucleosome positioning data and prediction of intrinsic nucleosome formation probabilities from the DNA sequence. A manually curated, up to date list of these resources will be maintained at http://generegulation.info.
description: To appear in Briefings in Bioinformatics
Study of cosmic ray events with high muon multiplicity using the ALICE detector at the CERN Large Hadron Collider
Creators: name: ALICE Collaboration
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: ALICE is one of four large experiments at the CERN Large Hadron Collider near Geneva, specially designed to study particle production in ultra-relativistic heavy-ion collisions. Located 52 meters underground with 28 meters of overburden rock, it has also been used to detect muons produced by cosmic ray interactions in the upper atmosphere. In this paper, we present the multiplicity distribution of these atmospheric muons and its comparison with Monte Carlo simulations. This analysis exploits the large size and excellent tracking capability of the ALICE Time Projection Chamber. A special emphasis is given to the study of high multiplicity events containing more than 100 reconstructed muons and corresponding to a muon areal density $ρ_μ > 5.9~$m$^{-2}$. Similar events have been studied in previous underground experiments such as ALEPH and DELPHI at LEP. While these experiments were able to reproduce the measured muon multiplicity distribution with Monte Carlo simulations at low and intermediate multiplicities, their simulations failed to describe the frequency of the highest multiplicity events. In this work we show that the high multiplicity events observed in ALICE stem from primary cosmic rays with energies above $10^{16}$ eV and that the frequency of these events can be successfully described by assuming a heavy mass composition of primary cosmic rays in this energy range. The development of the resulting air showers was simulated using the latest version of QGSJET to model hadronic interactions. This observation places significant constraints on alternative, more exotic, production mechanisms for these events.
description: 23 pages, 10 captioned figures, 3 tables, authors from page 18, published version, figures at http://aliceinfo.cern.ch/ArtSubmission/node/2419
Consensus Statements for Management of Barrett's Dysplasia and Early-Stage Esophageal Adenocarcinoma, Based on a Delphi Process
Creators: name: Kay, Elaine
name: Grabsch, Heike
name: Manner, Hendrik
name: Green, Susi
name: Loft, Duncan
name: Pech, Oliver
name: Inadomi, John
name: Ali, Haythem
name: Singh, Rajvinder
name: Rice, Thomas W.
name: Galmiche, Jean Paul
name: Hart, John
name: Anderson, Mark
name: Chak, Amitabh
name: Cestari, Renzo
name: Shaheen, Nicholas J.
name: Stein, Hubert J.
name: Longcroft-Wheaton, Gaius
name: Kaye, Philip
name: Lundell, Lars
name: Stuart, Robert
name: Nanji, Manoj
name: Corley, Douglas A.
name: Al Dulaimi, David
name: Attwood, Stephen
name: Waxman, Irving
name: Goldblum, John
name: Mairs, Philip
name: Johnston, David
name: Decaestecker, John
name: Sontag, Stephen
name: Jankowski, Janusz A.Z.
name: Odze, Robert
name: Murray, Iain
name: Going, James J.
name: Allen, John
name: Dunn, Lorna
name: Preston, Sean
name: Lerut, Toni
name: Lovat, Laurence B.
name: Bergman, Jacques
name: Gordon, Charles
name: Vakil, Nimish
name: Shimoda, Tadakuza
name: Sanders, Scott
name: Bennett, Cathy
name: Allum, Bill
name: Regula, Jaroslaw
name: Forbes-Young, Ricky
name: Abley, Chris
name: Moayyedi, Paul
name: Hochberger, Juergen
name: Curtis, Howard
name: Wang, Kenneth
name: Ferguson, Mark K.
name: Talley, Nicholas J.
name: Sampliner, Richard
name: Armstrong, David
name: Cengia, Gianpaolo
name: Malfertheiner, Peter
name: Poller, David
name: Krishnadath, Kausilia
name: Gay, Laura
name: Harrison, Rebecca
name: Fennerty, M. Brian
name: Tack, Jan
name: Meltzer, Stephen J.
name: Haigh, Chris
name: Romero, Yvonne
name: Watson, Peter
name: Griffin, S. Michael
name: Gittens, Stuart
name: Fullarton, Grant
name: Tham, Tony C.K.
name: Sharma, Prateek
name: Penman, Ian
name: Falk, Gary
name: Shepherd, Neil
name: Yerian, Lisa
name: Kahrilas, Peter
name: Falck-Ytter, Yngve
name: Barr, Hugh
name: Vieth, Michael
name: Bhandari, Pradeep
name: Hewin, David
name: Ganz, Robert
name: Hongo, Michio
name: Rugge, Massimo
name: Ragunath, Krish
name: Spechler, Stuart
name: Davies, Gareth
name: Ell, Christian
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Esophageal adenocarcinoma (EA) is increasingly common among patients with Barrett’s esophagus (BE). We aimed to provide consensus recommendations based on the medical literature that clinicians could use to manage patients with BE and low-grade dysplasia, high-grade dysplasia (HGD), or early-stage EA.
MPEC 2024-R201 : 2024 RL8
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 RL8

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Maximizing Opportunities and Avoiding Mistakes in Triple Therapy for Hepatitis C Virus
Creators: name: Barritt IV, A. Sidney
name: Fried, Michael W.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Recently developed drugs and innovative strategies for the treatment of chronic infection with genotype 1 hepatitis C virus (HCV) have become the standard of care. The protease inhibitors telaprevir (Incivek) and boceprevir (Victrelis) are the first direct-acting antiviral (DAA) agents approved, and many more are being developed. These drugs substantially increased rates of sustained virologic response in treatment-naïve and -experienced patients, in conjunction with peginterferon and ribavirin (triple therapy), in phase 3 trials. The efficacy of triple therapy depends on appropriate selection of patients, although the population of patients that receive triple therapy could be expanded as the risk/benefit ratio improves. Attention to details that reflect the standard of care, such as appropriate dosing, anticipation of adverse effects, and strict adherence to stopping rules, will insure the success of these drugs and lead the way for new combination therapies.
Ένας "ιδιαίτερος δρόμος" στο Σύμφωνο της Βαρσοβίας : η Ρουμανία επί Ν. Τσαουσέσκου, 1965-1989
Creators: name: Τσουρέκης Ορφανίδης, Κωνσταντίνος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2023
Subjects: subject: Σύμφωνο της Βαρσοβίας
subject: Ρουμανία
subject: Τσαουσέσκου
subject: Εθνικός κομμουνισμός
subject: Ψυχρός πόλεμος

description: Η παρούσα εργασία με τίτλο Ένας «ιδιαίτερος δρόμος» στο Σύμφωνο της Βαρσοβίας: Η Ρουμανία επί Ν. Τσαουσέσκου, 1965 – 1989 αποτελεί μια προσπάθεια να παρουσιαστεί ο ιδιαίτερος χειρισμός των εξωτερικών σχέσεων της Ρουμανίας επί της προεδρίας του Νικολάε Τσαουσέσκου κατά την κομμουνιστική περίοδο αλλά και να αναλυθούν οι συνθήκες στο εσωτερικό της χώρας όπου ουσιαστικά διαμορφώθηκαν έπειτα από υιοθέτηση προτύπων διακυβέρνησης άλλων κρατών. Έμπνευση για το θέμα αποτέλεσε μια σύντομη μελέτη της ρουμανικής εξωτερικής πολιτικής όπου με ενδιαφέρον διαπιστώθηκε η άρνηση υπακοής στις οδηγίες της Μόσχας, η μετάβαση στον εθνικό κομμουνισμό, η προσπάθεια ικανοποίησης τόσο των κομμουνιστών συμμάχων του, όσο και των Δυτικών, η μεγάλη επιρροή του μοντέλου της Βόρειας Κορέας στον κρατικό μηχανισμό κ.α.
Equivariant Fields in an $SU({\cal N})$ Gauge Theory with new Spontaneously Generated Fuzzy Extra Dimensions
Creators: name: Kurkcuoglu, S.
name: Unal, G.
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We find new spontaneously generated fuzzy extra dimensions emerging from a certain deformation of $N=4$ supersymmetric Yang-Mills (SYM) theory with cubic soft supersymmetry breaking and mass deformation terms. First, we determine a particular four dimensional fuzzy vacuum that may be expressed in terms of a direct sum of product of two fuzzy spheres, and denote it in short as $S_F^{2\, Int}\times S_F^{2\, Int}$. The direct sum structure of the vacuum is revealed by a suitable splitting of the scalar fields in the model in a manner that generalizes our approach in \cite{Seckinson}. Fluctuations around this vacuum have the structure of gauge fields over $S_F^{2\, Int}\times S_F^{2\, Int}$, and this enables us to conjecture the spontaneous broken model as an effective $U(n)$ $(n < {\cal N})$ gauge theory on the product manifold $M^4 \times S_F^{2\, Int} \times S_F^{2\, Int}$. We support this interpretation by examining the $U(4)$ theory and determining all of the $SU(2)\times SU(2)$ equivariant fields in the model, characterizing its low energy degrees of freedom. Monopole sectors with winding numbers $(\pm 1,0),\,(0,\pm1),\,(\pm1,\pm 1)$ are accessed from $S_F^{2\, Int}\times S_F^{2\, Int}$ after suitable projections and subsequently equivariant fields in these sectors are obtained. We indicate how Abelian Higgs type models with vortex solutions emerge after dimensionally reducing over the fuzzy monopole sectors as well. A family of fuzzy vacua is determined by giving a systematic treatment for the splitting of the scalar fields and it is made manifest that suitable projections of these vacuum solutions yield all higher winding number fuzzy monopole sectors. We observe that the vacuum configuration $S_F^{2\, Int}\times S_F^{2\, Int}$ identifies with the bosonic part of the product of two fuzzy superspheres with $OSP(2,2)\times OSP(2,2)$ supersymmetry and elaborate on this feature.
description: 38+1 pages, published version
Nonsteroidal Anti-inflammatory Drug Use Reduces Risk of Adenocarcinomas of the Esophagus and Esophagogastric Junction in a Pooled Analysis
Creators: name: Freedman, Neal D.
name: Murray, Liam J.
name: Gammon, Marilie D.
name: Pandeya, Nirmala
name: Vaughan, Thomas L.
name: Giffen, Carol
name: Bernstein, Leslie
name: Wu, Anna H.
name: Risch, Harvey A.
name: Cook, Michael B.
name: Corley, Douglas A.
name: Sadeghi, Shahram
name: Liao, Linda M.
name: Kamangar, Farin
name: Whiteman, David C.
name: Casson, Alan G.
name: Abnet, Christian C.
name: Chow, Wongho
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Regular use of aspirin and other non-steroidal anti-inflammatory drugs (NSAID) has been reported to reduce risks for esophageal adenocarcinoma (EAC) and esophagogastric junctional adenocarcinoma (EGJA). However, individual studies have been too small to accurately assess the effects of medication type, frequency, or duration of use. We performed a pooled analysis to investigate these associations.
Publication and collaboration anomalies in academic papers originating from a paper mill: Evidence from a Russia-based paper mill
Creators: name: Abalkina, Anna
Publisher: name: Freie Universität Berlin
Year: 2023
Subjects: subject: academic misconduct
subject: co-authorship for sale
subject: ghostwriting
subject: hijacked journals
subject: journals
subject: paper mills
subject: suspicious collaboration
subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::050 Zeitschriften, fortlaufende Sammelwerke::050 Zeitschriften, allgemeine fortlaufende Sammelwerke

description: This study attempts to detect papers originating from the Russia-based paper mill ‘International Publisher’ LLC. A total of 1,063 offers to purchase co-authorship on a fraudulent papers published from 2019 to mid-2022 on the 123mi.ru website were analysed. This study identifies at least 451 papers that are potentially linked to the paper mill, including one preprint, a duplication paper and 16 republications of papers erroneously published in hijacked journals. Evidence of suspicious provenance from the paper mill is provided: matches in title, number of co-authorship slots, year of publication, country of the journal, country of a co-authors and similarities of abstracts. These problematic papers are co-authored by scholars from at least 39 countries and are submitted to both predatory and reputable journals. This study also demonstrates collaboration anomalies in questionable papers and examines indicators of the Russia-based paper mill. The value of co-authorship slots offered by ‘International Publisher’ LLC from 2019 to 2021 is estimated at $6.5 million. Since this study only analysed a single paper mill, it is likely that the number of papers with forged authorship is much higher.
Additional file 5 of Accumulation of copy number alterations and clinical progression across advanced prostate cancer
Creators: name: Grist, Emily
name: Friedrich, Stefanie
name: Brawley, Christopher
name: Mendes, Larissa
name: Parry, Marina
name: Ali, Adnan
name: Haran, Aine
name: Hoyle, Alex
name: Gilson, Claire
name: Lall, Sharanpreet
name: Zakka, Leila
name: Bautista, Carla
name: Landless, Alex
name: Nowakowska, Karolina
name: Wingate, Anna
name: Wetterskog, Daniel
name: Hasan, A. M. Mahedi
name: Akato, Nafisah B.
name: Richmond, Malissa
name: Ishaq, Sofeya
name: Matthews, Nik
name: Hamid, Anis A.
name: Sweeney, Christopher J.
name: Sydes, Matthew R.
name: Berney, Daniel M.
name: Lise, Stefano
name: Parmar, Mahesh K. B.
name: Clarke, Noel W.
name: James, Nicholas D.
name: Cremaschi, Paolo
name: Brown, Louise C.
name: Attard, Gerhardt
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 5. List of STAMPEDE investigators.