bluuebunny/crossref_metadata_2025_split huggingface dataset:
Design and verification of a highly accurate in-situ hyperspectral radiometric measurement system (HyperNav)
Authors: Barnard Andrew , Boss Emmanuel , Haëntjens Nils , Orrico Cristina , Frouin Robert , Tan Jing , Klumpp Justin , Dewey Michael , Walter David , Mazloff Matthew , Chamberlain Paul 
Published: June 2024

Hyperspectral optical observations of the Earth’s surface oceans from space offer a means to improve our understanding of ocean biology and biogeochemistry. NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite mission, which includes a hyperspectral ocean color instrument (OCI), will provide radiometric observations of surface ocean with near continuous spectral resolution across the near UV to NIR range. Maintaining sufficient accuracy over the lifetime of satellite ocean color missions requires a robust program for system vicarious calibration (SVC) and product validation. The system vicarious calibration process combines satellite sensor data with in-situ radiometric/optical measurements to remove potential biases due to the combined errors from both satellite radiometric sensor calibration and atmospheric correction. As such, high accuracy, high-spectral resolution in-situ radiometric measurements are required to provide a principal source of truth for the satellite-derived products. To meet the requirements, a novel in-situ radiometric system, called HyperNav, has been developed, rigorously characterized and field tested. Key attributes of HyperNav are dual upwelling radiance heads coupled to individual spectrometers, spectral resolution of ∼2.2 nm (full width, half-maximum) across 320–900 nm, integrated shutter systems for dark measurements, and integrated tilt and pressure sensors. The HyperNav operational modes include traditional profiling and surface modes, as well as integration with an autonomous profiling float for unattended deployment, offering a new capability for a network of autonomous platforms to support the long-term needs for hyperspectral ocean color remote sensing observations. This paper describes the HyperNav design, in-situ operational modes, and field verification results.
Epirubicin and Non-Muscle Invasive Bladder Cancer Treatment: A Systematic Review
Authors: Chiujdea Sever , Ferro Matteo , Vartolomei Mihai Dorin , Lucarelli Giuseppe , Bekku Kensuke , Matsukawa Akihiro , Parizi Mehdi Kardoust , Klemm Jakob , Tsuboi Ichiro , Fazekas Tamas , Mancon Stefano , Shariat Shahrokh F. 
Published: June 2024

(1) Background: Intravesical chemotherapy is the standard of care in intermediate-risk non-muscleinvasive bladder cancer (NMIBC). Different agents are used across the world based on availability, cost, and practice patterns. Epirubicin (EPI), one of these agents, has been used by many centers over many decades. However, its true differential efficacy compared to other agents and its tolerability are still poorly reported. We aimed to assess the differential efficacy and safety of intravesical EPI in NMIBC patients. (2) Methods: This study aimed to systematically review the efficacy and safety profile of Epirubicin (EPI) in the management of non-muscle invasive bladder cancer (NMIBC) compared to other adjuvant therapies. A systematic search of the PUBMED, Web of Science, clinicaltrials.gov, and Google Scholar databases was conducted on 31 December 2023, using relevant terms related to EPI, bladder cancer, and NMIBC. The inclusion criteria targeted studies that evaluated patients treated with EPI following the transurethral resection of bladder tumors (TURBT) for NMIBC and compared oncological outcomes such as recurrence and progression with other adjuvant therapies, including Mitomycin C (MMC), Gemcitabine (GEM), and Bacillus Calmette-Guérin (BCG). Additionally, studies investigating the safety profile of EPI administered intravesically at room temperature and under hyperthermia, as well as oncological outcomes associated with hyperthermic intravesical EPI administration, were included. (3) Results: Eleven studies reported adverse events after adjuvant intravesical instillations with EPI; the most frequently reported adverse events included cystitis (34%), dysuria, pollakiuria, hematuria, bladder irritation/spasms, fever, nausea and vomiting, and generalized skin rash (2.3%). Nine studies compared EPI to BCG in terms of recurrence and progression rates; BCG instillations showed a lower recurrence rate compared to EPI, with limited or non-significant differences in progression rates. Two studies found no significant differences between EPI and MMC regarding progression and recurrence rates. One study showed statistically significant lower recurrence and progression rates with GEM in high-risk NMIBC patients. Another study found no significant differences between EPI and GEM regarding recurrence and progression. (4) Conclusions: EPI exhibits similar oncological performances to Gemcitabine and Mitomycin C currently used for adjuvant therapy in NMIBC. Novel delivery mechanisms such as hyperthermia are interesting newcomers.
A VARIANT OF BUILDING A FUZZY HELICOPTER AIR COLLISION AVOIDANCE SYSTEM BASED ON A LASER SCANNING SYSTEM (LIDAR)
Authors: Замыслов Михаил Александрович , Мальцев Александр Михайлович , Михайленко Сергей Борисович , Тарасов Сергей Васильевич , Штанькова Надежда Викторовна 
Published: June 2024

В статье рассматриваются вопросы построения нечеткой вертолетной системы предупреждения столкновений в воздухе с другими летательными аппаратами на основе использования данных, поступающих от бортовой лазерной сканирующей системы (лидара) вертолета. Разработаны алгоритм оценки опасности столкновения вертолетов на основе использования методов нечеткой логики и структурная схема нечеткого контроллера, формирующего информационные сигналы об опасности сближения для комплекса бортового оборудования вертолета. Проведено имитационное моделирования поведения нечеткой системы средствами расширения Simulink. Приводятся некоторые результаты моделирования, подтверждающие работоспособность вертолетной системы предупреждения столкновения, и вариант реализации рассматриваемой нечеткой системы в кодах программ Fuzzy Logic Toolbox.
The article discusses the construction of a fuzzy helicopter system for preventing collisions in the air with other aircraft based on the use of data received from the onboard laser scanning system (lidar) of the helicopter. An algorithm for assessing the danger of a helicopter collision based on the use of fuzzy logic methods and a structural diagram of a fuzzy controller that generates information signals about the danger of approaching for the helicopter's onboard equipment complex have been developed. Simulation modeling of the behavior of a fuzzy system by means of the Simulink extension was carried out. Some simulation results confirming the operability of the helicopter collision avoidance system and a variant of the implementation of the fuzzy system in the codes of the Fuzzy Logic Toolbox programs are presented.
The Role of Active Galactic Nucleus Winds in Galaxy Formation: Connecting AGN Outflows at Low Redshifts to the Formation/Evolution of Their Host Galaxies
Authors: Torres-Papaqui Juan Pablo , Coziol Roger , Robleto-Orús Aitor C. , Cutiva-Alvarez Karla A. , Roco-Avilez Paulina 
Published: June 2024

Abstract
Using Sloan Digital Sky Survey (SDSS) spectra, we applied an automatic method to search for outflows (OFs) in three large samples of narrow-line active galactic nuclei (AGN) at low redshifts (z < 0.4), separated into three spectral activity classes: radio-loud galaxies (RGs), 15,793; radio-quiet Seyfert 2 AGN (Sy2), 18,585; and LINERs, 25,656. In general, the probability of detecting an OF decreases along the sequence Sy1→Sy2→LINER/RG and independently of the AGN class, the wind velocity, traced by W80, increases with the AGN luminosity. Moreover W80 is systematically higher in RGs or any of the other AGN classes when detected in radio. These results support the idea that there are two main modes of production of OF, the radiative mode dominant in radio-quiet AGN and the jet mode dominant in RGs, although both modes could also happen simultaneously at different levels. From the spectra and SDSS photometry, the characteristics of the AGN host galaxies and their supermassive black holes (SMBHs) were also retrieved using the stellar population synthesis code STARLIGHT. This revealed that, independently of the AGN spectral class, (1) galaxy hosts with OFs have systematically later morphological types and higher star formation rates (SFRs) than their counterparts without OF, (2) the AGN occupy different positions in the specific diagnostic diagram (specific black hole accretion rate (sBHAR) versus specific SFR), which suggests they follow different evolutionary paths congruent with the morphology of their galaxy hosts, and (3) they show no evidence of AGN quenching or triggering of star formation. These results are consistent with a scenario explaining the different AGN classes as consequences of different formation processes of galaxies: early-type galaxies (LINERs and RGs) formed bigger bulges and more massive SMBHs, exhausting their reservoir of gas more rapidly than late-type galaxies (Sy2 and Sy1), and thereby quenching their star formation and starving their SMBHs.
The Nonsingular Estimator for Exoplanet Orbits: An Unscented Batch Estimation Method for Direct Imaging Measurements
Authors: Stojanovski Zvonimir , Savransky Dmitry 
Published: June 2024

Abstract
We present a new method for fitting exoplanet orbits to direct astrometric measurements, using nonlinear batch estimation and nonsingular orbital elements. Our estimation technique is based on the unscented transform, which approximates probability distributions using finite, deterministic sets of weighted sample points. Furthermore, we use Gaussian mixtures to account for the strong nonlinearities in the measurement model. As a fitting basis, we use a set of orbital elements developed specifically for directly observed exoplanets, combining features of the Thiele–Innes constants and the Cohen–Hubbard nonsingular elements. We validate the new method using simulated exoplanet orbits, and we demonstrate its use with real exoplanet data. Compared to state-of-the-art Markov Chain Monte Carlo and Bayesian rejection sampling techniques, the new method is found to give orbit estimates of comparable or higher accuracy but with much faster execution.
Physical Properties of Type II Supernovae Inferred from ZTF and ATLAS Photometric Data
Authors: Silva-Farfán Javier , Förster Francisco , Moriya Takashi J. , Hernández-García L. , Muñoz Arancibia A. M. , Sánchez-Sáez P. , Anderson Joseph P. , Tonry John L. , Clocchiatti Alejandro 
Published: June 2024

Abstract
We report an analysis of a sample of 186 spectroscopically confirmed Type II supernova (SN) light curves (LCs) obtained from a combination of Zwicky Transient Facility (ZTF) and Asteroid Terrestrial-impact Last Alert System observations. We implement a method to infer physical parameters from these LCs using hydrodynamic models that take into account the progenitor mass, the explosion energy, and the presence of circumstellar matter (CSM). The CSM is modeled via the mass-loss rate, wind acceleration at the surface of the progenitor star with a β velocity law, and the CSM radius. We also infer the time of explosion, attenuation (A

V
), and the redshift for each SN. Our results favor low-mass progenitor stars (M
ZAMS < 14 M
⊙) with a dense CSM (

M

̇

> 10−3
M
⊙ yr−1, CSM radius ∼ 1015 cm, and β > 2). Additionally, we find that the redshifts inferred from the SN LCs are significantly more accurate than those inferred using the host galaxy photometric redshift, suggesting that this method could be used to infer more accurate host galaxy redshifts from large samples of Type II SNe in the LSST era. Lastly, we compare our results with similar works from the literature.
The Galactic Center Lobe as an H ii Region
Authors: Anderson L. D. , Luisi Matteo , Liu B. , Linville Dylan J. , Benjamin Robert A. , Hurley-Walker Natasha , McClure-Griffiths N. M. , Zucker Catherine 
Published: June 2024

Abstract
The Galactic center lobe (GCL) is an object ∼1° across that is located north of the Galactic center. In the mid-infrared (MIR) the GCL appears as two 8.0 μm filaments between which there is strong 24 μm and radio continuum emission. Due to its morphology and location in the sky, previous authors have argued that the GCL is located in the Galactic center region, created by outflows from star formation or by activity of the central black hole Sagittarius A*. In an associated paper, low-frequency radio emission indicates that the GCL must instead lie foreground to the Galactic center. If the GCL is foreground to the Galactic center, it is likely to be a type of object common throughout the Galactic disk; we here investigate whether its properties are similar to those of Galactic H ii regions. We find that the GCL’s MIR morphology, MIR flux densities, dust temperatures, and radio recombination line properties as traced by the Green Bank Telescope Diffuse Ionized Gas Survey are consistent with those of known Galactic H ii regions, although the derived electron temperature is low. We search for the ionizing source(s) of the possible H ii region and identify a stellar cluster candidate (Camargo #1092/Ryu & Lee #532) and a cluster of young stellar objects (the SPICY cluster G359.3+0.3) whose members have Gaia parallaxes distances of 1.7 ± 0.4 kpc. Taken together, the results of our companion paper and those shown here suggest that the GCL has properties consistent with those of an H ii region located ∼2 kpc from the Sun.
Stellar X-Ray Activity and Habitability Revealed by the ROSAT Sky Survey
Authors: Han Henggeng , Wang Song , Zheng Chuanjie , Li Xue , Xiao Kai , Liu Jifeng 
Published: June 2024

Abstract
Using the homogeneous X-ray catalog from ROSAT observations, we conducted a comprehensive investigation into stellar X-ray activity–rotation relations for both single and binary stars. Generally, the relation for single stars consists of two distinct regions: a weak decay region, indicating a continued dependence of the magnetic dynamo on stellar rotation rather than a saturation regime with constant activity, and a rapid decay region, where X-ray activity is strongly correlated with the Rossby number. Detailed analysis reveals more fine structures within the relation: in the extremely fast-rotating regime, a decrease in X-ray activity was observed with increasing rotation rate, referred to as supersaturation, while in the extremely slow-rotating region, the relation flattens, mainly due to the scattering of F stars. This scattering may result from intrinsic variability in stellar activities over one stellar cycle or the presence of different dynamo mechanisms. Binaries exhibit a similar relation to that of single stars while the limited sample size prevented the identification of fine structures in the relation for binaries. We calculated the mass-loss rates of planetary atmospheres triggered by X-ray emissions from host stars. Our findings indicate that for an Earthlike planet within the stellar habitable zone, it would easily lose its entire primordial H/He envelope (equating to about 1% of the planetary mass).
Debris Disks Can Contaminate Mid-infrared Exoplanet Spectra: Evidence for a Circumstellar Debris Disk around Exoplanet Host WASP-39
Authors: Flagg Laura , Weinberger Alycia J. , Bell Taylor J. , Welbanks Luis , Morello Giuseppe , Powell Diana , Bean Jacob L. , Blecic Jasmina , Crouzet Nicolas , Gao Peter , Inglis Julie , Kirk James , López-Morales Mercedes , Molaverdikhani Karan , Nikolov Nikolay , Oza Apurva V. , Rackham Benjamin V. , Redfield Seth , Tsai Shang-Min , Jayawardhana Ray , Kreidberg Laura , Nixon Matthew C. , Stevenson Kevin B. , Turner Jake D. 
Published: June 2024

Abstract
The signal from a transiting planet can be diluted by astrophysical contamination. In the case of circumstellar debris disks, this contamination could start in the mid-infrared and vary as a function of wavelength, which would then change the observed transmission spectrum for any planet in the system. The MIRI/Low Resolution Spectrometer WASP-39b transmission spectrum shows an unexplained dip starting at ∼10 μm that could be caused by astrophysical contamination. The spectral energy distribution displays excess flux at similar levels to that which are needed to create the dip in the transmission spectrum. In this Letter, we show that this dip is consistent with the presence of a bright circumstellar debris disk, at a distance of >2 au. We discuss how a circumstellar debris disk like that could affect the atmosphere of WASP-39b. We also show that even faint debris disks can be a source of contamination in MIRI exoplanet spectra.
Reliability of the Mendonça Strabismus Forceps in Locating the Insertion of Extraocular Rectus Muscles in Patients Undergoing Strabismus Surgery
Authors: Borges Corrêa Alyne , Rossetto Júlia Dutra , Mendonça Tomás Scalamandré 
Published: June 2024

Purpose
To evaluate the reliability of Mendonça strabismus forceps in locating the extraocular rectus muscles in patients undergoing primary strabismus surgery or reoperation. The study also compared the method's efficacy in primary surgeries versus reoperations. The overall goal was to avoid unnecessary surgical exploration, thereby enabling more effective planning and safer surgery.

Methods
The study included 41 patients with strabismus undergoing surgical correction. The reliability of the Mendonça strabismus forceps in locating the extraocular rectus muscles was evaluated by comparing preoperative measurements using Mendonça strabismus forceps and Castroviejo forceps to intraoperative measurements made by direct muscle visualization. Differences of 1 mm or less were deemed acceptable.

Results
In patients without prior surgery, Mendonça strabismus forceps reliably located all muscles, with measurements consistently within the 1-mm limit. All muscles with previous surgeries were successfully grasped by the forceps, except for one medial rectus muscle with multiple interventions. In reoperations with satisfactory muscle grasp, 88.8% showed coincident measurements. Non-coincidence cases were attributed to anomalous scarring. The method demonstrated simplicity, cost-effectiveness, and no complications in this study.

Conclusions
The Mendonça strabismus forceps proved to be a reliable and non-invasive method for locating extraocular rectus muscles insertions without the need for additional imaging. It is a cost-effective, simple, and easily executed method that provides valuable information for surgical decision-making and planning. The method enhances surgical outcomes while reducing risks.

[
J Pediatr Ophthalmol Strabismus
. 2024;61(6):404–409.]
Histopathologic Change in the Anterior Part of the Posterior Fixation Suture After a Faden Operation in an Animal Model
Authors: Kim Seung-Hyun , Kang Eunseok , Kang Boram , Ha Suk-Gyu 
Published: June 2024

Purpose:
To observe postoperative histological changes in the anterior part of the posterior fixation suture after a Faden operation in an animal model.

Methods:
A posterior fixation suture was placed at two points 6 mm posterior to the insertion of the extraocular muscle on the superior rectus muscle of the right eye in eight rabbits. The superior rectus muscle of the left eye was used as a control. The eyes were enucleated and the anterior portion of the posterior fixation suture, including the myoscleral junction, was extracted 4 weeks after surgery. Postoperative adhesion was graded from 0 to 4 based on histologic findings (hematoxylin–eosin and Masson's trichrome staining).

Results:

Histological evaluation revealed diffuse fibrosis at the myoscleral junction and the anterior part of the posterior fixation suture after the Faden operation. The graded scores for fibrosis, acute inflammation, chronic inflammation, and foreign body reactions in the Faden operation group were significantly higher than those in the control group (
P
< .05). Postoperative diffuse fibrosis of the myoscleral junction and anterior-to-posterior fixation sutures were observed in an animal model.

Conclusions:
Histologic changes may affect ocular alignment and motility, making reoperation unpredictable after the Faden procedure.

[
J Pediatr Ophthalmol Strabismus
. 2024;61(5):371–375.]
Visokoentropijske zlitine za supertihe transformatorje
Authors: Luzar Jože 
Published: June 2024

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Traduction des miracles et miracle de la traduction : T. H. Huxley traducteur engagé
Authors: Coste Bénédicte 
Published: June 2024

Thomas H. Huxley n’est guère connu comme traducteur mais L’Histoire de la translation des bienheureux martyrs S. Marcellin et S. Pierre d’Éginhard, qu’il traduit partiellement en anglais, mérite un examen. Publié dans Nineteenth Century, l’article « The Value of Witness to the Miraculous » (1889) s’inscrit dans un débat fondamental sur le caractère révélé de la religion chrétienne que mène Huxley en partie contre le monde religieux. Fragmentaire, s’appuyant sur la traduction en français de Teulet et inscrite dans l’éthique de la croyance de W.K. Clifford, elle permet à Huxley d’invalider la valeur du témoignage d’Éginhard. Toujours commentée au fil de la plume, sa traduction sert également de couverture au véritable objet de la remise en cause d’Huxley : le Nouveau Testament.