Data Reduction Procedures Research Articles

HI line observations of 290 evolved stars made with the Nancay Radio Telescope. I. Data

We present a compendium of 21-cm line observations of circumstellar envelopes (CSEs) of 290 evolved stars, mostly (sim 84<!PCT!>) on the asymptotic giant branch (AGB), made with the 100m-class, single-dish Radio Telescope. The observational and data reduction procedures were optimised to separate genuine CSE emission from surrounding Galactic line features. For most targets (254), the results have not been previously published. Clear detections were made of 34 objects, for 33 of which the total flux and the size of the CSE could be determined. Possible detections were made of 21 objects, and upper limits could be determined for 95 undetected targets, while for 140 objects confusion from Galactic emission along the line of sight precluded meaningful upper limits. The collective results of this survey can provide guidance on the detectability of circumstellar gas for future mapping and imaging studies.

Scylla. I. A Pure-parallel, Multiwavelength Imaging Survey of the ULLYSES Fields in the LMC and SMC

Scylla is a deep Hubble Space Telescope (HST) survey of the stellar populations, interstellar medium, and star formation in the LMC and SMC. As a pure-parallel complement to the Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES) survey, Scylla obtained 342 orbits of ultraviolet (UV) through near-IR imaging of the LMC and SMC with Wide Field Camera 3. In this paper, we describe the science objectives, observing strategy, data reduction procedure, and initial results from our photometric analysis of 96 observed fields. Although our observations were constrained by ULLYSES primary exposures, we imaged all fields in at least two filters (F475W and F814W) and 64% of fields in at least three and as many as seven WFC3 filters spanning the UV to IR. Overall, we reach average 50% completeness of m F225W = 26.0, m F275W = 26.2, m F336W = 26.9, m F475W = 27.8, m F814W = 25.5, m F110W = 24.7, and m F160W = 24.0 Vega mag in our photometric catalogs, which is faintward of the ancient main-sequence turnoff in all filters. The primary science goals of Scylla include characterizing the structure and properties of dust in the MCs, as well as their spatially resolved star formation and chemical enrichment histories. Our images and photometric catalogs, which represent the widest-area coverage of MCs with HST photometry to date, are available as a high-level science product at the Barbara A. Mikulski Archive for Space Telescopes.

EDIG-CHANGE. III. The lagging eDIG revealed by multi-slit spectroscopy of NGC 891

The kinematic information of the extraplanar diffuse ionized gas (eDIG) around galaxies provides clues to the origin of the gas. The eDIG-CHANGES project studies the physical and kinematic properties of the eDIG around the CHANG-ES sample of nearby edge-on disk galaxies. We use a novel multi-slit narrow-band spectroscopy technique to obtain the spatial distribution of the spectral properties of the ionized gas around NGC 891, which is often regarded as an analogue of the Milky Way. We developed specific data reduction procedures for the multi-slit narrow-band spectroscopy data taken with the MDM 2.4m telescope. The data presented in this paper cover the Halpha and N II emission lines. The eDIG traced by the Halpha and N II lines shows an obvious asymmetric morphology, being brighter in the northeastern part of the galactic disk and extending a few kiloparsecs above and below the disk. Global variations in the N II /Halpha line ratio suggest additional heating mechanisms for the eDIG at large heights beyond photoionization. We also construct position-velocity (PV) diagrams of the eDIG based on our optical multi-slit spectroscopy data and compare them to similar PV diagrams constructed with the H I data. The dynamics of the two gas phases are generally consistent with each other. Modelling the rotation curves at different heights from the galactic mid-plane suggests a vertical negative gradient in turnover radius and maximum rotation velocity, with magnitudes of approximately $3 kpc kpc^ $ and $22-25 km s^ kpc^ $, respectively. Our measured vertical gradients of the rotation curve parameters suggest significant differential rotation of the ionized gas in the halo, often referred to as the lagging eDIG. Systematic study of the lagging eDIG, using the multi-slit narrow-band spectroscopy technique developed in our eDIG-CHANGES project, will help us to better understand the dynamics of the ionized gas in the halo.

Analisis Pengelolaan Alokasi Dana Desa dalam Pembangunan Infrastruktur di Desa Pangkoh Sari, Kecamatan Pandih Batu Kabupaten Pulang Pisau

This study aims to determine, analyze, and describe the extent to which the management of Village Fund Allocation (ADD) in Pangkoh Sari Village is conducted properly and in accordance with the applicable regulations, while also ensuring that the villagers understand its allocation and use. The research employs a descriptive qualitative approach, with data collected through observation, interviews, and documentation in Pangkoh Sari Village. Data analysis includes procedures for data reduction, data presentation, and drawing conclusions or verification. The findings indicate that the ADD in Pangkoh Sari Village has not been fully utilized for infrastructure development, instead focusing on improving social welfare, community services, and local income. However, one of the main obstacles identified is the lack of community awareness and participation in bureaucratic socialization efforts, leading to uneven development across the village. The study emphasizes the importance of communication and collaboration between the village government and the community to ensure more transparent and targeted use of the ADD. Improving socialization and community participation could help address these obstacles.

An activity coefficient model for mixed-solvent electrolyte mixtures based on Gibbs–Duhem’s equation: A case study of mixtures of water, KCl and ethanol

Thermodynamic properties of mixtures with several fluid components and electrolytes are challenging to model. Models are needed to develop and improve a wide range of electrochemical systems such as fuel cells, lithium-ion batteries, and processes with ion-exchange membranes. In the literature, activity coefficients are extracted using fundamentally different experimental methods that rely on electrochemical cells, vapour pressure measurements, solubility measurements, etc. The reference states of the activity coefficients obtained from these methods are likely to differ. This makes it difficult to combine or compare activity coefficient models from different sources. In this work, we present a method using Gibbs–Duhem’s equation for the development of activity coefficient models of mixtures that are based on experimental data from different methods. We use the ternary mixture of KCl, H2O and ethanol as example. First, empirical expressions are developed for the logarithm of the activity coefficients of KCl and ethanol. The expression for the activity coefficient of H2O is next derived using Gibbs–Duhem’s equation. The resulting three activity coefficient models are fitted to available experimentally data from several sources, generating linear and relatively low-complexity activity coefficient models. The empirical activity coefficient models are next compared to the electrolyte cubic plus association (e-CPA) equation of state. The models give saturation pressures in ternary mixtures that have average absolute relative deviations for water/ethanol of 8.3/3.4% for the empirical model and 11.8/3.3% for e-CPA. Experimental data reduction procedures for concentration cells, formation cells, and vapour pressure measurements are discussed, and the freedom to choose the reference state and the consequences are highlighted.

SPHERE RefPlanets: Search for ε Eridani b and warm dust

Context. Cold planets, including all habitable planets, produce only scattered light emission in the visual to near-infrared wavelength range. For this reason it is highly desirable to adapt the technique for the direct imaging of reflected light from extra-solar planets. Aims. For the nearby system ε Eri, we want to set much deeper detection limits for the expected scattered radiation from the radial velocity planet candidate (≈0.7 MJ) and the warm dust using the VLT/SPHERE adaptive optics (AO) instrument with the ZIMPOL imaging polarimeter. Methods. We carried out very deep imaging polarimetry of ε Eri based on 38.5 h of integration time with a broad-band filter (λc = 735 nm) for the search of the polarization signal from a planet or from circumstellar dust using AO, coronagraphy, high precision differential polarimetry, and angular differential imaging. The data were collected during 12 nights within four epochs distributed over 14 months and we searched for a signal in the individual epochs. We also combined the full data set to achieve an even higher contrast limit considering the Keplerian motion using the K-Stacker software. All data were also combined for the search of the scattering signal from extended dust clouds. We improved various data reduction and post-processing procedures and also developed new ones to enhance the sensitivity of SPHERE/ZIMPOL further. The final detection limits were quantified and we investigated the potential of SPHERE/ZIMPOL for deeper observations. Results. The data of ε Eridani provide unprecedented contrast limits but no significant detection of a point source or an extended signal from circumstellar dust. For each observing epoch, we achieved a 5 σ𝒩 point source contrast for the polarized intensity CP = Qϕ/I★ between 2 × 10−8 and 4 × 10−8 at a separation of ρ ≈ 1″, which is as expected for the proposed radial velocity planet at a quadrature phase. The polarimetric contrast limits are close to the photon noise limits for ρ > 0.6″ or about six times to 50 times better than the intensity limits because polarimetric imaging is much more efficient for speckle suppression. Combining the data for the search of a planet moving on a Keplerian orbit with the K-Stacker technique improves the contrast limits further by about a factor of two, when compared to an epoch, to about CP = 0.8 × 10−8 at ρ = 1″. This would allow the detection of a planet with a radius of about 2.5 RJ. Should future astrometry provide strong constraints on the position of the planet, then a 3 σ𝒩 detection at 1″ with CP ≈ 5 × 10−9 would be within reach of our data. The surface brightness contrast limits achieved for the polarized intensity from an extended scattering region is about 15 mag arcsec−2 at 1″ or up to 3 mag arcsec−2 deeper than previous limits. For ε Eri, these limits exclude the presence of a narrow dust ring and they constrain the dust properties. The photon statistics would allow deeper limits but we find a very weak systematic noise pattern probably introduced by polarimetric calibration errors. Conclusions. This ε Eri study shows that the polarimetric contrast limits for reflecting planets with SPHERE/ZIMPOL can be improved to a level below Cp < 10−8 by just collecting more data during many nights using software such as K-Stacker, which can combine all data considering the expected planet orbit. Contrast limits of Cp ≈ 10−9 are within reach for ε Eri if the search can be optimized for a planet with a well-known orbit. This limit is also attainable for other bright nearby stars, such as α Cen or Sirius A. Such data also provide unprecedented sensitivity for the search of extended polarized emission from warm circumstellar dust.

Approaches and challenges in whole-nanoparticle refinements from neutron total-scattering data

This study considers critical data reduction steps and data analysis approaches required to determine explicitly the atomic arrangements in nanoparticles from time-of-flight neutron total scattering. A practical procedure is described for removing parasitic backgrounds caused by the incoherent scattering of hydrogen inevitably present in most nanoparticle samples and normalizing the recovered coherent scattering intensities onto an absolute scale. A model-free analysis is presented of a pair-distribution function derived from total scattering that can be used to determine thermal expansion coefficients and particle sizes directly from experimental data without knowledge of the material's structure. Finally, atomistic whole-nanoparticle refinements of yttrium-doped ceria nanoparticles from neutron total-scattering data are demonstrated using the reverse Monte Carlo method implemented in the RMCProfile software. These results reveal a strong dependence of the cation–oxygen and oxygen–oxygen distances on the coordination numbers, which leads to gradients of these distances near the particle surface. The details are dependent on the surface coverage by ligands and adsorbates and on the structure of grain boundaries in nanocrystalline agglomerates. The refined models confirm the expectations of more substantial disorder at particle surfaces, with a distorted surface layer extending over several coordination shells. The results highlight the feasibility of whole-nanoparticle refinements from neutron data, calling for further development of data reduction and analysis procedures.

Thermo-osmotic coefficients in membrane distillation: Experiments and theory for three types of membranes

The thermo-osmotic coefficient of a porous medium is the ratio of the mass flow rate and the temperature difference that drives the flow. Thermo-osmotic coefficients of the Millipore DuraPore HVHP, GVHP and VVHP membranes have been measured using a new apparatus designed to provide accurate mass flux measurements with tightly controlled temperatures, pressures, and compositions on the feed and distillate side. To properly analyze the experimental data, recommendations on data reduction procedures anchored in non-equilibrium thermodynamics are discussed. An expression is presented for the apparent energy of activation of the transport process in terms of the derivative of the thermo-osmotic coefficient with respect to the inverse mean temperature. The expression is shown to accurately predict the temperature dependence of the thermo-osmotic coefficients from experiments. The expression is next used to explain observations in similar porous systems from the literature. Based on this, an optimization scheme to find the optimal mean pore radius to maximize the power density of a pressure-retarded membrane distillation (PRMD) process is presented. For membranes with properties similar to the Durapore XXHP series membranes, the optimal pore radius is found to be between 1 and 10 nm. It is shown that the power density can benefit greatly from a narrow pore size distribution and from membrane surface treatments that increase the liquid-solid contact angle, potentially exceeding a benchmark minimum power density of 5 W/m2 (set for the feasibility of pressure-retarded osmosis). An assessment of the second law efficiency of the PRMD process is also presented. A critical part of the process is due to the inevitably smaller water flux through smaller pores, required to maintain a high pressure difference and a feasible power density. This can only be alleviated by increasing the temperature difference across the membrane. We conclude that membranes designed for the PRMD process need increased overall thermal resistance to enhance performance.

Asteroid spin and shape properties from Gaia DR3 photometry

The third data release of in June 2022, included the first large sample of sparse photometric data for more than 150\,000 Solar System objects (SSOs), mainly asteroids. The SSO photometric data can be processed to derive information on the physical properties for a large number of objects, including spin properties, surface photometric behaviour in a variety of illumination conditions, and overall shape. After selecting a set of 22\,815 objects for which an adequate number of accurate photometric measurements had been obtained by we applied the 'genetic' algorithm of photometric inversion developed by the Data Processing and Analysis Consortium to process SSO photometric data. Given the need to minimise the required data processing time, the algorithm was set to adopt a simple triaxial ellipsoid shape model. Our results show that in spite of the limited variety of observing circumstances and the limited numbers of measurements per object at present (in the majority of cases no greater than $40$ and still far from the number expected at the end of the mission of about $60$ - $70$), the proportion of correct determinations for the spin period among the observed targets is about $85$<!PCT!>. This percentage is based on a comparison with reliable literature data following a moderate filtering procedure developed to remove dubious solutions. The analysis performed in this paper is important in the context of developing further improvements to the adopted data reduction procedure. This includes the possible development of better solution filtering procedures that take into account, for each object, the possible presence of multiple, equivalent spin period solutions that have not been systematically investigated in this preliminary application.

Strategi Promosi Perpustakaan dalam Meningkatkan Jumlah Kunjungan Pemustaka di Perpustakaan Daerah Deli Serdang

The purpose of this research is to find out how librarian tactics encourage library use and increase interest in visits. in the Deli Serdang regional library, to find out the causes of the low interest in visiting public libraries in Deli Serdang and the challenges of librarians in encouraging public library patronage in Deli Serdang Regency. This type of research combines field study methodology with qualitative research. Librarian The research topic is the Deli Serdang Regency Public Library. There are three techniques used to obtain data: observation, interviews, and documentation. Data presentation, data reduction procedures, and data analysis methods were all carried out in accordance with descriptive analysis. Based on the research results, the author can determine librarian tactics to encourage increased interest in visiting libraries in the Deli Serdang regional library, including by conducting mobile library activities, holding reading competitions for the community. Furthermore, knowing the lack of library collections, facilities and infrastructure, as well as inadequate library services is one of the factors causing the low interest in visiting public libraries in Deli Serdang. Librarians also face challenges in efforts to increase interest in visiting the Deli Serdang Regency public library.

TELAMON: Effelsberg monitoring of AGN jets with very-high-energy astroparticle emission

Aims. We introduce the TELAMON program which is using the Effelsberg 100-m telescope to monitor the radio spectra of active galactic nuclei (AGN) under scrutiny in astroparticle physics, specifically TeV blazars and candidate neutrino-associated AGN. Here, we present and characterize our main sample of TeV-detected blazars. Methods. We analyzed the data sample from the first ∼2.5 yr of observations between August 2020 and February 2023 in the range from 14 GHz to 45 GHz. During this pilot phase, we observed all 59 TeV-detected blazars in the Northern Hemisphere (i.e., Dec > 0°) known at the time of observation. We discuss the basic data reduction and calibration procedures used for all TELAMON data and introduce a sub-band averaging method used to calculate average light curves for the sources in our sample. Results. The TeV-selected sources in our sample exhibit a median flux density of 0.12 Jy at 20 mm, 0.20 Jy at 14 mm, and 0.60 Jy at 7 mm. The spectrum for most of the sources is consistent with a flat radio spectrum and we found a median spectral index (S(ν)∝να) of α = −0.11. Our results on flux density and spectral index are consistent with previous studies of TeV-selected blazars. Compared to the GeV-selected F-GAMMA sample, TELAMON sources are significantly fainter in the radio band. This is consistent with the double-humped spectrum of blazars being shifted towards higher frequencies for TeV-emitters (in particular for high-synchrotron peaked BL Lac type objects), which results in a lower radio flux density. The spectral index distribution of our TeV-selected blazar sample is not significantly different from the GeV-selected F-GAMMA sample. Moreover, we present a strategy to track the light curve evolution of sources in our sample for future variability and correlation analysis.

Application of the 187Re-187Os geochronometer to crustal materials: Systematics, methodology, data reporting, and interpretation

Abstract The rhenium-osmium (187Re-187Os) system is a highly versatile chronometer that is regularly applied to a wide range of geological and extraterrestrial materials. In addition to providing geo- or cosmo-chronological information, the Re-Os system can also be used as a tracer of processes across a range of temporal (millennial to gigayear) and spatial scales (lower mantle to cryosphere). An increasing number of sulfide minerals are now routinely dated, which further expands the ability of this system to refine mineral exploration models as society moves toward a new, green economy with related technological needs. An expanding range of natural materials amenable to Re-Os geochronology brings additional complexities in data interpretation and the resultant translation of measured isotopic ratios to a properly contextualized age. Herein, we provide an overview of the 187Re-187Os system as applied to sedimentary rocks, sulfides, and other crustal materials and highlight further innovations on the horizon. Additionally, we outline next steps and best practices required to improve the precision of the chronometer and establish community-wide data reduction procedures, such as the decay constant, regression technique, and software packages to use. These best practices will expand the utility and viability of published results and essential metadata to ensure that such data conform to evolving standards of being findable, accessible, interoperable, and reusable (FAIR).

Application of semester credit system curriculum in high school in Indonesia: Opportunities and challenges in the industrial age 4.0

One of the innovative efforts made to improve the quality of education in Indonesia during the industrial era 4.0 is the application of the Semester Credit System. The research objective in implementing the Semester Credit Unit system is intended to stimulate creativity and train children's intelligence in the learning process so that those who can complete it quickly, precisely and efficiently. This type of research is field research. The method used in this research is qualitative research. The kind of approach used is descriptive analysis with a phenomenological approach. The subjects of this study amounted to nine people consisting of the principal, vice-principal of the curriculum field, class teachers and students. The data analysis technique uses data reduction procedures, data presentation and data interpretation based on important collected themes. The findings of this study have three points. First, the Semester Credit Unit system learning application innovations can increase children's enthusiasm for learning, thus spurring students to complete on time. Second, the existing supporting factor is the extraordinary support from the government, especially the Ministry of Religion. Third, the constraining factor in implementing the Semester Credit System at Madrasah Aliyah (MA) Negeri 3 Palembang in facing industrial revolution 4.0 is overstressed and stress that accumulates in the students of MA Negeri Palembang so that it hurts their learning achievement. This research is theoretically expected to help increase intellectual treasures, especially in studying the Islamic education curriculum at MA. Meanwhile, practically, this research is expected to help prepare strategic plans for curriculum development. There are still many limitations in this research. Subsequent analysis can be minimised with more in-depth study. Keywords: Innovation, challenges, opportunities, semester credit units.

On Cyclic-Fatigue Crack Growth in Carbon-Fibre-Reinforced Epoxy-Polymer Composites.

The growth of cracks between plies, i.e., delamination, in continuous fibre polymer matrix composites under cyclic-fatigue loading in operational aircraft structures has always been a very important factor, which has the potential to significantly decrease the service life of such structures. Whilst current designs are based on a 'no growth' design philosophy, delamination growth can nevertheless arise in operational aircraft and compromise structural integrity. To this end, the present paper outlines experimental and data reduction procedures for continuous fibre polymer matrix composites, based on a linear elastic fracture mechanics approach, which are capable of (a) determining and computing the fatigue crack growth (FCG) rate, da/dN, curve; (b) providing two different methods for determining the mandated worst-case FCG rate curve; and (c) calculating the fatigue threshold limit, below which no significant FCG occurs. Two data reduction procedures are proposed, which are based upon the Hartman-Schijve approach and a novel simple-scaling approach. These two different methodologies provide similar worst-case curves, and both provide an upper bound for all the experimental data. The calculated FCG threshold values as determined from both methodologies are also in very good agreement.

Uncovering Budget Battle Practices: A Critical Study of Budget Participation in Indonesia

Purpose: This research aims to analyze the budget battle practices between local government (executive) and Regional People's Representative Council (DPRD or legislative) within the context of plenary sessions in North Toraja Regency. Theoretical framework: The theoretical framework of this article revolves around the concept of budget participation, influenced by the political environment, and inspired by Paulo Freire's ideas. Budget participation involves the engagement of the community in decisions regarding the allocation of public funds, with a normative emphasis on community involvement values. The influence of the political environment and the political will of the government plays a pivotal role in the success of budget participation. Design/methodology/approach: This study adopts a critical paradigm and employs the Habitus Theory as a tool for interpreting research data. The research also utilizes the data collection and reduction procedures outlined by Creswell (2014). The study was conducted in North Toraja Regency and involved ten informants selected through purposive sampling technique. Findings: The research findings reveal several aspects. Firstly, the practice of budgetary battles involves three models: negotiation, holding the Regional Budget Planning (RAPBD) hostage, and intimidation. Secondly, these three behaviors undergo transformation into a homogeneous institutional or group habitus among the actors. Thirdly, this group habitus is deeply internalized by the actors, shaping individual habits that are employed both during plenary sessions and outside the political context within the social realm. Research, Practical & Social implications: The social implications of these findings indicate that the existence of budgetary battle practices involving negotiation, holding the Regional Budget Planning (RAPBD) hostage, and intimidation can impact political dynamics and financial governance at the regional level. In terms of practice, these findings can provide guidance for policymakers at the local level to implement improvements in budgeting mechanisms. Originality/value: The originality of this article lies in its contribution to the understanding of how group habitus influences individual dispositions in budgetary battles. The findings concerning the three types of habitus also offer a novel contribution to the literature. This study provides crucial insights for further research in exploring the phenomenon of budgetary battles and their impact on budget participation within the context of local governance.

Data reduction and uncertainty assessment of the direct pulse heating technique with both contact and radiance temperature measurements

This work presents a data reduction procedure of the direct pulse heating technique with both contact and radiance temperature measurements. The technique is applied for the measurement of thermophysical properties of electroconductive solids over a wide temperature range, i.e., from room temperature up to about 2300°C. Absolute and radiance temperatures of a tested material are measured by thermocouple and radiation thermometer, respectively and these and other experimental data are then reduced to the values of specific heat, specific electrical resistivity, hemispherical total emissivity and normal spectral emissivity of the tested material. The related data reduction and corresponding uncertainty assessment for each property is described in detail. An example of uncertainty assessment is given for the recent measurement of specific heat, specific electrical resistivity, hemispherical total emissivity and normal spectral emissivity at 900 nm of molybdenum alloy TZM specimens.

(Invited) Considerations in Sample Environment and Data Processing for Operando Cell Studies by Neutron Depth Profiling

Neutron depth profiling (NDP) is a nominally non-destructive analytical technique used to measure select isotopes (6Li, 14N, 10B, etc...) in a diversity of materials. NDP can be conducted on operating Li-ion cells and be used to provide researchers real-time information about cell formation, conductance, and resilience. The increased use of NDP for electrochemical studies within the past decade has inspired the development of new sample preparation and data reduction strategies. Select topics that have been studied in the U.S. have included issues of neutron attenuation and scattering due to the addition of a protective capping layer over a cell, the possible need for matrix matched standards for complex materials, and the streamlining of the NDP data reduction procedure. Several challenges remain, however, including improving NDP data acquisition and reduction methods for detectable, low-Z isotopes such as 14N and 35Cl and improving upon the NDP data reduction and processing procedures so that they are more accessible to non-instrument specialists. All these topics will be discussed in this presentation.

MORAL LEARNING STRATEGIES AT MADRASAH MU'ALLIMAAT MUHAMMADIYAH YOGYAKARTA DURING THE COVID-19 PANDEMIC

Moral material becomes an essential thing in education. During the Covid-19 pandemic, the education sector changed policy. Every teacher must determine learning strategies following existing conditions, especially moral teachers who must use the right approach to transfer knowledge and instill morals in students optimally. This research was conducted to describe the learning strategies applied by the moral teachers of Madrasah Mu'allimaat Muhammadiyah Yogyakarta and the accompanying constraints. The type of research used is qualitative research with a descriptive approach. This study used respondents consisting of seven people as informants, namely two moral teachers, the deputy director of the curriculum section, and four students of Madrasah Mu'allimaat Muhammadiyah Yogyakarta. Then, interviews and documentations were data collection techniques used by researchers—analysis of data processing using data reduction procedures, data presentation and conclusion. Based on the research results obtained, the learning strategy used by the moral teachers at Mu'allimaat Muhammadiyah Yogyakarta during the Covid-19 pandemic was expository and active learning. As for the obstacles faced, namely the limitations of space, time (class hours), resources (network and IT devices), and the need for more motivation of the students. Even though there were several obstacles, they could be handled/appropriately resolved. This research has limitations, including the difficulty of arranging interview schedules because it is hindered by semester holidays and the school is busy accepting new students. The recommendation from this study is that teachers must be more able to manage classes optimally, especially by using suitable approaches and strategies. With this research, it is hoped that it can become a reference and reference for further similar research.

JWST Census for the Mass–Metallicity Star Formation Relations at z = 4–10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators

Abstract We present the evolution of the mass–metallicity (MZ) relation at z = 4–10 derived with 135 galaxies identified in JWST/NIRSpec data taken from the three major public spectroscopy programs of ERO, GLASS, and CEERS. Because there are many discrepancies between the flux measurements reported by the early ERO studies, we first establish our NIRSpec data reduction procedure for reliable emission-line flux measurements and errors, successfully explaining Balmer decrements with no statistical tensions thorough comparisons with the early ERO studies. Applying the reduction procedure to the 135 galaxies, we obtain emission-line fluxes for physical property measurements. We confirm that 10 out of the 135 galaxies with [O iii] λ4363 lines have electron temperatures of ≃(1.1–2.3) × 104 K, similar to lower-z star-forming galaxies, which can be explained by heating by young massive stars. We derive the metallicities of the 10 galaxies by a direct method and the rest of the galaxies with strong lines using the metallicity calibrations of Nakajima et al. applicable for these low-mass metal-poor galaxies, anchoring the metallicities with the direct-method measurements. We thus obtain the MZ relation and star formation rate (SFR)–MZ relation over z = 4–10. We find that there is a small evolution of the MZ relation from z ∼ 2–3 to z = 4–10, while interestingly the SFR–MZ relation shows no evolution up to z ∼ 8 but a significant decrease at z > 8 beyond the errors This SFR–MZ relation decrease at z > 8 may suggest a break of the metallicity equilibrium state via star formation, inflow, and outflow, while further statistical and local-baseline studies are needed for a conclusion.

Data reduction for spatially resolved reflectance anisotropy spectrometer.

We show that in spatially resolved reflectance anisotropy (RA) spectrometers, off-axis optical rays introduce a spurious signal component that cannot be addressed by optical alignment. Such a component is associated with the difference between the reflectivities s and p of the sample and depends, in a complex manner, on the incidence position of the incident light on the surface of the sample. We report a data-reduction procedure to easily identify and remove spurious RA signals associated with the off-axis optical rays, based on the singular value decomposition analysis of spatially resolved RA spectra. We validated this approach by developing a spatially resolved RA spectrometer based on an 8 × 8 multi-anode photomultiplier (PMT). The PMT allowed the use of phase-sensitive detection techniques to enhance the signal-to-noise ratio, which is essential for the evaluation of the proposed data reduction procedure.