bluuebunny/crossref_metadata_2025_split huggingface dataset:
Spatial Analysis of The Influence of Education And Income on Indonesia's Democracy Index In 2015 And 2019
Authors: Abiduloh Fauzan Zahid , Hasan Chotib 
Published: June 2021

Abstract:This research discusses the spatial effects of education and income influences on the 2015 and 2019 Democracy Index of Indonesia. The income variable used is Gross Regional Domestic Product (GRDP) per capita, and the education variable used is the average year of schooling. All of the data are collected from the website of the Indonesian Central Bureau of Statistics, namely www.bps.go.id. Using spatial econometrics, researchers found that the distribution of the democratic index value in each province forms a group spatial systemic pattern. Provinces with high democracy index scores tend to be surrounded by provinces that have high democracy index scores, while provinces with low democracy index scores tend to be surrounded by provinces that have low democracy index scores. Researchers also found a spatial dependence on the influence of education and income on the index of democracy in neighboring provinces. Thus, it can be concluded that the quality of democracy in a province is not only caused by the level of education and income in the province, but also by its neighboring provinces.Keywords: indonesia’s democracy index, education, income, spatial econometrics. Abstrak:Penelitian ini membahas pengaruh spasial variabel pendidikan dan pendapatan terhadap Indeks Demokrasi Indonesia 2015 dan 2019. Variabel pendapatan yang digunakan adalah Produk Domestik Regional Bruto (PDRB) perkapita, dan variabel pendidikan yang digunakan adalah rata-rata lama sekolah. Semua data dikumpulkan dari website Badan Pusat Statistik Indonesia, yaitu www.bps.go.id. Dengan menggunakan ekonometrik spasial, peneliti menemukan bahwa sebaran nilai indeks demokrasi di setiap provinsi membentuk pola sistemik spasial berkelompok. Provinsi dengan skor indeks demokrasi yang tinggi cenderung dikelilingi oleh provinsi yang memiliki skor indeks demokrasi yang tinggi pula, sedangkan provinsi dengan skor indeks demokrasi yang rendah cenderung dikelilingi oleh provinsi yang memiliki skor indeks demokrasi rendah. Peneliti juga menemukan adanya efek spasial dalam pengaruh pendidikan dan pendapatan terhadap indeks demokrasi di provinsi tetangga. Dengan demikian, dapat disimpulkan bahwa kualitas demokrasi di suatu provinsi tidak hanya disebabkan oleh tingkat pendidikan dan pendapatan di provinsi tersebut, tetapi juga oleh provinsi tetangganya.Kata kunci: indeks demokrasi indonesia, pendidikan, pendapatan, ekonometrika spasial
Diskriminasi Terhadap WNI Keturunan Tionghoa Terkait Kepemilikan Tanah di Yogyakarta
Authors: Pamungkas Brilian Satrio , Elfianta Febrio , Zulfana Kintan Anindita , Sabila Tanti 
Published: June 2021

AbstractThis scientific journal writing aims to analyze the land policy established by the Yogyakarta Special Region government regarding land rights ownership for Indonesian citizens of Chinese descent. The enactment of the UUAP in Jogja resulted in that individuals with Indonesian citizenship status were allowed to pocket or hold ownership rights to land. However, this is very inversely proportional to reality, first implementing the Deputy Governor's Instructions which made it impossible for Indonesian citizens of Chinese descent to own land rights in Jogja. The local government only allows Indonesian citizens of Chinese descent to only be allowed as use rights, building use rights, and business use. The Yogyakarta Regional Government seems to discriminate against its citizens, especially those of Chinese descent. This situation has made many Indonesian citizens of Chinese descent cast strong protests over the ownership of land rights for their groups to the local governmentKeywords: citizenship, restriction on the acquisition of rights, land ownership in Yogyakarta AbstrakPenulisan jurnal ilmiah ini bertujuan untuk menganalisis kebijakan pertanahan yang ditetapkan oleh Pemerintah Daerah Istimewa Yogyakarta mengenai kepemilikan hak atas tanah bagi warga negara Indonesia keturunan Tionghoa. Dengan berlakunya UUAP di Jogja, warga negara Indonesia diperbolehkan mengantongi atau memiliki hak kepemilikan atas tanah. Namun hal ini sangat berbanding terbalik dengan kenyataan, pertama melaksanakan Instruksi Wakil Gubernur yang tidak memungkinkan warga negara Indonesia keturunan Tionghoa memiliki hak atas tanah di Jogja. Pemerintah daerah hanya mengizinkan warga negara Indonesia keturunan Tionghoa untuk hanya diperbolehkan sebagai hak pakai, hak guna bangunan, dan guna usaha. Pemerintah Daerah Yogyakarta terlihat melakukan diskriminasi terhadap warganya, terutama yang keturunan Tionghoa. Situasi ini membuat banyak warga Indonesia keturunan Tionghoa melayangkan protes keras atas kepemilikan hak atas tanah bagi kelompoknya kepada pemerintah daerah.Kata kunci: kewarganegaraan, pembatasan perolehan hak, kepemilikan tanah di Yogyakarta
Spatial Barriers and the Tendency of the Utilization of Mediated Citizenship by Villagers in Accessing Public Services
Authors: Hidayat Rahmad , Akhyar Akhyar , Sauki Muhammad 
Published: June 2021

AbstractThis paper aims to discuss the dynamic intersection between the spatial barriers and the tendency of the utilization of "mediated citizenship" by villagers in accessing public services. It is important to map out how villagers interact with authoritative service providers at the local government level, which is not done directly, but through the mediation of a third party, namely a local NGO that is implementing a program in their village. Based on the context of Oi Bura Village, the tendency of the utilization of mediator services of "LAKPESDAM PCNU Kabupaten Bima" in accessing public services (especially the residential identities) began to take shape because it was triggered by the poor people's consideration about the spatial stretch of their village area with the site of the service provider that would have an impact on financial expenses and bureaucratic severity factors that must be passed when accessing these basic services. Although the residential identities should be obtained automatically based on formal status as an Indonesian citizen, in practice the access of the poor villagers to basic services is achieved through a third party mediation role. The limitations of the service providers' responsiveness, accountability and institutional capacity to act proactively in solving the public problems are increasingly opening up the chance for "permanence" of facilitation of the state-citizen interaction by third parties.Keywords: access, citizenship, mediator, service, space AbstrakMakalah ini bertujuan untuk membahas persimpangan dinamis antara hambatan spasial dan kecenderungan pemanfaatan "mediated citizenhip" oleh warga desa dalam mengakses layanan publik. Penting untuk memetakan bagaimana masyarakat desa berinteraksi dengan pemberi layanan otoritatif di tingkat pemerintah daerah, yang tidak dilakukan secara langsung, melainkan melalui mediasi pihak ketiga, yaitu LSM lokal yang melaksanakan program di desanya. Berdasarkan konteks Desa Oi Bura, kecenderungan pemanfaatan jasa mediator “LAKPESDAM PCNU Kabupaten Bima” dalam mengakses pelayanan publik (khususnya identitas permukiman) mulai terbentuk karena dipicu oleh pertimbangan masyarakat miskin terhadap tata ruang. hamparan wilayah desanya dengan lokasi penyedia layanan yang tentunya berdampak pada pengeluaran keuangan dan faktor keparahan birokrasi yang harus dilalui saat mengakses layanan dasar tersebut. Meskipun identitas kependudukan seharusnya diperoleh secara otomatis berdasarkan status formal sebagai warga negara Indonesia, pada praktiknya akses masyarakat miskin terhadap layanan dasar dicapai melalui peran mediasi pihak ketiga. Keterbatasan daya tanggap, akuntabilitas, dan kapasitas kelembagaan penyedia layanan untuk bertindak proaktif dalam menyelesaikan masalah publik semakin membuka peluang untuk "kelanggengan" fasilitasi interaksi negara-warga oleh pihak ketiga.Kata kunci: akses, citizenship, mediator, layanan, ruang.
Model Light Curves for Type Ib and Ic Supernovae
Authors: Woosley S. E. , Sukhbold Tuguldur , Kasen D. N. 
Published: June 2021

Abstract
Using the Monte Carlo code SEDONA, multiband photometry and spectra are calculated for supernovae derived from stripped helium stars with presupernova masses of 2.2 to 10.0 M
⊙. The models are representative of evolution in close binaries and have previously been exploded using a parameterized one-dimensional model for neutrino transport. A subset, those with presupernova masses in the range of 2.2–5.6 M
⊙, have many properties in common with observed Type Ib and Ic supernovae, including a median ejected mass near 2 M
⊙, explosion energies near 1 × 1051 erg, typical 56Ni masses of 0.07–0.09 M
⊙, peak times of about 20 days, and a narrow range for the V − R color index 10 days post-V-maximum near 0.3 mag. The median peak bolometric luminosity, near 1042.3 erg s−1, is fainter, however, than several observational tabulations, and the brightest explosion has a bolometric luminosity of only 1042.50 erg s−1. The brightest absolute B, V, and R magnitudes at peak are −17.2, −17.8, and −18.0. These limits are fainter than some allegedly typical Type Ib and Ic supernovae and could reflect problems in our models or in the observational analysis. Helium stars with lower and higher masses also produce interesting transients that may have been observed, including fast, faint, blue transients and long, red, faint Type Ic supernovae. New models are specifically presented for SN 2007Y, SN 2007gr, SN 2009jf, LSQ 13abf, SN 2008D, and SN 2010X.
The GADOT Galaxy Survey: Dense Gas and Feedback in Herschel-selected Starburst Galaxies at Redshifts 2 to 6
Authors: Riechers Dominik A. , Cooray Asantha , Pérez-Fournon Ismael , Neri Roberto 
Published: June 2021

Abstract
We report the detection of 23 OH+ 1 → 0 absorption, emission, or P-Cygni-shaped lines and CO(J = 9→8) emission lines in 18 Herschel-selected z = 2–6 starburst galaxies with the Atacama Large Millimeter/submillimeter Array and the NOrthern Extended Millimeter Array, taken as part of the Gas And Dust Over cosmic Time Galaxy Survey. We find that the CO(J = 9→8) luminosity is higher than expected based on the far-infrared luminosity when compared to nearby star-forming galaxies. Together with the strength of the OH+ emission components, this may suggest that shock excitation of warm, dense molecular gas is more prevalent in distant massive dusty starbursts than in nearby star-forming galaxies on average, perhaps due to an impact of galactic winds on the gas. OH+ absorption is found to be ubiquitous in massive high-redshift starbursts, and is detected toward 89% of the sample. The majority of the sample shows evidence for outflows or inflows based on the velocity shifts of the OH+ absorption/emission, with a comparable occurrence rate of both at the resolution of our observations. A small subsample appears to show outflow velocities in excess of their escape velocities. Thus, starburst-driven feedback appears to be important in the evolution of massive galaxies in their most active phases. We find a correlation between the OH+ absorption optical depth and the dust temperature, which may suggest that warmer starbursts are more compact and have higher cosmic-ray energy densities, leading to more efficient OH+ ion production. This is in agreement with a picture in which these high-redshift galaxies are “scaled-up” versions of the most intense nearby starbursts.
Comprehensive Laboratory Measurements Resolving the LMM Dielectronic Recombination Satellite Lines in Ne-like Fe xvii Ions
Authors: Grilo Filipe , Shah Chintan , Kühn Steffen , Steinbrügge René , Fujii Keisuke , Marques José , Feng Gu Ming , Paulo Santos José , Crespo López-Urrutia José R. , Amaro Pedro 
Published: June 2021

Abstract
We investigated experimentally and theoretically dielectronic recombination (DR) populating doubly excited configurations

(LMM) in Fe xvii, the strongest channel for soft X-ray line formation in this ubiquitous species. We used two different electron beam ion traps and two complementary measurement schemes for preparing the Fe xvii samples and evaluating their purity, observing negligible contamination effects. This allowed us to diagnose the electron density in both EBITs. We compared our experimental resonant energies and strengths with those of previous independent work at a storage ring as well as those of configuration interaction, multiconfiguration Dirac–Fock calculations, and many-body perturbation theory. This last approach showed outstanding predictive power in the comparison with the combined independent experimental results. From these we also inferred DR rate coefficients, unveiling discrepancies from those compiled in the OPEN-ADAS and AtomDB databases.
The Nuclear Region of NGC 1365: Star Formation, Negative Feedback, and Outflow Structure
Authors: Gao Yulong , Egusa Fumi , Liu Guilin , Kohno Kotaro , Bao Min , Morokuma-Matsui Kana , Kong Xu , Chen Xiaoyang 
Published: June 2021

Abstract
High-resolution observations of ionized and molecular gas in the nuclear regions of galaxies are indispensable for delineating the interplay of star formation, gaseous inflows, stellar radiation, and feedback processes. Combining our new Atacama Large Millimeter/submillimeter Array band 3 mapping and archival Very Large Telescope/MUSE data, we present a spatially resolved analysis of molecular and ionized gas in the central 5.4 kpc region of NGC 1365. We find the star formation rate/efficiency (SFR/SFE) in the inner circumnuclear ring is about 0.4/1.1 dex higher than in the outer regions. At a linear resolution of 180 pc, we obtain a superlinear Kennicutt–Schmidt law, demonstrating a steeper slope (1.96 ± 0.14) than previous results presumably based on lower-resolution observations. Compared to the northeastern counterpart, the southwestern dust lane shows lower SFE, but denser molecular gas and larger virial parameters. This is consistent with an interpretation of negative feedback from an active galactic nucleus (AGN) and/or starburst, in the sense that the radiation/winds can heat and interact with the molecular gas even in relatively dense regions. After subtracting the circular motion component of the molecular gas and the stellar rotation, we detect two prominent noncircular motion components of molecular and ionized hydrogen gas, reaching a line-of-sight velocity of up to 100 km s−1. We conclude that the winds or shocked gas from the central AGN may expel the low-density molecular gas and diffuse ionized gas on the surface of the rotating disk.
A New Identity Card for the Bulge Globular Cluster NGC 6440 from Resolved Star Counts*
Authors: Pallanca Cristina , Lanzoni Barbara , Ferraro Francesco R. , Casagrande Luca , Saracino Sara , Purohith Bhaskar Bhat Bhavana , Leanza Silvia , Dalessandro Emanuele , Vesperini Enrico 
Published: June 2021

Abstract
We present a new identity card for the cluster NGC 6440 in the Galactic Bulge. We have used a combination of high-resolution Hubble Space Telescope images, wide-field ground-based observations performed with the ESO-FORS2, and the public survey catalog Pan-STARRS to determine the gravitational center, projected density profile, and structural parameters of this globular from resolved star counts. The new determination of the cluster center differs by ∼2″ (corresponding to 0.08 pc) from the previous estimate, which was based on the surface brightness peak. The star density profile, extending out to 700″ from the center and suitably decontaminated from the Galactic field contribution, is best fit by a King model with a significantly higher concentration (c = 1.86 ± 0.06) and smaller core radius (r

c
= 6.″4 ± 0.″3) with respect to the literature values. By taking advantage of high-quality optical and near-IR color–magnitude diagrams, we also estimated the cluster age, distance, and reddening. The luminosity of the red giant branch bump was also determined. This study indicates that the extinction coefficient in the bulge in the direction of the cluster has a value (R

V
= 2.7) that is significantly lower than that traditionally used for the Galaxy (R

V
= 3.1). The corresponding best-fit values of the age, distance, and color excess of NGC 6440 are 13 Gyr, 8.3 kpc, and E(B − V) ∼ 1.27. These new determinations also allowed us to update the values of the central (t

rc
= 2.5 107 yr) and half-mass (t

rh
= 109 yr) relaxation times, suggesting that NGC 6440 is in a dynamically evolved stage.
EXOPLINES: Molecular Absorption Cross-section Database for Brown Dwarf and Giant Exoplanet Atmospheres
Authors: Gharib-Nezhad Ehsan , Iyer Aishwarya R. , Line Michael R. , Freedman Richard S. , Marley Mark S. , Batalha Natasha E. 
Published: June 2021

Abstract
Stellar, substellar, and planetary atmosphere models are all highly sensitive to the input opacities. Generational differences between various state-of-the-art stellar/planetary models arise primarily because of incomplete and outdated atomic/molecular line lists. Here we present a database of precomputed absorption cross sections for all isotopologues of key atmospheric molecules relevant to late-type stellar, brown dwarf, and planetary atmospheres: MgH, AlH, CaH, TiH, CrH, FeH, SiO, TiO, VO, and H2O. The pressure and temperature ranges of the computed opacities are 10−6–3000 bar and 75–4000 K, and their spectral ranges are 0.25–330 μm for many cases where possible. For cases with no pressure-broadening data, we use collision theory to bridge the gap. We also probe the effect of absorption cross sections calculated from different line lists in the context of ultrahot Jupiter and M-dwarf atmospheres. Using 1D self-consistent radiative–convective thermochemical equilibrium models, we report significant variations in the theoretical spectra and thermal profiles of substellar atmospheres. With a 2000 K representative ultrahot Jupiter, we report variations of up to 320 and 80 ppm in transmission and thermal emission spectra, respectively. For a 3000 K M-dwarf, we find differences of up to 125% in the spectra. We find that the most significant differences arise as a result of the choice of TiO line lists, primarily below 1 μm. In summary, (1) we present a database of precomputed molecular absorption cross sections, and (2) we quantify biases that arise when characterizing substellar/exoplanet atmospheres as a result of differences in the line lists, therefore highlighting the importance of correct and complete opacities for eventual applications to high-precision spectroscopy and photometry.
Probing M87 Globular Clusters for Flaring Ultraluminous X-Ray Sources
Authors: Huang Jeff , Sun Yifan , Dage Kristen , Haggard Daryl 
Published: June 2021

Abstract
We present X-ray analysis of three short Chandra observations of M87. The basis of this analysis is the search for possible new ultraluminous X-ray sources (ULXs) in M87's globular clusters (GCs) and attempt to quantify possible variability within the observations. We searched Chandra ObsIDs 1808 (2000 July 30, 14 ks) Wilson & Yang, 3975 (2002 November 17, 5 ks) and 3977 (2003 February 4, 5 ks) Harris et al. and identified one previously discovered GC ULX, and two new GC ULX candidates. Analysis of the light-curves revealed no new evidence of variability in these sources for the duration of the observations.
Donner sens et cohérence à la désertion en contexte de guerre : les émotions d’ex-militaires syriens
Authors: Napolitano Valentina 
Published: June 2021

Face à la répression sanglante des manifestations contre le régime de Bachar al-Assad et à la violence du conflit qui s’est ensuivi, plusieurs milliers de militaires syriens ont fait le choix de quitter l’armée régulière entre 2011 et 2013. En questionnant le processus de cette désertion, plutôt que ses causes, cette contribution s’inscrit dans la lignée de travaux récents qui ont envisagé les trajectoires des acteurs en guerre sur un continuum allant de l’avant-guerre à l’après-guerre. Elle analyse conjointement les mutations des statuts sociaux occupés par les déserteurs au fur et à mesure de l’évolution du conflit, ainsi que les émotions et sentiments moraux mis en avant dans leurs récits. Cette approche vise tout d’abord à mettre en relief les procédés de mise en cohérence de la désertion avec les trajectoires passées et présentes des ex-militaires ; ensuite à comprendre la redéfinition des frontières entre les groupes et les « communautés émotionnelles » dans un contexte de guerre interne.
Des « démobilisés » en quête de reconnaissance : le renouveau du combat politique des ex-combattants ivoiriens
Authors: Montaz Léo , Diallo Kamina 
Published: June 2021

À plusieurs reprises entre 2004 et 2012, la Côte d’Ivoire a engagé des programmes de « Désarmement, Démobilisation et Réintégration » (DDR) de ses combattants, qui se sont officiellement achevés en 2015 avec la fermeture de l’agence chargée du suivi des dossiers. Cependant, six ans plus tard, une partie des démobilisés considèrent toujours ne pas être réintégrés à la société civile et se plaignent de vivre dans des situations de grande précarité. Sur la base d’enquêtes de terrain menées dans différentes villes de la Côte d’Ivoire, nous proposons de suivre le parcours de ces démobilisés durant les cinq années qui ont suivi la fin des programmes. À travers l’analyse de leur quête de reconnaissance, nous interrogeons le rôle des émotions politiques dans la manière dont ces hommes, qui considèrent avoir été délaissés par l’État, se sont construits une identité politique nouvelle dans la Côte d’Ivoire « post-crise ». Nous questionnons également les processus qui concourent à la marginalisation et au déclassement social d’une partie d’entre eux, remettant ainsi en cause les visions normatives et positives des programmes de DDR.
Immigrés et descendants d’immigrés chinois face à l’épidémie de Covid-19 en France : des appartenances malmenées
Authors: Attané Isabelle , Chuang Ya-Han , Santos Aurélie , Wang Su 
Published: June 2021

Les immigrés et descendants d’immigrés chinois en France ont été affectés par la pandémie de Covid-19 à plusieurs titres. Indépendamment des désagréments qu’ils ont subis au même titre que l’ensemble de la population dans ce contexte de crise, ils ont été confrontés à des comportements de stigmatisation, voire de rejet ou de racisme, qui ont provoqué chez nombre d’entre eux un sentiment de malaise. Par ailleurs, pris en étau entre un discours médiatique régulièrement antichinois et la rhétorique triomphante du gouvernement chinois concernant sa lutte contre le virus, ils ont été ébranlés dans leurs sentiments d’appartenance et leurs représentations de soi. Nous documentons les processus à l’œuvre dans la fabrique d’une stigmatisation sur des bases a priori sanitaires, et restituons les manières dont nos interlocuteurs se sont positionnés en termes d’appartenance identitaire. Nous nous appuyons pour cela sur des entretiens qualitatifs réalisés pendant le premier confinement en France, et dont le contenu est confirmé par des extraits d’articles de presse. Dans ce contexte de crise, les personnes interrogées ont témoigné de vécus personnels différents selon la nature de leur lien avec la Chine. L’enjeu est d’examiner les différentes formes de ce sentiment d’appartenance face aux catégorisations véhiculées par les interactions avec la société majoritaire et les médias.