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Journal articles on the topic 'Acceptances. [from old catalog]'

Author: Grafiati

Published: 4 June 2021

Last updated: 28 July 2025

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1

Ksenzhik, G., and E. Karin. "Cartographic materials on the history of Kazakhstan of the XVII–early XX centuries: consolidated catalog." Bulletin of the Karaganda university History.Philosophy series 105, no. 1 (2022): 100–110. http://dx.doi.org/10.31489/2022hph1/100-110.

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The article is devoted to the analysis, cataloging of cartographic material of the consolidated catalog of “old” maps on the history of Kazakhstan in the XVII–early XX centuries. The funds for storage of cartographic materials in archives and libraries of Moscow and Orenburg are characterized. The functional values of the developed consolidated catalog of “old” maps have been substantiated. The consolidated catalog of cartographic materials can be considered as a kind of “guide” for potential users, with the help of which the user can get answers to the following questions: What archives, libr

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Urban, S. E., and G. L. Wycoff. "Densifying the Optical Reference Frame: The Tycho-2 Catalog of 2.5 Million Stars." International Astronomical Union Colloquium 180 (March 2000): 75–79. http://dx.doi.org/10.1017/s0252921100000130.

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AbstractSince the establishment of the Hipparcos Catalog as the defining source of the optical reference frame, densification beyond its ≈ 120,000 stars has been made possible by the utilization of the Tycho-1 Catalog. The ACT, combining the old Astrographic Catalog (AC) data with the Tycho-1 positions, is the best known example of this. The Tycho-2 consortium, led by E. Høg, has performed new reductions on the Tycho data. This not only has increased the astrometric and photometric accuracies of the original 1 million Tycho-1 stars, but also has added an additional 1.5 million stars. The U.S.

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Massaro, F., S. V. White, A. García-Pérez, et al. "Powerful Radio Sources in the Southern Sky. I. Optical Identifications." Astrophysical Journal Supplement Series 265, no. 2 (2023): 32. http://dx.doi.org/10.3847/1538-4365/acaf05.

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Abstract Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridge Catalog and its revised version (3CR). However, the largest fraction of data collected to date on 3CR sources was performed with relatively old instruments, rarely repeated and/or updated. Importantly, the 3CR contains only objects located in the Northern Hemisphere, thus having limited access to new and innovative astronomical facilities. To mitigate these limitations, we present a new catalog of powerful

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Chujo, Michio, and Michitaka Chujo. "A CATALOG OF THE EROTYLIDAE (INSECTA, COLEOPTERA) FROM THE OLD WORLD (EXCL. THE ETHIOPIAN REGION)." ESAKIA 26 (January 25, 1988): 139–85. http://dx.doi.org/10.5109/2510.

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Chujo, Michio, and Michitaka Chujo. "A CATALOG OF THE EROTYLIDAE (INSECTA, COLEOPTERA) FROM THE OLD WORLD (EXCL. THE ETHIOPIAN REGION)." ESAKIA 28 (March 3, 1989): 75–96. http://dx.doi.org/10.5109/2516.

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6

Malkin, Zinovy. "Improving Source Positions in the OCARS Catalog: A First Approach." Astronomical Journal 170, no. 1 (2025): 48. https://doi.org/10.3847/1538-3881/addc65.

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Abstract Optical Characteristics of Astrometric Radio Sources (OCARS) is a compiled catalog of various additional data associated with astrometric radio sources whose coordinates have been determined from very long baseline interferometry observations. It contains source coordinates, object type, redshift, optical, and near-infrared magnitudes. Until now, OCARS source coordinates were simply copied from input catalogs and, as a result, were systematically inhomogeneous. This work is the first attempt to obtain a unified set of radio source coordinates aligned to the International Celestial Ref

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Ivezić, Ž., D. G. Monet, N. Bond, et al. "Astrometry with digital sky surveys: from SDSS to LSST." Proceedings of the International Astronomical Union 3, S248 (2007): 537–43. http://dx.doi.org/10.1017/s1743921308020103.

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AbstractMajor advances in our understanding of the Universe have historically come from dramatic improvements in our ability to accurately measure astronomical quantities. The astrometric observations obtained by modern digital sky surveys are enabling unprecedentedly massive and robust studies of the kinematics of the Milky Way. For example, the astrometric data from the Sloan Digital Sky Survey (SDSS), together with half a century old astrometry from the Palomar Observatory Sky Survey (POSS), have enabled the construction of a catalog that includes absolute proper motions as accurate as 3 ma

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Chujo, Michio, and Michitaka Chujo. "A CATALOG OF THE EROTYLIDAE (INSECTA, COLEOPTERA) FROM THE OLD WORLD (EXCL. THE ETHIOPIAN REGION) III." ESAKIA 29 (September 30, 1990): 1–67. http://dx.doi.org/10.5109/2546.

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Yuan, Ye, Fan Li, Yanning Fu, and Shulin Ren. "New precise positions in 2013–2019 and a catalog of ground-based astrometric observations of 11 Neptunian satellites (1847–2019) based on Gaia-DR2." Astronomy & Astrophysics 645 (January 2021): A48. http://dx.doi.org/10.1051/0004-6361/202038776.

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Context. Developing high-precision ephemerides for Neptunian satellites requires not only the continuation of observing campaigns but also the collection and improvement of existing observations. So far, no complete catalogs of observations of Neptunian satellites are available. Aims. We aim to provide new, precise positions, and to compile a catalog including all available ground-based astrometric observations of Neptunian satellites. The observations are tabulated in a single and consistent format and given in the same timescale, the Terrestrial Time (TT), and reference system, the Internati

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Yuan, Ye, Fan Li, Yanning Fu, and Shulin Ren. "New precise positions in 2013–2019 and a catalog of ground-based astrometric observations of 11 Neptunian satellites (1847–2019) based on Gaia-DR2." Astronomy & Astrophysics 645 (January 2021): A48. http://dx.doi.org/10.1051/0004-6361/202038776.

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Context. Developing high-precision ephemerides for Neptunian satellites requires not only the continuation of observing campaigns but also the collection and improvement of existing observations. So far, no complete catalogs of observations of Neptunian satellites are available. Aims. We aim to provide new, precise positions, and to compile a catalog including all available ground-based astrometric observations of Neptunian satellites. The observations are tabulated in a single and consistent format and given in the same timescale, the Terrestrial Time (TT), and reference system, the Internati

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Girelli, Giacomo, Micol Bolzonella, and Andrea Cimatti. "Massive and old quiescent galaxies at high redshift." Astronomy & Astrophysics 632 (December 2019): A80. http://dx.doi.org/10.1051/0004-6361/201834547.

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Aims. Questions of how massive quiescent galaxies rapidly assembled and how abundant they are at high redshift are increasingly important in the study of galaxy formation. Looking at these systems can shed light on the processes of galaxy mass assembly and quenching of the star formation at early epochs. In order to address these questions, we aim to identify and characterize massive quiescent galaxies from z ∼ 2.5 out to the highest redshifts at which these systems can be found. The final purpose is to compare the results with the predictions of state-of-the-art semi-analytical models of gala

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Buser, Roland, and Jianxiang Rong. "Metallicity Structures of the Milky Way." Symposium - International Astronomical Union 169 (1996): 427–28. http://dx.doi.org/10.1017/s0074180900230040.

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The metallicity-sensitive (U – G) colors from the new homogeneous catalog of photographic RGU data in seven high-latitude fields have been used to determine the larger-scale metallicity distributions of the Galactic population components. For the thick disk, preliminary analysis based on our best structural models provides a mean metallicity 〈[M/H]〉 = −0.6 ± 0.3dex and a marginal vertical metallicity gradient ≈ −0.1dex/kpc. The observed color distributions are further consistent with the (old) thin disk having mean abundance 〈[M/H]〉 = −0.3 ± 0.2dex and abundance gradient ∂[M/H]/∂z = −0.6dex/kp

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Yendro, J. A., and D. Widyaningrum. "The development of vegetarian meatballs with oyster mushroom and tempeh flour using conjoint analysis and organoleptic test." IOP Conference Series: Earth and Environmental Science 1169, no. 1 (2023): 012085. http://dx.doi.org/10.1088/1755-1315/1169/1/012085.

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Abstract People are starting to implement a healthy lifestyle with a vegetarian consumption pattern. The study aimed to determine the importance level between attributes and the utility values of each level to design plant-based meatballs. Furthermore, we compared the sensory acceptances of prototypes product and commercial plant-based meatballs. The study consisted of three stages, which were a preliminary survey (n=51), a conjoint survey (n=163), and an organoleptic test (n=40). The surveys were conducted through online questionnaires. The characteristics of respondents were between the age

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Lewis, B. M. "Miras Without Masers are Symbiotic Stars." International Astronomical Union Colloquium 135 (1992): 241–43. http://dx.doi.org/10.1017/s0252921100006485.

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AbstractAbout 40% of potential OH / IR stars, color selected from the IRAS Point Source Catalog, have no 1612 MHz masers. While these objects are rarely carbon rich, they are usually associated with circumstellar shells. The natural explanation for these “OH / IR star color mimics” is that they are systems with a degenerate companion collecting an accretion disk from a red giant wind. This provides them with an extra source of UV for dissociating their molecules. The persistent absence of the usual complement of masers from an O-rich shell is then a pointer to the presence of a degenerate comp

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Marquis, Kathy. "Peter Devereaux and Carla Diane Hayden. The Card Catalog: Books, Cards, and Literary Treasures." RBM: A Journal of Rare Books, Manuscripts, and Cultural Heritage 19, no. 1 (2018): 71. http://dx.doi.org/10.5860/rbm.19.1.71.

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In an early archives job, I typed the name and subject entries at the top of card sets we received from the Library of Congress. It was exacting work and I really enjoyed it, including the filing. At a venerable manuscript repository, the cards ranged from the printed ones I placed on top of the rods (to be double-checked before they slipped into their forever homes) and those written in a spidery handwriting that could easily have been 100 years old. It made me feel part of a long tradition of information mavens.

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Law, Casey J., Kritti Sharma, Vikram Ravi, et al. "Deep Synoptic Array Science: First FRB and Host Galaxy Catalog." Astrophysical Journal 967, no. 1 (2024): 29. http://dx.doi.org/10.3847/1538-4357/ad3736.

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Abstract Fast radio bursts (FRBs) are a powerful and mysterious new class of transients that are luminous enough to be detected at cosmological distances. By associating FRBs to host galaxies, we can measure intrinsic and environmental properties that test FRB origin models, in addition to using them as precise probes of distant cosmic gas. The Deep Synoptic Array (DSA-110) is a radio interferometer built to maximize the rate at which it can simultaneously detect and localize FRBs. Here, we present the first sample of FRBs and host galaxies discovered by the DSA-110. This sample of 11 FRBs is

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Lin, Zehao, Ye Xu, Ligang Hou, et al. "Local Spiral Structure Traced by Red Clump Stars." Astrophysical Journal 931, no. 1 (2022): 72. http://dx.doi.org/10.3847/1538-4357/ac67a6.

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Abstract Using the cross-matched data of Gaia EDR3 and the Two Micron All Sky Survey Point Source Catalog, a sample of RC stars with parallax accuracies better than 20% is identified and used to reveal the nearby spiral pattern traced by old stars. As shown in the overdensity distribution of RC stars, there is an arc-like feature extending from l ∼ 90° to ∼243°, which passes close to the Sun. This feature is probably an arm segment traced by old stars, indicating the galaxy potential in the vicinity of the Sun. With a comparison to the spiral arms depicted by young objects, we found that there

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Kumkova, Irina I., Vadim V. Bobylev, and Nina M. Bronnikova. "Densification of ICRS in the Optical by use of Old Pulkovo Observation Sets." International Astronomical Union Colloquium 180 (March 2000): 61–67. http://dx.doi.org/10.1017/s0252921100000117.

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AbstractModern tasks of high precision astrometry demand optical coordinate systems including more faint stars than are available now in current conventional systems (Hipparcos). For this purpose it is suggested to use old photographic observations accumulated in the Pulkovo Observatory. Extensive observational data have been obtained at Pulkovo Observatory during the last century in the framework of several programs, e.g. Pulkovo Galaxy plan, etc. Observations have been made with the Normal Astrograph from 1894 to the present. The data are investigated with the aim of extending the Hipparcos

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TIAN, JIAHUI, and LIHONG TU. "A new species of the spider genus Solenysa from China (Araneae, Linyphiidae)." Zootaxa 4531, no. 1 (2018): 142. http://dx.doi.org/10.11646/zootaxa.4531.1.10.

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The genus Solenysa Simon, 1894 belongs to Linyphiidae Blackwall, 1859, which is a species-rich group, including 608 genera and 4,571 species (World Spider Catalog 2018). Solenysa currently includes 14 species from China, Japan and the Korean Peninsula (Simon 1894; Namkung 1986; Li & Song 1992; Gao, Zhu & Sha 1993; Tu, Ono & Li 2007; Ono 2011; Tu & Hormiga 2011; Wang, Ono & Tu 2015). The linyphiid phylogeny based on molecular data shows that Solenysa species forms one of the seven main clades within Linyphiidae (Wang et al. 2015). According to the phylogenetic analysis based

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Gupta, Om, Paz Beniamini, Pawan Kumar, and Steven L. Finkelstein. "The Cosmic Evolution of Fast Radio Bursts Inferred from the CHIME/FRB Baseband Catalog 1." Astrophysical Journal 986, no. 1 (2025): 100. https://doi.org/10.3847/1538-4357/add14c.

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Abstract Redshift and luminosity distributions are essential for understanding the cosmic evolution of extragalactic objects and phenomena, such as galaxies, gamma-ray bursts, and fast radio bursts (FRBs). For FRBs, these distributions are primarily estimated using the fluence and the dispersion measure (DM). Calibrating their joint distribution has been challenging due to a lack of accurate fluences in the intensity data of the CHIME/FRB survey. Using the baseband update of CHIME/FRB Catalog 1, we calibrate the 2D fluence–DM distribution for the first time. We find the energy distribution is

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Cisterna-Concha, Andrea, Camila Calderón-Quirgas, Fernanda Silva-Andrades, Richard Muñoz, and Heraldo V. Norambuena. "Reencounter with the past: occurrence of sei whale (Balaenoptera borealis) in an old hunting area in the south-eastern Pacific Ocean." Nature Conservation 51 (January 26, 2023): 1–12. http://dx.doi.org/10.3897/natureconservation.51.95690.

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The sei whale (Balaenoptera borealis) was intensively exploited throughout its range, with about 110.000 individuals hunted by pelagic fleets in Antarctic waters between 1960 and 1970. In addition, basic information on its distribution, migratory routes, and feeding grounds in the southeastern Pacific, has been poorly documented. In the case of Chile, recent information consists mainly of accidental records. This research presents the first sei whale photo-identification catalog for south-central Chile. From November 2019 to January 2020, 88 individuals were recorded from land-based and boat s

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Cisterna-Concha, Andrea, Camila Calderón-Quirgas, Fernanda Silva-Andrades, Richard Muñoz, and Heraldo V. Norambuena. "Reencounter with the past: occurrence of sei whale (Balaenoptera borealis) in an old hunting area in the south-eastern Pacific Ocean." Nature Conservation 51 (January 26, 2023): 1–12. https://doi.org/10.3897/natureconservation.51.95690.

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The sei whale (Balaenoptera borealis) was intensively exploited throughout its range, with about 110.000 individuals hunted by pelagic fleets in Antarctic waters between 1960 and 1970. In addition, basic information on its distribution, migratory routes, and feeding grounds in the southeastern Pacific, has been poorly documented. In the case of Chile, recent information consists mainly of accidental records. This research presents the first sei whale photo-identification catalog for south-central Chile. From November 2019 to January 2020, 88 individuals were recorded from land-based and boat s

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Kwak, Han Sub, Misook Kim, and Yoonhwa Jeong. "Different or similar? Acceptability of aseptic-packaged cooked rice among consumers, researchers and experts." British Food Journal 117, no. 5 (2015): 1564–80. http://dx.doi.org/10.1108/bfj-09-2014-0330.

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Purpose – The purpose of this paper is to compare the acceptance ratings and drivers of liking and disliking attributes of aseptic-packaged cooked rice by consumers, researchers and experts. Design/methodology/approach – Descriptive analysis (DA) was conducted using trained panelists. Acceptability was measured by consumers, researchers and experts. The results of DA and acceptability were analyzed using partial least square regression. Findings – There was no strong relationship among the three groups in their rating patterns for the samples (r=−0.342-0.445). The liking factors for each group

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Khomutov, Sergey Y., and Manjula Lingala. "Some problems with old magnetic data processing." E3S Web of Conferences 196 (2020): 02029. http://dx.doi.org/10.1051/e3sconf/202019602029.

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Continues magnetic measurements at the IKIR FEB RAS obser-vatories Magadan (MGD), Paratunka (PET), Yuzhno-Sakhalinsk (YSS), Cape Schmidt (CPS) and Khabarovsk (KHB) and CSIR-NGRI observatories Hyder-abad (HYB) and Choutuppal (CPL) have been started almost since their formation. A significant part of the results obtained is presented in the WDC and INTERMAGNET databases. However, a large amount of raw data remains un-processed and unavailable for using by scientific community. In the past few years, institutes has been making efforts to process and reprocess old magnetic data. Digital images of

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Zhong, Jing, Li Chen, Di Wu, Lu Li, Leya Bai, and Jinliang Hou. "Exploring open cluster properties with Gaia and LAMOST." Astronomy & Astrophysics 640 (August 2020): A127. http://dx.doi.org/10.1051/0004-6361/201937131.

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Context. In Gaia DR2, an unprecedented high level of precision has been reached at sub-milliarcsecond for astrometry and millimagnitudes for photometry. Using cluster members identified with the astrometry and photometry in Gaia DR2, we can obtain a reliable determination of cluster properties. However, because of the shortcomings of Gaia spectroscopic observations in dealing with densely crowded cluster regions, the RVs and metallicity values for cluster member stars from Gaia DR2 are still lacking. It is necessary to combine the Gaia data with the data from large spectroscopic surveys, such

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Westerhout, Gart. "Archiving of Data in Positional Astronomy." Highlights of Astronomy 9 (1992): 711–12. http://dx.doi.org/10.1017/s1539299600010121.

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Astrometry is the oldest of the astronomical endeavors. Indeed, we still have the observing journals of Galileo, the journals of Flamsteed, and those of most of the other old transit-circle astronomers. We have most of the early photographic plates taken for the astrographic catalog project, and almost all the parallax plates. However, as technology progressed, we have become somewhat less precise in recording what we did. It is for this reason that this joint meeting was called: to impress on the modern astronomer that, in general, he only extracts a fraction of the information from his obser

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Bo, M. Del, M. G. Lattanzi, G. Massone, et al. "The TOCAMM Project." International Astronomical Union Colloquium 178 (2000): 317–20. http://dx.doi.org/10.1017/s0252921100061431.

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AbstractThe TOCAMM (TOrino CAgliari Measuring Machine) project undertaken jointly between Torino and Cagliari Astronomical Observatories aimed to convert the old measuring machine ASCORECORD into an automatic and impersonal one. This program is intended to contribute to the link of the HIPPARCOS Catalogue to the ICRS through the determination of precise position of optical counterparts of 80 extragalactic radiosources taken from the IERS list and to investigate the astrometric accuracy of the Guide Star Catalog (version 1 and 2). The calibration test phase, carried out first at the Astronomica

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Mo, Jian-feng, Weishan Zhu, and Long-Long Feng. "The Dispersion Measure and Scattering of Fast Radio Bursts: Contributions from Multicomponents, and Clues for the Intrinsic Properties." Astrophysical Journal Supplement Series 277, no. 2 (2025): 43. https://doi.org/10.3847/1538-4365/adb616.

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Abstract Fast radio bursts (FRBs) are luminous, millisecond-duration transients that offer great potential for probing the Universe, yet their physical origins remain unclear. The dispersion measure (DM) and scattering time (τ) distributions provide key insights into FRBs’ properties, including source population, redshift, and energy distribution. We use a simplified model of FRB source population and intrinsic Schechter function–like energy distribution, coupled with a thorough assessment of various contributors to dispersion and scattering, to replicate the joint distribution of DM and τ in

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Verdu-Candela, Alvaro, Carmen Femenia-Ribera, Gaspar Mora-Navarro, and Rafael Sierra-Requena. "Implementation of Web Map Services for Old Cadastral Maps." ISPRS International Journal of Geo-Information 12, no. 10 (2023): 413. http://dx.doi.org/10.3390/ijgi12100413.

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It is widely accepted that old cadastral maps have multiple uses, such as reestablishing cadastral parcel boundaries, municipality boundaries, and coastal limits, or conducting historical, economic, and social studies. In Spain, the Directorate General for Cadastre, and the National Geographic Institute, has numerous digitized old maps that are accessible to users. In the Comunidad Valenciana, the georeferencing of certain series of old cadastral maps is being carried out in phases, which is one of the subjects of this study. A metric analysis of two series of old cadastral maps from a municip

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Lépine, Sébastien. "Where the Wild Young M Dwarfs Are: the SUPERBLINK Proper Motion Survey and a Search for Low-mass Moving Group Candidates." Proceedings of the International Astronomical Union 10, S314 (2015): 69–70. http://dx.doi.org/10.1017/s1743921315006365.

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AbstractThe SUPERBLINK survey catalogs all stars brighter than R = 19 mag and with proper motions larger than 40 mas yr−1, down to a declination of −33○. The catalog inevitably includes a significant fraction of the presumed low-mass members of several nearby young moving groups (Beta Pic, AB Dor, Tuc-Hor, Argus), or low-mass escapees from the Hyades and Pleiades clusters. We discuss opportunities and challenges in identifying the missing M dwarf members of these moving groups. While rounding up the majority of the potential M dwarf members of these groups, such samples are significantly affec

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Barmby, P., and M. Rafiei Ravandi. "Stellar populations in the outskirts of M31: the mid-infrared view." Proceedings of the International Astronomical Union 11, S321 (2016): 19–21. http://dx.doi.org/10.1017/s1743921316011054.

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AbstractThe mid-infrared provides a unique view of galaxy stellar populations, sensitive to both the integrated light of old, low-mass stars and to individual dusty mass-losing stars. We present results from an extended Spitzer/IRAC survey of M31 with total lengths of 6.6 and 4.4 degrees along the major and minor axes, respectively. The integrated surface brightness profile proves to be surprisingly difficult to trace in the outskirts of the galaxy, but we can also investigate the disk/halo transition via a star count profile, with careful correction for foreground and background contamination

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Dias, W. S., and H. Monteiro. "DISCOVERY OF 28 OPEN CLUSTERS WITH GAIA DR3." Revista Mexicana de Astronomía y Astrofísica 61, no. 1 (2025): 3–13. https://doi.org/10.22201/ia.01851101p.2025.61.01.01.

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In this work we searched for open clusters in the fields of star-forming regions in the Galaxy using the HDBSCAN applied to the astrometric data from the Gaia DR3 catalog. We identified 28 new open clusters, of which the real existence is supported by the membership probability determined from astrometric data and by the presence of cluster sequences in their color-magnitude diagrams, which allows for a reliable isochrone fit. Of the open clusters identified, 3 are younger than 50 Myr, 19 are of intermediate age, and 6 are old clusters. The clusters have apparent radii ranging from 3 to 20 arc

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Ugleva, Natalia V. "Attribution of old russian furniture in museums in the first quarter of the twentieth-first century." Vestnik Tomskogo gosudarstvennogo universiteta. Kul'turologiya i iskusstvovedenie, no. 54 (2024): 239–52. https://doi.org/10.17223/22220836/54/21.

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Attribution of Old Russian furniture in museums begins in the first third of the twentieth century, and its active development continues in the next century. In 2000, a catalog for the exhibition “One Hundred and Twelve Chairs” was published. For the first time, it includes images of several ancient artifacts and their brief annotations. The next edition on the topic of interest to us was published in St. Petersburg in 2003. Its Old Russian section includes a selective bibliography and two articles in which information about furniture production from antiquity to the XVII centuries is presente

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van Reijmersdal, Eva A., Esther Rozendaal, and Moniek Buijzen. "Boys’ responses to the integration of advertising and entertaining content." Young Consumers 16, no. 3 (2015): 251–63. http://dx.doi.org/10.1108/yc-10-2014-00487.

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Purpose – The purposes of this paper are to investigate the effects of integrated advertising formats on the persuasion of children, children’s awareness of the persuasive intent of these formats and how this awareness mediates the level of persuasion. Design/methodology/approach – An one-factor between-subjects experiment was conducted among 117 boys from 8 to 12 years old. Findings – This study showed that boys were more aware of the persuasive intent of a non-integrated catalog than of a brand-integrated magazine. In addition, higher awareness of the persuasive intent of the catalog enhance

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Davis, Marc, and Adi Nusser. "Re-examination of Large Scale Structure & Cosmic Flows." Proceedings of the International Astronomical Union 11, S308 (2014): 310–17. http://dx.doi.org/10.1017/s1743921316010061.

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AbstractComparison of galaxy flows with those predicted from the local galaxy distribution ended as an active field after two analyses came to vastly different conclusions 25 years ago, but that was due to faulty data. All the old results are therefore suspect. With new data collected in the last several years, the problem deserves another look. The goal is to explain the 640 km/s dipole anisotropy of the CMBR. For this we analyze the gravity field inferred from the enormous data set derived from the 2MASS collection of galaxies (Huchra et al. 2005), and compare it to the velocity field derive

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Hasan, Selim Kıroğlu. "Colors in Arabic Lexicology." Eskiyeni 41 (September 20, 2020): 757–74. https://doi.org/10.37697/eskiyeni.764352.

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Colors are one of the most important phenomena allowing the man to recognize the world and communicate with the beings around it. Color is one of the main arguments shaping our world, allowing us to relate to the environment in which we exist, and mediate in perceiving the environment. It is necessary to review the Arabian history, poetry and literature, not only to understand the Arabian perception or Arabian values, but also the old poems of the society in which the Qur’an was revealed. In addition to colors, images and connotations used in ancient Arabic poetry, it is also worth knowi

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Calienes, Raúl Fernández. "Bibliography of the Writings of Orlando E. Costas." Missiology: An International Review 17, no. 1 (1989): 87–105. http://dx.doi.org/10.1177/009182968901700111.

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During his life, the Rev. Dr. Orlando E. Costas made significant contributions to the literature of missiology and theology. Though he was only 45 years old at the time of his death, he personally authored over 100 books and articles, and made over thirty contributions (e.g., chapters, articles, prologues) to the books of other people from around the world. His own interests were varied, but centered mostly on mission, evangelism, and Latin America. This bibliography is an attempt to collect and record his writings, all in one place. It is offered as a tribute to his life and ministry. Whereve

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Fuchs, B., C. Dettbarn, and R. Wielen. "The Scatter of Metallicities of Stars in the Solar Neighbourhood." Symposium - International Astronomical Union 169 (1996): 431–32. http://dx.doi.org/10.1017/s0074180900230064.

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It is well known that the velocity dispersions of the stars in the solar neighbourhood increase with their ages (Wielen 1977). In Fig.1 we show |W| weighted velocity dispersions (cf. Wielen 1977) of the stars in the Third Catalog of Nearby Stars (Gliese and Jahreiß 1994). Open symbols indicate main sequence stars and crosses indicate McCormick stars, a kinematically unbiased subset of the CNS3, respectively, whereas the filled symbols are the Edvardsson et al. (1993) data. Stars older than 14 Gyr are not shown because they are probably thick disk stars (Freeman 1991). We have assumed a maximum

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Usenko, I. A., A. S. Miroshnichenko, S. Danford, D. G. Turner, D. J. Majaess, and D. D. Balam. "SPECTROSCOPIC INVESTIGATIONS OF POLARIS FIELD STARS." Odessa Astronomical Publications 36 (December 4, 2023): 88–95. http://dx.doi.org/10.18524/1810-4215.2023.36.290534.

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We present the results of an analysis of 28 spectra of 18 Polaris field A–G V stars obtained in 2016–2023. Derived radial velocities and Teff along with distances and reddenings from the Gaia DR3 catalog allowed us to calculate radii of the stars and compare them with calibration relationships “Spectral type – Luminosity” for MS stars. As a result, radii and distances for 9 stars were found overestimated compared to those determined photometrically. Therefore, the DR3 distances are unreliable and should be revisited. According to our data for these stars and their photometric distances, 15 obj

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Leal Rodrigues, Sofia. "“Vision in motion”: László Moholy-Nagy and the Genesis of the Visual Book." Disegno, no. 1-2 (2021): 86–109. http://dx.doi.org/10.21096/disegno_2021_1-2slr.

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This essay aims to analyze the ways in which László Moholy-Nagy’s concepts of “new typography” and “typophoto” were essential to the creation of a new typology of publications: visual books, which have a strong image component, resulting from the popularization of photography and cinema. New typography was defined in 1923 by László Moholy-Nagy in a short text for the catalog of the Bauhaus exhibition Staatliches Bauhaus in Weimar 1919–1923. New typography resulted from a new graphical orientation by Bauhaus, influenced by the ideology of several avant-garde movements, such as De Stijl and Russ

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Biswas, Pralay, and Yogesh Wadadekar. "Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGA." Astrophysical Journal 970, no. 1 (2024): 83. http://dx.doi.org/10.3847/1538-4357/ad4ee3.

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Abstract Using “spatially” resolved spectroscopy, we investigated the characteristics and different modes of formation of stars in elliptical galaxies. We identified an unusual population of 59 star-forming elliptical (SF-E) galaxies in SDSS-MaNGA, our primary sample. To identify these rare star-forming ellipticals, we combined GSWLC-A2 containing outputs of stellar population synthesis models with morphological results from the deep-learning catalog and resolved and integrated properties from the MaNGA Pipe3D value-added catalog. We have also constructed two control samples of star-forming sp

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ALfakar, Suha Abdullah Oudah, Khalil Ismail Abid Mohammed, Ameen Abdul Hasan Al-Alwany, and Jinan Mousa. "Detection of IL-27 in Patients with Visceral leishmaniasis." University of Thi-Qar Journal of Science 12, no. 1 (2025): 151–56. https://doi.org/10.32792/utq/utjsci/v12i1.1356.

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Visceral leishmaniasis (VL), caused by the protozoan parasites of the Leishmania donovani complex, remains one of the most significant neglected tropical diseases. Immune response mechanisms play a critical role in both resistance and pathogenesis of VL This study included 32 VL patients (19 females, 13 males, 2 months to 5 years old) and 30 healthy controls (1 month to 11 years old). Blood samples were obtained from the Central Public Health Laboratories (CPHL). The serum was isolated by centrifuging blood samples at 1000g for 5 minutes. Human IL-27 levels were quantified using an ELISA kit (

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Pascal, A. D. "Cyrillic writing system: from Slavic to Romanian." Proceedings of SPSTL SB RAS, no. 3 (September 17, 2020): 5–10. http://dx.doi.org/10.20913/2618-7515-2020-3-5-10.

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The article is devoted to Cyrillic handwritten books of the XIII–XIX centuries, created in the Romanian principalities, and stored today in the manuscript collections of the Russian State Library. The uniqueness of the writing system, functioning in the principalities (Wallachia, Moldavia, Transylvania) since their political formation, is that it was a Cyrillic script based on the old Slavic language with a predominant Roman-speaking population. In course of the writing system’ development in the principalities, there was a transition from the Slavic font to the Latin one; the intermediate res

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Mogheisi, Meisam, Hamidreza Tavakoli, and Elnaz Peyghaleh. "Probability Assessment of the Seismic Risk of Highway Bridges with Various Structural Systems (Case Study: Tehran City)." Sustainability 15, no. 12 (2023): 9783. http://dx.doi.org/10.3390/su15129783.

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Considering the development of urban transportation systems and the importance of highway bridges in a city’s resilience against earthquakes, it is critical to pay special attention to the seismic risk evaluation of highway bridges. The most significant issue to consider is the assessment of possible direct and indirect damages imposed on bridges before an earthquake. After this, the best practices for bridge rehabilitation can be adopted to minimize the induced damage. In this paper, we assessed the seismic risks associated with all 713 highway bridges in Tehran province (the capital of Iran)

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Benkortem, Saruta, Nahathai Tanakul, and Chutipong Suwannajak. "RR Lyrae analysis in the Local Group globular clusters and dwarf galaxies." Proceedings of the International Astronomical Union 14, S351 (2019): 56–59. http://dx.doi.org/10.1017/s1743921319007336.

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AbstractRR Lyrae variables are powerful tools to study their host stellar populations. Globular clusters and dwarf galaxies are old and usually host this type of variables. With a growing number of low luminosity objects discovered in the halo of the Milky Way, classifying stars clusters and galaxies has become more challenging. In this study, we examine the properties of RR Lyrae stars in globular clusters and dwarf galaxies in the Local Group. We construct a catalog of RR Lyrae variables in the Local Group globular clusters and dwarf galaxies from previously published data and compare the pr

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van Altena, William F., Vladimir I. Korchagin, Terrence M. Girard, Dana I. Dinescu, and Tatiana V. Borkova. "Galactic Disk Surface Density in the Solar Neighbourhood." Symposium - International Astronomical Union 220 (2004): 201–6. http://dx.doi.org/10.1017/s0074180900183214.

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Using parallaxes and proper motions of a kinematically and spatially unbiased sample of old bright red giant stars from the Hipparcos catalog with measured radial velocities from Barbier-Brossat & Figon (2000), we have re-estimated the surface density of the Galactic disk in the solar neighbourhood within ±0.4 kpc of the Sun. We determine the vertical distribution of the red giants as well as the vertical velocity dispersion of the sample, (14.4±0.26 km/sec), and combine these to derive the surface density of gravitating matter in the Galactic disk. Using these data, we determine the surfa

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Varga, Attila, Joel H. Kastner, D. Annie Dickson-Vandervelde, and Alex Binks. "Walking the Line: Young Stars on the Boundary of the Epsilon Cha and Lower Centaurus Crux Associations." Astronomical Journal 168, no. 6 (2024): 251. http://dx.doi.org/10.3847/1538-3881/ad7deb.

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Abstract Gaia Data Release 3 (DR3) has provided the largest and most astrometrically precise catalog of nearby stars to date, allowing for a more complete membership census of nearby, young stellar moving groups. These loose associations of young (age <100 Myr) stars within ∼100 pc are vital laboratories for the study of the early evolution of low-mass stars and planetary systems. We have exploited DR3 data to examine the boundary region between two of the youngest nearby moving groups, the ∼3–8 Myr-old ϵ Cha Association (ECA) and an ∼8 Myr-old subpopulation of the sprawling Lower Centaurus

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LEVKO, Oleksandr. "Formation of the Ukrainian religious and ethical lexicon in the 16th and 17th centuries (based on the Epistle to Galatians)." Linguistic and Conceptual Views of the World, no. 74 (2) (2023): 72–89. http://dx.doi.org/10.17721/2520-6397.2023.2.05.

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The article explores the origins of the Ukrainian language ethical lexicon in biblical written monuments of the early modern period. It traces the rendition of the vices and virtues catalog in the Epistle to the Galatians (Gal. 5:19–23) in the Krekhiv Apostle, a manuscript of the 2nd half of the 16th century, in comparison with the Church Slavonic Ostroh Bible of 1581, as well as lexicographical works of the 17th century, in particular Pamva Berynda’s “Lexicon”, and Ukrainian translations of the Bible of the 19th and 20th centuries. The Epistle to the Galatians contains one of the most extensi

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Emanov, Alexander G. "The Tatar World’s peoples catalog by Iohannes of Sulthanyeh in the early 15th century." Golden Horde Review 13, no. 1 (2025): 346–66. https://doi.org/10.22378/2313-6197.2025-13-2.346-366.

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The purpose of this article is to study the Tatar World’s Peoples Catalog in the Manuscript Versions of “Libellus de notitia orbis” by Iohannes of Sulthanyeh in the early 15th century.Research materials: The “Libellus de notitia orbis” by Iohannes of Sulthanyeh in 1404, preserved in manuscripts of the Austrian National Library in Vienna (ÖNB Cod. Ser. n. 39086), the University Library of Basel (BUB EIII17; BUB AV25), the University Library of Graz (GUB Ms. 1221), the Monastery Library of Klostenburg (KSB Cod. 1099), the University Library of Leipzig (LUB Ms. 1225), and the Diocesan Library of

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Tantalo, Maria, Massimo Dall’Ora, Giuseppe Bono, et al. "On the Dwarf Irregular Galaxy NGC 6822. I. Young, Intermediate, and Old Stellar Populations." Astrophysical Journal 933, no. 2 (2022): 197. http://dx.doi.org/10.3847/1538-4357/ac7468.

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Abstract We present accurate and deep multiband (g, r, i) photometry of the Local Group dwarf irregular galaxy NGC 6822. The images were collected with wide-field cameras at 2 m/4 m (INT, CTIO, CFHT) and 8 m class telescopes (Subaru) covering a 2 deg2 field of view across the center of the galaxy. We performed point-spread function photometry of ≈7000 CCD images, and the final catalog includes more than 1 million objects. We developed a new approach to identify candidate field and galaxy stars and performed a new estimate of the galaxy center by using old stellar tracers, finding that it diffe

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