cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Radial Age and Metal Abundance Gradients in the Stellar Content of M32
Creators: name: Schiavon, Ricardo P.
name: Caldwell, Nelson
name: Yamada, Yoshihiko
name: Vazdekis, Alexandre
name: Arimoto, Nobuo
name: Rose, James A.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2005

description: We present long-slit spectroscopy of the elliptical galaxy M32, obtained with the 8 m Subaru telescope at Mauna Kea, the 1.5 m Tillinghast telescope at the F. L. Whipple Observatory, and the 4 m Mayall telescope at the Kitt Peak National Observatory. The spectra cover the Lick index red spectral region, as well as higher order Balmer lines in the blue. Spectra have been taken with the slit offset from the nucleus to avoid scattered-light contamination from the bright nucleus of M32. An analysis of numerous absorption features, particularly involving the Hγ and Hβ Balmer lines, reveals that systematic radial trends are evident in the integrated spectrum of M32. Population synthesis models indicate a radial change in both the age and chemical composition of the light-weighted mean stellar population in M32, from the nucleus out to 33'', i.e., an approximately 1.0 effective radius, Re. Specifically, the light-weighted mean stellar population at 1Re is older by ~3 Gyr and more metal-poor by about -0.25 dex in [Fe/H] than the central value of ~4 Gyr and [Fe/H] ~ 0.0. We show that this apparent population trend cannot be attributed to a varying contribution from either hot stars or emission-line contamination. The increase in age and decrease in metal abundance with radius are sufficiently well matched to explain the flat radial color profiles previously observed in M32. In addition, the ratio of Mg to Fe abundance, [Mg/Fe], increases from about -0.25 in the nucleus to about -0.08 at 1Re. Finally, we find spuriously pronounced line-strength gradients in the Mayall data that are an artifact of scattered light from the bright nucleus. Scattered-light issues may explain the lack of consistency among previously published studies of radial line strength gradients in M32.
Figure S9 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: Heatmap of the presence or absence of Wolbachia and Rickettsia classified OTUs that appear in at least five individuals in the five Lasioglossum species used in the between-species comparisons. Species boundaries are somewhat apparent based on the presence of these bacterial taxa.
The C4 Clustering Algorithm: Clusters of Galaxies in the Sloan Digital Sky Survey
Creators: name: Evrard, August E.
name: Goto, Tomotsugu
name: Wechsler, Risa H.
name: Annis, James
name: Reichart, Daniel
name: Voges, Wolfgang
name: Bernardi, Mariangela
name: Connolly, Andrew J.
name: Kniazev, Alexie
name: Bahcall, Neta A.
name: Schneider, Donald P.
name: McKay, Timothy A.
name: Boehringer, Hans
name: Nichol, Robert C.
name: Postman, Marc
name: Miller, Christopher J.
name: Lamb, Donald
name: Sheth, Ravi K.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2005

description: We present the C4 Cluster Catalog, a new sample of 748 clusters of galaxies identified in the spectroscopic sample of the Second Data Release (DR2) of the Sloan Digital Sky Survey (SDSS). The C4 cluster-finding algorithm identifies clusters as overdensities in a seven-dimensional position and color space, thus minimizing projection effects that have plagued previous optical cluster selection. The present C4 catalog covers similar to 2600 deg(2) of sky and ranges in redshift from z = 0: 02 to 0.17. The mean cluster membership is 36 galaxies (with measured redshifts) brighter than r = 17: 7, but the catalog includes a range of systems, from groups containing 10 members to massive clusters with over 200 cluster members with measured redshifts. The catalog provides a large number of measured cluster properties including sky location, mean redshift, galaxy membership, summed r-band optical luminosity (L-r), and velocity dispersion, as well as quantitative measures of substructure and the surrounding large-scale environment. We use new, multicolor mock SDSS galaxy catalogs, empirically constructed from the Lambda CDM Hubble Volume (HV) Sky Survey output, to investigate the sensitivity of the C4 catalog to the various algorithm parameters ( detection threshold, choice of passbands, and search aperture), as well as to quantify the purity and completeness of the C4 cluster catalog. These mock catalogs indicate that the C4 catalog is similar or equal to 90% complete and 95% pure above M-200 = 1 x 10(14) h(-1) M circle dot and within 0.03 <= z <= 0.12. Using the SDSS DR2 data, we show that the C4 algorithm finds 98% of X-ray-identified clusters and 90% of Abell clusters within 0.03 <= z <= 0.12. Using the mock galaxy catalogs and the full HV dark matter simulations, we show that the L-r of a cluster is a more robust estimator of the halo mass ( M200) than the galaxy line-of-sight velocity dispersion or the richness of the cluster. However, if we exclude clusters embedded in complex large-scale environments, we find that the velocity dispersion of the remaining clusters is as good an estimator of M-200 as Lr. The final C4 catalog will contain similar or equal to 2500 clusters using the full SDSS data set and will represent one of the largest and most homogeneous samples of local clusters.
OHEJP BIOPIGEE Checklists for Salmonella and HEV
Creators: name: Burow, Elke
name: Smith, Richard
name: Tobias, Tijs
name: Meester, Marina
name: Sassu, Elena
name: Prigge, Christopher
Publisher: name: Zenodo
Year: 2022
Subjects: biosecurity
pig
salmonella
HEV
checklist

description: These are the BIOPIGEE checklists to assess biosecurity against Salmonella and HEV on pig farms from the deliverable D-JRP21-WP5.21 Benchmark system for effectiveness of biosecurity practice finished and forwarded to WP1 and WP6 (“BIOPIGEE Benchmark System”). The checklists can be downloaded individually in the respective languages or all together as a zip-file. Available languages are: Bulgarian, Czech, Dutch, English, Estonian, German, Italian, and Polish. The English version is the original upon which all other translations are based.
Chemical Composition of the Planet-harboring Star TrES-1
Creators: name: Sozzetti, Alessandro
name: Torres, Guillermo
name: Carney, Bruce W.
name: Laird, John B.
name: Latham, David W.
name: Yong, David
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: We present a detailed chemical abundance analysis of the parent star of the transiting extrasolar planet TrES-1. Based on high-resolution Keck HIRES and Hobby-Eberly Telescope HRS spectra, we have determined abundances relative to the Sun for 16 elements
Aurel Croissant, Gabriele Bruns und Marei John (eds.): Electoral Politics in Southeast & East Asia; Erfried Adam, Michael von Hauff und Marei John (eds.): Social Protection in Southeast & East Asia
Creators: name: Köllner, Patrick
Publisher: name: ASIEN: The German Journal on Contemporary Asia
Year: 2022

description: ASIEN: The German Journal on Contemporary Asia, Nr. 94 (2005): ASIEN (Januar)
Collision geometry effect on free spectator nucleons in relativistic heavy-ion collisions
Creators: name: Liu, Lu-Meng
name: Xu, Jun
name: Peng, Guang-Xiong
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Based on the deformed nucleon distributions obtained from the constrained Skyrme-Hartree-Fock-Bogolyubov calculation using different nuclear symmetry energies, we have investigated the effects of the neutron skin and the collision geometry on the yield of free spectator nucleons as well as the yield ratio $N_n/N_p$ of free spectator neutrons to protons in collisions of deformed nuclei at RHIC energies. We found that tip-tip (body-body) collisions with prolate (oblate) nuclei lead to fewest free spectator nucleons, compared to other collision configurations. While the $N_n/N_p$ ratio is sensitive to the average neutron-skin thickness of colliding nuclei and the symmetry energy, it is affected by the polar angular distribution of the neutron skin in different collision configurations. We also found that the collision geometry effect can be as large as 50% the symmetry energy effect in some collision systems. Due to the particular deformed neutron skin in $^{238}$U and $^{96}$Zr, the symmetry energy effect on the $N_n/N_p$ ratio is enhanced in tip-tip $^{238}$U+$^{238}$U collisions and body-body $^{96}$Zr+$^{96}$Zr collisions compared to other collision orientations in the same collision system. Our study may shed light on probing deformed neutron skin by selecting desired configurations in high-energy collisions with deformed nuclei.
description: 7 pages, 6 figures. arXiv admin note: text overlap with arXiv:2301.07893
Water transport through functionalized nanotubes with tunable hydrophobicity
Creators: name: Moskowitz, Ian
name: Snyder, Mark A.
name: Mittal, Jeetain
Publisher: name: arXiv
Year: 2015
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Molecular dynamics simulations are used to study the occupancy and flow of water through nanotubes comprised of hydrophobic and hydrophilic atoms, which are arranged on a honeycomb lattice to mimic functionalized carbon nanotubes (CNTs). We consider single-file motion of TIP3P water through narrow channels of (6,6) CNTs with varying fractions (f) of hydrophilic atoms. Various arrangements of hydrophilic atoms are used to create heterogeneous nanotubes with separate hydrophobic/hydrophilic domains along the tube as well as random mixtures of the two types of atoms. The water occupancy inside the nanotube channel is found to vary nonlinearly as a function of f, and a small fraction of hydrophilic atoms (f ~ 0.4) are sufficient to induce spontaneous and continuous filling of the nanotube. Interestingly, the average number of water molecules inside the channel and water flux through the nanotube are less sensitive to the specific arrangement of hydrophilic atoms than to the fraction, f. Two different regimes are observed for the water flux dependence on f - an approximately linear increase in flux as a function of f for f < 0.4, and almost no change in flux for higher f values, similar to the change in water occupancy. We are able to define an effective interaction strength between nanotube atoms and water's oxygen, based on a linear combination of interaction strengths between hydrophobic and hydrophilic nanotube atoms and water, that can quantitatively capture the observed behavior.
description: 6 pages, 4 figures
Elemental Abundance Ratios in Stars of the Outer Galactic Disk. III. Cepheids
Creators: name: Carney, Bruck W.
name: Pohi, Brian L.
name: Yong, David
name: De Almeida, Maria Luísa Teixera
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: We present metallicities, [Fe/H], and elemental abundance ratios, [X/Fe], for a sample of 24 Cepheids in the outer Galactic disk based on high-resolution echelle spectra. The sample members have galactocentric distances covering 12 kpc ≤ RGC ≤ 17.2 kp
Figure S2 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts.
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: A. Distributions of community dispersion in all social and solitary samples as well as those species represented by at least 10 individuals. The polymorphic L. albipes is split into social and solitary categories (n=19 solitary, n=6 social). Dispersions are not significantly different between social and solitary bees based on Wilcoxon rank-sum tests. The same test was used to compare all strictly social species to the strictly solitary species L. leucozonium and, again, none were significant. Data for L. albipes are included for reference; they were not included in statistical comparisons. B. Boxplots showing the number of copies of the bacterial 16S rRNA gene per nanogram of DNA.
(2151) Francis Joseph Young
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Appendix 3: A non-annotated checklist of Iranian spiders (i.e., 935 species, 324 genera, 55 families), excluding unpublished data, records of doubtful species previously rejected from the checklist of Iranian spiders, and those not identified to the species-level. The species that are known only from records in border areas are accompanied with a question mark. The order of listed families is based on their currently accepted evolutionary relationships. Within each family, species are listed alphabetically.
Creators: name: Zamani, Alireza
Publisher: name: Zenodo
Year: 2023

description: Appendix 3 of my doctoral dissertation.
Supplementary text S1 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: Detailed additional methods and results
"Asiens neue Wirtschaftsdynamik: Regionale und internationale Dimensionen" Tagung des Asien-Pazifik-Ausschusses der Deutschen Wirtschaft
Creators: name: Willmann, Katrin
Publisher: name: ASIEN: The German Journal on Contemporary Asia
Year: 2022

description: ASIEN: The German Journal on Contemporary Asia, Nr. 94 (2005): ASIEN (Januar)
Fermi surfaces and orbital polarization in superconducting CeO$_{0.5}$F$_{0.5}$BiS$_{2}$ revealed by angle-resolved photoemission spectroscopy
Creators: name: Sugimoto, T.
name: Ootsuki, D.
name: Morice, C.
name: Artacho, E.
name: Saxena, S. S.
name: Schwier, E. F.
name: Zheng, M.
name: Kojima, Y.
name: Iwasawa, H.
name: Shimada, K.
name: Arita, M.
name: Namatame, H.
name: Taniguchi, M.
name: Takahashi, M.
name: Saini, N. L.
name: Asano, T.
name: Nakajima, T.
name: Higashinaka, R.
name: Matsuda, T. D.
name: Aoki, Y.
name: Mizokawa, T.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have investigated the electronic structure of BiS$_2$-based CeO$_{0.5}$F$_{0.5}$BiS$_2$ superconductor using polarization-dependent angle-resolved photoemission spectroscopy (ARPES), and succeeded in elucidating the orbital characters on the Fermi surfaces. In the rectangular Fermi pockets around X point, the straight portion parallel to the $k_y$ direction is dominated by Bi $6p_x$ character. The orbital polarization indicates the underlying quasi-one-dimensional electronic structure of the BiS$_2$ system. Moreover, distortions on tetragonally aligned Bi could give rise to the band Jahn-Teller effect.
description: 5 pages, 4 figures
Hot Populations in M87 Globular Clusters
Creators: name: Frogel, Jay A.
name: Burstein, David
name: Sohn, Sangmo T.
name: Bohlin, Ralph C.
name: Landsman, Wayne B.
name: Rose, James A.
name: Kundu, Arunav
name: O'Connell, Robert W.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: To explore the production of UV-bright stars in old, metal-rich populations like those in elliptical galaxies, we have obtained Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph far- and near-UV photometry of globular clusters (GCs) in four fields in the giant elliptical (gE) galaxy M87. To a limit of mFUV ~ 25 we detect a total of 66 GCs in common with the deep HST optical-band study of Kundu et al. Despite strong overlap in V- and I-band properties, the M87 GCs have UV-optical properties that are distinct from clusters in the Milky Way and in M31. M87 clusters, especially metal-poor ones, produce larger hot horizontal-branch populations than do Milky Way analogs. In color plots including the near-UV band, the M87 clusters appear to represent an extension of the Milky Way sequence. Cluster mass is probably not a factor in these distinctions. The most metal-rich M87 GCs in our sample are near solar metallicity and overlap the local E galaxy sample in estimated Mg2 line indices. Nonetheless, the clusters produce much more UV light at a given Mg2, being up to 1 mag bluer than any gE galaxy in (FUV - V) color. The M87 GCs do not appear to represent a transition between Milky Way-type clusters and E galaxies. The differences are in the correct sense if the clusters are significantly older than the E galaxies. Comparisons with Galactic open clusters indicate that the hot stars lie on the extreme horizontal branch, rather than being blue stragglers, and that the extreme horizontal branch becomes well populated for ages 5 Gyr. Existing model grids for clusters do not match the observations well, due to poorly understood giant branch mass loss or perhaps high helium abundances. We find that 41 of our UV detections have no optical-band counterparts. Most appear to be UV-bright background galaxies seen through M87. Eleven near-UV variable sources detected at only one epoch in the central field are probably classical novae. Two recurrent variable sources have no obvious explanation but could be related to activity in the relativistic jet.
9. Japanisch-Deutsche Geographenkonferenz "Shaping the Future of Metropolitan Regions in Japan and Germany: Governance, Institutions and Place in New Context"
Creators: name: Feldhoff, Thomas
name: Flüchter, Winfried
name: Hohn, Uta
Publisher: name: ASIEN: The German Journal on Contemporary Asia
Year: 2022

description: ASIEN: The German Journal on Contemporary Asia, Nr. 94 (2005): ASIEN (Januar)
Redshifts and Velocity Dispersions of Galaxy Clusters in the Horologium-Reticulum Supercluster
Creators: name: Drinkwater, Michael J.
name: Hunstead, Richard W.
name: Fleenor, Matthew C.
name: Rose, James A.
name: Johnston-Hollitt, Melanie
name: Christiansen, Wayne A.
name: Saunders, William
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: We present 118 new optical redshifts for galaxies in 12 clusters in the Horologium-Reticulum supercluster (HRS) of galaxies. For 76 galaxies, the data were obtained with the Dual Beam Spectrograph on the 2.3 m telescope of the Australian National University at Siding Spring Observatory. After combining 42 previously unpublished redshifts with our new sample, we determine mean redshifts and velocity dispersions for 13 clusters in which previous observational data were sparse. In 6 of the 13 clusters, the newly determined mean redshifts differ by more than 750 km s-1 from the published values. In three clusters, A3047, A3109, and A3120, the redshift data indicate the presence of multiple components along the line of sight. The new cluster redshifts, when combined with other reliable mean redshifts for clusters in the HRS, are found to be distinctly bimodal. Furthermore, the two redshift components are consistent with the bimodal redshift distribution found for the intercluster galaxies in the HRS by Fleenor and coworkers.
„Ich könnte mit normalen Leuten leben“ – Barrieren, Ressourcen und Wünsche an der Schnittstelle von Flucht, Migration und Behinderung
Creators: name: Westphal, Manuela
name: Boga, Olezia
Publisher: name: Universität Kassel
Year: 2022
Subjects: subject: Migration
subject: Behinderung
subject: Inklusion
subject: Integration
subject: Teilhabebarrieren
subject: 300
subject: 360
subject: Migration
subject: Inklusion
subject: Behinderung
subject: Teilhabe

description: Diese Publikation wird auch als barrierearme Version online bereitgestellt. Der Text ist im Flattersatz gesetzt und weicht dadurch in Seiteninhalt und -zahl von der Originalversion leicht ab.
(2152) Anne Elizabeth Iles Young
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
VI Photometry of Globular Clusters NGC 6293 and NGC 6541: The Formation of the Metal-poor Inner Halo Globular Clusters
Creators: name: Carney, Bruce W.
name: Lee, Jae Woo
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: We present VI photometry of the metal-poor inner halo globular clusters NGC 6293 and NGC 6541 using the WFPC2 on board the Hubble Space Telescope (HST). Our color-magnitude diagrams of the clusters show well-defined blue horizontal-branch populations, consistent with their low metallicities and old ages. NGC 6293 appears to have blue straggler stars in the cluster's central region. We discuss the interstellar reddening and the distance modulus of NGC 6293 and NGC 6541 and obtain E(B - V) = 0.40 and (m - M)0 = 14.61 for NGC 6293 and E(B - V) = 0.14 and (m - M)0 = 14.19 for NGC 6541. Our results confirm that NGC 6293 and NGC 6541 are clearly located in the Galaxy's central regions (RGC ≤ 3 kpc). We also discuss the differential reddening across NGC 6293. The interstellar reddening value of NGC 6293 appears to vary by ΔE(B - V) ≈ 0.02-0.04 mag within our small field of view. The most notable result of our study is that the inner halo clusters NGC 6293 and NGC 6541 essentially have the same ages as M92, confirming the previous result from the HST NIC3 observations of NGC 6287.
Digital Archives in the Classroom: The Challenge of Appropriating the CLARIAH Media Suite Into Tool-Supported Pedagogical Practices
Creators: name: Aasman, Susan
Publisher: name: Zenodo
Year: 2023

description: Poster presented at DH Benelux 2022: RE-MIX. Creation and alteration in DH, 1-3 June 2022 at the University of Luxembourg.
AN OVERVIEW ON EMERGING OF VIRAL DISEASES IN INDIA AND FUTURE PROSPECTIVES ON THEIR TREATMENT
Creators: name: D. Nagavalli, S. Shoba, F. Nishvanth*
Publisher: name: Zenodo
Year: 2024

description: A virus is comprised of nucleic acid, either DNA or RNA, surrounded by a protein coat. It requires to multiply a living cell. A viral infection can lead to a spectrum of symptoms from asymptomatic to severe disease. A virus is a small infectious organism—much smaller than a fungus or bacterium—that must invade a living cell to reproduce (replicate). The virus attaches to a cell (called the host cell), enters the cell, and releases its DNA or RNA inside the cell. The virus’s DNA or RNA is the genetic material containing the information needed to replicate the virus. The virus’s genetic material takes control of the host cell and forces it to replicate the virus. The infected cell usually dies because the virus keeps it from performing its normal functions. When the infected host cell dies, it releases new viruses, which go on to infect other cells. People may get viruses by swallowing or inhaling them, by being bitten by insects, through sexual contact, or congenitally (passed by a pregnant person to the fetus). Most commonly, viral infections involve the nose, throat, and upper airways, or systems such as the nervous, gastrointestinal, and reproductive systems. Doctors may base the diagnose on symptoms, blood tests and cultures were examined. Antiviral drugs may interfere and affect the reproduction of viruses or strengthen the host cell immune response to the viral infection.

Key words: Virus, Avian Influenza virus, Nipah Virus, Sars- Cov 19 (Covid-19), Zika Virus, Monkey Pox Virus and Chandipura Virus
Hubble Space Telescope Ultraviolet Spectroscopy of 14 Low-Redshift Quasars
Creators: name: Junkkarinen, Vesa T.
name: Michael Crenshaw, D.
name: Proga, Daniel
name: Aldcroft, Thomas L.
name: Canalizo, Gabriela
name: Heap, Sara R.
name: Ogle, Patrick
name: Kazanas, Demosthenes
name: Konigl, Arieh
name: Leighly, Karen M.
name: Galliano, Emmanuel
name: Brotherton, Michael S.
name: Alloin, Danielle
name: Kriss, Gerard A.
name: Korista, Kirk T.
name: Gabel, Jack
name: Cecil, Gerald
name: Hines, Dean C.
name: Kaastra, Jelle S.
name: Sivron, Ran
name: Snedden, Stephanie
name: Kaiser, Mary Elizabeth
name: Arav, Nahum
name: Evererr, John
name: Vestergaard, Marianne
name: Chambers, Kenneth
name: Behar, Ehud
name: Martin Gaskell, C.
name: De Kool, Martijn
name: Mathur, Smita
name: Wisotzki, Lutz
name: Sabra, Bassem
name: Telfer, Randal
name: Chatzichristou, Eleni
name: Ganguly, Rajib
name: Laor, Ari
name: Green, Richard F.
name: Hall, Patrick B.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2007

description: 133
Figure S4 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts.
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: Phylogeny of recovered Sodalis sequences. Bolded taxa represent genomes assembled de novo in this study. C. calcarata, L. vierecki, L. marginatum, L. malachurum, and H. ligatus all represent Sodalis sequences recovered from shotgun sequencing libraries derived from those bee taxa. So. glossinidius and So. pierantonius are previously assembled symbionts of tsetse flies and weevils, respectively. So. praecaptivus is the previously assembled free-living form of Sodalis. All other tips are derived from L. albipes shotgun sequencing libraries and are labeled with their location of origin and mitochondrial haplotype in parentheses. Each number represents a unique haplotype. We were not able to recover haplotypes for all samples.
Quantum correlations in Ising-XYZ diamond chain structure under an external magnetic field
Creators: name: Faizi, E.
name: Eftekhari, H.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this paper, we consider an entangled Ising-XYZ diamond chain structure. Quantum correlations for this model is investigated by using of quantum discord and trace distance discord. Quantum correlations is obtained for different values of the anisotropy parameter, magnetic field and temperature. By comparison between quantum correlations, we show trace distance discord is always larger than quantum discord. Finally, some novel effects, such as increasing the quantum correlations with temperature and constructive role of anisotropy parameter which may paly to the quantum correlations were observed.
Thrift and Credit Groups and Community Development: the Hope Project in New Delhi/India
Creators: name: Schrader, Heiko
Publisher: name: Asien
Year: 2022

description: Recent approaches to micro-finance hold that poor people are able to save. Access to capital by means of saving or credit opens up opportunities to participate in the street economy and helps bridging problems of everyday-life. Without savings people usually depend upon expensive credit from moneylenders. Various NGOs nowadays take the approach "savings first, then credit". In this paper the authors argue that such programs do not only provide an end by itself; they are also meansto achieve broader goals. The Hope Project in New Delhi puts such program into the context of community development. In first step Muslim women's thrift and credit groups are formed to increase mutual trust in the neighbourhood. In second step these women may join handicraft cooperative and escape domestic marginalization by productive activity. The paper describes the process of institutionalizing women's thrift and credit groups.
description: Asien, Nr. 94 (2005): ASIEN (Januar)
(2153) Herbert Hammerton Young
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Figure S3 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts.
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: Heatmap of the presence or absence of Sodalis classified OTUs that appear in at least 5 samples in all Lasioglossum used in the comparison of social and solitary samples.
Resolution of cosmological singularity in Hořava-Lifshitz cosmology
Creators: name: Czuchry, Ewa
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The standard $Λ$CDM model despite its agreement with observational data still has some issues unaddressed, lie the problem of initial singularity. Solving that problem usually requires modifications of general relativity. However, there appeared the Hořava-Lifshitz (HL) theory of gravity, in which equations governing cosmological evolution include a new term scaling similarly as dark radiation term in the Friedmann equations, enabling a bounce of the universe instead of initial singularity. This review describes past works on a stability of such a bounce in different formulations of HL theory, initial detailed balance scenario and further projectable versions containing higher than quadratic term to the original action.
description: Submitted to Universe. Rewritten in order to remove repetitions from the previous papers
Frieden in Sri Lanka
Creators: name: Weiberg, Mirjam
Publisher: name: ASIEN: The German Journal on Contemporary Asia
Year: 2022

description: Since 1983 Sri Lanka is torn apart by bloody civil war between rebels of the Tamil minority population and the Government formed by the majority Sinhalese. During the last decades various attempts at negotiating settlement between the two sides were made, which not only failed abysmally but led to further escalation of the conflict. By comparing these peace talks undertaken till now, the reasons for their failure can be pointed out and the prospects for success of the latest peace initiative assessed. Although the negotiations since 2001 have been welcomed by both the parties to the conflict, still their objectives diverged markedly. Another complicating factor in the peace process is the internal tension between the President and the Prime Minister.
description: ASIEN: The German Journal on Contemporary Asia, Nr. 94 (2005): ASIEN (Januar)
Der Weg in die Hungersnot: Erinnerungen chinesischer Intellektueller an den ländlichen "Großen Sprung nach vorne" (1958-1961)
Creators: name: Wemheuer, Felix
Publisher: name: ASIEN: The German Journal on Contemporary Asia
Year: 2022

description: In the autumn of 1958 the Chinese government declared that communism is "nothing of the far future". With the organization of the peasants in people's communes, mass movements, and the militarization of the rural workforce, it was believed that China could overtake Great Britain and the USA within few years. After four months the strategy seemed to be total defeat. The dream of direct transformation to communism produced the most serious economic catastrophe in the history of New China. In China and in the West the most research about the process to the famine focuses on the government or Mao Zedong. The Chinese Party History never researched the village or the normal people. To focus on the village and the masses the author held Oral History-Interviews with retired intellectuals in Beijing in summer 2002 who had been sent to villages in 1958 to support the Great Leap Forward. With the beginning of the famine in the winter of 1958 this intellectuals lost their believes in direct transformation to communism. The political pressure from above and below thwarted the cadres, intellectuals, and the peasants from standing up against the destructive policies.
description: ASIEN: The German Journal on Contemporary Asia, Nr. 94 (2005): ASIEN (Januar)
Hδ in the Integrated Light of Galaxies: What Are We Actually Measuring?
Creators: name: Prochaska, L. C.
name: Caldwell, Nelson
name: Morrison, Heather
name: Rose, James A.
name: Harding, Paul
name: Concannon, Kristi
name: Schiavon, Ricardo P.
name: Castilho, Bruno V.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2007

description: We present a cautionary study exploring the reliability of the Hδ line in the integrated spectra of galaxies for determining galaxy ages. Our database consists of the observed integrated spectra of ~120 early-type galaxies, 7 metal-rich globular clusters in M31 and the Galactic globular cluster 47 Tuc, and the open cluster M67. We have measured Hδ using index definitions designed to assess contamination from the CN molecule in and around Hδ by choosing combinations of bandpasses that both avoid and include a region of CN molecular lines redward of Hδ. We find systematic differences in the ages derived from Hδ measurements among the various definitions when extracting ages from Hδ in old stellar populations with enhanced CN bands due to nonsolar abundance ratios. We propose that neighboring CN lines have a strong effect on pseudocontinuum and central bandpass levels. For stellar populations that have nonsolar abundance ratios in C and/or N, population synthesis models that do not account for abundance ratio variations cannot accurately reproduce the CN 4216 Å band, which leads to a corresponding inaccuracy in reproducing the various Hδ indices. Hence, caution must be used when extracting galaxy ages from the Hδ line in old stellar populations with significant nonsolar abundance ratios.
Figure S6 from Social behaviour in bees influences the abundance of Sodalis (Enterobacteriaceae) symbionts.
Creators: name: Rubin, Benjamin E. R.
name: Sanders, Jon G.
name: Turner, Kyle M.
name: Pierce, Naomi E.
name: Kocher, Sarah D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60408 Genomics

description: Rarefaction curves for all halictids samples examined in this study.
The Effect of Cluster Environment on Galaxy Evolution in the Pegasus I Cluster
Creators: name: Levy, Lorenza
name: Rose, James A.
name: Chaboyer, Brian
name: Van Gorkom, Jacqueline H.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2007

description: We present neutral hydrogen observations of 54 galaxies in the Pegasus Cluster. The observations include single-dish H I measurements, obtained with the Arecibo telescope for all 54 galaxies in the sample, as well as H I images obtained with the Very Large Array (VLA) for 10 of these. The Arecibo profiles reveal an overall H I deficiency in the cluster, with ~40% of the galaxies in the core of the cluster showing modest deficiencies of typically a factor of 2-3. The H I morphology of some galaxies shows that the H I disk is smaller than the optical disk and slightly offset from the stars. We find a correlation between H I deficiency and the ratio of the H I disk size to optical disk size. More H I-deficient galaxies have relatively smaller H I disks, a configuration that is usually attributed to an interaction between the interstellar medium (ISM) of the galaxy and the hot intracluster medium (ICM). Such a result is surprising, since the Pegasus Cluster has a low level of X-ray emission and a low velocity dispersion. The low velocity dispersion, coupled with the lack of a dense hot ICM, indicate that ram pressure stripping should not play a significant role in this environment. In addition, two of the galaxies, NGC 7604 and NGC 7648, are morphologically peculiar. Their peculiarities indicate contradictory scenarios of what is triggering their unusual star formation. Hα imaging, along with long-slit spectroscopy of NGC 7648, reveal morphological features that point to a recent tidal interaction. On the other hand, Hα imaging of NGC 7604 reveals a strong episode of star formation concentrated into an asymmetric arc, preferentially located on one side of the galaxy. VLA H I mapping shows that H I is also highly concentrated into that region, suggestive of a ram pressure event. Our data indicate that ISM-ICM interactions may play a role in a wider variety of environments than suggested by simple ram pressure arguments.
LINE BROADENING IN FIELD METAL-POOR RED GIANT AND RED HORIZONTAL BRANCH STARS
Creators: name: Stefanik, Robert P.
name: Carney, Bruce W.
name: Laird, John B.
name: Latham, David W.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2008

description: We report 349 radial velocities for 45 metal-poor field red giant and red horizontal branch stars. We have have identified one new spectroscopic binary, HD 4306, and one possible such system, HD 184711. We also report 57 radial velocities for 11 of the 91 stars reported on previously by Carney et al. (2003). As was found in the previous study, radial velocity "jitter" is present in many of the most luminous stars. Excluding stars showing spectroscopic binary orbital motion, all 7 of the red giants with M(V) <= -2.0 display jitter, as well as 3 of the 14 stars with -2.0 <= M(V) <= -1.4. We have also measured line broadening in all of the new spectra, using synthetic spectra as templates. The most luminous red giants show significant line broadening, as do many of the red horizontal branch stars, and we discuss briefly possible causes.
ROTATION AND MACROTURBULENCE IN METAL-POOR FIELD RED GIANT AND RED HORIZONTAL BRANCH STARS
Creators: name: Gray, David F.
name: Zelman, Rachel
name: Manset, Nadine
name: Latham, David W.
name: Carney, Bruce W.
name: Yong, David
name: Laird, John B.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2008

description: We report the results for rotational velocities, Vrot sin i, and macroturbulence dispersions, ζRT, for 12 metal-poor field red giant branch (RGB) stars and 7 metal-poor field red horizontal branch (RHB) stars. The results are based on Fourier transform a
New XMM-Newton observation of the Phoenix cluster: properties of the cool core
Creators: name: Tozzi, P.
name: Gastaldello, F.
name: Molendi, S.
name: Ettori, S.
name: Santos, J. S.
name: De Grandi, S.
name: Balestra, I.
name: Rosati, P.
name: Altieri, B.
name: Cresci, G.
name: Menanteau, F.
name: Valtchanov, I.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: (Abridged) We present a spectral analysis of a deep (220 ks) XMM-Newton observation of the Phoenix cluster (SPT-CL J2344-4243), which we also combine with Chandra archival ACIS-I data. We extract CCD and RGS X-ray spectra from the core region to search for the signature of cold gas, and constrain the mass deposition rate in the cooling flow which is thought to be responsible of the massive star formation episode observed in the BCG. We find an average mass deposition rate of $\dot M = 620 (-190 +200)_{stat} (-50 +150)_{syst} M_\odot$/yr in the temperature range 0.3-3.0 keV from MOS data. A temperature-resolved analysis shows that a significant amount of gas is deposited only above 1.8 keV, while upper limits of the order of hundreds of $M_\odot$/yr can be put in the 0.3-1.8 keV temperature range. From pn data we obtain $\dot M = 210 (-80 +85)_{stat} ( -35 +60)_{syst} M_\odot$/yr, and the upper limits from the temperature-resolved analysis are typically a factor of 3 lower than MOS data. In the RGS spectrum, no line emission from ionization states below Fe XXIII is seen above $12 Å$, and the amount of gas cooling below $\sim 3$ keV has a best-fit value $\dot M = 122_{-122}^{+343}$ $M_{\odot}$/yr. In addition, our analysis of the FIR SED of the BCG based on Herschel data provides $SFR = (530 \pm 50) M_\odot$/yr, significantly lower than previous estimates by a factor 1.5. Current data are able to firmly identify substantial amount of cooling gas only above 1.8 keV in the core of the Phoenix cluster. While MOS data analysis is consistent with values as high as $\dot M \sim 1000$ within $1 σ$, pn data provide $\dot M < 500 M_\odot$ yr$^{-1}$ at $3σ$ c.l. at temperature below 1.8 keV. At present, this discrepancy cannot be explained on the basis of known calibration uncertainties or other sources of statistical noise.
description: A&A in press, typos corrected, revised text according to published version
(2149) Mary Loft
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Dynamics of cloud features on Uranus
Creators: name: Sromovsky, Lawrence
name: Fry, Patrick
Publisher: name: arXiv
Year: 2015
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Near-infrared adaptive optics imaging of Uranus by the Keck 2 telescope during 2003 and 2004 has revealed numerous discrete cloud features, 70 of which were used to extend the zonal wind profile of Uranus up to 60°N. We confirmed the presence of a north-south asymmetry in the circulation (Karkoschka, Science 111, 570-572, 1998), and improved its characterization. We found no clear indication of long term change in wind speed between 1986 and 2004, although results of Hammel et al. (2001, Icarus 153, 229-235) based on 2001 HST and Keck observations average ~10 m/s less westward than earlier and later results, and 2003 observations by Hammel et al. (2005, Icarus 175, 534-545) show increased wind speeds near 45°N, which we don't see in our 2003-2004 observations. We observed a wide range of lifetimes for discrete cloud features: some features evolve within ~1 hour, many have persisted at least one month, and one feature near 34°S (termed S34) seems to have persisted for nearly two decades, a conclusion derived with the help of Voyager 2 and HST observations. S34 oscillates in latitude between 32°S and 36.5°S, with a period of $\sim$1000 days, which may be a result of a non-barotropic Rossby wave. It also varied its longitudinal drift rate between -20°/day and -31°/day in approximate accord with the latitudinal gradient in the zonal wind profile, exhibiting behavior similar to that of the DS2 feature observed on Neptune (Sromovsky et al., Icarus 105, 110-141, 1993). S34 also exhibits a superimposed rapid oscillation with an amplitude of 0.57°in latitude and period of 0.7 days, which is approximately consistent with an inertial oscillation.
description: 25 pages, 18 figures, 11 tables
Barjols, place de la Rouguière, les gardians galopent devant la foule
Creators: name: Musée National Des Arts Et Traditions Populaires (Paris)
name: Centre D'ethnologie Française
Publisher: name: École des Hautes Études en Sciences Sociales; Institut  interdisciplinaire d'anthropologie du contemporain (Paris); Laboratoire d'anthropologie et d'histoire de l'institution de la culture (Paris)
Year: 2024

Abstract
DETECTION OF PHOTOMETRIC VARIATIONS IN THE sdBV Star JL 166
Creators: name: Dunlap, B. H.
name: Lynas-Gray, A. E.
name: Clemens, J. C.
name: Barlow, B. N.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2009

description: We report the discovery of oscillations in the hot subdwarf B (sdB) star JL 166 from time-series photometry using the Goodman Spectrograph on the 4.1 m Southern Astrophysical Research Telescope. Previous spectroscopic and photometric observations place the star near the hot end of the empirical sdB instability strip and imply the presence of a cool companion. Amplitude spectra of the stellar light curve reveal at least 10 independent pulsation modes with periods ranging from 97 to 178 s and amplitudes from 0.9 to 4 mma. We adopt atmospheric parameters of T eff = 34,350 K and log g = 5.75 from a model atmosphere analysis of our time-averaged, medium-resolution spectrum.