cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Time Resolved Spectroscopic Observations Of An M-Dwarf Flare Star Ev Lac During A Flare.
Creators: name: Honda, Satoshi
name: Notsu, Yuta
name: Notsu, Shota
name: Maehara, Hiroyuki
name: Namekata, Kosuke
name: Nogami, Daisaku
name: Shibata, Kazunari
Publisher: name: Zenodo
Year: 2016
Subjects: stellar flare
M-dwarf

description: Flares are explosions on the surface of the Sun and stars. We can find stellar flares frequently on M-dwarf stars. EV Lac, one of the M-dwarf flare stars, is a good target for investigation of stellar flares. We have carried out continuous spectroscopic observations of the Halpha line with medium wavelength resolution (R~10,000) by using 2m Nayuta telescope at Nishi-Harima Astronomical Observatory in Japan from August to December, 2015. EV Lac always has Halpha emission line and it was stronger on 15 August than on the other nights. In this night, we observed a rapid enhancement (~20min) and following slow decrease (~1.5h) of the emission-line intensity of Halpha, which was probably caused by a flare. We also found an asymmetrical change in the blue region of the Halpha line. In many cases, red asymmetry has been observed in the Halpha line profile during solar flares, but blue asymmetry has been sometimes observed during stellar flares.
description: Poster #176
description: {"references": ["Maehara, H., et al. 2012, Nature, 485, 478", "Sciortino, S,. et al. 1999, A&A, 342, 502", "Favata, F,. et al.  2000, A&A, 353, 987", "Osten, R., et al.  2008, Atel, No.1499", "Schmidt, S. J., et al.  2012, ApJ, 745, 14", "Ichimoto, K. & Kurokawa, H. 1984, SoPh, 93, 105", "Crespo-Chacon, I., et al. 2006, A&A, 452, 987", "Baranovskii, E. A., et al. 2001, ARep, 45, 309"]}
A hot Uranus transiting the nearby M dwarf GJ3470. Detected with HARPS velocimetry. Captured in transit with TRAPPIST photometry
Creators: name: Bonfils, X.
name: Gillon, M.
name: Udry, S.
name: Armstrong, D.
name: Bouchy, F.
name: Delfosse, X.
name: Forveille, T.
name: Jehin, E.
name: Lendl, M.
name: Lovis, C.
name: Mayor, M.
name: McCormac, J.
name: Neves, V.
name: Pepe, F.
name: Perrier, C.
name: Pollaco, D.
name: Queloz, D.
name: Santos, N. C.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report on the discovery of GJ3470b, a transiting hot Uranus of mass m_p = 14.0+-1.8 Mearth, radius R_p = 4.2+-0.6 Rearth and period P=3.3371+-0.0002 day. Its host star is a nearby (d=25.2+-2.9pc) M1.5 dwarf of mass M_s=0.54+-0.07 Msol and radius R_s=0.50+-0.06 Rsol. The detection originates from a radial-velocity campaign with HARPS that focused on the search for short-period planets orbiting M dwarfs. Once the planet was discovered and the transit-search window narrowed to about 10% of an orbital period, a photometric search started with TRAPPIST and quickly detected the ingress of the planet. Additional observations with TRAPPIST, EulerCam and NITES definitely confirmed the transiting nature of GJ3470b and allow for the determination of its true mass and radius. The star's visible or infrared brightness (V=12.3, K=8.0 mag), together with a large eclipse depth D=0.57+-0.05%, ranks GJ3470b among the most favorable planets for follow-up characterizations.
description: submitted to A&A on 18/05/2012 (revised version)
Prediction of equilibrium Li isotope fractionation between minerals and aqueous solutions at high P and T: an efficient ab initio approach
Creators: name: Kowalski, Piotr M.
name: Jahn, Sandro
Publisher: name: arXiv
Year: 2011
Subjects: subject: Geophysics (physics.geo-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Other Condensed Matter (cond-mat.other)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: The mass-dependent equilibrium stable isotope fractionation between different materials is an important geochemical process. Here we present an efficient method to compute the isotope fractionation between complex minerals and fluids at high pressure, P, and temperature, T, representative for the Earth's crust and mantle. The method is tested by computation of the equilibrium fractionation of lithium isotopes between aqueous fluids and various Li bearing minerals such as staurolite, spodumene and mica. We are able to correctly predict the direction of the isotope fractionation as observed in the experiments. On the quantitative level the computed fractionation factors agree within 1.0 permil with the experimental values indicating predictive power of ab initio methods. We show that with ab initio methods we are able to investigate the underlying mechanisms driving the equilibrium isotope fractionation process, such as coordination of the fractionating elements, their bond strengths to the neighboring atoms, compression of fluids and thermal expansion of solids. This gives valuable insight into the processes governing the isotope fractionation mechanisms on the atomic scale. The method is applicable to any state and does not require different treatment of crystals and fluids.
description: 14 pages, 10 figures, accepted for publication in Geochimica et Cosmochimica Acta
Dynamical modeling and the interactions with the ISM
Creators: name: Steffen, Wolfgang
Publisher: name: arXiv
Year: 2011
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: This paper is a review of some of the recent modeling efforts to improve our understanding of structure formation and evolution of planetary nebulae including their interaction with the interstellar medium. New propositions have been made for the formation mechanism of multi-polar PNe and PPNe. These mechanisms are based on the central engine with interacting binary stars or hole producing instabilities in expanding shock waves leading to illumination effects from the central star that change the appearance of the nebula. Furthermore, there has been a lot of progress in the observation and 3D modeling of the kinematics, which is key to the understanding of the dynamics. Extensive observational catalogs are coming online for the kinematics, as well as some very detailed proper motion measurements have been made. New techniques for morpho--kinematic 3D modeling help to make the interpretation of kinematic data more reliable and detailed. In addition to individual pointed observations, new surveys have lead to the discovery of many PNe that show clear signs of interaction with the interstellar medium. Systematic hydrodynamic models of the interaction have produced a general scheme for the observed structure that results from the interaction of an evolving planetary nebula with the ISM. Detailed modeling of the dust-gas dynamics during the interaction with the ISM have produced interesting predictions for future IR observations. Detailed models were worked out for the structure of the bowshock and tail of Mira that was recently discovered in the UV.
description: 8 pages, 6 figures, invited review article to be published in the proceedings of the IAU Symposium 283 "Planetary Nebulae: An Eye on the Future", eds. Manchado, Stanghellini, and Schoenberner
On the Role of Charmed Meson Loops in Charmonium Decays
Creators: name: Mehen, Thomas
name: Yang, Di-Lun
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the effect of intermediate charmed meson loops on the M1 radiative decays $J/ψ\to η_c γ$ and $ψ'\rightarrowη^{(\prime)}_cγ$ as well as the isospin violating hadronic decays $ψ'\rightarrow J/ψ\,π^0(η)$ using heavy hadron chiral perturbation theory (HH$χ$PT). The calculations include tree level as well as one loop diagrams and are compared to the latest data from CLEO and BES-III. Our fit constrains the couplings of 1S and 2S charmonium multiplets to charmed mesons, denoted $g_2$ and $g_2^\prime$, respectively. We find that there are two sets of solutions for $g_2$ and $g_2^\prime$. One set, which agrees with previous values of the product $g_2 g_2^\prime$ extracted from analyses that consider only loop contributions to $ψ'\rightarrow J/ψ\,π^0(η)$, can only fit data on radiative decays with fine-tuned cancellations between tree level diagrams and loops in that process. The other solution for $g_2$ and $g_2^\prime$ leads to couplings that are smaller by a factor of 2.3. In this case tree level and loop contributions are of comparable size and the numerical values of the tree level contributions to radiative decays are consistent with estimates based on the quark model as well as non-relativistic QCD (NRQCD). This result shows that tree level HH$χ$PT couplings are as important as the one loop graphs with charmed mesons in these charmonium decays. The couplings $g_2$ and $g_2^\prime$ are also important for the calculations of the decays of charmed meson bound states, such as the X(3872), to conventional charmonia.
description: 16 pages, 3 figures, minor modifications, more references added
Transgender and Gender Diverse (TGD) students’ experiences in Australian schools, including Alternative, Distance and/or Online education
Creators: name: Fletcher, Jessica
Publisher: name: Macquarie University
Year: 2023
Subjects: Other education not elsewhere classified

description: Whilst research into TGD students’ experiences of institutionalised marginalisation in Australian schools has increased significantly in the last decade, little is known about the experiences of this cohort in Alternative, Distance and/or Online Learning in or beyond pandemic times. To address the current gaps in research, the present study explores the experiences of TGD students who have accessed or are currently accessing Alternative, Distance and/or Online learning in Australia. The study proceeded from a trans-informed methodological approach privileging the experiential knowledge of TGD students. Survey methods focused directly on making space for their voices at times of their convenience. An online survey hosted on Qualtrics was utilised to collect both quantitative and qualitative data from a cohort of 1,670 TGD identifying students aged 14-25 years. Participants were recruited through established social media platforms such as Facebook and Instagram as well as through TGD youth support organisations. Descriptive statistics were generated using SPSS, and thematic analyses was applied with the aid of the computer software Leximancer. Data suggests that TGD students’ experiences in alternative settings were positive and improved their overall wellbeing as compared to mainstream face-to-face settings. TGD students who accessed online learning during the COVID-19 pandemic reported increased feelings of physical safety from bullying, while simultaneously reporting negative experiences of social isolation from peers, misgendering in online settings and a lack of structure and academic support as compared to mainstream face-to-face schooling. TGD students overwhelmingly reported that online learning during COVID-19 negatively impacted upon their wellbeing. Implications for policy making and education stakeholders including researchers, school administrators and educators are discussed, as results suggest that mainstream face-to-face schools and online settings may learn from alternative settings on how best to support TGD students.
The Dynamo Clinical Trial
Creators: name: Ayres, Thomas
Publisher: name: Zenodo
Year: 2016
Subjects: X-rays
coronae
stars

description: Poster concerning the coronal activity cycles of Alpha Centauri A and B, the nearest sun-like stars, as observed by several generations of X-ray observatories including ROSAT, XMM-Newton, and most recently Chandra.
description: Also presented at HEAD-15 meeting in Naples, Florida, 3-7 April 2016.
MPEC 2023-M160 : DAILY ORBIT UPDATE (2023 June 29)
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Counting systems and the First Hilbert problem
Creators: name: Sergeyev, Yaroslav D.
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Mathematics (math.GM)
subject: FOS: Mathematics
subject: 68U, 40A, 03E, 11B

description: The First Hilbert problem is studied in this paper by applying two instruments: a new methodology distinguishing between mathematical objects and mathematical languages used to describe these objects; and a new numeral system allowing one to express different infinite numbers and to use these numbers for measuring infinite sets. Several counting systems are taken into consideration. It is emphasized in the paper that different mathematical languages can describe mathematical objects (in particular, sets and the number of their elements) with different accuracies. The traditional and the new approaches are compared and discussed.
description: 16 pages, no figures
ข้อสังเกตการเลือกใช้เหตุผลทางนิติศาสตร์ในการเขียนตอบข้อสอบกฎหมายกับการเรียงคำพิพากษา
Creators: name: พลภวิษย์ พันธุ์คำเกิด
Publisher: name: สำนักวิชานิติศาสตร์ มหาวิทยาลัยแม่ฟ้าหลวง
Year: 2562
Subjects: การใช้เหตุผลทางนิติศาสตร์
วิชาชีพกฎหมาย
ข้อสอบกฎหมาย
คำพิพากษา

description: วารสารนิติศาสตร์ มหาวิทยาลัยแม่ฟ้าหลวง, 2, 1, 171-197
ระบบกฎหมายซีวิลลอว์ : จากกฎหมายสิบสองโต๊ะสู่ประมวลกฎหมายแพ่งและพาณิชย์
Creators: name: พลภวิษย์ พันธุ์คำเกิด
Publisher: name: สำนักวิชานิติศาสตร์ มหาวิทยาลัยแม่ฟ้าหลวง
Year: 2562
Subjects: ระบบกฎหมายซีวิลลอว์
กฎหมายสิบสองโต๊ะ
ประมวลกฎหมายแพ่งและพาณิชย์

description: วารสารนิติศาสตร์ มหาวิทยาลัยแม่ฟ้าหลวง, 2, 1, 199-208
Relation Between Brown Dwarfs And Exoplanets
Creators: name: Flor Torres, Lauren Melissa
name: Coziol, Roger
name: Schröeder, Klauss-Peter
name: Caretta, César A.
name: Jack, Dennis
Publisher: name: Zenodo
Year: 2016
Subjects: Star
Planets
Brown Dwarf
Astrobiology

description: One of the most debated subjects in Astronomy since the discovery of exoplanets is how can we distinguish the most massive of such objects from very-low mass stars like Brown Dwarfs (BDs)? We have been looking for evidences of a difference in physical characteristics that could be related to different formation processes. Using a new diagnostic diagram that compares the baryonic gravitational potential (BGP) with the distances from their host stars, we have classified a sample of 355 well-studied exoplanets according to their possible structures. We have then compared the exoplanets to a sample of 87 confirmed BDs, identifying a range in BGP that could be common to both objects. By analyzing the mass-radius relations (MRR) of the exoplanets and BDs in those different BGP ranges, we were able to distinguish different characteristic behaviors. By comparing with models in the literature, our results suggest that BDs and massive exoplanets might have similar structures dominated by liquid metallic hydrogen (LMH).
description: Poster #149
description: {"references": ["Batalha, N. M. 2014, Proceedings of the National Academy of Science, 111, 12647", "Basri, G., & Brown, M. E. 2006, Annual Review of Earth and Planetary Sciences, 34, 193", "Bate, M. R. 2006, in Planet Formation, Cap. 15, pp. 236, Cambridge University Press", "Boss, A. P. 1988, ApJ, 331, 370", "Burgasser, A. J. 2008, PhT, 61, 70", "Burrows, A., & Liebert, J. 1993, Reviews of Modern Physics, 65, 301", "Burrows, A., Hubbard, W. B., Lunine, J. I., & Liebert, J. 2001, Reviews of Modern Physics, 73, 719", "Cushing, M. C. 2014, ASSL, 401, 113", "Dalladay-Simpson, P., Howie R. T. & Gregoryanz, E. 2016, Nature, 529, 63", "Grether, D. & Lineweaver, C. H. 2006, ApJ, 640, 1051", "Hatzes, A. P. & Rauer, H. 2015, ApJ, 810, L25", "Hubbard, W. B., Guillot, T., Lunine, J. I., Burrows, A., Saumon,", "D., Marley, M. S. & Freedman, R. S. 1997, PhPl, 4, 2011", "Johnson, J. A. 2009, PASP, 21, 309", "Johnston, Wm. R. 2015, Johnston\u2019s Archive of BDs: http://www.johnstonsarchive.net/astro/browndwarflist.htmKoch, D. G., Borucki, W. J., Basri, G., et al. 2010, ApJL, 713,", "LL79", "Larson, R. B. 1969, MNRAS, 145, 271", "Lissauer, J. J. 1993, Planet formation. 1993, ARA&A, 31, 129", "Padmanabhan, T. 1993, in Structure Formation in the Universe, Cambridge, UK: Cambridge University Press,", "pp. 499", "Rees, M. J. 1976, MNRAS, 176, 483", "Santerne, A., Moutou, C., Tsantaki, M., et al. 2016, A&A, 587, A64", "Silk, J. 1977a, ApJ, 214, 718", "Silk, J. 1977b, ApJ, 214, 152", "Sorahana, S., Yamamura, I., & Murakami, H. 2013, ApJ, 767, 77", "Wigner, E. & Huntington, H. B. 1935, J. Chem. Phys. 3, 764", "Winn, J. N. 2010, Exoplanets, ed. S. Seager, University of Arizona Press, p55"]}
The Luminous Infrared Host Galaxy of Short-Duration GRB 100206A
Creators: name: Perley, Daniel A.
name: Modjaz, M.
name: Morgan, A. N.
name: Cenko, S. B.
name: Bloom, J. S.
name: Butler, N. R.
name: Filippenko, A. V.
name: Miller, A. A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The known host galaxies of short-hard gamma-ray bursts (GRBs) to date are characterized by low to moderate star-formation rates and a broad range of stellar masses. In this paper, we positionally associate the recent unambiguously short-hard Swift GRB 100206A with a disk galaxy at redshift z=0.4068 that is rapidly forming stars at a rate of ~30 M_sun/yr, almost an order of magnitude higher than any previously identified short GRB host. Using photometry from Gemini, Keck, PAIRITEL, and WISE, we show that the galaxy is very red (g-K = 4.3 AB mag), heavily obscured (A_V ~ 2 mag), and has the highest metallicity of any GRB host to date (12 + log[O/H]_KD02 = 9.2): it is a classical luminous infrared galaxy (LIRG), with L_IR ~ 4 x 10^11 L_sun. While these properties could be interpreted to support an association of this GRB with very recent star formation, modeling of the broadband spectral energy distribution also indicates that a substantial stellar mass of mostly older stars is present. The current specific star-formation rate is modest (specific SFR ~ 0.5 Gyr^-1), the current star-formation rate is not substantially elevated above its long-term average, and the host morphology shows no sign of recent merger activity. Our observations are therefore equally consistent with an older progenitor, similar to what is inferred for other short-hard GRBs. Given the precedent established by previous short GRB hosts and the significant fraction of the Universe's stellar mass in LIRG-like systems at z >~0.3, an older progenitor represents the most likely origin of this event.
description: Submitted to ApJ. 15 pages, 5 tables, 9 figures
QUALITY EVALUATION OF JEANS AT THREE PRICE CATEGORIES
Creators: name: Farashahi, Behnoosh Ghaani
Publisher: name: University of Kentucky
Year: 2016
Subjects: subject: Fashion Business
subject: Fiber, Textile, and Weaving Arts

description: The purpose of this study was to evaluate the specifications, appearance and performance characteristics of jeans at three price categories and to evaluate the relationship between price and product quality. Three brands; Lucky, Gap, and Faded Glory represented men’s jeans in the price categories of better, moderate, and mass merchant (budget). Jeans were inspected and the design, material, and construction specifications were identified and compared. The appearance and performance characteristics of jeans were evaluated initially and compared to the initial characteristics after one and five launderings. ASTM and AATCC test methods were used to evaluate color difference, colorfastness to dry and wet crocking, smoothness retention, fabric breaking strength, seam strength, and dimensional change. The results of the study found that Lucky jeans had more design, material, and construction details, which would be preferable for style focused consumers with less interest on durability characteristics. Gap jeans had the highest fabric breaking strength and would be suitable for price-conscious consumers interested in durability as well as style and design. Home laundering had less impact on the appearance and performance characteristics of Faded Glory jeans and the price-conscious consumers that are primarily interested in durability would prefer Faded Glory jeans.
Time Resolved X-Ray Spectral  Analysis Of Class Ii Ysos In Ngc 2264 During Optical Dips And Bursts
Creators: name: Guarcello, Mario Giuseppe
name: Flaccomio, Ettore
name: Micela, Giuseppina
name: Argiroffi, Costanza
name: Venuti, Laura
Publisher: name: Zenodo
Year: 2016
Subjects: pre-main sequence stars; variability, protoplanetary disks; accretion

description: Pre-Main Sequence stars are variable sources. The main mechanisms responsible for their variability are variable extinction, unsteady accretion, and rotational modulation of both hot and dark photospheric spots and X-ray active regions. In stars with disks this variability is thus related to the morphology of the inner circumstellar region  (<0.1 AU) and that of photosphere and corona, all impossible to be spatially resolved with present day techniques. This has been the main motivations of the Coordinated Synoptic Investigation of NGC2264, a set of simultaneous observations of NGC2264 with 15 different telescopes.

We analyze the X-ray spectral properties of stars with disks extracted during optical bursts and dips in order to unveil the nature of these phenomena.

Stars are analyzed in two different samples. In stars with variable extinction a simultaneous increase of optical extinction and X-ray absorption is searched during the optical dips; in stars

with accretion bursts we search for soft X-ray emission and increasing X-ray absorption during the bursts.

In 9/33 stars with variable extinction we observe simultaneous increase

 of X-ray absorption and optical extinction. In seven dips it is possible to calculate the NH/AV ratio in order to infer the composition of the obscuring material. In 5/27 stars with optical accretion bursts, we observe soft X-ray emission during the bursts that we associate to the emission of accreting gas. It is not surprising that these properties are not observed in all the stars with dips and bursts since favorable geometric configurations are required.

The observed variable absorption during the dips is mainly due to dust-free material in accretion streams. In stars with accretion bursts we observe in average a larger soft X-ray spectral component not observed in non accreting stars. This indicates that this soft X-ray emission arises from the accretion shocks.
Bars in hydrodynamical cosmological simulations
Creators: name: Scannapieco, Cecilia
name: Athanassoula, Evangelia
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the properties of two bars formed in fully cosmological hydrodynamical simulations of the formation of Milky Way-mass galaxies. In one case, the bar formed in a system with disc, bulge and halo components and is relatively strong and long, as could be expected for a system where the spheroid strongly influences the evolution. The second bar is less strong, shorter, and formed in a galaxy with no significant bulge component. We study the strength and length of the bars, the stellar density profiles along and across the bars and the velocity fields in the bar region. We compare them with the results of dynamical (idealised) simulations and with observations, and find, in general, a good agreement, although we detect some important differences as well. Our results show that more or less realistic bars can form naturally in a $Λ$CDM cosmology, and open up the possibility to study the bar formation process in a more consistent way than previously done, since the host galaxies grow, accrete matter and significantly evolve during the formation and evolution of the bar.
description: 5 pages, 4 figures, MNRAS accepted
Multiferroic coupling in nanoscale BiFeO3
Creators: name: Goswami, S.
name: Bhattacharya, Dipten
name: Choudhury, P.
name: Ouladdiaf, B.
name: Chatterji, T.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Using the results of x-ray and neutron diffraction experiments, we show that the ferroelectric polarization, in ~22 nm particles of BiFeO3, exhibits a jump by ~30% around the magnetic transition point T_N (~635 K) and a suppression by ~7% under 5T magnetic field at room temperature (<
description: 4 pages including 4 figures and supplementary data; accepted for publication in Appl. Phys. Lett
Autopost-D6.5: Dissemination Workshop
Creators: name: Caballero, Monica
Publisher: name: Zenodo
Year: 2016
Subjects: Dissemination, exhibitions

description: The main objective of this deliverable is to report about the dissemination of the project results to creative professionals and research communities in the film, broadcast, and advertisement sectors.

The initial plan was to organize a dissemination workshop as the primary way of presenting the project results. During the project it was decided to focus on the presentation of the AUTOPOST project by means of a project booth in the two major trade fairs in the post-production sector, the IBC 2015 and the NAB 2016. This was due to the great opportunities aroused when AUTOPOST was invited to these events taking into account the total alignment of the objectives of AUTOPOST dissemination plan with the impact provided by the participation in the fairs.

As a final deliverable for dissemination tasks, this deliverable includes the final dissemination plan followed during the project (updating the information of D6.2), and the several dissemination activities carried out during the project. This covers the creation of the particular means and tools for disseminating the project, such as the corporative image, the website, the Vimeo channel or the Zenodo repository; the creation of dissemination material, leaflet, poster, dissemination videos and press releases; the different scientific publications made; and the contributions to the Open Data Pilot. Finally this deliverable reports the active participation in events and its impact, and collaborations made.
description: AutoPost project is co-funded by the European Union’s Horizon 2020 research and innovation programme under grant agreement No 644629.
js.2020-00392 Supplemental Table 3
Creators: name: Adibi, Jennifer
name: Xiaoshuang Xun
name: Yaqi Zhao
name: Yin, Qing
name: LeWinn, Kaja
name: Bush, Nicole R.
name: Panigrahy, Ashok
name: Peddada, Shyamal
name: Alfthan, Henrik
name: Ulf-Håkan Stenman
name: Tylavsky, Frances
name: Koistinen, Hannu
Publisher: name: figshare
Year: 2020
Subjects: subject: Biomarkers
subject: 110306 Endocrinology
subject: FOS: Clinical medicine
subject: 111706 Epidemiology
subject: FOS: Health sciences
subject: 111403 Paediatrics
subject: 111404 Reproduction
subject: FOS: Medical biotechnology
subject: 111401 Foetal Development and Medicine

description: Supplemental Table 3
High precision transit observations of the exoplanet WASP-13b with the RISE instrument
Creators: name: Barros, S. C. C.
name: Pollacco, D. L.
name: Gibson, N. P.
name: Keenan, F. P.
name: Skillen, I.
name: Steele, I. A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: WASP-13b is a sub-Jupiter mass exoplanet orbiting a G1V type star with a period of 4.35 days. The current uncertainty in its impact parameter (0 < b < 0.46) resulted in poorly defined stellar and planetary radii. To better constrain the impact parameter we have obtained high precision transit observations with the RISE instrument mounted on 2.0 m Liverpool Telescope. We present four new transits which are fitted with an MCMC routine to derive accurate system parameters. We found an orbital inclination of 85.2 \pm 0.3 degrees resulting in stellar and planetary radii of 1.56 \pm 0.04 R\odot and 1.39 \pm 0.05 RJup, respectively. This suggests that the host star has evolved off the main-sequence and is in the shell hydrogen-burning phase. We also discuss how the limb darkening affects the derived system parameters. With a density of 0.17ρJ, WASP-13b joins the group of low density planets whose radii are too large to be explained by standard irradiation models. We derive a new ephemeris for the system, T0 = 2455575.5136 \pm 0.0016 (HJD) and P = 4.353011 \pm 0.000013 days. The planet equilibrium temperature (Tequ = 1500 K) and the bright host star (V = 10.4 mag) make it a good candidate for follow-up atmospheric studies.
description: 7pages, 4 figures, submitted to MNRAS
Mycomya tenuis
Creators: name: El Mouden, Mohamed Amin
name: Chandler, Peter J.
name: Saidoun, Imane
name: Driauach, Ouafaa
name: Belqat, Boutaïna
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Mycetophilidae
Mycomya
Mycomya tenuis

description: Mycomya tenuis (Walker, 1856)
Material examined.
Morocco – Middle Atlas Region • 1 ♂; Forêt Admam; 22/V/2022; K. Aattouch, M. El Ouahabi and M. A. El Mouden leg; UAE-FST MA 22/24204.
North African distribution.
New to Morocco and North Africa.
description: Published as part of El Mouden, Mohamed Amin, Chandler, Peter J., Saidoun, Imane, Driauach, Ouafaa & Belqat, Boutaïna, 2025, A new species of Docosia Winnertz, 1864 and new records of fungus gnats (Diptera, Bolitophilidae, Keroplatidae and Mycetophilidae) from North Africa, pp. 349-379 in ZooKeys 1233 on pages 349-379, DOI: 10.3897/zookeys.1233.130502
Autopost-D6.6: Publishable Report
Creators: name: Caballero, Monica
name: Goldmann, Lutz
Publisher: name: Zenodo
Year: 2016
Subjects: AutoPost , summary

description: TThis deliverable highlights the AutoPost project’s main objectives, its activities, main S&T results/foregrounds, their potential impact, and dissemination activities carried out since the beginning of the project’s life.
description: AutoPost project is co-funded by the European Union’s Horizon 2020 research and innovation programme under grant agreement No 644629.
js.2020-00392 Supplemental Figure 1
Creators: name: Adibi, Jennifer
name: Xiaoshuang Xun
name: Yaqi Zhao
name: Yin, Qing
name: LeWinn, Kaja
name: Bush, Nicole R.
name: Panigrahy, Ashok
name: Peddada, Shyamal
name: Alfthan, Henrik
name: Ulf-Håkan Stenman
name: Tylavsky, Frances
name: Koistinen, Hannu
Publisher: name: figshare
Year: 2020
Subjects: subject: Biomarkers
subject: 110306 Endocrinology
subject: FOS: Clinical medicine
subject: 111706 Epidemiology
subject: FOS: Health sciences
subject: 111401 Foetal Development and Medicine
subject: 111403 Paediatrics
subject: 111404 Reproduction
subject: FOS: Medical biotechnology

description: Supplemental Figure 1
Hydrodynamic approach to surface pattern formation by ion beams
Creators: name: Castro, Mario
name: Cuerno, Rodolfo
Publisher: name: arXiv
Year: 2011
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: On the proper timescale, amorphous solids can flow. Solid flow can be observed macroscopically in glaciers or lead pipes, but it can also be artificially enhanced by creating defects. Ion Beam Sputtering (IBS) is a technique in which ions with energies in the 0.1-10 keV range impact against a solid target inducing defect creation and dynamics, and eroding its surface leading to formation of ordered nanostructures. Despite its technological interest, a basic understanding of nanopattern formation processes occurring under IBS of amorphizable targets has not been clearly established, recent experiments on Si having largely questioned knowledge accumulated during the last two decades. A number of interfacial equations have been proposed in the past to describe these phenomena, typically by adding together different contributions coming from surface diffusion, ion sputtering or mass redistribution, etc. in a non-systematic way. Here, we exploit the general idea of solids flowing due to ion impacts in order to establish a general framework into which different mechanisms (such as viscous flow, stress, diffusion, or sputtering) can be incorporated, under generic physical conservation laws. As opposed to formulating phenomenological interfacial equations, this approach allows to assess systematically the relevance and interplay of different physical mechanisms influencing surface pattern formation by IBS.
description: Applied Surface Science (in press). Some errata have been corrected with respect to the published version
Hydrological regime of Australian lakes over the Late-Quaternary and Holocene
Creators: name: Clerke, Liam
Publisher: name: Macquarie University
Year: 2023
Subjects: Other education not elsewhere classified

description: By comparing numerous historical records of lake level change across a vast geographic area, we are able to produce continental-scale records of change in the hydroclimate. Early efforts in reconstructing past lake level variability in Australia utilised a step-based approach at 1000-year time intervals. Since then, there has been a significant improvement to the overall spatial and temporal coverage of data across Australia, in addition to the development of new analytical techniques capable of producing higher-resolution records. This study presents an updated lake level reconstruction for Australia on a regional- and continental-scale, through the application of uncertainty-based statistical modelling techniques. The results suggest that lake-status was variable between sites across Australia over the last 30,000 years, with amplifier lakes across arid and semi-arid Australia exhibiting opposing lake-status trends to rain gauge lakes across humid Australia. Consistency in these results across experiments utilising different site inclusion parameters suggest a robustness against chronological and lake-status uncertainties, proving the potential of these models in supporting future research into how Australia’s hydroclimate could change into the future under an uncertain climate.
Analysis of an aggregate loss model in a Markov renewal regime
Creators: name: Ramírez-Cobo, Pepa
name: Carrizosa, Emilio
name: Lillo, Rosa Elvira
Publisher: name: arXiv
Year: 2024
Subjects: subject: Risk Management (q-fin.RM)
subject: Applications (stat.AP)
subject: FOS: Economics and business
subject: FOS: Computer and information sciences

description: In this article we consider an aggregate loss model with dependent losses. The losses occurrence process is governed by a two-state Markovian arrival process (MAP2), a Markov renewal process process that allows for (1) correlated inter-losses times, (2) non-exponentially distributed inter-losses times and, (3) overdisperse losses counts. Some quantities of interest to measure persistence in the loss occurrence process are obtained. Given a real operational risk database, the aggregate loss model is estimated by fitting separately the inter-losses times and severities. The MAP2 is estimated via direct maximization of the likelihood function, and severities are modeled by the heavy-tailed, double-Pareto Lognormal distribution. In comparison with the fit provided by the Poisson process, the results point out that taking into account the dependence and overdispersion in the inter-losses times distribution leads to higher capital charges.
Search for new physics in events with opposite-sign dileptons and missing transverse energy with the CMS experiment
Creators: name: Sprenger, Daniel
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The results of a search for new physics in events with two opposite-sign isolated electrons or muons, hadronic activity, and missing transverse energy in the final state are presented. The results are based on analysis of a data sample with a corresponding integrated luminosity of 0.98 fb-1 produced in pp collisions at a center-of-mass energy of 7 TeV collected by the CMS experiment at the LHC. No evidence for an event yield beyond Standard-Model expectations is found, and constraints on supersymmetric models are deduced from these observations.
description: Presented at the 2011 Hadron Collider Physics symposium (HCP-2011), Paris, France, November 14-18 2011, 3 pages, 3 figures
Duae Orationes Paedagogicae Marci Antonii Mureti De Praestantia Litterarum Humaniorum in Universitate Saeculo Sexto Decimo
Creators: name: Manning, Laura A.
Publisher: name: University of Kentucky
Year: 2016
Subjects: subject: Classical Literature and Philology

description: Marcus Antonius Muretus, humanista aetatis renascentium artium et orator, qui floruit 1526-1585, dicitur fuisse inter optimos oratores suae aetatis. Orationes Mureti per multa saecula legebantur et magni aestimabantur. Haec editio duarum orationum Mureti de praestantia litterarum est apta ad usum discipulorum qui facultatem Latine legendi confirmare debeant, qui nondum satis multa de humanismo sciant, qui provehere litteras et Latinas et Graecas volunt. In praefatione huius commentarii vitam Mureti, humanismum, artes liberales, cultum civilem Europaeum qui tempore renascentium artium exstabat, ipsam orationem, litteras humaniores, et methodum commentarii parandi tractamus.  Marcus Antonius Muretus (1526-1585) was a Renaissance humanist acknowledged as the foremost Latin orator of his day. His speeches were a model of Latin oratory not only in his own time, but in the centuries that followed. This edition of two of Muret's pedagogical speeches on the excellence of literature provides commentary for students who seek more experience reading unadapted Latin prose, to know more about humanism and European culture during the Renaissance, and to better appreciate Latin and Greek studies. The preface to this commentary discusses Muret's life, Humanism, literature and belles-lettres, the liberal arts, Renaissance culture, the state of Latin education in the Renaissance, oratory, and the text of the orations for this edition.
Wind Models For M-Type Agb Stars In Lmc
Creators: name: Bladh, Sara
Publisher: name: Zenodo
Year: 2016
Subjects: cool stars 19
AGB/Supergiant splinter session

description: The power-presentation from my talk "Wind models for M-type AGB stars in LMC"
description: {"references": ["H\u00f6fner, S., Bladh, S. et al. 2016 http://adsabs.harvard.edu/abs/2016arXiv160509730H", "Eriksson, K., Nowotny, W. et al 2014, A&A,566,95", "Mattsson, L., H\u00f6fner, S. 2011, A&A, 533, 42", "Bladh, S., H\u00f6fner, S. et al. 2015, A&A, 575, 105", "Groenewegen, M., Sloan, G. et al. 2009, A&A, 506, 1277"]}
Additional file 1 of Personalized ventilatory strategy based on lung recruitablity in COVID-19-associated acute respiratory distress syndrome: a prospective clinical study
Creators: name: Taenaka, Hiroki
name: Yoshida, Takeshi
name: Hashimoto, Haruka
name: Firstiogusran, Andi Muhammad Fadlillah
name: Ishigaki, Suguru
name: Iwata, Hirofumi
name: Enokidani, Yusuke
name: Ebishima, Hironori
name: Kubo, Naoko
name: Koide, Moe
name: Koyama, Yukiko
name: Sakaguchi, Ryota
name: Tokuhira, Natsuko
name: Horiguchi, Yu
name: Uchiyama, Akinori
name: Fujino, Yuji
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy
subject: Hematology
subject: 60506 Virology

description: Additional file 1. Supplemental Methodology and Table.
The Space of Geometric Limits of Abelian Subgroups of PSL2C
Creators: name: Baik, Hyungryul
name: Clavier, Lucien
Publisher: name: arXiv
Year: 2012
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 30F40, 20H10

description: We describe the topology of the space of all geometric limits of closed abelian subgroups of PSL2C. Main tools and ideas come from the previous paper [BC12].
description: 41 pages, 14 figures
Superconformally Covariant OPE and General Gauge Mediation
Creators: name: Fortin, Jean-François
name: Intriligator, Kenneth
name: Stergiou, Andreas
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider using broken superconformal symmetry and the super operator product expansion (sOPE) to constrain and analyze hidden sector theories that couple to our gauge forces and are not necessarily weakly coupled. Conformal and supersymmetry breaking are IR effects, associated with field or spurion expectation values, whereas the sOPE is determined in the UV and hence does not notice the breaking. The broken superconformal symmetry relates OPE coefficients of superconformal descendant operators to those of the superconformal primaries. We apply these ideas to the current correlators of general gauge mediation (GGM). We also consider analyticity properties of these correlators, e.g. their discontinuities, and use the optical theorem to relate them to total scattering cross sections from visible to hidden sector states, e.g. sigma(vis + vis --> hidden), analogous to sigma(e+ e- --> hadrons) in QCD. We discuss how the current-current OPE can be truncated to the first few terms to get a good approximation to the visible sector soft masses of GGM.
description: 33 pages, 4 figures
California's northern anchovy fishery : biological and economic basis for fishery management
Creators: name: Huppert, Daniel D.
name: MacCall, Alec D.
name: Stauffer, Gary D.
name: Parker, Keith R.
name: McMillan, Jane A.
name: Frey, Herbert W.
Publisher: name: U.S. Department of Commerce, National Oceanic and Atmospheric Administration, National Marine Fisheries Service, Southwest Fisheries Science Center
Year: 1980
Subjects: subject: Northern anchovy--Research--Pacific coast (U.S.)

description: This report was prepared during 1977-78 for the Pacific Fishery Management Council. The Council is one of seven regional councils established by the Fishery Conservation and Management Act of 1976, and is responsible for developing management plans for marine fisheries off the coasts of California, Oregon and Washington. to come under management by the Federal government through Pacific Fishery Northern anchovy was the second species (after salmon) Management Council efforts. Regulations for northern anchovy fishing were first promulgated in September 1978 and have been twice amended since then.
Mycomya tumida
Creators: name: El Mouden, Mohamed Amin
name: Chandler, Peter J.
name: Saidoun, Imane
name: Driauach, Ouafaa
name: Belqat, Boutaïna
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Mycetophilidae
Mycomya
Mycomya tumida

description: Mycomya tumida (Winnertz, 1864)
Material examined.
Morocco – Middle Atlas Region • 1 ♂; Oued Taourirt; 20/V/2022; K. Aattouch, M. El Ouahabi and M. A. El Mouden leg; UAE-FST MA 22/24205.
North African distribution.
Morocco (Banamar et al. 2020).
description: Published as part of El Mouden, Mohamed Amin, Chandler, Peter J., Saidoun, Imane, Driauach, Ouafaa & Belqat, Boutaïna, 2025, A new species of Docosia Winnertz, 1864 and new records of fungus gnats (Diptera, Bolitophilidae, Keroplatidae and Mycetophilidae) from North Africa, pp. 349-379 in ZooKeys 1233 on pages 349-379, DOI: 10.3897/zookeys.1233.130502
Additional file 8 of Reintroducing genetic diversity in populations from cryopreserved material: the case of Abondance, a French local dairy cattle breed
Creators: name: Jacques, Alicia
name: Leroy, Grégoire
name: Rognon, Xavier
name: Verrier, Etienne
name: Tixier-Boichard, Michèle
name: Restoux, Gwendal
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 8: Figure S6. Evolution of GEBV for the three indices (INEL, ISU, REPRO) in the Abondance breed. GEBV were assessed in 2017 for all genotyped individuals. Error bars correspond to standard errors.
On accuracy of mathematical languages used to deal with the Riemann zeta function and the Dirichlet eta function
Creators: name: Sergeyev, Yaroslav D.
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Mathematics (math.GM)
subject: FOS: Mathematics
subject: 11M26, 11M41, 11F66

description: The Riemann Hypothesis has been of central interest to mathematicians for a long time and many unsuccessful attempts have been made to either prove or disprove it. Since the Riemann zeta function is defined as a sum of the infinite number of items, in this paper, we look at the Riemann Hypothesis using a new applied approach to infinity allowing one to easily execute numerical computations with various infinite and infinitesimal numbers in accordance with the principle `The part is less than the whole' observed in the physical world around us. The new approach allows one to work with functions and derivatives that can assume not only finite but also infinite and infinitesimal values and this possibility is used to study properties of the Riemann zeta function and the Dirichlet eta function. A new computational approach allowing one to evaluate these functions at certain points is proposed. Numerical examples are given. It is emphasized that different mathematical languages can be used to describe mathematical objects with different accuracies. The traditional and the new approaches are compared with respect to their application to the Riemann zeta function and the Dirichlet eta function. The accuracy of the obtained results is discussed in detail.
description: 27 pages, 1 figure
Some bounds and limits in the theory of Riemann's zeta function
Creators: name: de Reyna, J. Arias
name: van de Lune, J.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Number Theory (math.NT)
subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 11M06 (primary), 11M99, 30B50 (secondary)

description: For any real a>0 we determine the supremum of the real σ such that ζ(σ+it) = a for some real t. For 0 < a < 1, a = 1, and a > 1 the results turn out to be quite different.} We also determine the supremum E of the real parts of the `turning points', that is points σ+it where a curve Im ζ(σ+it) = 0 has a vertical tangent. This supremum E (also considered by Titchmarsh) coincides with the supremum of the real σ such that ζ'(σ+it) = 0 for some real t. We find a surprising connection between the three indicated problems: ζ(s) = 1, ζ'(s) = 0 and turning points of ζ(s). The almost extremal values for these three problems appear to be located at approximately the same height.
description: 28 pages 1 figure
Topological Edge and Corner States in Biphenylene Network
Creators: name: Koizumi, Keiki
name: Phan, Huyen Thanh
name: Nishigomi, Kento
name: Wakabayashi, Katsunori
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The electronic states and topological properties of the biphenylene network (BPN) are analyzed using a tight-binding model based on the $π$-electron network. It is shown that tuning the hopping parameters induces topological phase transitions, leading to the emergence of edge states owing to the nontrivial topological Zak phase of the bulk BPN. Elementary band analysis clearly gives the number of edge states, which are associated with the location of Wannier centers. In addition, we have presented the conditions for the emergence of corner states owing to the higher-order topological nature of BPN.
description: 11 pages, 10 figures