cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
On the Spectral Evolution of Helium-Atmosphere White Dwarfs Showing Traces of Hydrogen
Creators: name: Rolland, Benoit
name: Bergeron, Pierre
name: Fontaine, Gilles
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a detailed spectroscopic analysis of 115 helium-line (DB) and 28 cool, He-rich hydrogen-line (DA) white dwarfs based on atmosphere fits to optical spectroscopy and photometry. We find that 63% of our DB population show hydrogen lines, making them DBA stars. We also demonstrate the persistence of pure DB white dwarfs with no detectable hydrogen feature at low effective temperatures. Using state-of-the art envelope models, we next compute the total quantity of hydrogen, $M_{\rm{H}}$, that is contained in the outer convection zone as a function of effective temperature and atmospheric H/He ratio. We find that some $(T_{\rm{eff}},M_{\rm{H}})$ pairs cannot physically exist as a homogeneously mixed structure; such combination can only occur as stratified objects of the DA spectral type. On that basis, we show that the values of $M_{\rm{H}}$ inferred for the bulk of the DBA stars are too large and incompatible with the convective dilution scenario. We also present evidence that the hydrogen abundances measured in DBA and cool, helium-rich white dwarfs cannot be globally accounted for by any kind of accretion mechanism onto a pure DB star. We suggest that cool, He-rich DA white dwarfs are most likely created by the convective mixing of a DA star with a thin hydrogen envelope; they are not cooled down DBA's. We finally explore several scenarios that could account for the presence of hydrogen in DBA stars.
description: Accepted for publication in The Astrophysical Journal. 75 pages, 18 figures, 3 tables
Cosmic Music: A Jazz Suite Inspired by Italo Calvino's Cosmicomics
Creators: name: Sanchez, Telesmar
Publisher: name: The University of Texas at Austin
Year: 2021
Subjects: music
jazz
Telesmar
Sanchez
composition
suite
Italo
Calvino
Cosmicomics
Cosmic

description: For my Plan II thesis, I composed a suite of pieces based off of different stories from Italo Calvino's Cosmicomics. This idea was born out of a disconnect I feel between my Plan II experience and my studies in my Jazz Guitar Performance major. My two majors are different from each other far beyond their subject matter: Their social environments, class structures, teaching methods, facilities, and resources are all in stark contrast. In pursuing both majors, I have felt like I am living a double life in undergraduate school. Very few of my music classmates even have any idea I am in Plan II, and vise-versa. Oftentimes over the past four years, I have had to deliberately split my time in half between everything Plan II and everything music. While I love both areas of study, their differences have caused me to feel a sense of overall alienation. I have felt that in doing both Plan II and music, I have kept from fully immersing myself in either. Therefore, I wanted this thesis to combine music and composition with Plan II liberal arts discourse to counteract that divide and synthesize my interests and lifestyles. Frankly, this fulfils not only a scholastic need for me, but a social one as well. I want this project to subvert my imposter syndrome with both communities by being an act of synthesis I can be proud of. I first read Cosmicomics for a Voltaire's Coffee just before I began my freshman year of college. I absolutely loved it. It proved to be deeply influential in my taste and value set in literature for my entire time in Plan II. I now consider Calvino to be my favorite author and I've since read lots of his other works. My hope was that by closely studying the storytelling nuances of such a formative Plan II text and translating them to jazz composition, I would be able to execute that meaningful synthesis I've wanted for so long. My end product is a four-movement suite of through-composed jazz music for an octet of my UT jazz major friends. Each movement is based on a short story from Cosmicomics.
Solar Neutrinos
Creators: name: Langacker, Paul
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The status of the solar neutrino problem is reviewed. Attempts to explain the observed deficit and spectral distortion, both by astrophysical and particle physics methods, are described. It is argued that the comparison of all experiments strongly prefers the particle physics solutions.
description: Invited talk presented at 32nd International School of Subnuclear Physics, Erice, July 1994. 33 pages, Latex, 15 figures, not included; postscript file with embedded figures by anonymous ftp at ftp://dept.physics.upenn.edu/pub/Langacker/erice.ps
SABZAVOT-POLIZ EKINLARDA UCHRAYDIGAN FITOFAG QO`NG`IZLARINING  TARQALISHI.
Creators: name: Rayimov, A.R.
name: Ibodulloyev, M.U.
name: Asadova, S.N.
name: Shavkatova, D.Z.
Publisher: name: Zenodo
Year: 2024

description: Tadqiqotlarimizda Buxoro viloyati hududlarida uchraydigan fitofag sabzavot-poliz ekin qo`ng`izlarning  xilma-xilligi, soni, biotoplar bo‘yicha tarqalishi va tur tarkibining mavsumiy o’zgarishi tahlil etiladi. Turli xil biotik, abiotik va antropgen omillar qo`ng`izlar faunasiga o‘zining salbiy ta’sirini ko‘rsatmay qolmaydi. Keyingi yilliklarda yuz berayotgan iqlim sharoitidagi keskinlashuv hamda ekin turlarida bo‘lgan o‘zgarishlar Buxoro viloyati entomofaunasiga ham ta’sir ko‘rsatishi tabiiy.
The Efficacy of Film as a Tool for Social-Emotional Learning
Creators: name: Alley, Ellen
Publisher: name: The University of Texas at Austin
Year: 2021
Subjects: Emotion
film
learning
emotional intelligence
social emotional learning
teaching

description: The purpose of this study is to test the efficacy of using film and television clips as a tool for teaching emotion in conjunction with standard written materials. Developing and assessing the effectiveness of an educational tool for social-emotional learning is critical to address the gap in the literature regarding ways to improve emotional recognition, understanding, and labeling skills in adults. The specific goals of this study are threefold: 1. Develop an enhanced tool for social-emotional learning (as outlined in the ability model of emotional intelligence) that utilizes film and television clips to enhance learning. 2. Assess the efficacy of the enhanced learning approach by comparing measures on emotional granularity and recognition to the standard group. 3. Assess the retention of the acquired skills over time by additional comparisons between the enhanced learning and standard groups. For the purpose of testing the efficacy of this tool, four emotions have been selected to be tested: shame, guilt, humiliation, and embarrassment. These emotions were selected because existing research demonstrates a positive relationship between emotional recognition of these affects and adaptive mental health outcomes. Additionally, the literature shows increased emotional regulation benefits for distinguishing negative emotions compared to positive emotions. Last, these emotions are commonly used, conflated, and confused words. The study, which includes a pretest, standard and enhanced learning, posttest, and two-week follow-up posttest, will collect quantitative data from a sample of 118 participants. This thesis will first examine the relevant literature regarding emotional intelligence, storytelling and emotion, and teaching tools. Second, it will describe the creation of the current tool, including the selection of emotions and film clips. Next, it will describe how emotional granularity, understanding, and recognition will be tested. Finally, it will examine the results of the study and the larger implications for the findings. This study attempts to explore address the gap in the literature regarding strategies for teaching emotion recognition, labeling, and understanding.
Weak-Lensing Mass Calibration of ACTPol Sunyaev-Zel'dovich Clusters with the Hyper Suprime-Cam Survey
Creators: name: Miyatake, Hironao
name: Battaglia, Nicholas
name: Hilton, Matt
name: Medezinski, Elinor
name: Nishizawa, Atsushi J.
name: More, Surhud
name: Aiola, Simone
name: Bahcall, Neta
name: Bond, J. Richard
name: Calabrese, Erminia
name: Choi, Steve K.
name: Devlin, Mark J.
name: Dunkley, Joanna
name: Dunner, Rolando
name: Fuzia, Brittany
name: Gallardo, Patricio
name: Gralla, Megan
name: Hasselfield, Matthew
name: Halpern, Mark
name: Hikage, Chiaki
name: Hill, J. Colin
name: Hincks, Adam D.
name: Hložek, Renée
name: Huffenberger, Kevin
name: Hughes, John P.
name: Koopman, Brian
name: Kosowsky, Arthur
name: Louis, Thibaut
name: Madhavacheril, Mathew S.
name: McMahon, Jeff
name: Mandelbaum, Rachel
name: Marriage, Tobias A.
name: Maurin, Loïc
name: Miyazaki, Satoshi
name: Moodley, Kavilan
name: Murata, Ryoma
name: Naess, Sigurd
name: Newburgh, Laura
name: Niemack, Michael D.
name: Nishimichi, Takahiro
name: Okabe, Nobuhiro
name: Oguri, Masamune
name: Osato, Ken
name: Page, Lyman
name: Partridge, Bruce
name: Robertson, Naomi
name: Sehgal, Neelima
name: Shirasaki, Masato
name: Sievers, Jonathan
name: Sifón, Cristóbal
name: Simon, Sara
name: Sherwin, Blake
name: Spergel, David N.
name: Staggs, Suzanne T.
name: Stein, George
name: Takada, Masahiro
name: Trac, Hy
name: Umetsu, Keiichi
name: van Engelen, Alex
name: Wollack, Edward J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present weak-lensing measurements using the first-year data from the Hyper Suprime-Cam Strategic Survey Program on the Subaru telescope for eight galaxy clusters selected through their thermal Sunyaev-Zel'dovich (SZ) signal measured at 148 GHz with the Atacama Cosmology Telescope Polarimeter experiment. The overlap between the two surveys in this work is 33.8 square degrees, before masking bright stars. The signal-to-noise ratio of individual cluster lensing measurements ranges from 2.2 to 8.7, with a total of 11.1 for the stacked cluster weak-lensing signal. We fit for an average weak-lensing mass distribution using three different profiles, a Navarro-Frenk-White profile, a dark-matter-only emulated profile, and a full cosmological hydrodynamic emulated profile. We interpret the differences among the masses inferred by these models as a systematic error of 10\%, which is currently smaller than the statistical error. We obtain the ratio of the SZ-estimated mass to the lensing-estimated mass (the so-called hydrostatic mass bias $1-b$) of $0.74^{+0.13}_{-0.12}$, which is comparable to previous SZ-selected clusters from the Atacama Cosmology Telescope and from the {\sl Planck} Satellite. We conclude with a discussion of the implications for cosmological parameters inferred from cluster abundances compared to cosmic microwave background primary anisotropy measurements.
description: 19 pages, 11 figures, 2 tables, comments are welcome
Theory of Exploring the Dark Halo with Microlensing 1: Power--Law Models
Creators: name: Alcock, C.
name: Allsman, R. A.
name: Axelrod, T. S.
name: Bennett, D. P.
name: Cook, K. H.
name: Evans, N. W.
name: Freeman, K. C.
name: Griest, K.
name: Jijina, J.
name: Lehner, M.
name: Marshall, S. L.
name: Perlmutter, S.
name: Peterson, B. A.
name: Pratt, M. R.
name: Quinn, P. J.
name: Rodgers, A. W.
name: Stubbs, C. W.
name: Sutherland, W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The detection of microlensing has opened the way for the development of new methods in galactic astronomy. This series of papers investigates what microlensing can teach us about the structure and shape of the dark halo. In this paper we present formulas for the microlensing rate, optical depth and event duration distributions for a simple set of axisymmetric disk-halo models. The halos are based on the "power--law models" which have simple velocity distributions. Using these models, we show that there is a large uncertainty in the predicted microlensing rate because of uncertainty in the halo parameters. For example, models which reproduce the measured galactic observables to within their errors still differ in microlensing rate towards the Magellanic Clouds by more than a factor of ten. We find that while the more easily computed optical depth correlates well with microlensing rate, the ratio of optical depth to rate can vary by a factor of two (or greater if the disk is maximal). Comparison of microlensing rates towards the Large and Small Magellanic Clouds (LMC and SMC) and M31 can be used to aid determinations of the halo flattening and rotation curve slope. For example, the ratio of microlensing rates towards the LMC and SMC is $\sim 0.7-0.8$ for E0 halos and $\sim 1.0 - 1.2$ for E7 halos (c.f. Sackett \& Gould 1993). Once the flattening has been established, the ratio of microlensing rates towards M31 and the LMC may help to distinguish between models with rising, flat or falling rotation curves. Comparison of rates along LMC and galactic bulge lines-of-sight gives useful information on the halo core radius, although this may not be so easy to extract in practice. Maximal disk models provide substantially smaller halo optical depths, shorter event durations and even larger model uncertainties.
description: 19 pages, tex, 12 figures(uuencoded + text.ps)
Additional file 11: of Functional annotation and distribution overview of RNA families in 27Â Streptococcus agalactiae genomes
Creators: name: Wolf, Ivan
name: Paschoal, Alexandre
name: Quiroga, Cecilia
name: Domingues, Douglas
name: RogĂŠrio De Souza
name: Pretto-Giordano, Lucienne
name: Laurival Vilas-Boas
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: rli and RatA RNA families counts and phage association information. (DOCX 59 kb)
แถน:ความเชื่อ พิธีกรรมและภาพสะท้อนในสังคมยุคใหม่ ในบริบทพื้นที่ภาคตะวันออกเฉียงเหนือประเทศไทยและสาธารณรัฐประชาธิปไตยประชาชนลาว
Creators: name: สุกัญญา โพธิ์ทอง
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยกาฬสินธุ์
Year: 2024
Subjects: ความเชื่อและพิธีกรรม
แถน
ภาพสะท้อน
สังคมยุคใหม่

description: วารสารมนุษยศาสตร์ สังคมศาสตร์ และนวัตกรรม มหาวิทยาลัยกาฬสินธุ์, 3, 1, 112-124
Earth: Atmospheric Evolution of a Habitable Planet
Creators: name: Olson, Stephanie L.
name: Schwieterman, Edward W.
name: Reinhard, Christopher T.
name: Lyons, Timothy W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Our present-day atmosphere is often used as an analog for potentially habitable exoplanets, but Earth's atmosphere has changed dramatically throughout its 4.5 billion year history. For example, molecular oxygen is abundant in the atmosphere today but was absent on the early Earth. Meanwhile, the physical and chemical evolution of Earth's atmosphere has also resulted in major swings in surface temperature, at times resulting in extreme glaciation or warm greenhouse climates. Despite this dynamic and occasionally dramatic history, the Earth has been persistently habitable--and, in fact, inhabited--for roughly 4 billion years. Understanding Earth's momentous changes and its enduring habitability is essential as a guide to the diversity of habitable planetary environments that may exist beyond our solar system and for ultimately recognizing spectroscopic fingerprints of life elsewhere in the Universe. Here, we review long-term trends in the composition of Earth's atmosphere as it relates to both planetary habitability and inhabitation. We focus on gases that may serve as habitability markers (CO2, N2) or biosignatures (CH4, O2), especially as related to the redox evolution of the atmosphere and the coupled evolution of Earth's climate system. We emphasize that in the search for Earth-like planets we must be mindful that the example provided by the modern atmosphere merely represents a single snapshot of Earth's long-term evolution. In exploring the many former states of our own planet, we emphasize Earth's atmospheric evolution during the Archean, Proterozoic, and Phanerozoic eons, but we conclude with a brief discussion of potential atmospheric trajectories into the distant future, many millions to billions of years from now. All of these 'Alternative Earth' scenarios provide insight to the potential diversity of Earth-like, habitable, and inhabited worlds.
description: 34 pages, 4 figures, 4 tables. Review chapter to appear in Handbook of Exoplanets
“Burdened”: A Collection of Short Stories about Eldest-Born Daughters in Immigrant Families“Burdened”: A Collection of Short Stories about Eldest-Born Daughters in Immigrant Families
Creators: name: Ameena, Irene
Publisher: name: The University of Texas at Austin
Year: 2021
Subjects: immigration
daughters
stories
short stories
creative fiction
eldest daughters
oldest daughters
immigrants
women of color
female main characters
race
gender
trauma
family

description: Online discourse often paints eldest daughters in immigrant families as carrying an outsized burden within their homes. Many feel that there is a tendency for a larger portion of responsibility to fall on them, whether that is emotional weight or tangible tasks. The roles assigned to them are influenced by birth order, race, and gender. These factors intersect to give them a unique position in their families, influenced by the challenges of migration, the duties assigned to eldest children, and the patriarchal society around them. This collection of short stories depicts the lives of five eldest daughters in immigrant families: Minahil, Ty, Eniola, Vivian, and Luna. These characters come from different backgrounds and have specific family dynamics that affect the stories I tell about them. By sharing a slice of their lives, these stories function to tell about just a few of the experiences, joys, and pressures that oldest daughters face.
A driven-dissipative quantum Monte Carlo method for open quantum systems
Creators: name: Nagy, Alexandra
name: Savona, Vincenzo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We develop a real-time Full Configuration Interaction Quantum Monte Carlo approach for the modeling of driven-dissipative open quantum systems. The method enables stochastic sampling of the Liouville-von-Neumann time evolution of the density matrix, thanks to a massively parallel algorithm, thus providing estimates of observables on the non-equilibrium steady state. We present the underlying theory, and introduce initiator technique and importance sampling to reduce the statistical error. Finally, we demonstrate the efficiency of our approach by applying it to the driven- dissipative two-dimensional XYZ spin model on lattice.
Additional file 1: of Yoga and breathing technique training in patients with heart failure and preserved ejection fraction: study protocol for a randomized clinical trial
Creators: name: Lopes, Carla
name: Luiz Danzmann
name: Moraes, Ruy
name: Vieira, Paulo
name: Meurer, Francisco
name: Soares, Douglas
name: Chiappa, Gaspar
name: Guimarâes, Luciano
name: Leitão, Santiago
name: Ribeiro, Jorge
name: Biolo, Andreia
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: SPIRIT Table. SPIRIT checklist of the protocol study. (PDF 182 kb)
A new gamma-ray source unveiled by AGILE in the region of Orion
Creators: name: Marchili, N.
name: Piano, G.
name: Cardillo, M.
name: Giuliani, A.
name: Molinari, S.
name: Tavani, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Diffuse galactic gamma-ray emission is produced by the interaction of cosmic rays (CRs) with the interstellar environment. The study of gamma-ray emission is therefore a powerful tool to investigate the origin of CRs and the processes through which they are accelerated. We aim to gain deeper insights of the nature of gamma-ray emission in the region of Orion, which is one of the best studied sites of on-going star formation, by analysing data from the AGILE satellite. The diffuse gamma-ray emission expected from the Orion region is relatively high. Its separation from the galactic plane also ensures a very low contribution from foreground or background emission, which makes it an ideal site for studying the processes of particle acceleration in star forming environments. The AGILE data are modelled through a template that quantifies the gamma-ray diffuse emission expected from atomic and molecular hydrogen. Other sources of emission are modelled as an isotropic contribution. Gamma-ray emission exceeding the amount expected by the diffuse emission model is detected with high level of significance. The main excess is in the high-longitude part of Orion A. A thorough analysis of this feature suggests a connection between the observed gamma-ray emission and the B0.5 Ia star k Orionis. The location of the gamma-ray excess is compatible with the site where stellar wind collides with the ISM. Both scattering on dark gas and cosmic-ray acceleration at the shock between the two environments are discussed as possible explanations, with the latter hypothesis being supported by the hardness of the energy spectrum of the emission. If confirmed, this would be the first direct detection of gamma-ray emission from the interaction between ISM and a single star's stellar wind.
description: 7 pages, 6 figures, Accepted for publication in Astronomy & Astrophysics
การศึกษาระดับเอนไซม์คอลีนเอสเทอเรสในเลือดภายหลังตาย
Creators: name: พีรยุทธ เฟื่องฟุ้ง
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2009
Subjects: postmortem
serum cholinesterase
organophosphate
carbamate
insecticide poisoning

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 3, 1, 43-56
ถอดบทเรียน การบริหารจัดการผู้เสียชีวิตกรณีเหตุการณ์ซานติก้า
Creators: name: พงษ์รักษ์ ศรีบัณฑิตมงคล
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2009
Subjects: DVI
Santiga pub
Mass fatalities
Personal identification

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 3, 1, 57-69
HD 7977 and its possible influence on Solar System bodies
Creators: name: Dybczyński, Piotr A.
name: Królikowska, Małgorzata
name: Bartczak, Przemysław
name: Podlewska-Gaca, Edyta
name: Kamiński, Krzysztof
name: Tokarek, Jakub
name: Langner, Krzysztof
name: de Bruijne, Jos
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In the latest Gaia third data release one can find extremely small proper motion components for the star HD 7977. This, together with the radial velocity measurement lead to the conclusion that this star passed very close to the Sun in the recent past. Such a very close approach of a one solar mass star must result in noticeable changes in the motion of all Solar System bodies, especially those on less tight orbits, namely long-period comets (LPCs) and Kuiper belt objects. We estimate and present these effects. Our current knowledge on the stellar surroundings of the Sun found in the latest Gaia catalogues allowed us to perform numerical integrations and prepare a list of potential stellar perturbers of LPCs. We use this list, made available in the StePPeD database. To study the past motion of LPCs under the simultaneous action of the Galactic potential and passing stars, we use precise original cometary orbits taken from the current CODE catalogue. We examine the reliability of the extremely small proper motion of HD 7977 concluding that this star can be an unresolved binary but according to the astrometry covering more than a century, the current Gaia results cannot be ruled out. We present the parameters of a very close passage of this star near the Sun. We also show examples of the strong influence of this passage on the past motion of some LPCs. We also discuss the possible influence of this perturber on other Solar System bodies. It is possible that 2.47 Myr ago the one solar mass star HD 7977 passed as close as one thousand au from the Sun. Such an event constitutes a kind of dynamical horizon for all studies of the past Solar System bodies' dynamics.
description: 15 pages, 13 figures, 5 tables, submitted to A&A
Constraining cosmic ray acceleration in young star clusters using multi-wavelength observations
Creators: name: Gupta, Siddhartha
name: Nath, Biman B.
name: Sharma, Prateek
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We use $1$D and $3$D two-fluid cosmic ray (CR) hydrodynamic simulations to investigate the role of CRs in the vicinity of a compact young star cluster. We model a self-gravitating cloud (density profile $ρ\propto r^{-1}$), include important thermal and non-thermal processes, and explore two different CR injection scenarios. We show that if internal shocks in the wind-driving region are the main site for CR acceleration, then the resulting $γ$-ray luminosity ($L_{\rm γ}$) can reach $\approx 5\%$ of the mechanical luminosity ($L_{\rm w}$), independent of the fraction of wind energy ($\sim 1-20\%$) injected into CRs. In contrast, if the forward/reverse shock of a bubble is the injection site then $L_{\rm γ}$ increases linearly with the CR injection fraction, as expected analytically. We find that the X-ray luminosity ($L_{\rm x}$) in the forward/reverse shock injection scenario is $\gtrsim 10^{-3} L_{\rm w}$, which is $\sim 10$ times larger than in the central wind-driving injection case. We predict the corresponding range of the synchrotron radio luminosity. We show how multi-wavelength observations can constrain the CR parameters. Comparing the predicted multi-wavelength luminosities with those of 30 Doradus we identify the reverse shock as the most probable CR injection site, and that thermal conduction is important. We do not find significant dynamical impact of CRs in our models.
description: 16 pages, 14 figures, 2 tables; submitted to MNRAS, Comments welcome
การชันสูตรพลิกศพที่ยิงตัวตายในโรงพยาบาลศรีนครินทร์ คณะแพทยศาสตร์ มหาวิทยาลัยขอนแก่น
Creators: name: วิรุจน์ คุณกิตติ
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2010
Subjects: suicide
forensic autopsy
gunshot wound

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 4, 1, 2-16
Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
Creators: name: Fernández-Fernández, Rebeca
name: Bonavera, Laura
name: Crespo, David
name: González-Nuevo, Joaquín
name: Cueli, Marcos M.
name: Casas, José Manuel
name: Cabo, Sara R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Magnification bias, an observational effect of gravitational lensing in the weak regime, allows testing the cosmological model through angular correlations of sources at different redshifts. This effect has been observed in various contexts, particularly with sub-millimeter galaxies (SMGs), offering astrophysical and cosmological insights. The study aims to investigate the magnification bias effect exerted by galaxy clusters on SMGs and its implications for astrophysical and cosmological parameters within the $Λ$CDM model. Magnification bias was explored through quantifying the cross-correlation function, utilised to derive constraints on cosmological and astrophysical parameters with a Markov Chain Monte Carlo algorithm. Two distinct galaxy cluster samples were used to assess result robustness and understand the influence of sample characteristics. Cluster samples show higher cross-correlation values than galaxies, with an excess at larger scales suggesting contributions from additional large-scale structures. The parameters obtained, while consistent with galaxies, are less constrained due to broader redshift distributions and limited cluster statistics. Results align with weak lensing studies, hinting at slightly lower $σ_8$ and $Ω_m$ values than \emph{Planck}'s CMB data, emphasizing the need for enhanced precision and alternative low-redshift universe tests. While yielding constraints compatible with the $Λ$CDM model, limitations include broader redshift distributions and a limited number of lenses, resulting in less constrained parameters compared to previous galaxy studies. Nonetheless, the study underscores the potential of using galaxy clusters as lenses for magnification bias studies, capitalising on their elevated mass, providing a promising avenue to test current Cosmology theories. Further progress can be made by expanding the lens sample size.
Probing the mass function of halo dark matter via microlensing
Creators: name: Green, Anne M
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The simplest interpretation of the microlensing events observed towards the Large Magellanic Clouds is that approximately half of the mass of the Milky Way halo is in the form of MAssive Compact Halo Objects with $M \sim 0.5 M_{\odot}$. It is not possible, due to limits from star counts and chemical abundance arguments, for faint stars or white dwarves to comprise such a large fraction of the halo mass. This leads to the consideration of more exotic lens candidates, such as primordial black holes, or alternative lens locations. If the lenses are located in the halo of the Milky Way, then constraining their mass function will shed light on their nature. Using the current microlensing data we find, for four halo models, the best fit parameters for delta-function, primordial black hole and various power law mass functions. The best fit primordial black hole mass functions, despite having significant finite width, have likelihoods which are similar to, and for one particular halo model greater than, those of the best fit delta functions . We then use Monte Carlo simulations to investigate the number of microlensing events necessary to determine whether the MACHO mass function has significant finite width. If the correct halo model is known, then $\sim$ 500 microlensing events will be sufficient, and will also allow determination of the mass function parameters to $\sim 5%$.
description: 28 pages including 14 figures, version to appear in ApJ, minor changes to discussion
การวิเคราะห์การวินิจฉัยสาเหตุการเสียชีวิตที่แน่ชัดในศพผู้ใหญ่ที่เสียชีวิตทันทีโดยที่ไม่สามารถอธิบายสาเหตุการเสียชีวิต
Creators: name: สามารถ มณีรัตน์
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2010
Subjects: Sudden death
SUD
CVS
CNS
CAD
CVA
Myocardial infarction and Undetermined cause of death

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 4, 1, 17-23
Additional file 6 of A TP53 mutation model for the prediction of prognosis and therapeutic responses in head and neck squamous cell carcinoma
Creators: name: Shi, Congyu
name: Liu, Shan
name: Tian, Xudong
name: Wang, Xiaoyi
name: Gao, Pan
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 6: Supplemental Table 1. The immune and clinic characteristics between HPV negative patients and positive patients in TCGA HNSC. Briefly speaking HPV + HNSC has more infiltrated immune cells, especially tumor suppressive cells like memory B cell, CD8 T cells, activated memory CD4 T cells, T cells follicular helper, and less pro-tumor cells like Macrophages M2. Interestingly HPV + HNSC has a greater proportion of low risk group, and those HPV positive patients were younger (median age:57 vs 61) and of high pathological grade.
Do Climate Signals Matter? Evidence from Agriculture
Creators: name: Cui, Xiaomeng
name: Gammans, Matthew
name: Merel, Pierre
name: Cui, Xiaomeng
name: Gammans, Matthew
name: Merel, Pierre
Publisher: name: Unknown
Year: 2019
Subjects: subject: Environmental Economics and Policy
subject: climate change
subject: climate adaptation
subject: panel data
subject: crop yield

description: The foreseeable impacts of climate change on humans depend critically on the ability of societies to adapt to new climatic signals. Recent literature based on the US experience suggest little to no adaptation to climate trends in crop agriculture. We revisit this question with a novel panel econometrics framework that allows yearly outcomes to jointly respond to contemporaneous weather and climate signals, delivering estimates of both short-run and long-run climate change impacts within a single regression framework. In our most conservative model, which strictly relies on the existence of trends in climate to identify adaptation potential, we find evidence of adaptation to beneficial temperatures (as captured by growing degree days) and precipitation, for both corn and soybean yields. Evidence of adaptation to extreme heat is more nuanced, with suggestive evidence of adaptation for corn and no evidence for soybeans. The presence of adaptation matters for the calculation of warming impacts: the net counterfactual impacts of warming are negative in the short run but become positive in the long run.
Additional file 1: of Radiosurgery or hypofractionated stereotactic radiotherapy for brain metastases from radioresistant primaries (melanoma and renal cancer)
Creators: name: Lesueur, Paul
name: Lequesne, Justine
name: Barraux, Victor
name: Kao, William
name: Geffrelot, Julien
name: Jean-Michel Grellard
name: Jean-Louis Habrand
name: Emery, Evelyne
name: Marie, Brigitte
name: Thariat, Juliette
name: Stefan, Dinu
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Cancer

description: Table S1. Characteristics of treated metastases and radiotherapy for the pairs matched groups. (DOCX 16 kb)
Wolfenstein Parametrization Re-examined
Creators: name: Xing, Zhi-zhong
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Wolfenstein parametrization of the $3\times 3$ Kobayashi-Maskawa (KM) matrix $V$ is modified by keeping its unitarity up to the accuracy of $O(λ^{6})$. This modification can self-consistently lead to the off-diagonal asymmetry of $V$: $|V_{ij}|^{2}-|V_{ji}|^{2}$ = $Z\displaystyle\sum_{k}ε^{~}_{ijk}$ with $Z=\approx A^{2}λ^{6} (1-2ρ)$, which is comparable in magnitude with the Jarlskog parameter of $CP$ violation $J\approx A^{2}λ^{6}η$. We constrain the ranges of $J$ and $Z$ by using the current experimental data, and point out that the possibility of a symmetric KM matrix has almost been ruled out.
description: 5 Latex pages including a figure; Two references are added
Tips for Deciphering and Quick Calculation of Radiation Spectra
Creators: name: Bondarenco, M. V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Radiation spectra from ultra-relativistic electrons in thin [$T\ll l_f(ω)$] and thick [$T\gg l_f(ω)$] targets are discussed. The method of simplified averaging is described by examples of Landau-Pomeranchuk-Migdal effect and radiation at doughnut scattering. General infrared and ultraviolet asymptotic properties of radiation spectra are discussed.
description: 6 pages, 4 figures, Proceedings of RREPS-2017, DESY, Hamburg, Germany
ความจำเพาะเจาะจงของการตรวจไมโครแซทเทลไลท์จากสารพันธุกรรมของมนุษย์เปรียบเทียบกับสัตว์เลี้ยงและสัตว์ที่มีสายพันธุ์ใกล้เคียงกับมนุษย์
Creators: name: ณัฐสิทธิ์ เจริญสันติ
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2010
Subjects: Cross-species
STR
microsatellite
D3S1358
D5S818
D8S1179
D10S2325
D13S317
D16S539
D19S253
THO1
vWA
TPOX

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 4, 1, 24-33
Additional file 2: of Education-related disparities in reported physical activity during leisure-time, active transportation, and work among US adults: repeated cross-sectional analysis from the National Health and Nutrition Examination Surveys, 2007 to 2016
Creators: name: Scholes, Shaun
name: Bann, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy

description: Activity levels (â Ľ150Â min/week) by demographic subgroups (age, gender, and race/ethnicity). (DOCX 42 kb)
Nonleptonic three-body charmed baryon weak decays with H(15)
Creators: name: Geng, Chao-Qiang
name: Liu, Chia-Wei
name: Liu, Sheng-Lin
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the nonleptonic three-body charmed baryon weak decays of $\mathbf{B}_{c}\rightarrow\mathbf{B}_{n}PP^{\prime}$ under the $SU(3)_{F}$ flavor symmetry, where $\mathbf{B}_{c}$ denotes the anti-triplet charmed baryon, comprising $(Ξ^{0}_{c},-Ξ^{+}_{c},Λ^{+}_{c})$, and $\mathbf{B}_{n}$ and $P(P^{\prime})$ represent octet baryon and pseudoscalar meson states, respectively. In addition to 12 parameters from the contributions of the color-antisymmetric part of the effective Hamiltonian, denoted as $H(\bar{\mathbf{6}})$, there are 4 parameters from the color-symmetric one, $H(\mathbf{15})$, which were not included in the previous study. With 16 parameters in total and 28 experimental data points, we obtain the minimal $χ^2$ over degree of freedom of $χ^{2}/d.o.f=1.5$, which is a great improvement comparing to that without $H(\mathbf{15})$. With the better fitting values, we evaluate the branching ratios and up-down asymmetries of $\mathbf{B}_{c}\rightarrow\mathbf{B}_{n}PP^{\prime}$, which present some interesting results such as $\mathcal{B}\,(Λ^{+}_{c}\rightarrow(Ξ(1690)^{0}\rightarrowΣ^{+}K^{-})\,K^{+})\equiv(1.5\pm0.4)\times10^{-3}$ and potential $SU(3)$ breaking effects in $Ξ^{+}_{c}\rightarrow pπ^{+}K^{-}$ and $Λ^{+}_{c}\rightarrow Σ^{+}π^{-}K^{+}$ to be verified by the experiments at BESIII, Belle-II and LHCb.
description: 21 pages, 2 figures,14 tables
การศึกษาความคงตัวของความเข้มข้นของเมทแอมเฟตามีนในปัสสาวะที่เก็บที่อุณหภูมิห้องในแต่ละช่วงเวลา
Creators: name: ภัทรวรรณ รัตนาวิวัฒน์พงศ์
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2010
Subjects: stability
non-spiked urine methamphetamine
room temperature
postmortem

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 4, 1, 34-42
Toxicokinetic Profiling and Developmental Neurotoxicity of Long-Chain PFAS Exposure in Zebrafish as a Model for Human Health
Creators: name: Kraus, Paul G
Publisher: name: Purdue University Graduate School
Year: 2025
Subjects: classificationCode: 321407
subject: Toxicology (incl. clinical toxicology)
classificationCode: 429999
subject: Other health sciences not elsewhere classified
classificationCode: 520202
subject: Behavioural neuroscience

description: This thesis is concerned with the investigation of the health effects and toxicokinetic behavior of perfluorooctane sulfonate (PFOS), perfluorodecanoic acid (PFDA), and perfluoroundecanoic acid (PFUnDA), three legacy, long-chain per- and polyfluoroalkyl substances (PFAS). These substances are known to be highly persistent in the environment and generally believed to be highly bioaccumulative. Despite being phased out of production in favor of theoretically safer short-chain alternatives in the 2000s, a study found that many Americans are still being exposed to a number of long-chain PFAS, primarily PFOS, PFDA, and PFUnDA, to a substantial degree through the consumption of freshwater fish. In this thesis, zebrafish were used as a model organism to characterize toxicokinetics of these three PFAS and as a model for potential human developmental neurotoxicity, specifically as it pertains to dysregulation of dopamine. Mass spectrometer quantification of both water and tissue samples revealed that all three PFAS were rapidly absorbed by zebrafish during the early developmental window and bioconcentrated in the tissue to a substantial degree. Locomotor behavioral analysis of exposed larvae revealed a number of significant abnormalities, especially in PFDA and PFUnDA. ELISA quantification of dopamine indicated that these compounds induced significant changes in dopamine regulation at nearly every exposure concentration for each compound down to the lowest test concentration used in this study at 0.004 ppb (µg/L). These findings indicate that PFOS, PFDA, and PFUnDA all exhibit a substantial capacity for bioaccumulation. The present findings also demonstrate a need for further research into how developmental exposure to long-chain PFAS can impact neurological health, as well as further consideration for the legal regulation of this class of environmental pollutants.
Thermodynamics of charged black holes in Maxwell-dilaton-massive gravity
Creators: name: Yue, Rui-Hong
name: Qian, Kai-Qiang
name: Liu, Bo
name: Zou, De-Cheng
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Considering the nonminimal coupling of the dilaton field to the massive graviton field in Maxwell-dilaton-massive gravity, we obtain a class of analytical solutions of charged black holes, which are neither asymptotically flat nor (A)dS. The calculated thermodynamic quantities, such as mass, temperature and entropy, verify the validity of the first law of black hole thermodynamics. Moreover, we further investigate the critical behaviors of these black holes in the grand canonical and canonical ensemble, and find a novel critical phenomenon never before observed, known as the ``reverse" reentrant phase transition with a tricritical point. It implies that the system undergoes a novel ``SBH-LBH-SBH" phase transition process, and is the reverse of the ``LBH-SBH-LBH" process observed in reentrant phase transitions.
description: 20 Pages, 5 figures, 8 tables
การศึกษาการเปลี่ยนแปลงระดับความเข้มข้นของไซยาไนด์ในเลือดศพที่อุณหภูมิเก็บรักษา
Creators: name: มานะ บุญเต็ม
Publisher: name: สมาคมแพทย์นิติเวชแห่งประเทศไทย
Year: 2010
Subjects: postmortem
cyanide level
blood cyanide level
cyanide

description: วารสารสมาคมแพทย์นิติเวชแห่งประเทศไทย, 4, 1, 43-51
Uniform Substitution for Differential Game Logic
Creators: name: Platzer, André
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Computer Science and Game Theory (cs.GT)
subject: Programming Languages (cs.PL)
subject: Logic (math.LO)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: F.4.1; F.3.1; F.3.2; I.2.3
subject: 03F03, 03B70, 34A38, 91A25

description: This paper presents a uniform substitution calculus for differential game logic (dGL). Church's uniform substitutions substitute a term or formula for a function or predicate symbol everywhere. After generalizing them to differential game logic and allowing for the substitution of hybrid games for game symbols, uniform substitutions make it possible to only use axioms instead of axiom schemata, thereby substantially simplifying implementations. Instead of subtle schema variables and soundness-critical side conditions on the occurrence patterns of logical variables to restrict infinitely many axiom schema instances to sound ones, the resulting axiomatization adopts only a finite number of ordinary dGL formulas as axioms, which uniform substitutions instantiate soundly. This paper proves soundness and completeness of uniform substitutions for the monotone modal logic dGL. The resulting axiomatization admits a straightforward modular implementation of dGL in theorem provers.
The neutrino cross section and upward going muons
Creators: name: Lipari, Paolo
name: Lusignoli, Maurizio
name: Sartogo, Francesca
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The charged current cross section for neutrinos with energy of a few GeV is reanalysed. In this energy range the cross section for the lowest multiplicity exclusive channels is an important fraction of $σ_{CC}$ and the approximation of describing the cross section with deep inelastic scattering formulae may be inaccurate. Possible consequences of our reanalysis of the cross section in the interpretation of the data obtained by deep underground detectors on $ν$--induced upward going muons (both stopping and passing) are discussed.
description: 9 pages, REVTEX, 1 uu-encoded compressed file with 3 figures
Additional file 3: of Improving patient safety by enhancing raising concerns at medical school
Creators: name: Johnson, Luke
name: Malik, Natasha
name: Gafson, Irene
name: Gostelow, Naomi
name: Kavanagh, Jayne
name: Griffin, Ann
name: Gishen, Faye
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Appendix 3. The consent form received by focus group participants to understand what they were agreeing to by partaking in the focus group. (DOCX 14 kb)
Additional file 10 of MicroRNA-based signatures impacting clinical course and biology of ovarian cancer: a miRNOmics study
Creators: name: Krasniqi, E.
name: Sacconi, A.
name: Marinelli, D.
name: Pizzuti, L.
name: Mazzotta, M.
name: Sergi, D.
name: Capomolla, E.
name: Donzelli, S.
name: Carosi, M.
name: Bagnato, A.
name: Gamucci, T.
name: Tomao, S.
name: Natoli, C.
name: Marchetti, P.
name: Grassadonia, A.
name: Tinari, N.
name: De Tursi, M.
name: Vizza, E.
name: Ciliberto, G.
name: Landi, L.
name: Cappuzzo, F.
name: Barba, M.
name: Blandino, G.
name: Vici, P.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer

description: Additional file 10: Figure S2. Kaplan-Meier curves illustrating the performance of the IRE prognostic signature in the TCGA cohort for EFS (A), and OS (B). Kaplan-Meier curves showing the impact of miR-224-5p on EFS in the IRE cohort (C). Differences between curves were evaluated by logrank test. Box plots illustrating the expression level of miR-224-5p in tumor samples (T) versus normal tissue samples (N), in the TCGA cohort (D), and in the IRE cohort (E). Box plots showing the expression levels of miR-200a in platinum resistant tumors (resist) versus platinum sensitive tumors (resist), in the TCGA (F). Differences in miRNAs expression were assessed by Student’s T-test. For all the comparisons, the level of statistical significance was p