cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Polarization, Polarizing Efficiency, and Grain alignment towards the direction of the cluster NGC 2345
Creators: name: Singh, Sadhana
name: Pandey, Jeewan C.
name: Hoang, Thiem
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have investigated the grain alignment and dust properties towards the direction of the cluster NGC 2345 using the multi-band optical polarimetric observations. For the majority of the stars, the observed polarization is found to be due to the interstellar medium with average values of maximum polarization and wavelength corresponding to it as 1.55% and 0.58 $μm$, respectively. This reveals a similar size distribution of dust grains to that in the general interstellar medium in the direction of NGC 2345. Alteration of dust properties near the distance of 1.2 kpc towards the direction of NGC 2345 has been noticed. The dust grains located beyond this distance are found to be aligned with the Galactic magnetic field, whereas a dispersion in orientation of the dust grains lying in the foreground of this distance is found. Polarizing efficiency of grains in this direction is found to be close to the average efficiency for our Galaxy. The decreased grain size along with the increased polarizing efficiency towards the core region of the cluster indicates the local radiation field is higher within the cluster which is responsible for the increased alignment efficiency of small grains. The wavelength of maximum polarization (associated with the average size of aligned grains) is also found to increase with extinction and reduces with the increase in polarizing efficiency, which can be explained by the radiative torque alignment mechanism.
description: 15 pages, 9 figures, 2 tables. Accepted for publication in MNRAS
sj-docx-2-aas-10.1177_00953997221109308 – Supplemental material for Learning and Adaptation in Polycentric Transport Governance: The Case of the Dutch Brabant Accessibility Agenda
Creators: name: Bousema, Ingo
name: Busscher, Tim
name: Rauws, Ward
name: Leendertse, Wim
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160607 International Relations
subject: FOS: Political science
subject: 160509 Public Administration

description: Supplemental material, sj-docx-2-aas-10.1177_00953997221109308 for Learning and Adaptation in Polycentric Transport Governance: The Case of the Dutch Brabant Accessibility Agenda by Ingo Bousema, Tim Busscher, Ward Rauws and Wim Leendertse in Administration & Society
sj-docx-1-ahd-10.1177_00914150221112284 - Supplemental material for Longitudinal Associations of Perceived Mastery and Constraints With Coping and Their Implications for Functional Health for Aging Adults
Creators: name: Toyama, Masahiro
name: Hektner, Joel M.
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 110308 Geriatrics and Gerontology
subject: FOS: Clinical medicine

description: Supplemental material, sj-docx-1-ahd-10.1177_00914150221112284 for Longitudinal Associations of Perceived Mastery and Constraints With Coping and Their Implications for Functional Health for Aging Adults by Masahiro Toyama and Joel M. Hektner in The International Journal of Aging and Human Development
A semi-analytical solution to the forward-reverse shock hydrodynamics of the gamma-ray burst afterglow
Creators: name: Zhang, Ze-Lin
name: Liu, Ruo-Yu
name: Geng, Jin-Jun
name: Wu, Xue-Feng
name: Wang, Xiang-Yu
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We extend the standard model of forward-reverse shock (FS-RS) for gamma-ray burst (GRB) afterglow to more general cases. On one hand, we derive the analytical solution to the hydrodynamics of the shocks in two limiting cases, i.e., an ultra-relativistic reverse shock case and a Newtonian reverse shock case. Based on the asymptotic solutions in these two limiting cases, we constitute a semi-analytical solution for the hydrodynamics of the shocks in the generic case, covering the mildly-relativistic reverse shock case. On the other hand, we derive the evolution of the system taking into account the condition of energy conservation which is not satisfied in the standard FS-RS model. A generic solution of semi-analytical expressions is also given. In both the extended standard FS-RS model (satisfying pressure balance condition) and the model satisfying energy conservation, we find that the results in the ultra-relativistic reverse shock case and in the early stage of the Newtonian reverse shock case are different from those in the standard FS-RS model by only a factor that close to one while the same initial conditions adopted. However, the asymptotic solutions in the limiting cases are not good approximations to those in the intermediate case. Our semi-analytical results agree well with the numerical results for a large range of model parameters, and hence can be easily employed to diagnose the physical quantities of the GRB shell and circumburst environment.
description: 13 pages, 8 figures, Accepted for publication in MNRAS, Comments and questions are welcome!
Isotope velocimetry: Experimental and theoretical demonstration of the potential importance of gas flow for isotope fractionation during evaporation of protoplanetary material
Creators: name: Young, Edward D.
name: Macris, Catherine A.
name: Tang, Haolan
name: Hogan, Arielle A.
name: Shollenberger, Quinn R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Fluid Dynamics (physics.flu-dyn)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: We use new experiments and a theoretical analysis of the results to show that the isotopic fractionation associated with laser-heating aerodynamic levitation experiments is consistent with the velocity of flowing gas as the primary control on the fractionation. The new Fe and Mg isotope data are well explained where the gas is treated as a low-viscosity fluid that flows around the molten spheres with high Reynolds numbers and minimal drag. A relationship between the ratio of headwind velocity to thermal velocity and saturation is obtained on the basis of this analysis. The recognition that it is the ratio of flow velocity to thermal velocity that controls fractionation allows for extrapolation to other environments in which molten rock encounters gas with appreciable headwinds. In this way, in some circumstances, the degree of isotope fractionation attending evaporation is as much a velocimeter as it is a barometer.
description: Accepted for publication in Earth and Planetary Science Letters
sj-docx-2-cpc-10.1177_10556656211036316 - Supplemental material for Genome-Wide Scan for Parent-of-Origin Effects in a sub-Saharan African Cohort With Nonsyndromic Cleft Lip and/or Cleft Palate (CL/P)
Creators: name: Gowans, Lord J. J.
name: Comnick, Carissa L.
name: Mossey, Peter A.
name: Eshete, Mekonen A.
name: Adeyemo, Wasiu L.
name: Naicker, Thirona
name: Awotoye, Waheed A.
name: Petrin, Aline
name: Adeleke, Chinyere
name: Donkor, Peter
name: Busch, Tamara D.
name: James, Olutayo
name: Ogunlewe, Mobolanle O.
name: Li, Mary
name: Olotu, Joy
name: Hassan, Mohaned
name: Adeniyan, Oluwole A.
name: Obiri-Yeboah, Solomon
name: Arthur, Fareed K. N.
name: Agbenorku, Pius
name: Oti, Alexander A.
name: Olatosi, Olubukola
name: Adamson, Olawale O.
name: Fashina, Azeez A.
name: Zeng, Erliang
name: Marazita, Mary L.
name: Adeyemo, Adebowale A.
name: Murray, Jeffrey C.
name: Butali, Azeez
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 110323 Surgery
subject: FOS: Clinical medicine

description: Supplemental material, sj-docx-2-cpc-10.1177_10556656211036316 for Genome-Wide Scan for Parent-of-Origin Effects in a sub-Saharan African Cohort With Nonsyndromic Cleft Lip and/or Cleft Palate (CL/P) by Lord J. J. Gowans, Carissa L. Comnick, Peter A. Mossey, Mekonen A. Eshete, Wasiu L. Adeyemo, Thirona Naicker, Waheed A. Awotoye, Aline Petrin, Chinyere Adeleke, Peter Donkor, Tamara D. Busch, Olutayo James, Mobolanle O. Ogunlewe, Mary Li, Joy Olotu, Mohaned Hassan, Oluwole A. Adeniyan, Solomon Obiri-Yeboah, Fareed K. N. Arthur, Pius Agbenorku, Alexander A. Oti, Olubukola Olatosi, Olawale O. Adamson, Azeez A. Fashina, Erliang Zeng, Mary L. Marazita, Adebowale A. Adeyemo, Jeffrey C. Murray and Azeez Butali in The Cleft Palate-Craniofacial Journal
sj-docx-1-ejo-10.1177_11206721211049102 - Supplemental material for Combined transconjunctival sutureless three-port vitrectomy and scleral fixation of intraocular lens
Creators: name: Danese, Carla
name: Lanzetta, Paolo
Publisher: name: SAGE Journals
Year: 2022
Subjects: Medicine

description: Supplemental material, sj-docx-1-ejo-10.1177_11206721211049102 for Combined transconjunctival sutureless three-port vitrectomy and scleral fixation of intraocular lens by Carla Danese and Paolo Lanzetta in European Journal of Ophthalmology
Termination Shocks and the Extended X-ray Emission in MRK 78
Creators: name: Fornasini, Francesca M.
name: Elvis, Martin
name: Maksym, W. Peter
name: Fabbiano, Giuseppina
name: Bergmann, Thaisa Storchi
name: Gandhi, Poshak
name: Whittle, Mark
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Sub-arcsecond imaging of the X-ray emission in the type 2 AGN Mrk 78 with Chandra shows complex structure with spectral variations on scales from $\sim$200 pc to $\sim$ 2 kpc. Overall the X-ray emission is aligned E-W with the radio (3.6 cm) and narrow emission line region as mapped in [OIII], with a marked E-W asymmetry. The Eastern X-ray emission is mostly in a compact knot coincident with the location where the radio source is deflected, while the Western X-ray emission forms a loop or shell $\sim$2 kpc from the nucleus with radius $\sim$0.7 kpc. There is suggestive evidence of shocks in both the Eastern knot and the Western arc. Both these positions coincide with large changes in the velocities of the [OIII] outflow. We discuss possible reasons why the X-ray shocks on the Western side occur $\sim1$ kpc farther out than on the Eastern side. We estimate that the thermal energy injected by the shocks into the interstellar medium corresponds to $0.05-0.6$% of the AGN bolometric luminosity.
description: 23 pages, 14 figures, 6 tables
Determining the aberrations in a nearly diffraction-limited spectrograph
Creators: name: Sánchez, B.
name: Watson, A. M.
name: Cuevas, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a method to determine the static aberrations in a nearly diffraction-limited spectrograph introduced, for example, by alignment or manufacturing errors. We consider an instrument with two stages separated by a slit or image slicer located in the intermediate focal plane. In such a spectrograph, it is not trivial to distinguish aberrations in the first stage, before the slit, from those in the second, after the slit. However, our method achieves this. Measuring these aberrations separately opens the possibility of reducing them, by realignment or other means, and thereby improving the optical performance of the instrument. The method is based on fitting models to multiple images of a point source, with controlled displacements of the source perpendicular to the slit and controlled defocuses of the second stage or the detector. Fitting models to these images allows the determination of the aberrations in both stages. Our key discovery is that the displaced and defocused images provide additional information which allows us to break the ambiguity between the two stages. We present simulations that validate the performance of the method.
description: Accepted by MNRAS. 17 pages
57614: Bottom Wood and Quadrangle Wood
Creators: name: Project Team, First World War Poetry Digital Archive
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: This is a photograph taken from some high ground above Mametz Wood showing the location of Bottom Wood (left) and Quadrangle Wood (the small gathering of tress to the right)"
The attack by the 1st Royal Welch Fusiliers on the 4th July 1916 started at Bottom Wood and ended in the capture of Quadrangle Trench which ran from left to right in the photograph just behind Quadrangle Wood.
sj-docx-1-pie-10.1177_09544089211037443 - Supplemental material for Multi-response modeling for sliding wear behavior of AA5052/TiC composites by stir casting: A comparative analysis using response surface methodology and fuzzy logic system
Creators: name: Samal, Priyaranjan
name: Vundavilli, Pandu R
name: Meher, Arabinda
name: Mahapatra, Manas M
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, sj-docx-1-pie-10.1177_09544089211037443 for Multi-response modeling for sliding wear behavior of AA5052/TiC composites by stir casting: A comparative analysis using response surface methodology and fuzzy logic system by Priyaranjan Samal, Pandu R Vundavilli, Arabinda Meher and Manas M Mahapatra in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
Creators: name: Bohn, Thomas
name: Canalizo, Gabriela
name: Satyapal, Shobita
name: Sales, Laura
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: While it is generally believed that supermassive black holes (SMBH) lie in most galaxies with bulges, few SMBHs have been confirmed in bulgeless galaxies. Identifying such a population could provide important insights to the BH seed population and secular BH growth. To this end, we obtained near-infrared spectroscopic observations of a sample of low-redshift bulgeless galaxies with mid-infrared colors suggestive of AGN. We find additional evidence of AGN activity (such as coronal lines and broad permitted lines) in 69$\%$ (9/13) of the sample, demonstrating that mid-infrared selection is a powerful tool to detect AGN. More than half of the galaxies with confirmed AGN activity show fast outflows in [O III] in the optical and/or [Si VI] in the NIR, with the latter generally having much faster velocities that are also correlated to their spatial extent. We are also able to obtain virial BH masses for some targets and find they fall within the scatter of other late-type galaxies in the $M_{\rm{BH}}$-$M_{\rm{stellar}}$ relation. The fact that they lack a significant bulge component indicates that secular processes, likely independent of major mergers, grew these BHs to supermassive sizes. Finally, we analyze the rotational gas kinematics and find two notable exceptions: two AGN hosts with outflows that appear to be rotating faster than expected. There is an indication that these two galaxies have stellar masses significantly lower than expected from their dark matter halo masses. This, combined with the observed AGN activity and strong gas outflows may be evidence of the effects of AGN feedback.
description: Accepted by ApJ. 25 pages, 8 figures, and 6 tables
Unveiling non-gray surface of cloudy exoplanets: the influence of wavelength-dependent surface albedo and cloud scattering properties on retrieval solutions
Creators: name: Wang, Fei
name: Fujii, Yuka
name: He, Jinping
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Direct-imaging spectra hold rich information about a planet's atmosphere and surface, and several space-based missions aiming at such observations will become a reality in the near future. Previous spectral retrieval works have resulted in key atmospheric constraints under the assumption of a gray surface, but the effect of wavelength-dependent surface albedo on retrieval has not been shown. We explore the influence of the coupling effect of cloud and wavelength-dependent surface albedo on retrieval performance via modeling suites of Earth-like atmospheres with varying cloud and surface albedo parameterizations. Under the assumption of known cloud scattering properties, the surface spectral albedos can be reasonably recovered when the surface cover represents that of Earth-like vegetation or ocean, which may aid in characterizing the planet's habitability. When the cloud scattering properties cannot be assumed, we show that the degeneracy between the cloud properties and wavelength-dependent surface albedo leads to biased results of atmospheric and cloud properties. The multi-epoch visible band observations offer limited improvement in disentangling this degeneracy. However, the constraints on atmospheric properties from the combination of UV band (R $\sim 6$) $+$ visible band (R $\sim 140$) are consistent with input values to within 1 $σ$. If short bandpass data is not available, an alternative solution to reduce the retrieval uncertainties would be to have the prior constraints on planetary cloud fraction with less than 20% uncertainty.
Additional file 1 of Effect of exercise-based cancer rehabilitation via telehealth: a systematic review and meta-analysis
Creators: name: Batalik, Ladislav
name: Chamradova, Katerina
name: Winnige, Petr
name: Dosbaba, Filip
name: Batalikova, Katerina
name: Vlazna, Daniela
name: Janikova, Andrea
name: Pepera, Garyfallia
name: Abu-Odah, Hammoda
name: Su, Jing Jing
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Supplementary Material 1.
Additional file 1 of International study to develop a patient-reported outcome measure to evaluate outcomes of gender-affirming care - the GENDER-Q
Creators: name: Kaur, Manraj N.
name: Morrison, Shane D.
name: Kennedy, Shelby L.
name: van de Grift, Tim C.
name: Højgaard, Astrid
name: Jacobsen, Amalie Lind
name: Johnson, Natasha
name: Mullender, Margriet G.
name: Poulsen, Lotte
name: Satterwhite, Thomas
name: Santucci, Richard
name: Semple, John
name: Rae, Charlene
name: Savard, Kinusan
name: Sørensen, Jens Ahm
name: Young-Afat, Danny
name: Pusic, Andrea L.
name: Klassen, Anne F.
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biotechnology
Developmental Biology
Science Policy

description: Supplementary Material 1
sj-docx-1-pie-10.1177_09544089211037116 - Supplemental material for A review study on the performance of a parabolic trough receiver using twisted tape inserts
Creators: name: Thapa, Sashank
name: Samir, Sushant
name: Kumar, Khushmeet
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, sj-docx-1-pie-10.1177_09544089211037116 for A review study on the performance of a parabolic trough receiver using twisted tape inserts by Sashank Thapa, Sushant Samir and Khushmeet Kumar in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
Spin-glass-like behaviour in SmFeAsO0.8F0.2
Creators: name: Zhigadlo, Nikolai D.
name: Puzniak, Roman
Publisher: name: arXiv
Year: 2022
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The iron-based oxypnictide superconductor SmFeAsO0.8F0.2 was synthesized under high-pressure and investigated by measuring dc magnetic susceptibility. The zero-field cooled (ZFC) magnetic susceptibility confirmed the bulk superconductivity of the sample with a critical temperature of Tc = 50 K and a significant jump in the magnetization at 4.3 K, usually attributed to the antiferromagnetic ordering of Sm3+ ions in this system. Since the occurrence of the jump depends on the cooling history, our data strongly suggest a spin-glass-like behaviour.
Der Augustiner Felice Milensio als päpstlicher Berichterstatter am Regensburger Reichstag des Jahres 1698
Creators: name: Piper, Anton
Publisher: name: Römische Quartalschrift
Year: 1970

description: Römische Quartalschrift, Bd. 5 (1891): Römische Quartalschrift, Band 5
sj-docx-1-pie-10.1177_09544089211042524 - Supplemental material for An experimental study on design and performance of a waste heat recovery system with a thermoelectric generator to be used in exhaust systems of motorcycle engines
Creators: name: Kunt, M. Akif
name: Gunes, Haluk
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, sj-docx-1-pie-10.1177_09544089211042524 for An experimental study on design and performance of a waste heat recovery system with a thermoelectric generator to be used in exhaust systems of motorcycle engines by M. Akif Kunt and Haluk Gunes in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
Supplemental Material, sj-pdf-1-aje-10.1177_1098214020977692 - Statistical Power for Detecting Moderation in Partially Nested Designs
Creators: name: Cox, Kyle
name: Kelcey, Benjamin
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160807 Sociological Methodology and Research Methods
subject: FOS: Sociology

description: Supplemental Material, sj-pdf-1-aje-10.1177_1098214020977692 for Statistical Power for Detecting Moderation in Partially Nested Designs by Kyle Cox and Benjamin Kelcey in American Journal of Evaluation
Supplemental Material - Post-Communist Junctures, the Left, and Illiberalism: Theory with Evidence from Central and Eastern Europe
Creators: name: Binev, Binio S.
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: Supplemental Material for Post-Communist Junctures, the Left, and Illiberalism: Theory with Evidence from Central and Eastern Europe by Binio Binev in Comparative Political Studies
Nucleon and $Δ$ resonances in $γn \to K^+Σ^-$ photoproduction
Creators: name: Wei, Neng-Chang
name: Wang, Ai-Chao
name: Huang, Fei
name: Nakayama, Kanzo
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The most recent data on beam asymmetries, $Σ$, and beam-target asymmetries, $E$, from the CLAS Collaboration, together with the previous data on differential cross sections and beam asymmetries from the CLAS and LEPS Collaborations, for the $γn \to K^+Σ^-$ reaction are studied based on an effective Lagrangian approach in the tree-level Born approximation. The $t$-channel $K$ and $K^\ast(892)$ exchanges, the $u$-channel $Σ$ exchange, the interaction current, and the exchanges of $N$, $Δ$, and their excited states in the $s$ channel are considered in constructing the reaction amplitudes to describe the available experimental data. The reaction mechanisms of $γn \to K^+Σ^-$ are analyzed, and the associated resonances' parameters are extracted. The numerical results show that the $Δ$ exchange and the $N(1710)1/2^+$, $N(1880)1/2^+$, $N(1900)3/2^+$, and $Δ(1920)3/2^+$ resonance exchanges in the $s$-channel dominate the $γn \to K^+Σ^-$ reaction in the lower energy region, and the $t$-channel $K^\ast(892)$ exchange plays a crucial role at forward angles in the higher energy region.
description: To be published in Physical Review D; 11 pages, 5 figures
SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve
Creators: name: Zhang, Xinghan
name: Wang, Xiaofeng
name: Sai, Hanna
name: Mo, Jun
name: Nagy, A. P.
name: Zhang, Jicheng
name: Cai, Yongzhi
name: Lin, Han
name: Zhang, Jujia
name: Baron, E.
name: DerKacy, J. M.
name: Zhang, T. -M.
name: Li, Zhitong
name: Graham, Melissa
name: Huang, F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present multi-band photometric and spectroscopic observations of the type II supernova, (SN) 2019va, which shows an unusually flat plateau-phase evolution in its V-band light curve. Its pseudo-bolometric light curve even shows a weak brightening towards the end of the plateau phase. These uncommon features are related to the influence of 56Ni decay on the light curve during the plateau phase, when the SN emission is usually dominated by cooling of the envelope. The inferred 56Ni mass of SN 2019va is 0.088+/-0.018 solar mass, which is significantly larger than most SNe II. To estimate the influence of 56Ni decay on the plateau-phase light curve, we calculate the ratio (dubbed as eta_Ni) between the integrated time-weighted energy from 56Ni decay and that from envelope cooling within the plateau phase, obtaining a value of 0.8 for SN 2019va, which is the second largest value among SNe II that have been measured. After removing the influence of 56Ni decay on the plateau-phase light curve, we found that the progenitor/explosion parameters derived for SN 2019va are more reasonable. In addition, SN 2019va is found to have weaker metal lines in its spectra compared to other SNe IIP at similar epochs, implying a low-metallicity progenitor, which is consistent with the metal-poor environment inferred from the host-galaxy spectrum. We further discuss the possible reasons that might lead to SN 2019va-like events.
description: 19 pages, 16 figures, accepted by MNRAS
sj-pdf-1-opp-10.1177_10781552221114073 - Supplemental material for Pinnae and facial hypertrichosis induced by cetuximab
Creators: name: Alexandris, Dimitrios
name: Alevizopoulos, Nektarios
name: Palamaris, Kostas
name: Gakiopoulou, Charikleia
name: Theocharis, Stamatios
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111299 Oncology and Carcinogenesis not elsewhere classified
subject: FOS: Clinical medicine
subject: 111599 Pharmacology and Pharmaceutical Sciences not elsewhere classified

description: Supplemental material, sj-pdf-1-opp-10.1177_10781552221114073 for Pinnae and facial hypertrichosis induced by cetuximab by Dimitrios Alexandris, Nektarios Alevizopoulos, Kostas Palamaris, Charikleia Gakiopoulou and Stamatios Theocharis in Journal of Oncology Pharmacy Practice
title: Isotopic evidence (δ¹³C, δ³⁷Cl, δ²H) for distinct transformation mechanisms of chloroform: Catalyzed H₂-water system vs. zero-valent iron (ZVI)
Creators: name: Asfaw, Berhane Abrha
name: Sakaguchi-Söder, Kaori
name: Schiedek, Thomas
name: Michelsen, Nils
name: Bernstein, Anat
name: Siebner, Hagar
name: Schüth, Christoph
Publisher: name: Elsevier
Year: 2024

description: Catalytic hydrodechlorination is an efficient technology for degrading organochlorinated compounds, such as chloroform (CF), into harmless products. Compound-specific stable isotope analysis (CSIA) of multiple elements is widely used for the investigation of degradation mechanisms. Yet, its application in the study of catalytic hydrodechlorination is still limited. We have applied CSIA to derive chlorine, carbon, and hydrogen isotope enrichment factors (ε) during the degradation of CF over Pd/Al₂O₃ and over Rh/Al₂O₃. In addition, the enrichment factors for the same isotopes were derived for the reaction of CF with zero-valent iron (ZVI) for comparison. For the reactions of CF over Pd/Al₂O₃ and Rh/Al₂O₃, εC values (−21.9±0.25 ‰ and −23.4±2.3 ‰) and εCl values (−12.1±1.7 ‰ and −10.3±0.6 ‰) were determined, respectively. The corresponding εC and εCl values, for the dechlorination of CF with ZVI were −22.2±2.8 ‰ and −4.7±0.45 ‰, respectively. The apparent kinetic isotope effects (AKIE) of Cl suggest that the transformation mechanism in the catalyzed hydrogen-water system is a non-concerted reaction, unlike the known reductive dechlorination of CF with ZVI. Moreover, dual-isotope slopes (ΛC/Cl) for both catalyzed reactions (ΛPd = 1.8±0.13 and ΛRh = 2.1±0.14) are markedly different than for the ZVI (ΛZVI = 5.8±0.41), reflecting that the reactions proceed in different mechanisms. For hydrogen isotopes, while there was no clear trend for the catalyzed reactions, an inverse secondary hydrogen isotope effect was observed for the reaction of CF with ZVI.
Efficient and Automated Inversions of Magnetically-Sensitive Forbidden Coronal Lines: CLEDB -- The Coronal Line Emission DataBase Magnetic Field Inversion Algorithm
Creators: name: Paraschiv, Alin Razvan
name: Judge, Philip Gordon
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present CLEDB, a "single point inversion" algorithm for inferring magnetic parameters using I,Q,U, and V Stokes parameters of forbidden magnetic dipole lines formed in the solar corona. We select lines of interest and construct databases of Stokes parameters for combinations of plasma thermal and magnetic configurations. The size and complexity of such databases are drastically reduced by taking advantage of symmetries. Using wavelength-integrated line profiles, each of which might be decomposed beforehand into several line-of-sight components, we search for nearest matches to observed Stokes parameters computed for the elongation corresponding to the observed region. The method is intended to be applied to two or more lines observed simultaneously. The solutions initially yield magnetic orientation, thermal properties, and the spatial position of the emitting plasma in three dimensions. Multiple possible solutions for each observation are returned, including irreducible degeneracies, where usually sets of two solutions are compatible with the two input I,Q,U, and V measurements. In solving for the scattering geometry, this method avoids an additional degeneracy pointed out by Dima & Schad (2020). The magnetic field strength is separately derived from the simple ratio of observed to database Stokes V data, after the thermal properties and scattering geometry solutions have been determined.
description: Solar Physics, accepted for publication. 19 pages, 7 Figures, and 3 Tables
The Study of Biofield Energy Treatment Based Herbomineral Formulation in Skin Health and Function
Creators: name: Nayak, Gopal
Publisher: name: SMN - The ScienceMedia Network
Year: 2017
Subjects: Natural Sciences
Chemistry

description: The aim of the study was to evaluate the effect of the The Trivedi Effect®- Consciousness Energy Healing Treatment based new proprietary herbomineral formulation and cell medium (DMEM) on various skin health parameters using HFF-1, HaCaT, and B16-F10 cell lines. It contained minerals (zinc chloride, sodium selenate, and sodium molybdate), L-ascorbic acid, along with the mixture of Centella asiatica extract and tetrahydrocurcumin (THC). The test formulation and DMEM were divided into two parts each, one part of each was coded as untreated (UT), while the second part of each was treated with the Biofield Treatment by Johanne Dodon and denoted as the Biofield Energy Treated (BT) test items. MTT assay result showed that the test formulation was safe and nontoxic up to 80 µg/mL concentration. The fibroblast cell proliferation assay using BrdU method showed a significant increased cell proliferation at 2.13, 8.75, and 17.53 µg/mL by 3.90%, 14.68% and 29.54%, respectively in the BT-DMEM + BT-Test formulation group compared to the untreated group. The collagen data showed an increased synthesis by 7.42% and 3.84% in the UT-DMEM + BT-Test formulation and BT-DMEM + BT-Test formulation groups, respectively at 0.625 µg/mL with respect to the untreated group. Similarly, the elastin synthesis was increased by 19.8% and 25.8% in the UT-DMEM + BT-Test formulation and BT-DMEM + BT-Test formulation groups, respectively at 5 µg/mL with respect to the untreated group. However, the Biofield Energy Treated test formulation showed an increased level of hyaluronic acid by 1.7% in UT-DMEM + BT-Test formulation group compared to the untreated group. Melanin synthesis inhibition was observed by 15.21% and 11.43% in UT-DMEM + BT-Test Formulation and BT-DMEM + BT-Test Formulation groups, respectively at 0.125 µg/mL compared with the untreated group in B16-F10 melanoma cell line. Anti-wrinkling effects showed an improved cell viability by 7.65% at 1.25 µg/mL in the BT-DMEM + BT-Test formulation experimental group compared with the untreated test group. In addition, the Biofield Energy Treated Test formulation/DMEM showed a significant wound healing activity and high cellular migration of fibroblast and keratinocytes in HFF-1 and HaCaT cells, respectively. Overall, the data suggested that Biofield Treated formulation/DMEM could be helpful for skin healing, improvement the skin health, elasticity, and tightness, as well as, improving skin health issues such as wrinkling, pigmentation disorders, redness, swelling, skin cancer, aging, rashes, and skin sagging.
Revisiting the secondary eclipses of KELT-1b using TESS observations
Creators: name: Eftekhar, Mohammad
name: Abedini, Yousefali
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present the characterization of the transiting planet KELT-1b % ($R_p \simeq 1.15 R_J, M_p \simeq 27.23 M_J $) using data from the Transiting Exoplanet Survey Satellite (TESS). % during cycle $2$ and sector $17$. Our light curve model includes primary transit and secondary eclipse. Here, we model the systematic noise using Gaussian processes (GPs) and fit it to the data using the Markov Chain Monte Carlo (MCMC) method. Modelling of the TESS light curve returns a planet-to-star radius ratio, $p =$ $0.07652_{-0.00028}^{+0.00029}$ and a relatively large secondary eclipse depth of $388_{-13}^{+12}$ ppm. The transit ephemeris of KELT-1b is updated using the MCMC method. Finally, we complement our work by searching for transit timing variations (TTVs) for KELT-1b. We do not find significant variations from the constant-period models in our transit time data.
description: Accepted for publication
sj-pdf-2-tmj-10.1177_03008916231157837 – Supplemental material for Breast implant associated anaplastic large cell lymphoma: Evidence for an efficient diagnostic workup
Creators: name: Vittoria, Laura
name: Sala, Laura
name: Summo, Valeria
name: Capone, Iolanda
name: Conca, Elena
name: Toma, Martina
name: Ottolenghi, Joseph
name: Testa, Francesca
name: Cortinovis, Umberto
name: Paolini, Biagio
name: Cabras, Antonello
name: Aiello, Antonella
name: Bozzi, Fabio
Publisher: name: SAGE Journals
Year: 2023
Subjects: Medicine

description: Supplemental material, sj-pdf-2-tmj-10.1177_03008916231157837 for Breast implant associated anaplastic large cell lymphoma: Evidence for an efficient diagnostic workup by Laura Vittoria, Laura Sala, Valeria Summo, Iolanda Capone, Elena Conca, Martina Toma, Joseph Ottolenghi, Francesca Testa, Umberto Cortinovis, Biagio Paolini, Antonello Cabras, Antonella Aiello and Fabio Bozzi in Tumori Journal
Skin Nourishing Effects of Biofield Energy Healing Treatment Based Herbomineral Formulation
Creators: name: Nayak, Gopal
Publisher: name: SMN - The ScienceMedia Network
Year: 2017
Subjects: Natural Sciences
Chemistry

description: The aim of the present study was undertaken to evaluate the effects of a Consciousness Energy Healing (The Trivedi Effect®) Treatment based test formulation on skin health. The test formulation and DMEM were separated into two parts. One part of each received the Consciousness Energy Healing Treatment by Shirley Theresa Holmlund and were termed as the Biofield Energy Treated samples, while the other parts were considered as the untreated test samples. MTT assay showed more than 70% cells were viable in all the tested concentrations in three cell lines and that the test formulation was safe and nontoxic. The percent cell proliferation using BrdU assay was significantly increased by 343.57%, 100.29%, and 132.6% in the UT-DMEM + BT-Test formulation, BT-DMEM + UT-Test formulation, and BT-DMEM + BT-Test formulation groups, respectively at 8.75 µg/mL compared to the UT-DMEM + UT-Test formulation group. The collagen synthesis was significantly increased by 5.94% and 10.84% in the UT-DMEM + BT-Test formulation and BT-DMEM + BT-Test formulation groups, respectively at 0.625 µg/mL with respect to the untreated group. Elastin level was significantly (p≤0.001) increased by 15.95%, 58.31%, and 47.18% at 2.5 µg/mL in the UT-DMEM + BT-Test formulation, BT-DMEM + UT-Test formulation, and BT-DMEM + BT-Test formulation groups, respectively compared to the untreated group. The level of hyaluronic acid was significantly increased by 15.13% and 68.56% in the BT-DMEM + UT-Test formulation and BT-DMEM + BT-Test formulation groups, respectively at 0.625 µg/mL compared to the untreated group. The level of melanin was significantly reduced by 17.06%, 6.94%, and 13.07% in the UT-DMEM + BT-Test formulation, BT-DMEM + UT-Test formulation, and BT-DMEM + BT-Test formulation groups, respectively at 0.063 µg/mL compared to untreated group. The effect of skin protection upon exposure with UV-B rays displayed some alteration of the percent cell viability in all the tested groups. The wound healing activity by scratch assay exhibited significant wound closure and cell migration in the test formulation and DMEM in HFF-1 cells compared to the untreated group. Altogether, the data suggests that the Consciousness Energy Healing Treated DMEM and test formulation exhibited better skin protective responses compared to the untreated DMEM and test formulation group with respect to the skin health parameters. Therefore, the Biofield Energy Treated test formulation could be developed as a potential cosmetic product against various skin problems viz. eczema, vitiligo, psoriasis, acne, hives, rosacea, ichthyosis, seborrheic dermatitis, erythema, contact dermatitis, skin aging, wrinkles, etc.
Additional file 5 of Co-expression gene module analysis in response to attenuated cercaria vaccine reveals a critical role for NK cells in protection against Schistosoma mansoni
Creators: name: Neto, Almiro Pires da Silva
name: Vitoriano-Souza, Juliana
name: Khouri, Mariana Ivo
name: Favaro, Regiane Degan
name: Wilson, Robert Alan
name: Leite, Luciana Cezar de Cerqueira
name: Ramos, Pablo Ivan Pereira
name: Farias, Leonardo Paiva
Publisher: name: figshare
Year: 2024
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 5: Fig. 3. Cell type prediction using genes from modules M2 (a) and M6 (b) with WebCSEA. Each point in the Jitter plots represents a tissue cell type, with the y-axis indicating the significance of detection as – log10 (combined p-value). The dashed red line represents the Bonferroni-corrected significance cutoff (P = 3.69 × 10–5) across 1355 tissue cell types.
sj-docx-1-pie-10.1177_09544089231165128 - Supplemental material for Casing failure mechanism and slip anchoring optimization of the compression packer in the oil and gas well
Creators: name: Tang, Yang
name: Wang, Jie
name: Zhou, Minghai
name: Li, Guangyao
name: Xiao, Xiao
Publisher: name: SAGE Journals
Year: 2023
Subjects: Engineering not elsewhere classified
Materials Engineering not elsewhere classified

description: Supplemental material, sj-docx-1-pie-10.1177_09544089231165128 for Casing failure mechanism and slip anchoring optimization of the compression packer in the oil and gas well by Yang Tang, Jie Wang, Minghai Zhou, Guangyao Li and Xiao Xiao in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
title: "Ritratto di giovane su busto moderno", Arte romana, inv. LXXVI-bis (ITA/EN)
title: Scheda catalogo digitale Borghese
titleType: AlternativeTitle
Creators: name: Clementi, Jessica
name: Galleria Borghese
Publisher: name: Galleria Borghese
Year: 2024

description: Pubblicazione delle schede delle opere conservate nel museo ed estratte dal catalogo digitale di Galleria Borghese, nelle due versioni esistenti online, in italiano e inglese.

Collegamento al catalogo digitale:

ITA: https://www.collezionegalleriaborghese.it/

EN: https://www.collezionegalleriaborghese.it/en
Additional file 1 of Comparing effectiveness of physiotherapy versus drug management on fatigue, physical functioning, and episodic disability for myalgic encephalomyelitis in post-COVID-19 condition: a study protocol of randomized control trial
Creators: name: Sarker, Altaf Hossain
name: Hossain, K.M. Amran
name: Kabir, Md. Feroz
name: Jahan, Sharmila
name: Hossain, Md. Zahid
name: Hossain, Tofajjal
name: Jahid, Iqbal Kabir
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cancer
Mental Health
Virology

description: Supplementary Material 1.
Stellar and black hole assembly in z<0.3 infrared-luminous mergers: intermittent starbursts vs. super-Eddington accretion
Creators: name: Farrah, Duncan
name: Efstathiou, Andreas
name: Afonso, Jose
name: Bernard-Salas, Jeronimo
name: Cairns, Joe
name: Clements, David L
name: Croker, Kevin
name: Hatziminaoglou, Evanthia
name: Joyce, Maya
name: Lacy, Mark
name: Lebouteiller, Vianney
name: Lieblich, Alix
name: Lonsdale, Carol
name: Oliver, Seb
name: Pearson, Chris
name: Petty, Sara
name: Pitchford, Lura K
name: Rigopoulou, Dimitra
name: Rowan-Robinson, Michael
name: Runburg, Jack
name: Spoon, Henrik
name: Verma, Aprajita
name: Wang, Lingyu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy mergers at z<0.3 by combining results from radiative transfer modelling with archival measures of molecular gas and black hole mass. The ratios of stellar mass, molecular gas mass, and black hole mass to each other are consistent with those of massive gas-rich galaxies at z<0.3. The advanced mergers may show increased black hole mass to stellar mass ratios, consistent with the transition from AGN to ellipticals and implying substantial black hole mass growth over the course of the merger. Star formation rates are enhanced relative to the local main sequence, by factors of ~100 in the starburst and ~1.8 in the host. The starburst star formation rates appear distinct to star formation in the main sequence at all redshifts up to at least z~5. Starbursts may prefer late-stage mergers, but are observed at any merger stage. We do not find evidence that the starbursts in these low-redshift systems substantially increase the total stellar mass, with a soft upper limit on the stellar mass increase from starburst activity of about a factor of two. In contrast, 12 objects show evidence for super-Eddington accretion, associated with late-stage mergers, suggesting that many AGN in infrared-luminous mergers go through a super-Eddington phase. The super-Eddington phase may increase black hole mass by up to an order of magnitude at an accretion efficiency of 42+/-33% over a period of 44+/-22Myr. Our results imply that super-Eddington accretion is an important black hole growth channel in infrared-luminous galaxies at all redshifts.
description: MNRAS Accepted
Geologic context of the bright MARSIS reflectors in Ultimi Scopuli, South Polar Layered Deposits, Mars
Creators: name: Landis, M. E.
name: Whitten, J. L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Radar-bright basal reflectors have been detected below the South Polar Layered Deposits (SPLD), Mars using Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) data and have an exciting but controversial interpretation: liquid water from subglacial lakes. We mapped the surface of the SPLD immediately above and surrounding the putative lakes (1:2M map scale) in order to provide geologic context for interpretation of the bright basal reflectors. We use THEMIS daytime IR (100 m/pixel), CTX (6 m/pixel), and HiRISE (25 cm/pixel) data to characterize geologic units and typical surface roughness. We find evidence for multiple geologic units with features due to CO2 and aeolian-related processes. We do not find evidence for surface modification linked to the postulated lake locations. This is not consistent with the interpretation of the MARSIS basal radar reflector as subglacial lakes.
description: 29 pages, 2 figures (main paper), 4 (supplement), accepted 4/29/2022 at Geophysical Research Letters
On the origin of molecular oxygen on the surface of Ganymede
Creators: name: Migliorini, A.
name: Kanuchova, Z.
name: Ioppolo, S.
name: Barbieri, M.
name: Jones, N. C.
name: Hoffmann, S. V.
name: Strazzulla, G.
name: Tosi, F.
name: Piccioni, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Since its first identification on the surface of Ganymede in 1995, molecular oxygen (O2) ice has been at the center of a scientific debate as the surface temperature of the Jovian moon is on average well above the freezing point of O2. Laboratory evidence suggested that solid O2 may either exist in a cold (<50 K) subsurface layer of the icy surface of Ganymede, or it is in an atmospheric haze of the moon. Alternatively, O2 is constantly replenished at the surface through ion irradiation of water-containing ices. A conclusive answer on the existence of solid O2 on the surface of Ganymede is hampered by the lack of detailed, extensive observational datasets. We present new ground-based, high-resolution spectroscopic observations of Ganymede's surface obtained at the Telescopio Nazionale Galileo. These are combined with dedicated laboratory measurements of ultraviolet-visible (UV-vis) photoabsorption spectra of O2 ice, both pure and mixed with other species of potential interest for the Galilean satellites. Our study confirms that the two bands identified in the visible spectra of Ganymede's surface are due to the (1,0) and (0,0) transition bands of O2 ice. Oxygen-rich ice mixtures including water (H2O) and carbon dioxide (CO2) can reproduce observational reflectance data of the Ganymede's surface better than pure O2 ice in the temperature range 20-35 K. Solid H2O and CO2 also provide an environment where O2 ice can be trapped at higher temperatures than its pure ice desorption under vacuum space conditions. Our experiments at different temperatures show also that the (1,0)/(0,0) ratio in case of the CO2:O2=1:2 ice mixture at 35 K has the closest value to observations, while at 30 K the (1,0)/(0,0) ratio seems to be mixture independent with the exception of the N2:O2=1:2 ice mixture. The present work will support the ESA/JUICE mission to the Jovian system.
description: Accepted for publication in Icarus