cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
Creators: name: Ansarinejad, B.
name: Murphy, D. N. A.
name: Shanks, T.
name: Metcalfe, N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Taking advantage of $\sim4700$ deg$^2$ optical coverage of the Southern sky offered by the VST ATLAS survey, we construct a new catalogue of photometrically selected galaxy groups and clusters using the {\sc orca} cluster detection algorithm. The catalogue contains $\sim 22,000$ detections with $N_{200}>10$ and $\sim9,000$ with $N_{200}>20$. We estimate the photometric redshifts of the clusters using machine learning and find the redshift distribution of the sample to extend to $z\sim0.7$, peaking at $z\sim0.25$. We calibrate the ATLAS cluster mass-richness scaling relation using masses from the MCXC, Planck, ACT DR5 and SDSS redMaPPer cluster samples. We estimate the ATLAS sample to be $>95\%$ complete and $>85\%$ pure at $z<0.35$ and in the $M_{\rm 200m}$>$1\times10^{14}h^{-1}{\rm M}_\odot$ mass range. At $z<0.35$, we also find the ATLAS sample to be more complete than redMaPPer, recovering a $\sim40\%$ higher fraction of Abell clusters. This higher sample completeness places the amplitude of the $z<0.35$ ATLAS cluster mass function closer to the predictions of a $Λ$CDM model with parameters based on the Planck CMB analyses, compared to the mass functions of the other cluster samples. However, strong tensions between the observed ATLAS mass functions and models remain. We shall present a detailed cosmological analysis of the ATLAS cluster mass functions in paper II. In the future, optical counterparts to X-ray-detected eROSITA clusters can be identified using the ATLAS sample. The catalogue is also well suited for auxiliary spectroscopic target selection in 4MOST. The ATLAS cluster catalogue is publicly available at http://astro.dur.ac.uk/cosmology/vstatlas/cluster_catalogue/.
description: 21 pages, 17 figures. v2 contains moderate revisions in response to the MNRAS referee report. In addition, cluster galaxy magnitudes have now been added to the updated catalogue. The updated manuscript has been re-submitted to MNRAS
The formation of the W43 complex: constraining its atomic-to-molecular transition and searching for colliding clouds
Creators: name: Bontemps, S.
name: Glover, S.
name: Heitsch, F.
name: Beuther, H.
name: Didelon, P.
name: Carlhoff, P.
name: Schneider, N.
name: Motte, F.
name: Louvet, F.
name: Nguyên Luong, Q.
name: Hennemann, M.
name: Hill, T.
name: Schilke, P.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: Context. Numerical simulations have explored the possibility of forming molecular clouds through either a quasi-static, self-gravitating mechanism or the collision of gas streams or lower density clouds. They also quantitatively predict the distribution of matter at the transition from atomic to molecular gases.
Sparse Ellipsometry: Portable Acquisition of Polarimetric SVBRDF and Shape with Unstructured Flash Photography
Creators: name: Hwang, Inseung
name: Jeon, Daniel S.
name: Muñoz, Adolfo
name: Gutierrez, Diego
name: Tong, Xin
name: Kim, Min H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Graphics (cs.GR)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Ellipsometry techniques allow to measure polarization information of materials, requiring precise rotations of optical components with different configurations of lights and sensors. This results in cumbersome capture devices, carefully calibrated in lab conditions, and in very long acquisition times, usually in the order of a few days per object. Recent techniques allow to capture polarimetric spatially-varying reflectance information, but limited to a single view, or to cover all view directions, but limited to spherical objects made of a single homogeneous material. We present sparse ellipsometry, a portable polarimetric acquisition method that captures both polarimetric SVBRDF and 3D shape simultaneously. Our handheld device consists of off-the-shelf, fixed optical components. Instead of days, the total acquisition time varies between twenty and thirty minutes per object. We develop a complete polarimetric SVBRDF model that includes diffuse and specular components, as well as single scattering, and devise a novel polarimetric inverse rendering algorithm with data augmentation of specular reflection samples via generative modeling. Our results show a strong agreement with a recent ground-truth dataset of captured polarimetric BRDFs of real-world objects.
Additional file 2 of Debriefing interaction patterns and learning outcomes in simulation: an observational mixed-methods network study
Creators: name: Abegglen, Sandra
name: Greif, Robert
name: Balmer, Yves
name: Znoj, Hans Joerg
name: Nabecker, Sabine
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Network metrics and dyad census for the different interaction patterns.
Descargar PDF LA NOCHE SEXUAL
Creators: name: Mckinney
Publisher: name: Zenodo
Year: 2024

description: LA NOCHE SEXUAL de PASCAL QUIGNARD

Descargar eBook gratis ➡ Link

Ficha técnica

LA NOCHE SEXUAL

PASCAL QUIGNARD

Número de páginas: 227

Idioma: CASTELLANO

Formatos: Pdf, ePub, MOBI, FB2

ISBN: 9788494302640

Editorial: FUNAMBULISTA

Año de edición: 2014

 

 

 

 

 

Descargar libros electrónicos para nook gratis LA NOCHE SEXUAL 9788494302640

 

Overview

«Cuando en el silencio de la noche sondamos las profundidades del corazón la indigencia de las imágenes que nos hemos formado sobre el gozo nos llena de vergüenza.Yo no estaba allí la noche de mi concepción.Es difícil asistir al día que nos precede.Una imagen falta en el alma. Dependemos de una postura que tuvo lugar necesariamente pero que nunca se nos revelará. A esta imagen que falta la llamamos «el origen. La buscamos detrás de todo lo que vemos. Y a esta falta que arrastran los días la llamamos «el destino. La buscamos detrás de todo lo que vivimos. Es allí donde acaban perdiéndose los gestos que repetimos inadvertidamente, las mismas palabras que fallan.Mi intención es dar un paso más hacia el origen del espanto que sienten los hombres cuando piensan en lo que fueron antes de que su cuerpo proyectara una sombra en este mundo. Si tras la fascinación está la imagen que falta, tras la imagen que falta, hay algo más: la noche. (Pascal Quignard, Nota preliminar)
Additional file 3 of Debriefing interaction patterns and learning outcomes in simulation: an observational mixed-methods network study
Creators: name: Abegglen, Sandra
name: Greif, Robert
name: Balmer, Yves
name: Znoj, Hans Joerg
name: Nabecker, Sabine
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3. All network structures Pattern 1: Fan.
Generation and delivery of free hydroxyl radicals using a remote plasma
Creators: name: McQuaid, Harold
name: Rutherford, David
name: Mariotti, Davide
name: Maguire, Paul
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We demonstrate a new gas-based OH generation source using a low power RF-driven atmospheric pressure plasma configured to deliver the radical flux into the far effluent region, well away from interference from other plasma factors such as electric fields, currents, and UV radiation. Using He-H2O gas chemistry isolated from the laboratory air, the plasma generated flux consists of H2O2 and OH, varying with H2O vapour content and absorbed power density. Peak flux values were 2.3 nmol s-1 and 0.23 nmol s-1 for H2O2 and OH respectively at a distance of 50 mm from the plasma, with 790 ppmv H2O and a power density of 1E8 W m-3. The maximum OH flux density was 4.5 x 1E19 m-2 s-1 falling to 1.7 x 1E19 m-2 s-1 at 110 mm, equivalent to generation rates of 74 uM s-1 and 28 uM s-1. Despite high OH recombination rates at the plasma exit, the escaping flux is still significant, indicating a viable delivery capability to downstream targets. Its performance with regard to OH generation rates compares well with traditional OH generation techniques such as radiolysis, advanced oxidation processes and enhanced Fenton-chemistry approaches where OH production rates are sub-uM s-1. Delivering precisely quantifiable OH fluxes provides new opportunities for scientific studies and technological opportunities in cell biology, atmospheric chemistry, protein unfolding and systematic dose studies for plasma-based and other OH related potential medical treatments.
description: 19 pages, 7 figures, 88 references
(3069) Joshua Nicholson
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
LA LIBRERÍA DE LOS CORAZONES ROTOS leer epub PETRA HULSMANN
Creators: name: Gordon
Publisher: name: Zenodo
Year: 2024

description: LA LIBRERÍA DE LOS CORAZONES ROTOS de PETRA HULSMANN

Descargar eBook gratis ➡ Link

Ficha técnica

LA LIBRERÍA DE LOS CORAZONES ROTOS

PETRA HULSMANN

Número de páginas: 432

Idioma: CASTELLANO

Formatos: Pdf, ePub, MOBI, FB2

ISBN: 9788416673698

Editorial: CATEDRAL

Año de edición: 2018

 

 

 

 

 

Descarga gratuita de libros electrónicos para teléfonos móviles. LA LIBRERÍA DE LOS CORAZONES ROTOS

 

Overview

Lena está a punto de cumplir treinta años, su novio la planta justo antes de la boda, y al cabo de poco, la despiden del trabajo a causa de un embarazoso error. Pero decide no rendirse, y se refugia en el piso compartido en el que vive su hermano Michel, la novia de este, Juli (que es a su vez la mejor amiga de Lena), y Ben, un viejo amigo de su hermano. A la espera de encontrar algo mejor, acepta un trabajo provisional en una librería, y va apareciendo gente nueva en su vida como Otto, el anciano y arisco librero, o Jan, un estudiante apasionado de la literatura que se gana la vida sirviendo copas. Lena sigue siendo un desastre, pero esta vorágine de cambios puede que la ayude a encontrarse a sí misma. Y tal vez, también, al amor de su vida
Searches for dark matter signals in simplified models at future hadron colliders
Creators: name: Xiang, Qian-Fei
name: Bi, Xiao-Jun
name: Yin, Peng-Fei
name: Yu, Zhao-Huan
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the prospect of dark matter (DM) searches in the monojet channel at future $pp$ colliders with center-of-mass energies of 33, 50, and 100~TeV. We consider a class of simplified models in which a vector boson connecting DM particles to quarks is introduced. Comparing with studies in the effective field theory, the present framework gives more reasonable production rates and kinematics of the DM signatures. We estimate the sensitivities of future colliders with an integrated luminosity of 3 $ab^{-1}$ to the DM-induced monojet signature and show the parameter space that can be explored. The constraints from direct and indirect DM detection experiments are compared with the future collider sensitivities. We find that the future collider detection will be much more sensitive than the indirect detection for the vector interaction, and have better sensitivities than those of the direct detection by several orders of magnitude for the axial vector interaction.
description: 24 papes, 6 figures
An eclipsing post common-envelope system consisting of a pulsating hot subdwarf B star and a brown dwarf companion
Creators: name: Drechsel, H.
name: Barlow, B. N.
name: Dunlap, B. H.
name: Schaffenroth, V.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2015

description: Hot subdwarf B stars (sdBs) are evolved, core helium-burning objects located on the extreme horizontal branch. Their formation history is still puzzling as the sdB progenitors must lose nearly all of their hydrogen envelope during the red-giant phase. About half of the known sdBs are in close binaries with periods from 1.2 h to a few days, a fact that implies they experienced a common-envelope phase. Eclipsing hot subdwarf binaries (also called HW Virginis systems) are rare but important objects for determining fundamental stellar parameters. Even more significant and uncommon are those binaries containing a pulsating sdB, as the mass can be determined independently by asteroseismology. Here we present a first analysis of the eclipsing hot subdwarf binary V2008-1753. The light curve shows a total eclipse, a prominent reflection effect, and low--amplitude pulsations with periods from 150 to 180 s. An analysis of the light-- and radial velocity (RV) curves indicates a mass ratio close to $ q = 0.146$, an RV semi-amplitude of $K=54.6 \,\rm kms^{-1}$, and an inclination of $i=86.8^\circ$. Combining these results with our spectroscopic determination of the surface gravity, $\log \,g = 5.83$, the best--fitting model yields an sdB mass of 0.47$M_{\rm \odot}$ and a companion mass of $69 M_{\rm Jup}$. As the latter mass is below the hydrogen-burning limit, V2008-1753 represents the first HW Vir system known consisting of a pulsating sdB and a brown dwarf companion. Consequently, it holds great potential for better constraining models of sdB binary evolution and asteroseismology.
Additional file 4 of Debriefing interaction patterns and learning outcomes in simulation: an observational mixed-methods network study
Creators: name: Abegglen, Sandra
name: Greif, Robert
name: Balmer, Yves
name: Znoj, Hans Joerg
name: Nabecker, Sabine
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 4. All network structures Pattern 2: Triangle.
Relaxation approximation of Friedrich's systems under convex constraints
Creators: name: Babadjian, Jean-François
name: Mifsud, Clément
name: Seguin, Nicolas
Publisher: name: arXiv
Year: 2015
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: This paper is devoted to present an approximation of a Cauchy problem for Friedrichs' systems under convex constraints. It is proved the strong convergence in L^2\_{loc} of a parabolic-relaxed approximation towards the unique constrained solution.
(3071) Arthur Nicholson
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Supplementary Information from A dynamically diluted alignment model reveals the impact of cell turnover on the plasticity of tissue polarity patterns.
Creators: name: Hoffmann, Karl B.
name: Voss–Böhme, Anja
name: Rink, Jochen C.
name: Brusch, Lutz
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: 10202 Biological Mathematics
subject: FOS: Mathematics
subject: Computational Biology
subject: 60114 Systems Biology
subject: FOS: Biological sciences

description: Supplementary Information to Hoffmann, Voss-Böhme, Rink and Brusch 2017: “A Dynamically Diluted Alignment Model Reveals the Impact of Cell Turnover on the Plasticity of Tissue Polarity Patterns” with detailed derivations of equations that are used in the main text, a table summarising all variable names and notations and additional results in 7 supplementary figures: Fig.S1, Lattice size effects. Fig.S2, Effects of de-novo polarisation rate beta on the time of minimal order. Fig.S3, Statistical robustness of time of minimal order. Fig.S4, Bistability of mean-field ODE system for very high neighbour coupling strength. Fig.S5, Time of minimal order for vanishing neighbour coupling strength. Fig.S6, Time of minimal order collapses to linear function of the effective neighbour coupling strength. Fig.S7, Effects of coupling strength to global signal epsilon_s on the time of minimal order.
Rel leaves of the Arnoux-Yoccoz surfaces
Creators: name: Hooper, W. Patrick
name: Weiss, Barak
Publisher: name: arXiv
Year: 2015
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 37Exx

description: We analyze the rel leaves of the Arnoux-Yoccoz translation surfaces. We show that for any genus $g \geq 3$, the leaf is dense in the connected component of the stratum $H(g -1 , g -1)$ to which it belongs, and the one-sided imaginary-rel trajectory of the surface is divergent. For one surface on this trajectory, namely the Arnoux-Yoccoz surface itself, the horizontal foliation is invariant under a pseudo-Anosov map (and in particular is uniquely ergodic), but for all other surfaces, the horizontal foliation is completely periodic. The appendix proves a field theoretic result needed for denseness of the leaf: for any $n \geq 3$, the field extension of the rationals obtained by adjoining a root of $X^n-X^{n-1}-\ldots-X-1$ has no totally real subfields other than the rationals.
description: Appendix by Lior Bary-Soroker, Mark Shusterman and Umberto Zannier. The prior version was published, but had errors in \S 6. Erroneous statements have been indicated and an erratum was included as Appendix B which corrects the errors. Main results are still correct. 70 pages, 9 figures. arXiv admin note: text overlap with arXiv:1506.06773
Additional file 5 of Debriefing interaction patterns and learning outcomes in simulation: an observational mixed-methods network study
Creators: name: Abegglen, Sandra
name: Greif, Robert
name: Balmer, Yves
name: Znoj, Hans Joerg
name: Nabecker, Sabine
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 5. All network structures Pattern 3: Net.
Evidence of coupling between the thermal and nonthermal emission in the gamma-ray binary LS I +61 303
Creators: name: Ribó, M.
name: Casares, J.
name: Núñez, J.
name: Fors, O.
name: Paredes-Fortuny, X.
name: Bosch-Ramon, V.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2015

description: The gamma-ray binary LS I +61 303 is composed of a Be star and a compact companion orbiting in an eccentric orbit. Variable flux modulated with the orbital period of ~26.5 d has been detected from radio to very high-energy gamma rays. In addition, the system presents a superorbital variability of the phase and amplitude of the radio outburst with a period of ~4.6 yr. We present optical photometric observations of LS I +61 303 spanning ~1.5 yr and contemporaneous Halpha equivalent width (EW Halpha) data. The optical photometry shows, for the first time, that the known orbital modulation suffers a positive orbital phase shift and an increase in flux for data obtained 1-yr apart. This behavior is similar to that already known at radio wavelengths, indicating that the optical flux follows the superorbital variability as well. The orbital modulation of the EW Halpha presents the already known superorbital flux variability but shows, also for the first time, a positive orbital phase shift. In addition, the optical photometry exhibits a lag of ~0.1-0.2 in orbital phase with respect to the EW Halpha measurements at similar superorbital phases, and presents a lag of ~0.1 and ~0.3 orbital phases with respect noncontemperaneous radio and X-ray outbursts, respectively. The phase shifts detected in the orbital modulation of thermal indicators, such as the optical flux and the EW Halpha, are in line with the observed behavior for nonthermal indicators, such as X-ray or radio emission. This shows that there is a strong coupling between the thermal and nonthermal emission processes in the gamma-ray binary LS I +61 303. The orbital phase lag between the optical flux and the EW Halpha is naturally explained considering different emitting regions in the circumstellar disk, whereas the secular evolution might be caused by the presence of a moving one-armed spiral density wave in the disk.
Effective field theory of magnetogenesis identify necessary and sufficient conditions
Creators: name: Kushwaha, Ashu
name: Naskar, Abhishek
name: Nandi, Debottam
name: Shankaranarayanan, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: At astrophysical and cosmological scales, there is a detectable amount of magnetic field. There are several probable origins for this observed magnetic field, including the possibility of its origin in the early Universe. There are several models for primordial magnetogenesis, and if the inflationary background is taken into account, broken conformal invariance is required to generate a sufficient amount of magnetic field. The breaking of conformal invariance is introduced either by new couplings between electromagnetic field and inflaton field or including higher derivative terms to the theory. As a step to unify these different approaches in the literature, we propose an Effective Field Theory (EFT) approach based on expansion about the Hubble parameter $(H)$ and its derivatives, where EFT parameters describe the magnetogenesis scenario in the early Universe, and different choices of parameters correspond to different models. We explicitly show that the generation of primordial magnetic fields requires two necessary conditions -- conformal invariance breaking and causal propagation. While broken conformal invariance is a common requirement for primordial magnetogenesis, for the first time, we show that causal propagation is also a necessary condition. We confirm this by considering a specific model of primordial magnetogenesis.
description: V2: 35 pages, 2 figures, added two appendices, version accepted in JCAP
I Could Never Be a Succubus! Volume 2 by Nora Kohigashi, Wasabi, Roy Nukia on Audiobook New
Creators: name: Steffes
Publisher: name: Zenodo
Year: 2024

description: I Could Never Be a Succubus! Volume 2 by Nora Kohigashi, Wasabi, Roy Nukia

 

 

Download Book ➡ Link

Read Book Online ➡ Link

 

 

I Could Never Be a Succubus! Volume 2

Nora Kohigashi, Wasabi, Roy Nukia

Page: 250

Format: pdf, ePub, mobi, fb2

ISBN: 9781718336629

Publisher: J-Novel Club

 

Download ebook for kindle I Could Never Be a Succubus! Volume 2 English version PDB

MARK OF THE SUCCUBUS GN VOLUME 2 (OF 3) She now has a choice to save her first target or defy demon law! If she tries to bend the Rules, there may be a chance that neither of them will survive. Thoughts on I'm Not a Succubus! Volume 2 - Rory Muses Feb 13, 2023 — Chapter 2 - being a Succubus in a new world Souma was lucky enough to have been chosen as someon action adventure demon ecchi fantasy femaleprotagonist genderbender goddess isekai  I Could Never Be a Succubus! [Light Novel] | Series SeriesI Could Never Be a Succubus! [Light Novel] Series author: Nora Kohigashi. 2 Works Popularity 178,643 (2 Members) 3 Books 0 Reviews [Light Novel] Volume  I'm Not a Succubus! Vol. 2 - Horitomo Jan 31, 2023 — I Am Not A Succubus Manga Volume 2 (Mature) ever-ready sex demon, or her days at the academy could be numbered! I Am Not A Succubus Manga Volume 2 (Mature). Publisher Seven Seas Entertainment LLC; Genre  I'm Not a Succubus! Vol. 2 (Paperback) Jan 31, 2023 — I'm Not a Succubus!. Vol. 2 riding practice, or helping a horny harpy lay an egg, Sakura has to be the hands-on ever-ready sex demon, or her days at the academy could be numbered! I Could Never Be a Succubus! Volume 2 - Nora Kohigashi In the midst of a battle with a demon lord, Liz lost her memories and succubus powers, but somehow her reunion with the great hero Cain has caused something to  Saki the Succubus Hungers Tonight Manga Volume 2 She cooks, she cleans, and she's the cutest thing he's ever seen! Unfortunately, roommate Saki is a succubus who emits aphrodisiac pheromones that drive him  I'm Not a Succubus! Vol. 2 (Paperback) Jan 31, 2023 — I Could Never Be a Succubus! Volume 2 eBook In the midst of a battle with a demon lord, Liz lost her memories and succubus powers, but somehow her reunion with the great hero Cain has caused something to
THOR: The H i, OH, Recombination line survey of the Milky Way: The pilot study: H i observations of the giant molecular cloud W43⋆
Creators: name: Bihr, S.
name: Hughes, A.
name: Walsh, A. J.
name: Johnston, K. G.
name: Urquhart, J. S.
name: Klessen, R. S.
name: Henning, T.
name: Menten, K. M.
name: Smith, R. J.
name: Schilke, P.
name: Anderson, L. D.
name: Glover, S. C.O.
name: Ott, J.
name: Bigiel, F.
name: Heyer, M. H.
name: Heitsch, F.
name: Churchwell, E.
name: Linz, H.
name: Beuther, H.
name: Motte, F.
name: Goldsmith, P. F.
name: Plume, R.
name: Schneider, N.
name: Nguyen-Luong, Q.
name: Walter, F.
name: Ragan, S. E.
name: Carlhoff, P.
name: Brunthaler, A.
name: Longmore, S. N.
name: Hill, T.
name: Roy, N.
name: Stil, J. M.
name: McClure-Griffiths, N. M.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2015

description: To study the atomic, molecular and ionized emission of Giant Molecular Clouds (GMCs), we have initiated a Large Program with the VLA: 'THOR - The HI, OH, Recombination Line survey of the Milky Way'. We map the 21cm HI line, 4 OH lines, 19 H_alpha recombination lines and the continuum from 1 to 2 GHz of a significant fraction of the Milky Way (l=15-67deg, |b|<1deg) at ~20" resolution. In this paper, we focus on the HI emission from the W43 star-formation complex. Classically, the HI 21cm line is treated as optically thin with column densities calculated under this assumption. This might give reasonable results for regions of low-mass star-formation, however, it is not sufficient to describe GMCs. We analyzed strong continuum sources to measure the optical depth, and thus correct the HI 21cm emission for optical depth effects and weak diffuse continuum emission. Hence, we are able to measure the HI mass of W43 more accurately and our analysis reveals a lower limit of M=6.6x10^6 M_sun, which is a factor of 2.4 larger than the mass estimated with the assumption of optically thin emission. The HI column densities are as high as N(HI)~150 M_sun/pc^2 ~ 1.9x10^22 cm^-2, which is an order of magnitude higher than for low mass star formation regions. This result challenges theoretical models that predict a threshold for the HI column density of ~10 M_sun/pc^2, at which the formation of molecular hydrogen should set in. By assuming an elliptical layered structure for W43, we estimate the particle density profiles. While at the cloud edge atomic and molecular hydrogen are well mixed, the center of the cloud is strongly dominated by molecular hydrogen. We do not identify a sharp transition between hydrogen in atomic and molecular form. Our results are an important characterization of the atomic to molecular hydrogen transition in an extreme environment and challenges current theoretical models.
Radio and X-rays From SN 2013df Enlighten Progenitors of Type IIb Supernovae
Creators: name: Kamble, Atish
name: Margutti, Raffaella
name: Soderberg, Alicia M.
name: Chakraborti, Sayan
name: Fransson, Claes
name: Chevalier, Roger
name: Powell, Diana
name: Milisavljevic, Dan
name: Parrent, Jerod
name: Bietenholz, Michael
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present radio and X-ray observations of the nearby Type IIb Supernova 2013df in NGC4414 from 10 to 250 days after the explosion. The radio emission showed a peculiar soft-to-hard spectral evolution. We present a model in which inverse Compton cooling of synchrotron emitting electrons can account for the observed spectral and light curve evolution. A significant mass loss rate, $\dot{M} \approx 8 \times 10^{-5}\,\rm M_{\odot}/yr$ for a wind velocity of 10 km/s, is estimated from the detailed modeling of radio and X-ray emission, which are primarily due to synchrotron and bremsstrahlung, respectively. We show that SN 2013df is similar to SN 1993J in various ways. The shock wave speed of SN 2013df was found to be average among the radio supernovae; $v_{sh}/c \sim 0.07$. We did not find any significant deviation from smooth decline in the light curve of SN 2013df. One of the main results of our self-consistent multiband modeling is the significant deviation from energy equipartition between magnetic fields and relativistic electrons behind the shock. We estimate $ε_{e} = 200 ε_{B}$. In general for Type IIb SNe, we find that the presence of bright optical cooling envelope emission is linked with free-free radio absorption and bright thermal X-ray emission. This finding suggests that more extended progenitors, similar to that of SN 2013df, suffer from substantial mass loss in the years before the supernova.
description: 15 pages, 7 figures, 1 table; Submitted to The Astrophysical Journal
Higgs, Coulomb, and Hall-Littlewood
Creators: name: Kang, Monica Jinwoo
name: Lawrie, Craig
name: Lee, Ki-Hong
name: Sacchi, Matteo
name: Song, Jaewon
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Higgs branch of 4d $\mathcal{N}=2$ SCFTs can be analyzed via the Hilbert series of the Higgs branch or, in special cases, by computing the Hall-Littlewood index. For any class $\mathcal{S}$ theory corresponding to a genus-zero Riemann surface, they are conjectured to be identical. We present several families of counterexamples. We find that for any class $\mathcal{S}$ theory with four or more $\mathbb{Z}_2$-twisted punctures, they do not match. We construct 3d mirrors for such theories and analyze their Coulomb branch Hilbert series to compute the Higgs branch Hilbert series of the 4d theory. We further construct $a=c$ theories in class $\mathcal{S}$ using the twisted punctures, and these theories, which includes the $\hat{D}_4(SU(2n+1))$ theories, have Hall--Littlewood index different from the Hilbert series of the Higgs branch. We conjecture that this is the case for all $a=c$ theories with non-empty Higgs branch, including $\mathcal{N}\ge 3$ SCFTs.
description: 49 pages + appendices + references, 20 figures, and 5 tables
Direct numerical simulations of turbulent jets: vortex-interface-surfactant interactions
Creators: name: Constante-Amores, C. R.
name: Abadie, T.
name: Kahouadji, L.
name: Shin, S.
name: Chergui, J.
name: Juric, D.
name: Castrejon-Pita, A. A.
name: Matar, O. K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the effect of insoluble surfactants on the spatio-temporal evolution of turbulent jets. We use three-dimensional numerical simulations and employ an interface-tracking/level-set method that accounts for surfactant-induced Marangoni stresses. The present study builds on our previous work (Constante et al., 2021, J. Fluid Mech., 922, A6) in which we examined in detail the vortex-surface interaction in the absence of surfactants. Numerical solutions are obtained for a wide range of Weber and elasticity numbers in which vorticity production is generated by surface deformation and surfactant-induced Marangoni stresses. The present work demonstrates, for the first time, the crucial role of Marangoni stresses, brought about by surfactant concentration gradients, in the formation of coherent, hairpin-like vortex structures. These structures have a profound influence on the development of the three-dimensional interfacial dynamics. We also present theoretical expressions for the mechanisms that influence the rate of production of circulation in the presence of surfactants for a general, three-dimensional, two-phase flow and highlight the dominant contribution of Marangoni stresses.
New arcs in projective Hjelmslev planes over Galois rings
Creators: name: Kiermaier, Michael
name: Kohnert, Axel
Publisher: name: arXiv
Year: 2015
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: It is known that some good linear codes over a finite ring (R-linear codes) arise from interesting point constellations in certain projective geometries. For example, the expurgated Nordstrom-Robinson code, a nonlinear binary [14,6,6]-code which has higher minimum distance than any linear binary [14,6]-code, can be constructed from a maximal 2-arc in the projective Hjelmslev plane over Z_4.
Supplementary Information from A dynamically diluted alignment model reveals the impact of cell turnover on the plasticity of tissue polarity patterns
Creators: name: Hoffmann, Karl B.
name: Voss–Böhme, Anja
name: Rink, Jochen C.
name: Brusch, Lutz
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: 10202 Biological Mathematics
subject: FOS: Mathematics
subject: Computational Biology
subject: 60114 Systems Biology
subject: FOS: Biological sciences

description: Supplementary Information to Hoffmann, Voss-Böhme, Rink and Brusch 2017: “A Dynamically Diluted Alignment Model Reveals the Impact of Cell Turnover on the Plasticity of Tissue Polarity Patterns” with detailed derivations of equations that are used in the main text, a table summarising all variable names and notations and additional results in 7 supplementary figures: Fig.S1, Lattice size effects. Fig.S2, Effects of de-novo polarisation rate beta on the time of minimal order. Fig.S3, Statistical robustness of time of minimal order. Fig.S4, Bistability of mean-field ODE system for very high neighbour coupling strength. Fig.S5, Time of minimal order for vanishing neighbour coupling strength. Fig.S6, Time of minimal order collapses to linear function of the effective neighbour coupling strength. Fig.S7, Effects of coupling strength to global signal epsilon_s on the time of minimal order.
Superfluidity vs prethermalisation in a nonlinear Floquet system
Creators: name: Mu, Sen
name: Macé, Nicolas
name: Gong, Jiangbin
name: Miniatura, Christian
name: Lemarié, Gabriel
name: Albert, Mathias
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We show that superfluidity can be used to prevent thermalisation in a nonlinear Floquet system. Generically, periodic driving boils an interacting system to a featureless infinite temperature state. Fast driving is a known strategy to postpone Floquet heating with a large but always finite boiling time. In contrast, using a nonlinear periodically-driven system on a lattice, we show the existence of a continuous class of initial states which do not thermalise at all. This absence of thermalisation is associated to the existence and persistence of a stable superflow motion.
description: 7 pages, 5 figures, Supplementary material
[PDF] Les espaces à scénario  - Cycle 1 by Mélanie Rambaud, Coeur d'artiflo, Léa Lallinec, André Kister
Creators: name: Macdonald
Publisher: name: Zenodo
Year: 2024

description: Les espaces à scénario - Cycle 1 pan Mélanie Rambaud, Coeur d'artiflo, Léa Lallinec, André Kister

Télécharger eBook gratuit ➡ Link

Caractéristiques

Les espaces à scénario - Cycle 1

Mélanie Rambaud, Coeur d'artiflo, Léa Lallinec, André Kister

Nb. de pages: 200

Format: Pdf, ePub, MOBI, FB2

ISBN: 9782492471100

Editeur: Sésames (Les Editions)

Date de parution: 2022

 

 

 

Téléchargements ebook gratuits google Les espaces à scénario - Cycle 1 9782492471100 en francais

 

Overview

Donnez une autre dimension aux coins jeux de votre classe en les transformant en espaces à scénario ! Le travail est mis en scène dans un cadre motivant pour l'enfant, reprenant une situation concrète de la vie réelle afin de donner du sens aux apprentissages. Chaque scénario est pensé et conçu comme une activité d'entraînement pour renforcer l'acquisition d'une compétence en particulier, tout en tenant compte du niveau des enfants. Cet ouvrage permet de travailler les domaines fondamentaux qui sont Mobiliser le langage dans toutes ses dimensions et Acquérir les premiers outils mathématiques. Ces scénarios permettent tous de développer également des compétences langagières. Le livre vous présente pas à pas le fonctionnement de dix espaces, imaginés par une enseignante expérimentée.
(3067) Frederick Eastwood
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Thermal photon radiation in high multiplicity p+Pb collisions at the Large Hadron Collider
Creators: name: Shen, C.
name: Paquet, J. -F.
name: Denicol, G. S.
name: Jeon, S.
name: Gale, C.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The collective behaviour of hadronic particles has been observed in high multiplicity proton-lead collisions at the Large Hadron Collider (LHC), as well as in deuteron-gold collisions at the Relativistic Heavy-Ion Collider (RHIC). In this work we present the first calculation, in the hydrodynamic framework, of thermal photon radiation from such small collision systems. Owing to their compact size, these systems can reach temperatures comparable to those in central nucleus-nucleus collisions. The thermal photons can thus shine over the prompt background, and increase the low $p_T$ direct photon spectrum by a factor of 2-3 in 0-1% p+Pb collisions at 5.02 TeV. This thermal photon enhancement can therefore serve as a clean signature of the existence of a hot quark-gluon plasma during the evolution of these small collision systems, as well as validate hydrodynamic behavior in small systems.
description: 6 pages, 4 figures
(3070) Rachel [Nicholson]
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Additional file 1 of What implementation strategies and outcome measures are used to transform healthcare organizations into learning health systems? A mixed-methods review protocol
Creators: name: Somerville, Mari
name: Cassidy, Christine
name: Curran, Janet
name: Rothfus, Melissa
name: Sinclair, Doug
name: Elliott Rose, Annette
Publisher: name: figshare
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Appendix 1. Search strategy. Appendix 2. Data extraction instruments.
Mass Production of 2021 KMTNet Microlensing Planets II
Creators: name: Ryu, Yoon-Hyun
name: Shin, In-Gu
name: Yang, Hongjing
name: Gould, Andrew
name: Albrow, Michael D.
name: Chung, Sun-Ju
name: Han, Cheongho
name: Hwang, Kyu-Ha
name: Jung, Youn Kil
name: Shvartzvald, Yossi
name: Yee, Jennifer C.
name: Zang, Weicheng
name: Cha, Sang-Mok
name: Kim, Dong-Jin
name: Kim, %Hyoun-Woo
name: Kim, Seung-Lee
name: Lee, Chung-Uk
name: Lee, Dong-Joo
name: Lee, Yongseok
name: Park, Byeong-Gon
name: Pogge, Richard W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We continue our program of publishing all planets (and possible planets) found by eye in 2021 Korea Microlensing Telescope Network (KMTNet) online data. We present 4 planets, (KMT-2021-BLG-0712Lb, KMT-2021-BLG-0909Lb, KMT-2021-BLG-2478Lb, and KMT-2021-BLG-1105Lb), with planet-host mass ratios in the range -3.3 < log q < -2.2. This brings the total of secure, by-eye, 2021 KMTNet planets to 16, including 8 in this series. The by-eye sample is an important check of the completeness of semi-automated detections, which are the basis for statistical analyses. One of the planets, KMT-2021-BLG-1105Lb, is blended with a relatively bright $(I,V)\sim (18.9,21.6)$ star that may be the host. This could be verified immediately by high-resolution imaging. If so, the host is an early G dwarf, and the planet could be characterized by radial-velocity observations on 30m class telescopes.
PDF [DOWNLOAD] Temper by Layne Fargo on Iphone
Creators: name: Cecil
Publisher: name: Zenodo
Year: 2024

description: Temper by Layne Fargo

 

 

Download Book ➡ Link

Read Book Online ➡ Link

 

 

Temper

Layne Fargo

Page: 353

Format: pdf, ePub, mobi, fb2

ISBN: 9781982106737

Publisher: Simon & Schuster

 

Download book from amazon Temper 9781982106737 by Layne Fargo PDB PDF FB2 in English

Download it once and read it on your PC or mobile device PDF Temper by Layne Fargo EPUB Download. Uploaded fiction and nonfiction Temper EPUB PDF Download Read Layne Fargo. PDF Temper by Layne Fargo EPUB Download Kindle, PC, mobile phones or tablets. Ready for reading and downloading. HQ EPUB/MOBI/KINDLE/PDF/Doc Read EPUB Temper By Layne Fargo PDF Download ISBN. Check this ebook now Pages Published Publisher. Facebook share full length digital edition Temper EPUB PDF Download Read Layne Fargo.

Share link here and get free ebooks to read online. Kindle, iPhone, Android, Symbian, iPad FB2, PDF, Mobi, TXT. Synopsis PDF Temper by Layne Fargo EPUB Download zip file. Download at full speed with unlimited bandwidth PDF Temper by Layne Fargo EPUB Download just one click. eBook reading shares EPUB Temper By Layne Fargo PDF Download free link for reading and reviewing PDF EPUB MOBI documents. Uploaded fiction and nonfiction PDF Temper by Layne Fargo EPUB Download.

Reviews in epub, pdf and mobi formats. Novels - upcoming Temper EPUB PDF Download Read Layne Fargo. PDF Temper by Layne Fargo EPUB Download Open now in any browser there's no registration and complete book is free. PDF Temper by Layne Fargo EPUB Download You will be able to download it easily. PDF Temper by Layne Fargo EPUB Download ISBN novel zip, rar. Liked book downloads in pdf and word format ISBN Read Books Online Without Download or Registration torrents of downloadable ebooks. PDF Temper by Layne Fargo EPUB Download Share link here and get free ebooks to read online. Read book in your browser Temper EPUB PDF Download Read Layne Fargo.

You should be able to download your books shared forum Temper EPUB PDF Download Read Layne Fargo Review. New PDF Temper by Layne Fargo EPUB Download - Downloading to Kindle - Download to iPad/iPhone/iOS or Download to B&N nook. Today I'm sharing to you EPUB Temper By Layne Fargo PDF Download and this ebook is ready for read and download. Bestseller author of Temper new ebook or audio book available for download. Novels - upcoming Temper EPUB PDF Download Read Layne Fargo. Today I'm sharing to youTemper EPUB PDF Download Read Layne Fargoand this ebook is ready for read and download. PDF Temper by Layne Fargo EPUB Download review, torrent download locations. You should be able to download your books shared forum Temper Review.
Spin dynamics of a solid-state qubit in proximity to a superconductor
Creators: name: Monge, Richard
name: Delord, Tom
name: Proscia, Nicholas
name: Shotan, Zav
name: Jayakumar, Harishankar
name: Henshaw, Jacob
name: Zangara, Pablo R.
name: Lozovoi, Artur
name: Pagliero, Daniela
name: Esquinazi, Pablo D.
name: An, Toshu
name: Sodemann, Inti
name: Menon, Vinod M.
name: Meriles, Carlos A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A broad effort is underway to understand and harness the interaction between superconductors and spin-active color centers with an eye on the realization of hybrid quantum devices and novel imaging modalities of superconducting materials. Most work, however, overlooks the complex interplay between either system and the environment created by the color center host. Here we use an all-diamond scanning probe to investigate the spin dynamics of a single nitrogen-vacancy (NV) center proximal to a high-critical-temperature superconducting film in the presence of a weak magnetic field. We find that the presence of the superconductor increases the NV spin coherence lifetime, a phenomenon we tentatively rationalize as a change in the electric noise due to a superconductor-induced redistribution of charge carriers near the NV site. We build on these findings to demonstrate transverse-relaxation-time-weighted imaging of the superconductor film. These results shed light on the complex surface dynamics governing the spin coherence of shallow NVs while simultaneously paving the route to new forms of noise spectroscopy and imaging of superconductors.