cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Coevolution of the olfactory organ and its receptor repertoire in ray-finned fishes
Creators: name: Policarpo, Maxime
name: Bemis, Katherine E.
name: Laurenti, Patrick
name: Legendre, Laurent
name: Sandoz, Jean-Christophe
name: Rétaux, Sylvie
name: Casane, Didier
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Diversity of the olfactory receptor gene repertoire in ray-finned fishes. Figure S2. Distribution of ORA7 and ORA8 subfamilies in ray-finned fishes. Figure S3. Distribution of birth and death rates of OR, TAAR, OlfC and ORA genes in ray-finned fishes. Figure S4. Correlation of the number of gene losses (or gene gains) between gene families, estimated using the 368 branches of the phylogenetic tree. Figure S5. Correlation between the number of OR, TAAR and OlfC pseudogenes in 185 ray-finned fishes. Figure S6. Narial tubes of four species of ray-finned fishes with complex olfactory organs and large gene repertoires. Figure S7. Takifugu rubripes, USNM 57620, 290 mm TL.
Analytical Phase Reduction for Weakly Nonlinear Oscillators
Creators: name: León, Iván
name: Nakao, Hiroya
Publisher: name: arXiv
Year: 2023
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: FOS: Physical sciences

description: Phase reduction is a dimensionality reduction scheme to describe the dynamics of nonlinear oscillators with a single phase variable. While it is crucial in synchronization analysis of coupled oscillators, analytical results are limited to few systems. In this letter, we analytically perform phase reduction for a wide class of oscillators by extending the Poincaré-Lindstedt perturbation theory. We exemplify the utility of our approach by analyzing an ensemble of Van der Pol oscillators, where the derived phase model provides analytical predictions of their collective synchronization dynamics
description: 10 pages, 5 figures
THE RESOLVE SURVEY ATOMIC GAS CENSUS AND ENVIRONMENTAL INFLUENCES ON GALAXY GAS RESERVOIRS
Creators: name: Baker, Ashley D.
name: Calderon, Victor F.
name: Burchett, Joseph N.
name: Norris, Mark A.
name: Hoversten, Erik A.
name: Hall, Kirsten R.
name: Giovanelli, Riccardo
name: Florez, Jonathan
name: Kannappan, Sheila J.
name: Stark, David V.
name: Moffett, Amanda J.
name: Eckert, Kathleen D.
name: Leroy, Adam K.
name: Haynes, Martha P.
name: Gonzalez, Roberto E.
name: Watson, Linda C.
name: Wei, Lisa H.
name: Berlind, Andreas A.
name: Guynn, David T.
name: Pisano,
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2016

description: We present the H i mass inventory for the REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey, a volume-limited, multi-wavelength census of >1500 z = 0 galaxies spanning diverse environments and complete in baryonic mass down to dwarfs of ~109 ${M}_{\odot }$. This first 21 cm data release provides robust detections or strong upper limits (1.4M H i < 5%–10% of stellar mass M *) for ~94% of RESOLVE. We examine global atomic gas-to-stellar mass ratios (G/S) in relation to galaxy environment using several metrics: group dark matter halo mass M h, central/satellite designation, relative mass density of the cosmic web, and distance to the nearest massive group. We find that at fixed M *, satellites have decreasing G/S with increasing M h starting clearly at M h ~ 1012 ${M}_{\odot }$, suggesting the presence of starvation and/or stripping mechanisms associated with halo gas heating in intermediate-mass groups. The analogous relationship for centrals is uncertain because halo abundance matching builds in relationships between central G/S, stellar mass, and halo mass, which depend on the integrated group property used as a proxy for halo mass (stellar or baryonic mass). On larger scales G/S trends are less sensitive to the abundance matching method. At fixed M h ≤ 1012 ${M}_{\odot }$, the fraction of gas-poor centrals increases with large-scale structure density. In overdense regions, we identify a rare population of gas-poor centrals in low-mass (M h < 1011.4 ${M}_{\odot }$) halos primarily located within ~1.5× the virial radius of more massive (M h > 1012 ${M}_{\odot }$) halos, suggesting that gas stripping and/or starvation may be induced by interactions with larger halos or the surrounding cosmic web. We find that the detailed relationship between G/S and environment varies when we examine different subvolumes of RESOLVE independently, which we suggest may be a signature of assembly bias.
title: Differential Diagnosis of Endobronchial Lesions in Childhood with a Surprising Diagnosis: Langerhans' Cell Histiocytosis
Creators: name: Agirlar Trabzonlu, Tugce
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Thorax
subject: Paediatric
subject: CT
subject: PET-CT
subject: Screening
subject: Pathology
subject: Haematologic diseases

description: Purpose Methods and Materials Results Conclusions References Personal Information
description: Purpose: Primary endobronchial tumours are rare in pediatric practice and are appropriately not the first consideration when a child presents with recurrent atelectasis or respiratory tract infection. In children the commonest neoplasm is the carcinoid tumor...
Variable Selection for Modeling the Absolute Magnitude at Maximum of Type Ia Supernovae
Creators: name: Uemura, Makoto
name: Koji
name: Kawabata, S.
name: Ikeda, Shiro
name: Maeda, Keiichi
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We discuss what is an appropriate set of explanatory variables in order to predict the absolute magnitude at the maximum of Type Ia supernovae. In order to have a good prediction, the error for future data, which is called the "generalization error," should be small. We use cross-validation in order to control the generalization error and LASSO-type estimator in order to choose the set of variables. This approach can be used even in the case that the number of samples is smaller than the number of candidate variables. We studied the Berkeley supernova database with our approach. Candidates of the explanatory variables include normalized spectral data, variables about lines, and previously proposed flux-ratios, as well as the color and light-curve widths. As a result, we confirmed the past understanding about Type Ia supernova: i) The absolute magnitude at maximum depends on the color and light-curve width. ii) The light-curve width depends on the strength of Si II. Recent studies have suggested to add more variables in order to explain the absolute magnitude. However, our analysis does not support to add any other variables in order to have a better generalization error.
description: 9 pages, 7 figures, accepted for publication in PASJ
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1746
Subjects: Argenson, Marc-Pierre de Voyer d'1696-1764Marc Pierre de Voyer de PaulmyArgeson
Bousquet, Marc Michel1696-1762Marc-MichelBousquet
Jaquier, François1711-1788
Le MercierBuchhändler in Paris
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
Maupertuis, René Moreau de1664-1746RenéMoreau deMaupertuis
Moula, Frédéric1703-1782
Newton, Isaac1643-1727I.Newton
Voltaire1694-1778François-MarieArouet

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit schwarzem Siegel
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, pp.152-154; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.279-280
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
title: Imaging of acute thoracic aortic disease: typical and atypical features and complications
Creators: name: Mnari, Walid
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Cardiovascular system
subject: CT-Angiography
subject: MR
subject: Ultrasound-Colour Doppler
subject: Education
subject: Acute
subject: Dissection
subject: Aneurysms

description: Learning objectives Background Imaging findings OR Procedure details Conclusion References Personal Information
description: Learning objectives: - To review the pathophysiology of acute aortic syndrome (AAS) especially the new concept of aortic hematoma. - To present the spectrum of multi-modality radiological findings in AAS, with an emphasis on multidetector CT angiography. - Illustrate...
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1745
Subjects: Bernoulli, Jacob1712-1769JacobBernoulli-Debary
FriedrichII. Preußen, König1712-1786FredericGuillaume
Maupertuis, René Moreau de1664-1746RenéMoreau deMaupertuis
Voltaire1694-1778François-MarieArouet

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit rotem Siegel
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, pp.146-147; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.274-275
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
title: Percutaneous cutting needle biopsy and fine needle aspiration cytology for diffuse micronodular lung disease using the same coaxial guide needle under a C-arm cone-beam CT system
Creators: name: Park, Choong-Ki
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Infection
subject: Foreign bodies
subject: Cancer
subject: Biopsy
subject: Cone beam CT
subject: Thorax

description: Purpose Methods and Materials Results Conclusions References Personal Information
description: Purpose: Micronodule is a term used for discrete, small, round, focal opacity. And diverse cutoff diameters of micronodule have been used according to the references.(1) We defined micronodule as same or less than 10mm diameter in this article. There are...
Brief an [Johann II Bernoulli]
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1739
Subjects: Bernoulli, Johann1667-1748JohannBernoulli
Clairaut, Alexis Claude1713-1765...Clairaut
König, Samuel1712-1757SamuelKoenig
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
Voltaire1694-1778François-MarieArouet

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.260-262
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'Etudes III, Genève 1958, I, pp.385-387; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.212-214
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
title: Diagnosis of Pulmonary Alveolar Microlithiasis, Can Imaging Alone Help?
Creators: name: Alhassan, Donya
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Calcifications / Calculi
subject: Diagnostic procedure
subject: CT-High Resolution
subject: Conventional radiography
subject: Lung

description: Learning objectives Background Imaging findings OR Procedure details Conclusion References Personal Information
description: Learning objectives: To Identify the radiological manifestations of pulmonary alveolar microlithiasis (PAM) on chest radiography and to illustrate the characteristic pattern on HRCT. To illustrate this, we report a case of symptomatic PAM in whom imaging findings prove...
Brief an [Johann II] Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1739
Subjects: Bernoulli, Daniel1700-1782DanielBernoulli
Bernoulli, Nicolaus1687-1759NicolasBernoulli
Clairaut, Alexis Claude1713-1765...Clairaut
Fontenelle, Bernard Le Bovier de1657-1757Bernard Le BouierFontenelle
König, Daniel1725-1747
König, Samuel1712-1757SamuelKoenig
Mairan, Jean Jacques de1678-1771Jean-JacquesMairan
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
Picard, Jean1620-1682JoannesPicard
Réaumur, René Antoine Ferchault de1683-1757René AntoineFerchault de Reaumur
Voltaire1694-1778François-MarieArouet

description: Emilie du Châtelet spricht von der Rückkehr Maupertuis nach Paris und von den Bedenken Fontenelles und Réaumurs hinsichtlich der Wahl eines associé étranger in die Académie. Dies deutet auf 1739 hin. Samuel König wurde damals in die Académie gewählt.
description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'Etudes III, Genève 1958, I, pp.376-378; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.204-206
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.252-253
Brief an [Johann II Bernoulli]
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1739
Subjects: Bernoulli, Daniel1700-1782DanielBernoulli
Bernoulli, Johann1667-1748JohannBernoulli
Bernoulli, Nicolaus1687-1759NicolasBernoulli
König, Samuel1712-1757SamuelKoenig
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
Voltaire1694-1778François-MarieArouet

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Monat und Jahr im Datum von Joh. III B. ergänzt
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.244-245
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études III, Genéve 1958, I, pp.352-353; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.196-197
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
Regge trajectories for the heavy-light diquarks
Creators: name: Chen, Jiao-Kai
name: Feng, Xia
name: Xie, Jia-Qi
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We attempt to apply the Regge trajectory approach to the heavy-light diquarks composed of one heavy quark and one light quark. However, we find that the direct application of the usual Regge trajectory formula for the heavy-light mesons and baryons fails. In order to correctly estimate the masses of the heavy-light diquarks, it is needed to consider the light quark mass correction and the parameter $C$ in the Cornell potential within the Regge trajectory formula. By using the modified Regge trajectory formulas, we are able to estimate the masses of the heavy-light diquarks $(cu)$, $(cs)$, $(bu)$ and $(bs)$, which agree with other theoretical results. It is illustrated that the heavy-light diquarks satisfy the universal descriptions irrespective of heavy quark flavors, similar to other heavy-light systems such as the heavy-light mesons, the heavy-light baryons composed of one heavy quark (diquark) and one light diquark (quark), and the heavy-light tetraquarks composed of one heavy diquark (antidiquark) and one light antidiquark (diquark). The diquark Regge trajectory provides a new and very simple approach for estimating the spectra of the heavy-light diquarks.
description: 10 pages, 3 figures, 7 tables
TWO SMALL TEMPERATE PLANETS TRANSITING NEARBY M DWARFS IN K2 CAMPAIGNS 0 AND 1
Creators: name: Beichman, Charles A.
name: Henning, Thomas
name: Baranec, Christoph
name: Obermeier, Christian
name: Isaacson, Howard T.
name: Fulton, Benjamin J.
name: Hinz, Philip
name: Bonnefoy, Mickaël
name: Crossfield, Ian J. M.
name: Schlieder, Joshua E.
name: Skemer, Andrew
name: Lépine, Sébastien
name: Bailey, Vanessa P.
name: Law, Nicholas
name: Petigura, Erik A.
name: Ciardi, David R.
name: Sinukoff, Evan
name: Liu, Michael C.
name: Riddle, Reed
name: Ziegler, Carl
name: Howard, Andrew W.
name: Aller, Kimberly M.
name: Morton, Timothy D.
name: Defrère, Denis
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2016

description: The prime Kepler mission revealed that small planets (<4 ) are common, especially around low-mass M dwarfs. K2, the repurposed Kepler mission, continues this exploration of small planets around small stars. Here we combine K2 photometry with spectroscopy, adaptive optics imaging, and archival survey images to analyze two small planets orbiting the nearby field-age M dwarfs, K2-26 (EPIC 202083828) and K2-9. K2-26 is an dwarf at 93 ± 7 pc from K2 Campaign 0. We validate its planet with a day period of 14.5665 and estimate a radius of . K2-9 is an dwarf at 110 ± 12 pc from K2 Campaign 1. K2-9b was first identified by Montet et al.; here we present spectra and adaptive optics imaging of the host star and independently validate and characterize the planet. Our analyses indicate K2-9b is a planet with a 18.4498 day period. K2-26b exhibits a transit duration that is too long to be consistent with a circular orbit given its measured stellar radius. Thus, the long transits are likely due to the photoeccentric effect and our transit fits hint at an eccentric orbit. Both planets receive low incident flux from their host stars and have estimated equilibrium temperatures <500 K. K2-9b may receive approximately Earth-like insolation. However, its host star exhibits strong GALEX UV emission which could affect any atmosphere it harbors. K2-26b and K2-9b are representatives of a poorly studied class of small planets with cool temperatures that have radii intermediate to Earth and Neptune. Future study of these systems can provide key insight into trends in bulk composition and atmospheric properties at the transition from silicate dominated to volatile rich bodies.
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1740
Subjects: FriedrichII. Preußen, König1712-1786FredericGuillaume
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit schwarzem Siegel
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.276
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, pp.34-35; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.229-230
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
description: Konservierung=Preservation=Conservation Juli 2014 Sämtliche Seiten sind durch Tintenfrass beschädigt. Bestandserhaltung
title: The role of fetal MRI in planning for the ex-utero intrapartum (EXIT) procedure
Creators: name: Semple, Thomas
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Foetus
subject: Congenital
subject: Diagnostic procedure
subject: MR
subject: Thorax
subject: Paediatric
subject: Foetal imaging

description: Purpose Methods and Materials Results Conclusions References Personal Information
description: Purpose: Purpose: Following a retrospective review of cases, we present a previously unreported MRI sign of fetal airway obstruction that could represent a useful tool in prenatal assessment and planning for the ex-utero intrapartum (EXIT) procedure....
Polarization Transfer in Wide-Angle Compton Scattering and Single-Pion Photoproduction from the Proton
Creators: name: Fanelli, C.
name: Cisbani, E.
name: Hamilton, D. J.
name: Salme, G.
name: Wojtsekhowski, B.
name: Ahmidouch, A.
name: Annand, J. R. M.
name: Baghdasaryan, H.
name: Beaufait, J.
name: Bosted, P.
name: Brash, E. J.
name: Butuceanu, C.
name: Carter, P.
name: Christy, E.
name: Chudakov, E.
name: Danagoulian, S.
name: Day, D.
name: Degtyarenko, P.
name: Ent, R.
name: Fenker, H.
name: Fowler, M.
name: Frlez, E.
name: Gaskell, D.
name: Gilman, R.
name: Horn, T.
name: Huber, G. M.
name: de Jager, C. W.
name: Jensen, E.
name: Jones, M. K.
name: Kelleher, A.
name: Keppel, C.
name: Khandaker, M.
name: Kohl, M.
name: Kumbartzki, G.
name: Lassiter, S.
name: Li, Y.
name: Lindgren, R.
name: Lovelace, H.
name: Luo, W.
name: Mack, D.
name: Mamyan, V.
name: Margaziotis, D. J.
name: Markowitz, P.
name: Maxwell, J.
name: Mbianda, G.
name: Meekins, D.
name: Meziane, M.
name: Miller, J.
name: Mkrtchyan, A.
name: Mkrtchyan, H.
name: Mulholland, J.
name: Nelyubin, V.
name: Pentchev, L.
name: Perdrisat, C. F.
name: Piasetzky, E.
name: Prok, Y.
name: Puckett, A. J. R.
name: Punjabi, V.
name: Shabestari, M.
name: Shahinyan, A.
name: Slifer, K.
name: Smith, G.
name: Solvignon, P.
name: Subedi, R.
name: Wesselmann, F. R.
name: Wood, S.
name: Ye, Z.
name: Zheng, X.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Wide-angle exclusive Compton scattering and single-pion photoproduction from the proton have been investigated via measurement of the polarization transfer from a circularly polarized photon beam to the recoil proton. The wide-angle Compton scattering polarization transfer was analyzed at an incident photon energy of 3.7~GeV at a proton scattering angle of \cma$= 70^\circ$. The longitudinal transfer \KLL, measured to be $0.645 \pm 0.059 \pm 0.048$, where the first error is statistical and the second is systematic, has the same sign as predicted for the reaction mechanism in which the photon interacts with a single quark carrying the spin of the proton. However, the observed value is $\sim$3~times larger than predicted by the generalized-parton-distribution-based calculations, which indicates a significant unknown contribution to the scattering amplitude.
description: 6 pages, 5 figures, the text has been made consistent with the published
Brightness and mass accretion rate evolution during the 2022 burst of EX~Lupi
Creators: name: de Miera, F. Cruz-Sáenz
name: Kóspál, Á.
name: Ábrahám, P.
name: Claes, R. A. B.
name: Manara, C. F.
name: Wendeborn, J.
name: Fiorellino, E.
name: Giannini, T.
name: Nisini, B.
name: Sicilia-Aguilar, A.
name: Campbell-White, J.
name: Alcalá, J. M.
name: Banzatti, A.
name: Szabó, Zs. M.
name: Lykou, F.
name: Antoniucci, S.
name: Varga, J.
name: Siwak, M.
name: Park, S.
name: Nagy, Zs.
name: Kun, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: EX Lupi is the prototype by which EXor-type outbursts were defined. It has experienced multiple accretion-related bursts and outbursts throughout the last decades, whose study have greatly extended our knowledge about the effects of these types of events. This star experienced a new burst in 2022. We used multi-band photometry to create color-color and color-magnitude diagrams to exclude the possibility that the brightening could be explained by a decrease in extinction. We obtained VLT/X-shooter spectra to determine the Lacc and Macc during the peak of the burst and after its return to quiescence using 2 methods: empirical relationships between line luminosity and Lacc, and a slab model of the whole spectrum. We examined the 130 year light curve of EX Lupi to provide statistics on the number of outbursts experienced during this period of time. Our analysis of the data taken during the 2022 burst confirmed that a change in extinction is not responsible for the brightening. Our two approaches in calculating the Macc were in agreement, and resulted in values that are 2 orders of magnitude above what had previously been estimated, thus suggesting that EX Lupi is a strong accretor even when in quiescence. We determined that in 2022 March the Macc increased by a factor of 7 with respect to the quiescent level. We also found hints that even though the Macc had returned to almost its pre-outburst levels, certain physical properties of the gas had not returned to the quiescent values. We found that the mass accreted during this three month event was 0.8 lunar masses, which is approximately half of what is accreted during a year of quiescence. We calculated that if EX Lupi remains as active as it has been for the past 130 years, during which it has experienced at least 3 outbursts and 10 bursts, then it will deplete the mass of its circumstellar material in less than 160000 yr.
description: 18 pages, 12 figures, 4 tables. Accepted for publication in A&A
title: Dual-Energy CT in Pulmonary Hypertension
Creators: name: Benegas Urteaga, Mariana
Publisher: name: European Society of Thoracic Imaging
Year: 2016
Subjects: subject: Hypertension
subject: Computer Applications-Virtual imaging
subject: CT-Angiography
subject: CT
subject: Thorax

description: Learning objectives Background Imaging findings OR Procedure details Conclusion References Personal Information
description: Learning objectives: To describe the radiologic evaluation of patients with Pulmonary Hypertension (PH) with the introduction of Dual-Energy CT (DECT) imaging. To illustrate different causes of PH on Dual-CT images To show the utility and the potential advantages and...
WHY ARE RAPIDLY ROTATING M DWARFS IN THE PLEIADES SO (INFRA)RED? NEW PERIOD MEASUREMENTS CONFIRM ROTATION-DEPENDENT COLOR OFFSETS FROM THE CLUSTER SEQUENCE
Creators: name: Agüeros, Marcel A.
name: Law, Nicholas M.
name: Levitan, David
name: Surace, Jason
name: Laher, Russ
name: Sesar, Branimir
name: Liu, Jiyu
name: Covey, Kevin R.
name: Ahmadi, Aida
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2016

description: Stellar rotation periods ( P {sub rot}) measured in open clusters have proved to be extremely useful for studying stars’ angular momentum content and rotationally driven magnetic activity, which are both age- and mass-dependent processes. While P {sub rot} measurements have been obtained for hundreds of solar-mass members of the Pleiades, measurements exist for only a few low-mass (<0.5 M {sub ⊙}) members of this key laboratory for stellar evolution theory. To fill this gap, we report P {sub rot} for 132 low-mass Pleiades members (including nearly 100 with M ≤ 0.45 M {sub ⊙}), measured from photometric monitoring of the cluster conducted by the Palomar Transient Factory in late 2011 and early 2012. These periods extend the portrait of stellar rotation at 125 Myr to the lowest-mass stars and re-establish the Pleiades as a key benchmark for models of the transport and evolution of stellar angular momentum. Combining our new P {sub rot} with precise BVIJHK photometry reported by Stauffer et al. and Kamai et al., we investigate known anomalies in the photometric properties of K and M Pleiades members. We confirm the correlation detected by Kamai et al. between a star's P {sub rot} and position relative tomore » the main sequence in the cluster's color–magnitude diagram. We find that rapid rotators have redder ( V − K ) colors than slower rotators at the same V , indicating that rapid and slow rotators have different binary frequencies and/or photospheric properties. We find no difference in the photometric amplitudes of rapid and slow rotators, indicating that asymmetries in the longitudinal distribution of starspots do not scale grossly with rotation rate.« less
A Deep Test of Radial Differential Rotation in a Helium-atmosphere White Dwarf.I. Discovery of Pulsations in PG 0112+104
Creators: name: Clemens,
name: Hermes,
name: Dunlap,
name: Bischoff-Kim,
name: Kawaler, Steven D.
name: Provencal,
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2017

description: We present the detection of non-radial oscillations in a hot, helium-atmosphere white dwarf using 78.7 days of nearly uninterrupted photometry from the Kepler space telescope. With an effective temperature >30,000 K, PG 0112+104 becomes the hottest helium-atmosphere white dwarf known to pulsate. The rich oscillation spectrum of low-order g-modes includes clear patterns of rotational splittings from consecutive sequences of dipole and quadrupole modes, which can be used to probe the rotation rate with depth in this highly evolved stellar remnant. We also measure a surface rotation rate of 10.17404 hr from an apparent spot modulation in the K2 data. With two independent measures of rotation, PG 0112+104 provides a remarkable test of asteroseismic inference.
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1742
Subjects: Bourbon, Louis-Auguste de1700-1755Louis AugusteBourbon
Grandvillars, de
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
Pourfour du Petit, François1664-1741François PourfourPetit

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit rotem Siegel
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, pp.85-86; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.245-246
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
Metrewave Galactic Plane with the uGMRT (MeGaPluG) Survey: Lessons from the Pilot Study
Creators: name: Dokara, Rohit
name: Roy, Nirupam
name: Menten, Karl
name: Vig, Sarita
name: Dutta, Prasun
name: Beuther, Henrik
name: Pandian, Jagadheep D.
name: Rugel, Michael
name: Rashid, Md
name: Brunthaler, Andreas
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. The advent of wide-band receiver systems on interferometer arrays enables one to undertake high-sensitivity and high-resolution radio continuum surveys of the Galactic plane in a reasonable amount of telescope time. However, to date, there are only a few such studies of the first quadrant of the Milky Way that have been carried out at frequencies below 1 GHz. The Giant Metrewave Radio Telescope (GMRT) has recently upgraded its receivers with wide-band capabilities (now called the uGMRT) and provides a good opportunity to conduct high resolution surveys, while also being sensitive to the extended structures. Aims. We wish to assess the feasibility of conducting a large-scale snapshot survey, the Metrewave Galactic Plane with the uGMRT Survey (MeGaPluG), to simultaneously map extended sources and compact objects at an angular resolution lower than $10''$ and a point source sensitivity of 0.15 mJy/beam. Methods. We performed an unbiased survey of a small portion of the Galactic plane, covering the W43/W44 regions ($l=29^\circ-35^\circ$ and $|b|<1^\circ$) in two frequency bands: 300$-$500 MHz and 550$-$750 MHz. The 200 MHz wide-band receivers on the uGMRT are employed to observe the target field in several pointings, spending nearly 14 minutes on each pointing in two separate scans. We developed an automated pipeline for the calibration, and a semi-automated self-calibration procedure is used to image each pointing using multi-scale CLEAN and outlier fields. Results. We produced continuum mosaics of the surveyed region at a final common resolution of $25''$ in the two bands that have central frequencies of 400 MHz and 650 MHz, with a point source sensitivity better than 5 mJy/beam. We plan to cover a larger footprint of the Galactic plane in the near future based on the lessons learnt from this study. (Abridged)
description: To be published in A&A. 13 pages, 10 figures
Additional file 3 of Coevolution of the olfactory organ and its receptor repertoire in ray-finned fishes
Creators: name: Policarpo, Maxime
name: Bemis, Katherine E.
name: Laurenti, Patrick
name: Legendre, Laurent
name: Sandoz, Jean-Christophe
name: Rétaux, Sylvie
name: Casane, Didier
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Supplementary Data 2. Comparison of olfactory receptor gene repertoires from the present and previous studies. (A) Summary of the number of TAAR genes retrieved in our study and previous studies of four teleost species. (B) Summary of the number of OlfC genes retrieved in our study and previous studies of four teleost species. (C) Summary of the number of ORA genes retrieved in our study and previous studies of four teleost species. (D) Phylogenetic tree of Danio rerio TAAR genes retrieved in Hashiguchi and Nishida 2007 and our study. (E) Phylogenetic tree of Gasterosteus aculeatus TAAR genes retrieved in Azzouzi et al. 2015 and our study. (F) Phylogenetic tree of Oryzias latipes TAAR genes retrieved in Azzouzi et al. 2015 and our study. (G) Phylogenetic tree of Takifugu rubripes TAAR genes retrieved in Hashiguchi and Nishida 2007 and our study. (H) Phylogenetic tree of Danio rerio OlfC genes retrieved in Yang et al. 2019 and our study. (I) Phylogenetic tree of Gasterosteus aculeatus OlfC genes retrieved in Yang et al. 2019 and our study. (J) Phylogenetic tree of Oryzias latipes OlfC genes retrieved in Yang et al. 2019 and our study. (K) Phylogenetic tree of Takifugu rubripes OlfC genes retrieved in Yang et al. 2019 and our study. (L) Phylogenetic tree of Danio rerio ORA genes retrieved in Zapilko and Korsching 2016 and our study. (M) Phylogenetic tree of Gasterosteus aculeatus ORA genes retrieved in Zapilko and Korsching 2016 and our study. (N) Phylogenetic tree of Oryzias latipes ORA genes retrieved in Zapilko and Korsching 2016 and our study. (O) Phylogenetic tree of Takifugu rubripes ORA genes retrieved in Zapilko and Korsching 2016 and our study. (P) Phylogenetic tree of Polypterus senegalus OR genes retrieved in Bi X et al. 2021 and our study.
Brief an [Johann II] Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1740
Subjects: Cassini, Jacques1677-1756JacquesCassini de Glos
Du Châtelet, Louis-Marie-Florent1727-1793Louis Marie FlorentDu Châtelet
Erlach, Abraham von1716-1782
König, Samuel1712-1757SamuelKoenig
Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius
TrichateauMarquis de

description: von [Gabrielle Emilie Le Tonnellier de Breteuil] Du Châtelet
description: "Copie de lettre", vermutlich Signatur L Ia 768:Bl.268-269 (dort ist der 24. April anggegeben)
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, pp.14-16; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.224-225
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
description: Briefkatalog UB Basel: 24. April 1740; "Copie de lettre", L Ia 768:Bl.268-269, ebenso (09.01.2017/A100/bot2)
A review of planetary systems around HD 99492, HD 147379 and HD 190007 with HARPS-N
Creators: name: Stalport, M.
name: Cretignier, M.
name: Udry, S.
name: John, A. Anna
name: Wilson, T. G.
name: Delisle, J. -B.
name: Bonomo, A. S.
name: Buchhave, L. A.
name: Charbonneau, D.
name: Dalal, S.
name: Damasso, M.
name: Di Fabrizio, L.
name: Dumusque, X.
name: Fiorenzano, A.
name: Harutyunyan, A.
name: Haywood, R. D.
name: Latham, D. W.
name: López-Morales, M.
name: Lorenzi, V.
name: Lovis, C.
name: Malavolta, L.
name: Molinari, E.
name: Mortier, A.
name: Pedani, M.
name: Pepe, F.
name: Pinamonti, M.
name: Poretti, E.
name: Rice, K.
name: Sozzetti, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The Rocky Planet Search (RPS) program is dedicated to a blind radial velocity (RV) search of planets around bright stars in the Northern hemisphere, using the high-resolution echelle spectrograph HARPS-N installed on the Telescopio Nazionale Galileo (TNG). The goal of this work is to revise and update the properties of three planetary systems by analysing the HARPS-N data with state-of-the-art stellar activity mitigation tools. The stars considered are HD 99492 (83Leo B), HD 147379 (Gl617 A) and HD 190007. We employ a systematic process of data modelling, that we selected from the comparison of different approaches. We use YARARA to remove instrumental systematics from the RV, and then use SPLEAF to further mitigate the stellar noise with a multidimensional correlated noise model. We also search for transit features in the Transiting Exoplanets Survey Satellite (TESS) data of these stars. We report on the discovery of a new planet around HD 99492, namely HD 99492 c, with an orbital period of 95.2 days and a minimum mass of msin i = 17.9 M_Earth, and refine the parameters of HD 99492 b. We also update and refine the Keplerian solutions for the planets around HD 147379 and HD 190007, but do not detect additional planetary signals. We discard the transiting geometry for the planets, but stress that TESS did not exhaustively cover all the orbital phases. The addition of the HARPS-N data, and the use of advanced data analysis tools, has allowed us to present a more precise view of these three planetary systems. It demonstrates once again the importance of long observational efforts such as the RPS program. Added to the RV exoplanet sample, these planets populate two apparently distinct populations revealed by a bimodality in the planets minimum mass distribution. The separation is located between 30 and 50 M_Earth.
description: 27 pages, 26 figures (13 in Appendix); Accepted for publication in A&A
Polycyclic Aromatic Hydrocarbons in Exoplanet Atmospheres I. Thermochemical Equilibrium Models
Creators: name: Dubey, Dwaipayan
name: Grübel, Fabian
name: Arenales-Lope, Rosa
name: Molaverdikhani, Karan
name: Ercolano, Barbara
name: Rab, Christian
name: Trapp, Oliver
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Context: Polycyclic Aromatic Hydrocarbons, largely known as PAHs, are widespread in the universe and have been identified in a vast array of astronomical observations from the interstellar medium to protoplanetary discs. They are likely to be associated with the chemical history of the universe and the emergence of life on Earth. However, their abundance on exoplanets remains unknown. Aims: We aim to investigate the feasibility of PAH formation in the thermalized atmospheres of irradiated and non-irradiated hot Jupiters around Sun-like stars. Methods: To this aim, we introduced PAHs in the 1-D self-consistent forward modeling code petitCODE. We simulated a large number of planet atmospheres with different parameters (e.g. carbon to oxygen ratio, metallicity, and effective planetary temperature) to study PAH formation. By coupling the thermochemical equilibrium solution from petitCODE with the 1-D radiative transfer code, petitRADTRANS, we calculated the synthetic transmission and emission spectra for irradiated and non-irradiated planets, respectively, and explored the role of PAHs on planet spectra. Results: Our models show strong correlations between PAH abundance and the aforementioned parameters. In thermochemical equilibrium scenarios, an optimal temperature, elevated carbon to oxygen ratio, and increased metallicity values are conducive to the formation of PAHs, with the carbon to oxygen ratio having the largest effect.
description: 10 pages, 10 figures
Additional file 4 of Coevolution of the olfactory organ and its receptor repertoire in ray-finned fishes
Creators: name: Policarpo, Maxime
name: Bemis, Katherine E.
name: Laurenti, Patrick
name: Legendre, Laurent
name: Sandoz, Jean-Christophe
name: Rétaux, Sylvie
name: Casane, Didier
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4. Supplementary Data 3. (A) Phylogeny of OR genes from 44 species representing 44 orders of ray-finned fishes sampled in this study. Branches are colored according to the gene subfamily classification. (B) Phylogeny of all TAAR genes retrieved from 185 ray-finned fishes. Branches are colored according to gene family classification. Outgroup sequences (nonTAAR GPCRs) are colored in black. (C) Phylogeny of all OlfC genes retrieved from 185 ray-finned fish. Branches are colored according to the gene subfamily classification. Outgroup sequences (CasR and V2R2 genes) are colored in black. (D) Phylogeny of all ORA genes retrieved from 185 ray-finned fishes. Branches are colored according to the gene subfamily classification. Outgroup sequences (T2R genes) are colored in black.
Brief an [Johann II Bernoulli]
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1739
Subjects: Maupertuis, Pierre Louis Moreau de1698-1759Pierre Louis MoreauMaupertius

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit rotem Siegel
description: S. 379 leer
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.254
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'Etudes III, Genève 1958, I, pp.381-382; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.207-208
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
Experimental study of balanced optical homodyne and heterodyne detection by controlling sideband modulation
Creators: name: Li, Wei
name: Meng, Zengming
name: Yu, Xudong
name: Zhang, Jing
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We experimentally study optical homodyne and heterodyne detections with a same setup, which is flexible to manipulate the signal sideband modulation. When the modulation only generate a single signal sideband, the light field measurement by mixing the single sideband at $ω_{0}+Ω$ with a strong local oscillator at the carrier frequency $ω_{0}$ on a beam splitter become balanced heterodyne detection. When two signal sidebands at $ω_{0}\pmΩ$ are generated and the relative phase of the two sidebands is locked, this measurement corresponds to optical balanced homodyne detection. With this setup, we may confirm directly that the signal-to-noise ratio with heterodyne detection is two-fold worse than that with homodyne detection. This work will have important applications in quantum state measurement and quantum information.
description: This paper includes 5 pages and 6 figures
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1740
Subjects: König, Samuel1712-1757SamuelKoenig

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit rotem Siegel
description: "Copie de lettre", siehe Signatur L Ia 768:Bl.263
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, p.7; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, p.215
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
Brief an Johann II Bernoulli / Brief an Johann II Bernoulli
Creators: name: Du Châtelet, Gabrielle Émilie Le Tonnelier de Breteuil
Publisher: name: [s.n.]
Year: 1743
Subjects: Bernoulli, Daniel1700-1782DanielBernoulli
Bernoulli, Johann1667-1748JohannBernoulli
Voltaire1694-1778François-MarieArouet

description: von [Gabrielle Emilie Le Tonnellier de] Breteuil Du Châtelet
description: Mit rotem Siegel
description: Briefumschlag auf S. 460/461
description: Öffentliche Bibliothek der Universität Basel
description: Französisch
description: Druck: Publications de l'Institut et Musée Voltaire, Série d'études IV, Genève 1958, II, p.101; Studies on Voltaire and the Eighteenth Century, vol. IV, Genève 1957, pp.250-251
description: Datenimport aus LIDOS / Bernoulli (2004-07-02)
A Search for Rapidly Pulsating Hot Subdwarf Stars in the GALEX Survey
Creators: name: Haislip, Josh B.
name: Linder, Tyler R.
name: Boudreaux, Thomas M.
name: Reichart, Dan E.
name: Barlow, Brad N.
name: Moore, Justin P.
name: Fleming, Scott W.
name: Soto, Alan Vasquez
name: Million, Chase
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2017

description: NASA’s Galaxy Evolution Explorer ( GALEX ) provided near- and far-UV observations for approximately 77% of the sky over a 10-year period; however, the data reduction pipeline initially only released single NUV and FUV images to the community. The recently released Python module gPhoton changes this, allowing calibrated time-series aperture photometry to be extracted easily from the raw GALEX data set. Here we use gPhoton to generate light curves for all hot subdwarf B (sdB) stars that were observed by GALEX , with the intention of identifying short-period, p-mode pulsations. We find that the spacecraft’s short visit durations, uneven gaps between visits, and dither pattern make the detection of hot subdwarf pulsations difficult. Nonetheless, we detect UV variations in four previously known pulsating targets and report their UV pulsation amplitudes and frequencies. Additionally, we find that several other sdB targets not previously known to vary show promising signals in their periodograms. Using optical follow-up photometry with the Skynet Robotic Telescope Network, we confirm p-mode pulsations in one of these targets, LAMOST J082517.99+113106.3, and report it as the most recent addition to the sdBV{sub r} class of variable stars.
LHC $τ$-rich Tests of Lepton-specific 2HDM for $(g-2)_μ$
Creators: name: Chun, Eung Jin
name: Kang, Zhaofeng
name: Takeuchi, Michihisa
name: Tsai, Yue-Lin Sming
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The lepton-sepcific (or type X) 2HDM (L2HDM) is an attractive new physics candidate explaining the muon $g-2$ anomaly requiring a light CP-odd boson $A$ and large $\tanβ$. This scenario leads to $τ$-rich signatures, such as $3τ$, $4τ$ and $4τ+W/Z$, which can be readily accessible at the LHC. We first study the whole L2HDM parameter space to identify allowed regions of extra Higgs boson masses as well as two couplings $λ_{hAA}$ and $ξ_h^l$ which determine the 125 GeV Higgs boson decays $h\to τ^+τ^-$ and $h\to AA/AA^*(τ^+τ^-)$, respectively. This motivates us to set up two regions of interest: (A) $m_A \ll m_{H} \sim m_{H^\pm}$, and (B) $m_A \sim m_{H^\pm} \sim {\cal O}(100) \mbox{GeV} \ll m_H$, for which derive the current constraints by adopting the chargino-neutralino search at the LHC8, and then analyze the LHC14 prospects by implementing $τ$-tagging algorithm. A correlated study of the upcoming precision determination of the 125 GeV Higgs boson decay properties as well as the observation of multi-tau events at the next runs of LHC will be able to shed light on the L2HDM option for the muon $g-2$.
description: 21 pages, 9 figures
Additional file 1 of COVID-19 and the transition to virtual teaching sessions in an orthopaedic surgery training program: a survey of resident perspectives
Creators: name: Kruse, Colin
name: Gouveia, Kyle
name: Thornley, Patrick
name: Yan, James R.
name: McCarthy, Colm
name: Chan, Teresa
name: Kishta, Waleed
name: Khanna, Vickas
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1.
Clustering community science data to infer songbird migratory connectivity in the Western Hemisphere
Creators: name: Vincent, Jaimie
Publisher: name: Open Science Framework
Year: 2022

description: Related to Vincent, Jaimie G., Schuster, Richard, Wilson, Scott, Fink, Daniel, and Bennett, Joseph R.. 2022. “ Clustering Community Science Data to Infer Songbird Migratory Connectivity in the Western Hemisphere.” Ecosphere 13( 4): e4011. https://doi.org/10.1002/ecs2.4011