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description Publicationkeyboard_double_arrow_right Preprint , Article 2019 United States, United Kingdom, ItalyAmerican Physical Society (APS) EC | COGS, NSF | Collaborative Research: E..., NSF | Physics Frontier Center a... +6 projectsEC| COGS ,NSF| Collaborative Research: Elements: Software: NSCI: HDR: Building An HPC/HTC Infrastructure For The Synthesis And Analysis Of Current And Future Cosmic Microwave Background Datasets ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| Exploring the Time-Varying Universe at Millimeter Wavelengths with the South Pole Telescope ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,ARC| Discovery Projects - Grant ID: DP150103208 ,NSF| Collaborative Research: The Dark Energy Survey Data Management Operations ,EC| COSMICDAWN ,EC| TESTDESrinivasan Raghunathan; S. Patil; Eric J. Baxter; Bradford Benson; Lindsey Bleem; T. M. Crawford; G. P. Holder; T. McClintock; Christian L. Reichardt; T. N. Varga; Nathan Whitehorn; Peter A. R. Ade; S. Allam; Adam Anderson; Jason E. Austermann; Santiago Avila; Jessica Avva; David Bacon; J. A. Beall; Amy N. Bender; Federico Bianchini; Sebastian Bocquet; David Brooks; D. L. Burke; John E. Carlstrom; J. Carretero; F. J. Castander; C. L. Chang; H. C. Chiang; Robert I. Citron; M. Costanzi; A. T. Crites; L. N. da Costa; Shantanu Desai; H. T. Diehl; J. P. Dietrich; Matt Dobbs; Peter Doel; S. Everett; August E. Evrard; Chang Feng; B. Flaugher; Pablo Fosalba; Joshua A. Frieman; Jason Gallicchio; Juan Garcia-Bellido; Enrique Gaztanaga; Elizabeth George; Tommaso Giannantonio; A. J. Gilbert; Robert A. Gruendl; J. Gschwend; Nikhel Gupta; G. Gutierrez; T. de Haan; N. W. Halverson; N. L. Harrington; Jason W. Henning; Gene C. Hilton; Devon L. Hollowood; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; N. Huang; Johannes Hubmayr; Kent D. Irwin; Tesla E. Jeltema; M. Carrasco Kind; Lloyd Knox; N. Kuropatkin; Ofer Lahav; Adrian T. Lee; Dale Li; Marcos Lima; A. E. Lowitz; M. A. G. Maia; Jennifer L. Marshall; Jeff McMahon; Peter Melchior; Felipe Menanteau; S. S. Meyer; Ramon Miquel; L. M. Mocanu; Joseph J. Mohr; Joshua Montgomery; C. Corbett Moran; Andrew Nadolski; T. Natoli; John P. Nibarger; G. I. Noble; Valentine Novosad; R. L. C. Ogando; Stephen Padin; A. A. Plazas; C. Pryke; David Rapetti; A. K. Romer; A. Roodman; A. Carnero Rosell; Eduardo Rozo; J. E. Ruhl; Eli S. Rykoff; Benjamin Saliwanchik; E. J. Sanchez; J. T. Sayre; V. Scarpine; K. K. Schaffer; Michael Schubnell; S. Serrano; I. Sevilla-Noarbe; C. Sievers; Graeme Smecher; Mathew Smith; Marcelle Soares-Santos; Antony A. Stark; K. T. Story; E. Suchyta; M. E. C. Swanson; Gregory Tarle; Carole Tucker; K. Vanderlinde; T. Veach; J. De Vicente; Joaquin Vieira; Vinu Vikram; Gensheng Wang; W. L. K. Wu; V. G. Yefremenko; Yanxi Zhang;pmid: 31763885
handle: 11368/2970925
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from stacked images formed by rotating the cluster-centered Stokes $Q/U$ map cutouts along the direction of the locally measured background CMB polarization gradient. Using data from the SPTpol 500 deg$^{2}$ survey at the locations of roughly 18,000 clusters with richness $\lambda \ge 10$ from the Dark Energy Survey (DES) Year-3 full galaxy cluster catalog, we detect lensing at $4.8\sigma$. The mean stacked mass of the selected sample is found to be $(1.43 \pm 0.4)\ \times 10^{14}\ {\rm M_{\odot}}$ which is in good agreement with optical weak lensing based estimates using DES data and CMB-lensing based estimates using SPTpol temperature data. This measurement is a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements. Comment: 10 pages, 3 figures, 1 table; typos fixed; accepted for publication in PRL
Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
visibility 0visibility views 0 download downloads 5 Powered bymore_vert Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020Oxford University Press (OUP) ARC | ARC Centres of Excellence..., UKRI | BRIdging Disciplines of G..., UKRI | Hertfordshire Astronomy 2... +2 projectsARC| ARC Centres of Excellence - Grant ID: CE170100013 ,UKRI| BRIdging Disciplines of Galactic Chemical Evolution (BRIDGCE): The Rise of the Chemical Elements ,UKRI| Hertfordshire Astronomy 2018-2021 ,NSF| Enabling a New Instrument 'IGRINS' for the Gemini South Telescope User Community ,NSF| MRI: Development of a High Resolution Infrared Spectrograph with a Large Spectral GraspAldo Mura-Guzmán; David Yong; C. Abate; Amanda I. Karakas; Chiaki Kobayashi; Heeyoung Oh; S. H. Chun; Gregory N. Mace;We present new fluorine abundance estimations in two carbon enhanced metal-poor (CEMP) stars, HE 1429-0551 and HE 1305+0007. HE 1429-0551 is also enriched in slow neutron-capture process (s-process) elements, a CEMP-s, and HE 1305+0007 is enhanced in both, slow and rapid neutron-capture process elements, a CEMP-s/r. The F abundances estimates are derived from the vibration-rotation transition of the HF molecule at 23358.6 A using high-resolution infrared spectra obtained with the Immersion Grating Infrared Spectrometer (IGRINS) at the 4m-class Lowell Discovery Telescope. Our results include a F abundance measurement in HE 1429-0551 of A(F) = +3.93 ([F/Fe] = +1.90) at [Fe/H] = -2.53, and a F upper limit in HE 1305+0007 of A(F) < +3.28 ([F/Fe] < +1.00) at [Fe/H] = -2.28. Our new derived F abundance in HE 1429-0551 makes this object the most metal-poor star where F has been detected. We carefully compare these results with literature values and state-of-the-art CEMP-s model predictions including detailed AGB nucleosynthesis and binary evolution. The modelled fluorine abundance for HE 1429-0551 is within reasonable agreement with our observed abundance, although is slightly higher than our observed value. For HE 1429-0551, our findings support the scenario via mass transfer by a primary companion during its thermally-pulsing phase. Our estimated upper limit in HE 1305+0007, along with data from the literature, shows large discrepancies compared with AGB models. The discrepancy is principally due to the simultaneous s- and r-process element enhancements which the model struggles to reproduce. 12 pages, 5 Figures -- Accepted in MNRAS
Monthly Notices of t... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2016American Chemical Society (ACS) ARC | Development of the next g...ARC| Development of the next generation of organo-mineral fertilisers utilising domestic and commercial waste productsAditya Rawal; Stephen Joseph; James M. Hook; C. H. Chia; Paul Munroe; Scott W. Donne; Yun Lin; David Phelan; David R. G. Mitchell; Ben Pace; Joseph Horvat; J. Beau W. Webber;pmid: 27284608
Dramatic changes in molecular structure, degradation pathway, and porosity of biochar are observed at pyrolysis temperatures ranging from 250 to 550 °C when bamboo biomass is pretreated by iron-sulfate-clay slurries (iron-clay biochar), as compared to untreated bamboo biochar. Electron microscopy analysis of the biochar reveals the infusion of mineral species into the pores of the biochar and the formation of mineral nanostructures. Quantitative (13)C nuclear magnetic resonance (NMR) spectroscopy shows that the presence of the iron clay prevents degradation of the cellulosic fraction at pyrolysis temperatures of 250 °C, whereas at higher temperatures (350-550 °C), the clay promotes biomass degradation, resulting in an increase in both the concentrations of condensed aromatic, acidic, and phenolic carbon species. The porosity of the biochar, as measured by NMR cryoporosimetry, is altered by the iron-clay pretreatment. In the presence of the clay, at lower pyrolysis temperatures, the biochar develops a higher pore volume, while at higher temperature, the presence of clay causes a reduction in the biochar pore volume. The most dramatic reduction in pore volume is observed in the kaolinite-infiltrated biochar at 550 °C, which is attributed to the blocking of the mesopores (2-50 nm pore) by the nonporous metakaolinite formed from kaolinite.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu142 citations 142 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2016IOP Publishing ARC | Representation theory of ..., NSERCARC| Representation theory of diagram algebras and logarithmic conformal field theory ,NSERCAuthors: Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;The central charge of the dimer model on the square lattice is still being debated in the literature. In this paper, we provide evidence supporting the consistency of a $c=-2$ description. Using Lieb's transfer matrix and its description in terms of the Temperley-Lieb algebra $TL_n$ at $\beta = 0$, we provide a new solution of the dimer model in terms of the model of critical dense polymers on a tilted lattice and offer an understanding of the lattice integrability of the dimer model. The dimer transfer matrix is analysed in the scaling limit and the result for $L_0-\frac c{24}$ is expressed in terms of fermions. Higher Virasoro modes are likewise constructed as limits of elements of $TL_n$ and are found to yield a $c=-2$ realisation of the Virasoro algebra, familiar from fermionic $bc$ ghost systems. In this realisation, the dimer Fock spaces are shown to decompose, as Virasoro modules, into direct sums of Feigin-Fuchs modules, themselves exhibiting reducible yet indecomposable structures. In the scaling limit, the eigenvalues of the lattice integrals of motion are found to agree exactly with those of the $c=-2$ conformal integrals of motion. Consistent with the expression for $L_0-\frac c{24}$ obtained from the transfer matrix, we also construct higher Virasoro modes with $c=1$ and find that the dimer Fock space is completely reducible under their action. However, the transfer matrix is found not to be a generating function for the $c=1$ integrals of motion. Although this indicates that Lieb's transfer matrix description is incompatible with the $c=1$ interpretation, it does not rule out the existence of an alternative, $c=1$ compatible, transfer matrix description of the dimer model. Comment: 54 pages. v2: minor corrections
Journal of Physics A... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu15 citations 15 popularity Average influence Average impulse Top 10% Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2015 CanadaPublic Library of Science (PLoS) SSHRC, ARC | Voyaging, Trade and the D..., ARC | The future of palaeoclima...SSHRC ,ARC| Voyaging, Trade and the Development of Ancient Complex Societies in East Polynesia: An Interdisciplinary Approach ,ARC| The future of palaeoclimate and archaeological research in Australia: next generation instrumentation for chronology and environmental reconstructionAuthors: David V. Burley; Kevan Edinborough; Marshall I. Weisler; Jian-xin Zhao;David V. Burley; Kevan Edinborough; Marshall I. Weisler; Jian-xin Zhao;First settlement of Polynesia, and population expansion throughout the ancestral Polynesian homeland are foundation events for global history. A precise chronology is paramount to informed archaeological interpretation of these events and their consequences. Recently applied chronometric hygiene protocols excluding radiocarbon dates on wood charcoal without species identification all but eliminates this chronology as it has been built for the Kingdom of Tonga, the initial islands to be settled in Polynesia. In this paper we re-examine and redevelop this chronology through application of Bayesian models to the questioned suite of radiocarbon dates, but also incorporating short-lived wood charcoal dates from archived samples and high precision U/Th dates on coral artifacts. These models provide generation level precision allowing us to track population migration from first Lapita occupation on the island of Tongatapu through Tonga’s central and northern island groups. They further illustrate an exceptionally short duration for the initial colonizing Lapita phase and a somewhat abrupt transition to ancestral Polynesian society as it is currently defined.
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For further information contact us at helpdesk@openaire.eu66 citations 66 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020Proceedings of the National Academy of Sciences ARC | Discovery Projects - Gran..., ARC | ARC Future Fellowships - ..., ARC | The genomics of adaptatio...ARC| Discovery Projects - Grant ID: DP150102903 ,ARC| ARC Future Fellowships - Grant ID: FT130101068 ,ARC| The genomics of adaptation to environmental change in an ecologically important non-model aquatic organismJonathan Sandoval-Castillo; Katie Gates; Chris J. Brauer; Steve Smith; Louis Bernatchez; Luciano B. Beheregaray;Resilience to environmental stressors due to climate warming is influenced by local adaptations, including plastic responses. The recent literature has focused on genomic signatures of climatic adaptation, but little is known about how plastic capacity may be influenced by biogeographic and evolutionary processes. We investigate phenotypic plasticity as a target of climatic selection, hypothesizing that lineages that evolved in warmer climates will exhibit greater plastic adaptive resilience to upper thermal stress. This was experimentally tested by comparing transcriptomic responses within and among temperate, subtropical, and desert ecotypes of Australian rainbowfish subjected to contemporary and projected summer temperatures. Critical thermal maxima were estimated, and ecological niches delineated using bioclimatic modeling. A comparative phylogenetic expression variance and evolution model was used to assess plastic and evolved changes in gene expression. Although 82% of all expressed genes were found in the three ecotypes, they shared expression patterns in only 5 out of 236 genes that responded to the climate change experiment. A total of 532 genes showed signals of adaptive (i.e., genetic-based) plasticity due to ecotype-specific directional selection, and 23 of those responded to projected summer temperatures. Network analyses demonstrated centrality of these genes in thermal response pathways. The greatest adaptive resilience to upper thermal stress was shown by the subtropical ecotype, followed by the desert and temperate ecotypes. Our findings indicate that vulnerability to climate change will be highly influenced by biogeographic factors, emphasizing the value of integrative assessments of climatic adaptive traits for accurate estimation of population and ecosystem responses. Significance Adaptation to climate change is expected to be influenced by thermal conditions experienced by species during their evolutionary history. We studied plastic capacity as a target of climatic selection, hypothesizing that populations that evolved under warmer climates have greater plastic adaptive resilience to climate change. This was tested experimentally by comparing upper thermal tolerance and gene expression in fish populations from desert, temperate, and subtropical regions of Australia. Divergent adaptive plastic responses to future climates were found across different bioregions, including in key heat stress genes. The greatest adaptive resilience was shown by the subtropical ecotype, followed by the desert and temperate ecotypes. These results have implications for large-scale assessments of climate impacts and for predictions of species distribution changes.
Europe PubMed Centra... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu38 citations 38 popularity Top 1% influence Average impulse Top 1% Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2019Elsevier BV ARC | ARC Future Fellowships - ...ARC| ARC Future Fellowships - Grant ID: FT180100652Miguel F. Frohlich; Timothy F. Smith; Chris Jacobson; Pedro Fidelman; Rosalynn Carter; Claudia Baldwin;Adaptive management has been advocated as an appropriate approach for the management of social-ecological systems, although its implementation has proven to be a challenge. Legal systems can hinder or facilitate adaptive management. Focusing on legal arrangements, this article explores how adaptive management can be better operationalised in the context of coastal management. Byron Shire, a local government area in New South Wales, Australia, was selected as a case study where we: (a) analysed how the concept of adaptive management has emerged within the evolution of coastal management and its applicable legal framework, and (b) identified juridical constraints to adaptive coastal management. Qualitative methods were used for the analysis of relevant documents and semi-structured interviews with 23 key informants. The results show that a distorted version of adaptive management has been adopted in Byron Shire's draft coastal management plans, which fails to adhere to the formal, structured, and iterative process of adaptive management. A legacy created by the legal effects of past decisions affecting coastal management has led to a path dependency towards protective measures to manage coastal erosion, constraining other management options, particularly managed realignment strategies. Failure to address juridical constraints in the early stages of the adaptive management process can result in stakeholder conflict and litigation. Overlitigation harms adaptive coastal management by pushing the decision-making process away from the pathway offered by the legal framework for preparing and implementing coastal management plans. After recent legislative coastal reform at the state level, there is momentum for the Byron Shire Council to refocus its adaptive management approach. However, overcoming existing juridical constraints will require adaptive governance, in which all levels of government must work collaboratively with the affected stakeholders in the design and implementation of the adaptive management process.
Ocean & Coastal Mana... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu15 citations 15 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
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You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.ocecoaman.2019.104909&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2021American Astronomical Society NSF | ZWICKY TRANSIENT FACILITY, NSF | Graduate Research Fellows..., NSF | CAREER: A Holistic Study ... +14 projectsNSF| ZWICKY TRANSIENT FACILITY ,NSF| Graduate Research Fellowship Program (GRFP) ,NSF| CAREER: A Holistic Study of Compact-Object Mergers across the Electromagnetic Spectrum ,NSF| REU Site: The Lamat Summer Research Program on High Performance Computing in Astrophysics ,NSF| Graduate Research Fellowship Program(GRFP) ,UKRI| UK Involvement in LSST: Phase B (QUB component) ,NSF| The Progenitors and Explosions of Type Ia Supernovae and Exotic Transients ,NSF| Gradute Research Fellowship Program (GRFP) ,UKRI| Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2020-2023 ,ARC| ARC Centres of Excellence - Grant ID: CE170100013 ,NSF| Collaborative Research: A Multi-Wavelength Observational and Theoretical Study of the Fastest Evolving Stellar Explosions ,UKRI| Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2017-2020 ,NSF| Next-Generation Supernova Cosmology ,NSF| Multiple Approaches to Multiple-Messenger Astronomy ,NSF| Pan-STARRS1: Operations; Public Data Release; Education and Outreach ,NSF| Graduate Research Fellowship Program (GRFP) ,EC| CR-GASDavid O. Jones; Ryan J. Foley; Gautham Narayan; Jens Hjorth; M. E. Huber; P. Aleo; Kate D. Alexander; C. R. Angus; Katie Auchettl; Vivienne Baldassare; S. H. Bruun; K. C. Chambers; Deep Chatterjee; Deanne L. Coppejans; D. A. Coulter; Lindsay DeMarchi; Georgios Dimitriadis; Maria R. Drout; Andrew Engel; K. D. French; Alexander Gagliano; Christa Gall; Tiara Hung; Luca Izzo; Wynn V. Jacobson-Galán; Charles D. Kilpatrick; Heidi Korhonen; Raffaella Margutti; S. I. Raimundo; Enrico Ramirez-Ruiz; Armin Rest; César Rojas-Bravo; Matthew R. Siebert; S. J. Smartt; K. W. Smith; Giacomo Terreran; Q. Wang; Radosław Wojtak; Adriano Agnello; Z. Ansari; N. Arendse; A. Baldeschi; P. K. Blanchard; D. Brethauer; J. S. Bright; J. S. Brown; T. J. L. de Boer; Sierra A. Dodd; J. R. Fairlamb; Claudio Grillo; A. Hajela; C. Hede; A. N. Kolborg; Jamie Law-Smith; C. C. Lin; E. A. Magnier; Konstantin Malanchev; David Matthews; Brenna Mockler; Daniel Muthukrishna; Y. C. Pan; Hugo Pfister; D. K. Ramanah; Sofia Rest; A. Sarangi; S. L. Schr der; Candice Stauffer; M. C. Stroh; Kirsty Taggart; S. Tinyanont; R. J. Wainscoat;Time domain science has undergone a revolution over the past decade, with tens of thousands of new supernovae (SNe) discovered each year. However, several observational domains, including SNe within days or hours of explosion and faint, red transients, are just beginning to be explored. Here, we present the Young Supernova Experiment (YSE), a novel optical time-domain survey on the Pan-STARRS telescopes. Our survey is designed to obtain well-sampled $griz$ light curves for thousands of transient events up to $z \approx 0.2$. This large sample of transients with 4-band light curves will lay the foundation for the Vera C. Rubin Observatory and the Nancy Grace Roman Space Telescope, providing a critical training set in similar filters and a well-calibrated low-redshift anchor of cosmologically useful SNe Ia to benefit dark energy science. As the name suggests, YSE complements and extends other ongoing time-domain surveys by discovering fast-rising SNe within a few hours to days of explosion. YSE is the only current four-band time-domain survey and is able to discover transients as faint $\sim$21.5 mag in $gri$ and $\sim$20.5 mag in $z$, depths that allow us to probe the earliest epochs of stellar explosions. YSE is currently observing approximately 750 square degrees of sky every three days and we plan to increase the area to 1500 square degrees in the near future. When operating at full capacity, survey simulations show that YSE will find $\sim$5000 new SNe per year and at least two SNe within three days of explosion per month. To date, YSE has discovered or observed 8.3% of the transient candidates reported to the International Astronomical Union in 2020. We present an overview of YSE, including science goals, survey characteristics and a summary of our transient discoveries to date. Comment: ApJ, in press; more information at https://yse.ucsc.edu/
arXiv.org e-Print Ar... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/abd7f5&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu44 citations 44 popularity Top 1% influence Average impulse Top 1% Powered by BIP!
more_vert arXiv.org e-Print Ar... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/abd7f5&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017Springer Science and Business Media LLC NSERC, EC | THREEPLE, ARC | Discovery Projects - Gran... +2 projectsNSERC ,EC| THREEPLE ,ARC| Discovery Projects - Grant ID: DP150104327 ,ARC| Quantum entanglement using slow-light-enhanced nonlinearity ,ARC| Nonlinear optical phononics: harnessing sound and light in nonlinear nanoscale circuitsLucia Caspani; Chunle Xiong; Benjamin J. Eggleton; Daniele Bajoni; Marco Liscidini; Matteo Galli; Roberto Morandotti; David J. Moss;AbstractThe ability to generate complex optical photon states involving entanglement between multiple optical modes is not only critical to advancing our understanding of quantum mechanics but will play a key role in generating many applications in quantum technologies. These include quantum communications, computation, imaging, microscopy and many other novel technologies that are constantly being proposed. However, approaches to generating parallel multiple, customisable bi- and multi-entangled quantum bits (qubits) on a chip are still in the early stages of development. Here, we review recent advances in the realisation of integrated sources of photonic quantum states, focusing on approaches based on nonlinear optics that are compatible with contemporary optical fibre telecommunications and quantum memory platforms as well as with chip-scale semiconductor technology. These new and exciting platforms hold the promise of compact, low-cost, scalable and practical implementations of sources for the generation and manipulation of complex quantum optical states on a chip, which will play a major role in bringing quantum technologies out of the laboratory and into the real world.
CORE (RIOXX-UK Aggre... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/lsa.2017.100&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu182 citations 182 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
visibility 17visibility views 17 download downloads 195 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/lsa.2017.100&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2018American Chemical Society (ACS) ARC | Discovery Early Career Re...ARC| Discovery Early Career Researcher Award - Grant ID: DE170100417Authors: Scarlett C. Southall; Steven Micklethwaite; Siobhan A. Wilson; Andrew J. Frierdich;Scarlett C. Southall; Steven Micklethwaite; Siobhan A. Wilson; Andrew J. Frierdich;Goethite (α-FeOOH) is a source and sink for trace elements in surficial environments. Its elemental and isotopic composition may be perturbed during recrystallization, particularly when accelerated by aqueous Fe(II), but the factors that control such reactivity and the extent to which it occurs are poorly understood. Here we react goethite samples of varying crystallinity in 57Fe-enriched Fe(II) solutions and detail the temporal distribution of the tracer isotope and the evolution of goethite crystallites. Consistent with earlier work, isotope exchange occurs between dissolved Fe(II) and goethite. By completely dissolving Fe(II)-reacted goethite in sequential steps while measuring the tracer isotope, we reconstructed the goethite recrystallized with time. Initially, the tracer isotope is enriched at the goethite surface. With continued reaction, however, the 57Fe tracer-isotope becomes distributed throughout the bulk goethite with an isotopic composition equal to that of Fe(II) dissolved in solution. Crys...
ACS Earth and Space ... arrow_drop_down ACS Earth and Space ChemistryArticle . 2018License: https://doi.org/10.15223/policy-029Data sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1021/acsearthspacechem.8b00100&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu28 citations 28 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
more_vert ACS Earth and Space ... arrow_drop_down ACS Earth and Space ChemistryArticle . 2018License: https://doi.org/10.15223/policy-029Data sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1021/acsearthspacechem.8b00100&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Preprint , Article 2019 United States, United Kingdom, ItalyAmerican Physical Society (APS) EC | COGS, NSF | Collaborative Research: E..., NSF | Physics Frontier Center a... +6 projectsEC| COGS ,NSF| Collaborative Research: Elements: Software: NSCI: HDR: Building An HPC/HTC Infrastructure For The Synthesis And Analysis Of Current And Future Cosmic Microwave Background Datasets ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| Exploring the Time-Varying Universe at Millimeter Wavelengths with the South Pole Telescope ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,ARC| Discovery Projects - Grant ID: DP150103208 ,NSF| Collaborative Research: The Dark Energy Survey Data Management Operations ,EC| COSMICDAWN ,EC| TESTDESrinivasan Raghunathan; S. Patil; Eric J. Baxter; Bradford Benson; Lindsey Bleem; T. M. Crawford; G. P. Holder; T. McClintock; Christian L. Reichardt; T. N. Varga; Nathan Whitehorn; Peter A. R. Ade; S. Allam; Adam Anderson; Jason E. Austermann; Santiago Avila; Jessica Avva; David Bacon; J. A. Beall; Amy N. Bender; Federico Bianchini; Sebastian Bocquet; David Brooks; D. L. Burke; John E. Carlstrom; J. Carretero; F. J. Castander; C. L. Chang; H. C. Chiang; Robert I. Citron; M. Costanzi; A. T. Crites; L. N. da Costa; Shantanu Desai; H. T. Diehl; J. P. Dietrich; Matt Dobbs; Peter Doel; S. Everett; August E. Evrard; Chang Feng; B. Flaugher; Pablo Fosalba; Joshua A. Frieman; Jason Gallicchio; Juan Garcia-Bellido; Enrique Gaztanaga; Elizabeth George; Tommaso Giannantonio; A. J. Gilbert; Robert A. Gruendl; J. Gschwend; Nikhel Gupta; G. Gutierrez; T. de Haan; N. W. Halverson; N. L. Harrington; Jason W. Henning; Gene C. Hilton; Devon L. Hollowood; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; N. Huang; Johannes Hubmayr; Kent D. Irwin; Tesla E. Jeltema; M. Carrasco Kind; Lloyd Knox; N. Kuropatkin; Ofer Lahav; Adrian T. Lee; Dale Li; Marcos Lima; A. E. Lowitz; M. A. G. Maia; Jennifer L. Marshall; Jeff McMahon; Peter Melchior; Felipe Menanteau; S. S. Meyer; Ramon Miquel; L. M. Mocanu; Joseph J. Mohr; Joshua Montgomery; C. Corbett Moran; Andrew Nadolski; T. Natoli; John P. Nibarger; G. I. Noble; Valentine Novosad; R. L. C. Ogando; Stephen Padin; A. A. Plazas; C. Pryke; David Rapetti; A. K. Romer; A. Roodman; A. Carnero Rosell; Eduardo Rozo; J. E. Ruhl; Eli S. Rykoff; Benjamin Saliwanchik; E. J. Sanchez; J. T. Sayre; V. Scarpine; K. K. Schaffer; Michael Schubnell; S. Serrano; I. Sevilla-Noarbe; C. Sievers; Graeme Smecher; Mathew Smith; Marcelle Soares-Santos; Antony A. Stark; K. T. Story; E. Suchyta; M. E. C. Swanson; Gregory Tarle; Carole Tucker; K. Vanderlinde; T. Veach; J. De Vicente; Joaquin Vieira; Vinu Vikram; Gensheng Wang; W. L. K. Wu; V. G. Yefremenko; Yanxi Zhang;pmid: 31763885
handle: 11368/2970925
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from stacked images formed by rotating the cluster-centered Stokes $Q/U$ map cutouts along the direction of the locally measured background CMB polarization gradient. Using data from the SPTpol 500 deg$^{2}$ survey at the locations of roughly 18,000 clusters with richness $\lambda \ge 10$ from the Dark Energy Survey (DES) Year-3 full galaxy cluster catalog, we detect lensing at $4.8\sigma$. The mean stacked mass of the selected sample is found to be $(1.43 \pm 0.4)\ \times 10^{14}\ {\rm M_{\odot}}$ which is in good agreement with optical weak lensing based estimates using DES data and CMB-lensing based estimates using SPTpol temperature data. This measurement is a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements. Comment: 10 pages, 3 figures, 1 table; typos fixed; accepted for publication in PRL
Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.123.181301&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
visibility 0visibility views 0 download downloads 5 Powered bymore_vert Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWall