Delivering Science: Effective Communications Skills to Become a Successful Scientist
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Effective communication skills are essential to scientists being successful. Scientists give talks, write papers and proposals; they must communicate with peers, students, policy makers, and the general public. This session discussed strategies and resources to help scientists become better communicators and how effective communication skills can support professional advancement. Presented at the 2015 SACNAS National Conference by Dr. Mónica I. Feliú-Mójer, Dr. Amy Vashlishan-Murray and Ms. Liz Neeley.
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This document discusses leadership in the 21st century and the need for innovation in schools. It argues that schools need to move beyond standardization and focus more on design, story, empathy and meaning. It provides examples of concepts from authors like Collins that could help define and measure success. The document suggests creating frameworks and opportunities for rigorous debate about challenging questions to stimulate cultural change. It proposes using Web 2.0 tools and social media to build curiosity and engage in real debates about technology and differentiation. The goal is to walk the talk of 21st century learning.
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Social Media for Scientists
Social media can be an invaluable tool to increase the impact and visibility of scientific research. For example, papers shared on social media have increased citations and downloads. Social media offers new ways to expand your professional network; connect with policymakers and the public; to communicate scientific research; and to advance your professional career. This session will provide 1) an introduction to social media platforms, particularly Twitter; 2) tangible examples of how social media use can benefit your research and career; and 3) resources and strategies to use social media effectively. Offered at the 2015 American Society for Cell Biology (ASCB) Annual Meeting.
Expand Your Network: How to Identify Advisors, Mentors, Sponsors and Collabo...
Expand Your Network: How to Identify Advisors, Mentors, Sponsors and Collabo...Monica Feliu-Mojer, Ph.D.
This workshop offered tips and advice on how you can support your career advancement by cultivating a professional and personal network by identifying advisors, mentors and sponsors. Presented at the 2015 SACNAS National Conference by Drs. Mary García-Cazarín, Yaihara Fortis-Santiago, Kermin Martínez-Hernández, Nahyr Rovira-Figueroa, and Mónica Feliú-Mójer.
Identity, Academia & Community: Research & Implications for Broadening Partic...
Identity, Academia & Community: Research & Implications for Broadening Partic...Monica Feliu-Mojer, Ph.D.
Social identity, or the intersection between race/ethnicity and gender identity, strongly influences women and underrepresented minority (URM) students’ interest and persistence in STEM. This session discussed recent research findings and discuss how they can be translated into programs and practices to broaden participation in STEM. Presented at the 2015 SACNAS National Conference by Dr. Paul Hernandez, Dr. Kenny Gibbs, Jr. and Dr. Giovanna Guerrero-Medina. Moderated by Dr. Mónica I. Feliú-Mójer and Dr. Yaihara Fortis-Santiago.Storytelling, Meaningful Connections and Making Science More Inclusive
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Communicating Science to Underserved Communities
Communicating science to underserved communities is important. Scientists can play a key role by contextualizing science and making it relevant and relatable through storytelling. Ciencia Puerto Rico is a model for this, as it leverages the scientific community to produce crowdsourced science content in Spanish for Puerto Rican media and communities. It has helped increase students' interest in science by providing local and relatable examples.
Women in Science: Challenges at the Intersection of Gender, Race & Culture
Presentation by Dr. Mónica I. Feliú-Mójer, Manager of Outreach, Department of Biostatistics, University of Washington, Seattle at open forum discussing the challenges faced by women in science, particularly at the intersection of gender, race and culture.
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Recently uploaded
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
Anti-Universe And Emergent Gravity and the Dark Universe
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
Methods of grain storage Structures in India.pdf
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Video mentioned at page no. 23 as summary for better understanding
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Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
Signatures of wave erosion in Titan’s coasts
The shorelines of Titan’s hydrocarbon seas trace flooded erosional landforms such as river valleys; however, it isunclear whether coastal erosion has subsequently altered these shorelines. Spacecraft observations and theo-retical models suggest that wind may cause waves to form on Titan’s seas, potentially driving coastal erosion,but the observational evidence of waves is indirect, and the processes affecting shoreline evolution on Titanremain unknown. No widely accepted framework exists for using shoreline morphology to quantitatively dis-cern coastal erosion mechanisms, even on Earth, where the dominant mechanisms are known. We combinelandscape evolution models with measurements of shoreline shape on Earth to characterize how differentcoastal erosion mechanisms affect shoreline morphology. Applying this framework to Titan, we find that theshorelines of Titan’s seas are most consistent with flooded landscapes that subsequently have been eroded bywaves, rather than a uniform erosional process or no coastal erosion, particularly if wave growth saturates atfetch lengths of tens of kilometers.
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Sustainable Land Management - Climate Smart AgricultureInternational Food Policy Research Institute- South Asia Office
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Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
Direct Seeded Rice - Climate Smart Agriculture
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Recently uploaded (20)
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Anti-Universe And Emergent Gravity and the Dark Universe
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Holsinger, Bruce W. - Music, body and desire in medieval culture [2001].pdf
Holsinger, Bruce W. - Music, body and desire in medieval culture [2001].pdf
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Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
Quality assurance B.pharm 6th semester BP606T UNIT 5
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Juaristi, Jon. - El canon espanol. El legado de la cultura española a la civi...
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Sustainable Land Management - Climate Smart Agriculture
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Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
Delivering Science: Effective Communications Skills to Become a Successful Scientist
- 7. www.cienciapr.org/yca • Professional Development • Career Advancement • Mentoring • Science Outreach
- 16. IMPORTANT 2 mins