Podcasts about oii

This week, Andrew is joined once again by the ever-ready, ever-fit Oli—because let's be honest, he's always on standby when the usual suspects drop the ball. Together, they take a deep dive into crate digging, both in the literal sense of flicking through dusty vinyl sleeves and in the modern-day algorithm-fueled digital rabbit hole of obscure musical discoveries.

Back in 2021, following calls for police reform after the murder of George Floyd, Washington state did something unique. Legislators created a state-funded agency to investigate instances of serious or fatal police use of force – even ones that had happened in the past. Many believe the Office of Independent Investigations has potential to improve trust between marginalized communities and law enforcement. But some say it's taking the office too long to get going. So far, the OII hasn't officially launched a single investigation. Melanie Henshaw, an Indigenous Affairs reporter at InvestigateWest, spoke to reform advocates and agency officials about the obstacles that are keeping the office from quickly meeting its intended purpose.  Thank you to the supporters of KUOW, you help make this show possible! If you want to help out, go to kuow.org/donate/soundsidenotes Soundside is a production of KUOW in Seattle, a proud member of the NPR Network. GUEST: Melanie Henshaw, Indigenous Affairs reporter for InvestigateWest RELATED LINKS: Three years, no investigations: A slow start for Washington office tasked with probing police violence - InvestigateWest  See omnystudio.com/listener for privacy information.

This week on Inside Olympia...Roger Rogoff, director of the state's Office of Independent Investigations, which is set to begin examining police deadly force cases.

How can you leverage the principles of physics to grow your business? In this episode, Rich sits down with Bob Rogers, CEO of Oii.ai and a PhD in physics who studied supermassive black holes. They discuss how Bob's background as a scientist informs how he thinks about business, how to know when to pivot in a startup, and how cross-pollinating ideas from different domains leads to innovation for customers and patent-worthy ideas. ---------Key Quotes:“It's literally just finding the right level of granularity and detail to tell your story effectively. And that's a physics concept, but it's also a storytelling concept, and it's a business concept for me.”“I've seen a couple of organizations just, we're putting AI into this, this, this, and this. And it's like, ooh, it's a huge mistake. Because you really want to think of it as just another tool. It's not like, oh, let's go hammer everything and see what happens, you wouldn't do that just because you got a new hammer, right?” “The main thing is, every single person in your organization has patents inside them. That's the starting point. Start with that mindset. Everybody has patents inside them.”“Here's the tricky thing about the pivot. When you're building a business, a bullseye is a two dimensional object, like X axis and Y axis. But in business, it's a multidimensional space. So you're pivoting two degrees in an unknown direction. You've got to figure out the orientation and the angle, which is why it's not simple.”Practice Makes Profit segment: How to use a prioritization matrix.The League of Strategic Minds segment [listener question]: What is the difference between strategic thinking and strategic planning? Winsight: Idea for Advantage segment:  Gary Kasparov, the  world chess champion from 1985 to 200, said, “What separates a winner from a loser at the grandmaster level is a willingness to do the unthinkable. A brilliant strategy is certainly a matter of intelligence, but intelligence without audacity is not enough. You must have the guts to explode the game, to upend your opponent's thinking, and in doing so, unnerve them.” What are you doing to explode the game in your field? What are you doing? That's innovative. That's different. And that's going to upend  your opponent's thinking.---------Time stamps:(00:42) Deep Dive Interview with Bob Rogers(49:54)  Practice Makes Profit(52:05) The League of Strategic Minds (53:50) Winsights, Ideas for Advantage  ---------Links:Submit a question for Rich to the League of Strategic Minds Bob Rogers LinkedInOii.aiRich Horwath on LinkedInRich Horwath on YouTubeRich Horwath on InstagramStrategic Thinking Institute WebsiteInc. Magazine's Top 4 book for 2024: STRATEGIC  BookNew executive development platform: Strategic Fitness System Sign up for Rich's free Strategic Thinker Newsletter[Subscribe to the Podcast] On Apple PodcastsOn Spotify---------

Oii, sou uma pessoa que gosta muito de animações, por isso decidi falar sobre minha obra favorita, Nana. Neste podcast tem um pequeno resumo do início da obra, opiniões minhas e algumas curiosidades, também pode ser considerado um convite para você assistir caso se interesse. Espero que gostem!

Legislative Review features highlights from Thursday's legislative activity (2/15/24).On this episode: A bill to authorize the WA Attorney General to investigate police deadly force incidents; a bill proposing public utility tax exemptions for green hydrogen; and a bill to make EpiPen more available in schools for emergency care for allergic reactions.

The Big 5 Model of Personality is perhaps the most consistently reliable model of personality used in research around the world. Focusing on the key elements of conscientiousness, agreeableness, neuroticism, openness to experience and extraversion, the Big 5 model has been applied to evaluate personality traits in my contexts including not least leadership. A recent paper – co-authored by our guest today on Brain for Business – Dr Fabian Braesemann – considered the Big 5 traits most commonly found in entrepreneurs and founders, assessing amongst other things what are the personality characteristics of typical of founders and how they contribute to start-up success.About our guest…Dr Fabian Braesemann is a Departmental Research Lecturer in AI & Work at the Oxford Internet Institute at the University of Oxford.Fabian's research focuses on the Science of Success. He uses data science methods to quantify the determinants of success in different fields:1. The Science of Success in Business2. Success and the Future of Work, and 3. Quantifying success online and offlineBefore Fabian started to work as a Departmental Research Lecturer at the OII, he worked as a Research Fellow & Data Scientist in the Future of Real Estate Initiative at the Saïd Business School, University of Oxford, and as a Data Scientist at the OII on projects that applied data science to understand human development and labour markets The article co-authored by Fabian is available here: https://www.nature.com/articles/s41598-023-41980-yThe 2019 Nature article discussed in the podcast (“Quantifying the dynamics of failure across science, startups and security” by Yin et al.) is available here: https://arxiv.org/pdf/1903.07562.pdfYou can find out more about Fabian via his Linkedin page (https://www.linkedin.com/in/fabian-braesemann-210645138/_ or else via the OII website (https://www.oii.ox.ac.uk/people/profiles/fabian-braesemann/) Hosted on Acast. See acast.com/privacy for more information.

This week on Inside Olympia ... It's been two years since lawmakers created an Office of Independent Investigations to investigate police deadly force incidents. How many investigators have been hired and trained and when will investigations begin? We get an update from Director Roger Rogoff.

Oii, me chamo Mirella, tenho 18 anos (faço 19 no dia 12/11), esse é o meu 3° ano tentando medicina, fiz enem apenas três vezes, a primeira vez no 3° ano do ensino médio em 2021, primeira vez como questionadora em 2022 e o enem de agora 2023 como questionado tbm. Conheci o método questiona através de uma conversa sobre cursinhos online com um amigo, na época que conversamos sobre estávamos no 3° ano do EM, já tinha decidido que iria assinar algum cursinho pro ano seguinte, mas estava pesquisando MUITOOOO para não perder dinheiro com oq não fosse me ajudar. Estudo em escola militar/estadual (o colegio militar da minha cidade pertence ao estado pois é da PM, alem disso é colegio público) desde o ensino fundamental II. O primeiro enem q fiz na vida eu já sabia que não ia conseguir passar em med devido as várias interferências que tive (pandemia, falta de apoio escolar e tudo mais) no meu último ano do colégio assim como todos os estudantes do colégio os professores tbm estavam perdidos, afinal ficamos o ano de 2020 INTEIRO sem aula nenhuma. Isso me deixou com uma lacuna enorme nos assuntos que deveria ter sido estudado no 2° do EM. E bom, quando comecei com o medo tô questiona em 2022 tive um pouco de insegurança, mas tinha decidido que ou eu aprendia, ou eu aprendia e a proposta do método me permitia ter uma maior flexibilidade nos estudos e me joguei de cabeça, msm com medo. Tive resultados ótimos, aumentei 102 pontos na média geral, e como consequência passei com bolsa de 50% na MELHOR faculdade particular de saúde da minha cidade, além de vários outros cursos na federal.

Oii, meu nome é Bruno tenho 27 anos e moro em Porto Alegre - RS. Minha primeira graduação foi Ciências Biológicas na UFRGS, queria muito ser Professor, comecei a dar aula aos 20 em pré vestibular e colégio e me formei aos 24. Logo percebi que queria fazer outra graduação, desde então entrei na Ed. Física, no Jornalismo e por fim na Odonto, todos na UFRGS. Mas percebi que não ia ter jeito, queria fazer Medicina e graças ao Questiona eu vi que era possível estudar de uma maneira eficiente, sem ter que voltar ao ambiente dos cursinhos. Desde o início do ano fui me desvinculando dos lugares onde eu trabalhava para conseguir me dedicar, fiz uma reserva financeira durante esses anos como prof. e atualmente to com total disposição e foco pra alcançar o meu objetivo, acho que é isso. :)

Oii, meu nome é Vivian, tenho 20 anos, estou no meu quarto ano de cursinho, entrei no método esse ano e finalmente consegui chegar nos 80% no ENEM, tenho buscado evoluir mais ainda e espero fazer minha entrevista de aprovação logo ❤️ Eu preciso conseguir evoluir nas provas mais difíceis, sinto muita dificuldade e encontro diversas lacunas teóricas, além de lidar com o cansaço, estou a 9 meses estudando direto, estou bem cansada

Oii, Sarah! Sou a Ágata, conheci o método no início do ano e foi a melhor coisa que me aconteceu! Quero Medicina e este já é o meu segundo ano tentando - ano passado eu estudei também, mas estava no terceiro ano.

Oii, meu nome é Jayane, @estudoroxo, tenho 20 anos, moro em Campina Grande - PB. Estou no meu quarto ano tentando passar em Medicina pelo ENEM, comecei a seguir as dicas da Sarah ano passado e depois do último ENEM assinei o método, o hospital me ajuda diariamente na caminhada até a prova.

Oii, Sarah ! Meu nome é Manuela, @manuzinhacom, tenho 22 anos e estou no meu quinto ano de preparação.  Dentro desse tempo, fiz dois anos de cursinho presencial e os outros dois anos estudei por conta. Entretanto, percebi uma queda no rendimento, além de ter tido um desânimo incessante por conta de não ver uma evolução no processo. Estagnei na casa dos 70% e não sabia como mudar isso, porque não tinha ninguém para me mostrar onde estava errando.  Ao começar o hospital este ano, isso mudou muito! Comecei a visualizar os pontos que realmente seriam diferenciais e estudar coisas que nesses quatro anos ainda não tinha aprendido. Tem sido incrível ver que não preciso ficar o dia todo em função do estudo e ainda assim ver pouco a pouco a evolução que eu não via por meio de outro método de estudo

Descriçawwwwwwww: Oii gente! No rap de hoje tem a ascensão do Threads, já aproveita pra seguir a gente lá rs. E sim também falamos sobre o assunto que deu o que falar neste fim de semana no Twitter e em todo lugar. IG do Podcast: @falagaypodcast | E-mail: falagaypodcast@gmail.com Hosts: @cleytonleite8 | @davidcsta @hiroshitakeuti --- Send in a voice message: https://podcasters.spotify.com/pod/show/falagaypodcast/message

Oii, suave na nave? Tranquilo como esquilo? De boa na lagoa? Se sim, por que não aprender alguma coisa nova e se aventurar no mundo da música? Se não, te garanto que conhecer um pouco sobre teoria musical vai te deixar suave!!! Te convido a escutar esse podcast feito com carinho, te garanto que você vai gostar, vamos lá? *Este podcast foi criado, elaborado e produzido pelos estudantes do segundo ano do Ensino Médio na Escola S Blumenau, em 2023. As aulas de Mídias Digitais são uma unidade curricular do STEAM e permitem que os estudantes desenvolvam habilidades voltadas à criação de roteiro, edição de áudio e design. O objetivo geral é compreender o funcionamento de diferentes linguagens e práticas culturais. Estamos na 3ª edição do projeto.

Oii, você assistiu a série da Rainha Charlotte no Netflix?⚠️Esse episódio contém spoilers! Veja 3 pontos fortes de autoestima baseados na personagem:1° Saber o que quer;2° Se posicionar e apoiar o que acredita;3° Sair do papel de vítima, entender que é capaz e não aceitar menos do que merece.E aí, gostou do episódio de hoje? Me siga no insta para mais dicas de Psicologia: @psicojessicarodriguez Abraço da psi Jéssica Rodriguez - CRP 01/21148 Agende sua sessão (61) 98258-6968

Bob Rogers, AI pioneer, entrpreneur, and author, started Oii in 2019 to automate supply chain design. The company uses advanced modeling and AI to optimize supply chain planning and automate the configuration of complex networks. Bob started his career as a Harvard physicist using neural networks to measure activity near black holes in deep space. During his 35 year career Bob has been a trailblazer in using AI to solve complex problems. He's also an Expert in Residence for AI at UCSF Smarter Health and was Chief Data Scientist in the Data Center Group at Intel as well as co-founder and Chief Scientist at Apixio, a Healthcare AI company. Additionally, he co-authored the books Artificial Neural Networks: Forecasting Time Series and “De-mystifying Big Data and Machine Learning for Healthcare“. Bob received his BA in physics at UC Berkeley and his PhD in physics at Harvard. Listen and learn...How neural nets work... from a pioneerWhat it was like to co-author a book with ChatGPTWhat surprised Bob most when he tested the boundaries of ChatGPTWhy ChatGPT spews credible nonsenseThe ethics of using generative AI to sell content derived from copyrighted materialsWhy ChatGPT became an instant global phenomenonHow OpenAI trained ChatGPT "to be nice"Is there another "AI winter" ahead?References in this episode:The book Bob co-authored with ChatGPTCan AI be an author of a publication in a scientific journal?Bob's previous book: Demystifying AI for the enterpriseStanford's Dr. Fei-Fei Li in conversation with OpenAI CTO Mira MuratiFuturists Peter Scott and David Wood on AI and the Future of WorkBob's company: Oii.ai

In 2020, the murder of George Floyd brought national attention to the use of deadly force by police throughout the country. In Washington state's legislature, the killing of Manuel Ellis by Tacoma Police helped propel a police reform package of more than a dozen bills. One of those bills created The Office of Independent Investigations, or OII. This is the first office of its kind in the nation, and it plans to train civilian investigators to watchdog the use of deadly force by police throughout the state.

Chemical abundances in the dwarf galaxy NGC 4163 based on the nebular and auroral emission lines by I. A. Zinchenko et al. on Wednesday 30 November We constructed an oxygen abundance map and N/O ratio map of the unusually low excitation dwarf irregular galaxy NGC 4163 based on publicly available spectroscopy obtained by the MaNGA survey. We detected auroral emission line [OII]$lambdalambda$7320,7330 which allows us to measure chemical abundance by direct T$_e$ method. We found that the scatter of the oxygen abundance derived by the strong line method is large. The oxygen abundances 12 + log(O/H) derived by strong line method vary from ~7.3 to ~7.8 with a mean value of ~7.55. The oxygen abundances derived in two apertures of 2 arcseconds by the direct T$_e$ method using our measurements of the O$^+$ auroral line is about 7.8 dex. The nitrogen-to-oxygen ratio log(N/O) of about -1.5 is typical value for a low metallicity galaxy, maybe slightly shifted towards higher N/O ratios with respect to the N/O values in the HII regions in nearby galaxies. An unusual negative trend between log(N/O) and oxygen abundance is detected. NGC 4163 is a gas-poor galaxy with a neutral atomic gas mass fraction of around 0.25. The oxygen abundance in the galaxy is only around 0.1 of the oxygen abundance potentially attainable in a galaxy with such a gas mass fraction. The low metallicity coupled with the low gas mass fraction implies that either the metallicity of the interstellar medium of the galaxy was reduced by pristine gas infall in the recent epoch or the evolution of this galaxy was accompanied by strong galactic winds. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15710v1

Chemical abundances in the dwarf galaxy NGC 4163 based on the nebular and auroral emission lines by I. A. Zinchenko et al. on Tuesday 29 November We constructed an oxygen abundance map and N/O ratio map of the unusually low excitation dwarf irregular galaxy NGC 4163 based on publicly available spectroscopy obtained by the MaNGA survey. We detected auroral emission line [OII]$lambdalambda$7320,7330 which allows us to measure chemical abundance by direct T$_e$ method. We found that the scatter of the oxygen abundance derived by the strong line method is large. The oxygen abundances 12 + log(O/H) derived by strong line method vary from ~7.3 to ~7.8 with a mean value of ~7.55. The oxygen abundances derived in two apertures of 2 arcseconds by the direct T$_e$ method using our measurements of the O$^+$ auroral line is about 7.8 dex. The nitrogen-to-oxygen ratio log(N/O) of about -1.5 is typical value for a low metallicity galaxy, maybe slightly shifted towards higher N/O ratios with respect to the N/O values in the HII regions in nearby galaxies. An unusual negative trend between log(N/O) and oxygen abundance is detected. NGC 4163 is a gas-poor galaxy with a neutral atomic gas mass fraction of around 0.25. The oxygen abundance in the galaxy is only around 0.1 of the oxygen abundance potentially attainable in a galaxy with such a gas mass fraction. The low metallicity coupled with the low gas mass fraction implies that either the metallicity of the interstellar medium of the galaxy was reduced by pristine gas infall in the recent epoch or the evolution of this galaxy was accompanied by strong galactic winds. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15710v1

This week we are joined by Bob Rogers and Trevor Miles.  Trevor Miles is one of the most revered thought leaders in the supply chain space. Throughout his career Trevor has worked for well-respected brands such as Kinaxis, i2 Technologies and SAP. What makes Trevor so unique is his global understanding of not only market needs but also customer requirements.  Bob Rogers is the co-founder and CEO of Oii.ai, an AI powered cognitive modelling solution, which is looking to help prevent supply chain disruption. Bob actually began his career as an astrophysicist before going on to work for the likes of Intel and AI Healthcare company, Apixio. Bob is now one the leading figures in the nascent world of Artificial Intelligence. On this week's episode Bob, Trevor and Maria discuss:   How Oii.ai can benefit the supply chain   Why the continued dissemination of AI is an inevitability  How close we are to being able to predict and navigate uncertainty  The ways in which businesses can support technological innovation  New episodes are released every Wednesday. Make sure to like and subscribe to the Transform Talks podcast never to miss the supply chain conversations that matter. ↓ Bob Rogers ↓ https://www.linkedin.com/in/bob-rogers-0a00441/ ↓ Trevor Miles ↓ https://www.linkedin.com/in/milesahead/ ↓ FOLLOW US ON LINKEDIN ↓ Maria Villablanca (Host) https://www.linkedin.com/in/mariavillablanca/ Transform Talks  https://www.linkedin.com/showcase/transform-talks/ ↓ FIND US ONLINE ↓ https://futureinsights.org/ https://futureinsights.org/transform-talks/ Get more on-demand supply chain content https://sctvplus.com/pages/sctv-individual Apply to be a guest on the show https://futureinsights.org/speaker-form/ Apply be a sponsor on the show https://futureinsights.org/sponsor-form/

EPISODE DESCRIPTION  My guests today are Vishnu Vyas and Bob Rogers, co-founders of OII. OII uses AI to deliver end-to-end supply chain modeling. It combines simulation with optimization to deliver cost-efficient supply chains.  They share their insights into how they help small businesses improve discards, inventory costs, and financing terms, and reduce chargebacks. Find more details about OII at www.oii.ai, or reach out directly to Bob Rogers at bob@oii.ai, or to Vishnu at vishnu@oii.ai.  SHOW NOTES  Find the guests and their bios on LinkedIn: Bob Rogers: https://www.linkedin.com/in/bob-rogers-0a00441/ Vishnu Vyas: https://www.linkedin.com/in/vishnuvyas/ Key topics   Introduction to today's episode and guests  How does OII help with Supply Chain optimization  OII Tech and the Observe, Measure, Optimize approach  Identifying supply chain failure modes using AI  Using OII to rate the resilience in your current supply chain  OII operating model  A few successful cases  CALL TO ACTION  Thank you for listening!  Follow me on Linkedin at https://www.linkedin.com/in/chandhrika/  Sharing is caring! Spread the word about this show to your network  Leave us a rating and feedback  Email me at chandhrika@source-refresh.com if you would like to be a guest on my show    

Question: what do black holes, AI, and digital twins of supply chains have in common? Answer: Bob Rogers, CEO of OII.ai - a company using AI to create digital twins of supply chains, allowing planners to quickly and accurately run what-if scenarios to improve their planning. And the black holes? Bob cut his AI teeth creating digital twins of black holes to understand what was happening around supermassive black holes in space.I invited him to come on the podcast to talk about how that work can be translated (many years later) into supply chain digital twins.He graciously agreed and we had a fascinating conversation covering how the research on black holes led to supply chain digital twins, how having a digital twin of your supply chain can help, and why an AI is necessary to do that. I learned loads, I hope you do too...If you have any comments/suggestions or questions for the podcast - feel free to leave me a voice message over on my SpeakPipe page or just send it to me as a direct message on Twitter/LinkedIn. Audio messages will get played (unless you specifically ask me not to).If you liked this show, please don't forget to rate and/or review it. It makes a big difference to help new people discover it. Thanks.Dev InterruptedWhat the smartest minds in engineering are thinking about, working on and investing in.Listen on: Apple Podcasts SpotifySupport the show

In 2020, the police-involved killings of Manuel Ellis in Tacoma and George Floyd in Minneapolis were two cases among many incidents across the nation which led to the recent establishment of the Office of Independent Investigations (OII) earlier this summer in Olympia. Signed into law by Governor Inslee, the OII is a civilian-led agency that conducts investigations into police-involved incidents of serious harm or death. The agency's creation offers an opportunity to improve public faith in police accountability.   In June 2022, Roger Rogoff became director of the new OII. Rogoff's career in the criminal justice system spans 27 years, including roles as judge in King County Superior Court as well as in the juvenile courts, and as both prosecuting and criminal defense attorney. In addition to serving as assistant U.S. attorney, Rogoff most recently served as legal counsel for Microsoft on matters of data privacy and public safety. As Gov. Inslee stated, “Roger's experiences make him exceptionally suited to lead an agency, independent of law enforcement or the governor's office, to investigate cases.”  In this episode, Rogoff details how the OII is working thoughtfully and efficiently to fulfill its mission. He explains the office's priorities for its first six months, law enforcement's response to the agency's creation, the way the OII will work with other parties, employment prospects, and how OII roles like family liaisons and community liaisons address the need for transparency around investigations of police use of force. 

Oii! aqui é o GeoCast, feito pelas alunas Lorena, Letícia, Bruna, Emilly, Manuela e Mariah do 8° ano B. O tema que vamos falar é sobre a geleira Thwaites, que é capaz de elevar o nível do mar em vários metros e está derretendo à medida que o planeta aquece. Espero que vocês gostem e lembre-se de compartilhar o podcast para que as pessoas tenham consciência e evitem o aquecimento global

Washington state is creating a first-in-the-nation independent state office which will investigate police use-of-force incidents. Host Austin Jenkins interviews Roger Rogoff, tapped by Gov. Jay Inslee to be the first director of the new Washington Office of Independent Investigations.

Oii meninas, tutupom? E no programa de hoje vamos receber nossa primeira convidada internacional, ela que abriu um espacinho na agenda de compromissos a blogueira, influenciadora, youtuber, cantora BLOGUEIRINHA! Vamos fofocar muito sobre vida, carreira, internet e muito mais. @blogueirinha @poddelas @boounzueta @tata

Oii meninas, tutupom? E no programa de hoje vamos receber nossa primeira convidada internacional, ela que abriu um espacinho na agenda de compromissos a blogueira, influenciadora, youtuber, cantora BLOGUEIRINHA! Vamos fofocar muito sobre vida, carreira, internet e muito mais. @blogueirinha @poddelas @boounzueta @tata

On the Origin of the Strong Optical Variability of Emission-line Galaxies by Ruqiu Lin et al. on Thursday 22 September Emission-line galaxies (ELGs) are crucial in understanding the formation and evolution of galaxies, while little is known about their variability. Here we report the study on the optical variability of a sample of ELGs selected in the COSMOS field, which has narrow-band observations in two epochs separated by $gtrsim$ 12 years. This sample was observed with Suprime-Cam (SC) and Hyper Suprime-Cam (HSC) on the $Subaru$ telescope in NB816 and $i'/i$ bands, respectively. After carefully removing the wing effect of a narrow-band filter, we check the optical variability in a sample of 181 spectroscopically confirmed ELGs. We find that 0 (0/68) Ha emitters, 11.9% (5/42) [OIII] emitters, and 0 (0/71) [OII] emitters show significant variability ($|Delta m_{NB}| geq 3,sigma_{Delta m_{NB,AGN}} = 0.20, mag$) in the two-epoch narrow-band observations. We investigate the presence of active galactic nucleus (AGN) in this variable ELG (var-ELG) sample with three methods, including X-ray luminosity, mid-infrared activity, and radio-excess. We find zero bright AGN in this var-ELG sample, but cannot rule out the contribution from faint AGN. We find that SNe could also dominate the variability of the var-ELG sample. The merger morphology shown in the HST/F814W images of all the var-ELG sample is in agreement with the enhancement of star formation, i.e., the SNe activity. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.07087v2

This week we are joined by Callum Cant, Author of Riding for Deliveroo, editor for NFP and Postdoc researcher at the OII, To discuss the recent Amazon wildcat strikes in the UK; why the british media is steadfastly ignoring them, and what they tell us about organising in the modern era. But first, why is it that the first month of september generates some of the most memorable tweets? Read Callum's piece on the strikes: https://notesfrombelow.org/article/mapping-amazon-strikes -------- This show is supported by Patreon. Sign up for as little as $5 a month to gain access to a new bonus episode every week, and our entire backlog of bonus episodes! Thats https://www.patreon.com/10kpostspodcast -------- Ten Thousand Posts is a show about how everything is posting. It's hosted by Hussein (@HKesvani), Phoebe (@PRHRoy) and produced by Devon (@Devon_onEarth).  

On the Origin of the Strong Optical Variability of Emission-line Galaxie by Ruqiu Lin et al. on Thursday 15 September Emission-line galaxies (ELGs) are crucial in understanding the formation and evolution of galaxies, while little is known about their variability. Here we report the study on the optical variability of a sample of ELGs selected in the COSMOS field, which has narrow-band observations in two epochs separated by $gtrsim$ 12 years. This sample was observed with Suprime-Cam (SC) and Hyper Suprime-Cam (HSC) on the $Subaru$ telescope in NB816 and $i'/i$ bands, respectively. After carefully removing the wing effect of a narrow-band filter, we check the optical variability in a sample of 181 spectroscopically confirmed ELGs. We find that 0 (0/68) Ha emitters, 11.9% (5/42) [OIII] emitters, and 0 (0/71) [OII] emitters show significant variability ($|Delta m_{NB}| geq 3,sigma_{Delta m_{NB,AGN}} = 0.20, mag$) in the two-epoch narrow-band observations. We investigate the presence of active galactic nucleus (AGN) in this variable ELG (var-ELG) sample with three methods, including X-ray luminosity, mid-infrared activity, and radio-excess. We find zero bright AGN in this var-ELG sample, but cannot rule out the contribution from faint AGN. We find that SNe could also dominate the variability of the var-ELG sample. The merger morphology shown in the HST/F814W images of all the var-ELG sample is in agreement with the enhancement of star formation, i.e., the SNe activity. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.07087v1

Statistical analysis of AlIII 1860 and CIII 1909 emission lines as virial black hole mass estimators in quasars by T. M. Buendia-Rios et al. on Tuesday 13 September We test the usefulness of the intermediate ionisation lines AlIII 1860 and CIII] 1909 as reliable virial mass estimators for quasars. We identify a sample of 309 quasars from the SDSS DR16 in the redshift range 1.2 < z < 1.4 to have [OII] 3728 recorded on the same spectrum of AlIII 1860, SiIII 1890, and CIII] 1909. We set the systemic quasar redshift using careful measurements of [OII]. We then classified the sources as Population A, extreme Population A (xA) and Population B, and analysed the 1900AA blend using multi-component models to look for systematic line shifts of the AlIII and CIII] along the quasar main sequence. We do not find significant shifts of the AlIII line peak in Pop. B and the wide majority of Pop. A. For Pop. xA, a small median blueshift of -250 km/s was observed, motivating a decomposition of the AlIII line profile into a virialized component centred at rest-frame and a blueshifted component for an outflow emission. For Pop. B objects, we proved the empirical necessity to fit a redshifted very broad component (VBC), clearly seen in CIII], and analysed the physical implications on a Pop. B composite spectrum using CLOUDY simulations. We find consistent black hole mass estimations using AlIII and CIII] as virial estimators for the bulk of Population A. AlIII (and even CIII]) is a reliable virial black hole mass estimator for Pop. A and B objects. xA sources deserve special attention due to the significant blueshifted excess observed in the line profile of AlIII, although not as large as those observed in CIV 1549. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.05526v1

Empirical constraints on the turbulence in QSO host nebulae from velocity structure function measurements by Mandy C. Chen et al. on Monday 12 September We present the first empirical constraints on the turbulent velocity field of the diffuse circumgalactic medium around four luminous QSOs at $z!approx!0.5$--1.1. Spatially extended nebulae of $approx!50$--100 physical kpc in diameter centered on the QSOs are revealed in [OII]$lambdalambda,3727,3729$ and/or [OIII]$lambda,5008$ emission lines in integral field spectroscopic observations obtained using MUSE on the VLT. We measure the second- and third-order velocity structure functions (VSFs) over a range of scales, from $lesssim!5$ kpc to $approx!20$--50 kpc, to quantify the turbulent energy transfer between different scales in these nebulae. While no constraints on the energy injection and dissipation scales can be obtained from the current data, we show that robust constraints on the power-law slope of the VSFs can be determined after accounting for the effects of atmospheric seeing, spatial smoothing, and large-scale bulk flows. Out of the four QSO nebulae studied, one exhibits VSFs in spectacular agreement with the Kolmogorov law, expected for isotropic, homogeneous, and incompressible turbulent flows. The other three fields exhibit a shallower decline in the VSFs from large to small scales but with loose constraints, in part due to a limited dynamic range in the spatial scales in seeing-limited data. For the QSO nebula consistent with the Kolmogorov law, we determine a turbulence energy cascade rate of $approx!0.2$ cm$^{2}$ s$^{-3}$. We discuss the implication of the observed VSFs in the context of QSO feeding and feedback in the circumgalactic medium. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.04344v1

SFR estimations from z=0 to z=0 9 -- A comparison of SFR calibrators for star-forming galaxies by M. Figueira et al. on Monday 12 September Using VIPERS, we estimated a set of SFR based on photometric and spectroscopic data. We used, as estimators, photometric bands from ultraviolet to mid-infrared, and spectral lines. Assuming a reference SFR obtained from the spectral energy distribution reconstructed with Code Investigating GALaxy Emission, we estimated the reliability of each band as an SFR tracer. We used GSWLC to trace the dependence of these SFR calibrators with redshift. The far and near UV, u-band and 24-$mu$m bands, as well as $L_{TIR}$, are found to be good SFR tracers up to $zsim0.9$ with a strong dependence on the attenuation prescription used for the bluest bands (scatter of SFR of 0.26, 0.14, 0.15, 0.23, and 0.24dex for VIPERS, and 0.25, 0.24, 0.09, 0.12, and 0.12dex for GSWLC). The 8-$mu$m band provides only a rough estimate of the SFR as it depends on metallicity and polycyclic aromatic hydrocarbon properties (scatter of 0.23dex for VIPERS). We estimated the scatter of rest-frame luminosity estimations from CIGALE to be 0.26, 0.14, 0.12, 0.15, and 0.20dex for FUV, NUV, ugriz, K$_{mathrm{s}}$, and 8-24$mu$m-$L_{mathrm{TIR}}$). At intermediate redshift, the H$beta$ line is a reliable SFR tracer (scatter of 0.19dex) and the [OII] line gives an equally good estimation when the metallicity from the $R_{23}$ parameter is taken into account (0.17 for VIPERS and 0.20dex for GSWLC). A calibration based on [OIII] retrieves the SFR only when additional information such as the metallicity or the ionization parameter of galaxies are used (0.26 for VIPERS and 0.20dex for GSWLC), diminishing its usability as a direct SFR tracer. Based on rest-frame luminosities estimated with CIGALE, we propose our own set of calibrations from FUV, NUV, u-band, 8, 24$mu$m, $L_{TIR}$, H$beta$, [OII], and [OIII]. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.04390v1

Empirical constraints on the turbulence in QSO host nebulae from velocity structure function measurements by Mandy C. Chen et al. on Monday 12 September We present the first empirical constraints on the turbulent velocity field of the diffuse circumgalactic medium around four luminous QSOs at $z!approx!0.5$--1.1. Spatially extended nebulae of $approx!50$--100 physical kpc in diameter centered on the QSOs are revealed in [OII]$lambdalambda,3727,3729$ and/or [OIII]$lambda,5008$ emission lines in integral field spectroscopic observations obtained using MUSE on the VLT. We measure the second- and third-order velocity structure functions (VSFs) over a range of scales, from $lesssim!5$ kpc to $approx!20$--50 kpc, to quantify the turbulent energy transfer between different scales in these nebulae. While no constraints on the energy injection and dissipation scales can be obtained from the current data, we show that robust constraints on the power-law slope of the VSFs can be determined after accounting for the effects of atmospheric seeing, spatial smoothing, and large-scale bulk flows. Out of the four QSO nebulae studied, one exhibits VSFs in spectacular agreement with the Kolmogorov law, expected for isotropic, homogeneous, and incompressible turbulent flows. The other three fields exhibit a shallower decline in the VSFs from large to small scales but with loose constraints, in part due to a limited dynamic range in the spatial scales in seeing-limited data. For the QSO nebula consistent with the Kolmogorov law, we determine a turbulence energy cascade rate of $approx!0.2$ cm$^{2}$ s$^{-3}$. We discuss the implication of the observed VSFs in the context of QSO feeding and feedback in the circumgalactic medium. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.04344v1

SFR estimations from z=0 to z=0 9 -- A comparison of SFR calibrators for star-forming galaxies by M. Figueira et al. on Monday 12 September Using VIPERS, we estimated a set of SFR based on photometric and spectroscopic data. We used, as estimators, photometric bands from ultraviolet to mid-infrared, and spectral lines. Assuming a reference SFR obtained from the spectral energy distribution reconstructed with Code Investigating GALaxy Emission, we estimated the reliability of each band as an SFR tracer. We used GSWLC to trace the dependence of these SFR calibrators with redshift. The far and near UV, u-band and 24-$mu$m bands, as well as $L_{TIR}$, are found to be good SFR tracers up to $zsim0.9$ with a strong dependence on the attenuation prescription used for the bluest bands (scatter of SFR of 0.26, 0.14, 0.15, 0.23, and 0.24dex for VIPERS, and 0.25, 0.24, 0.09, 0.12, and 0.12dex for GSWLC). The 8-$mu$m band provides only a rough estimate of the SFR as it depends on metallicity and polycyclic aromatic hydrocarbon properties (scatter of 0.23dex for VIPERS). We estimated the scatter of rest-frame luminosity estimations from CIGALE to be 0.26, 0.14, 0.12, 0.15, and 0.20dex for FUV, NUV, ugriz, K$_{mathrm{s}}$, and 8-24$mu$m-$L_{mathrm{TIR}}$). At intermediate redshift, the H$beta$ line is a reliable SFR tracer (scatter of 0.19dex) and the [OII] line gives an equally good estimation when the metallicity from the $R_{23}$ parameter is taken into account (0.17 for VIPERS and 0.20dex for GSWLC). A calibration based on [OIII] retrieves the SFR only when additional information such as the metallicity or the ionization parameter of galaxies are used (0.26 for VIPERS and 0.20dex for GSWLC), diminishing its usability as a direct SFR tracer. Based on rest-frame luminosities estimated with CIGALE, we propose our own set of calibrations from FUV, NUV, u-band, 8, 24$mu$m, $L_{TIR}$, H$beta$, [OII], and [OIII]. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.04390v1

Metal-Enriched Neutral Gas Reservoir around a Strongly-lensed, Low-mass Galaxy at z=4 Identified by JWST NIRISS and VLT MUSE by Xiaojing Lin et al. on Thursday 08 September Direct observations of low-mass, low-metallicity galaxies at $zgtrsim4$ provide an indispensable opportunity for detailed inspection of the ionization radiation, gas flow, and metal enrichment in sources similar to those that reionized the Universe. Combining the James Webb Space Telescope (JWST), VLT/MUSE, and ALMA, we present detailed observations of a strongly lensed, low-mass ($approx 10^{7.6}$ ${rm M}_odot$) galaxy at $z=3.98$ (also see Vanzella et al. 2022). We identify strong narrow nebular emission, including CIV $lambdalambda1548,1550$, HeII $lambda1640$, OIII] $lambdalambda1661,1666$, [NeIII] $lambda3868$, [OII] $lambda3727$, and Balmer series of Hydrogen from this galaxy, indicating a metal-poor HII region ($lesssim 0.12 {rm Z}_odot$) powered by massive stars. Further, we detect a metal-enriched damped Ly$alpha$ system (DLA) associated with the galaxy with the HI column density of $N_{rm{HI}}approx 10^{21.8}$ cm$^{-2}$. The metallicity of the associated DLA may reach the super solar metallicity (${gtrsim Z}_odot$). Moreover, thanks to JWST and gravitational lensing, we present the resolved UV slope ($beta$) map at the spatial resolution of $approx 100$ pc at $z=4$, with steep UV slopes reaching $beta approx -2.5$ around three star-forming clumps. Combining with low-redshift analogs, our observations suggest that low-mass, low-metallicity galaxies, which dominate reionization, could be surrounded by a high covering fraction of the metal-enriched, neutral-gaseous clouds. This implies that the metal enrichment of low-mass galaxies is highly efficient, and further support that in low-mass galaxies, only a small fraction of ionizing radiation can escape through the interstellar or circumgalactic channels with low column-density neutral gas. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.03376v1

Oii! Esse é o nosso primeiro devocional

Oii minhas Riquezas

#khangchienchongmy #chongmy1954 #nghethuatquansuthoichongmy Cuộc kháng chiến chống Mỹ, cứu nước của nhân dân ta đã trải qua hơn 2 thập kỷ, là cuộc chiến tranh cứu nước dài ngày nhất, ác liệt và phức tạp nhất trong lịch sử chống ngoại xâm của dân tộc Việt Nam. Trong cuộc chiến tranh lâu dài ấy, đế quốc Mỹ đã nhiều kéoII thất bại phải bị động thay đổi chiến lược; ta đánh thắng từng chiến lược chiến tranh của địch, giành thắng lợi từng bước làm thay đổi cục diện chiến trường, tiến tới giành thắng lợi hoàn toàn. --- Send in a voice message: https://anchor.fm/tu-dien-lich-su/message

Oii minhas Riquezas

Oii pessoal ! Tudo bem ? E ai, anda procastinando demais , esta sem foco e sem produtividade?! Vem comigo nesta dica incrível, uma técnica eficaz para seus estudos, trabalhos e projetos. Aproveitem a dica !

Oii gente, tudo bem? Estou muito feliz em finalmente voltar com mais um episódio :) Dessa vez, vamos falar sobre as pessoas com deficiência do movimento LGBT, como forma de continuarmos a discussão sobre sexualidade (abordada no primeiro episódio) e pensarmos em como os preconceitos se aplicam no Brasil. Espero que vocês gostem e compartilhem com os amigos. Para mais informações, acompanhe o @aacessibilizando no Instagram. Beijinhos!

Berlins Nummer 1! ... zumindest vorerst. Michel, OIi und Benni sprechen angeschlagen, nach negativen Testungen aber mit positiver Stimmung über alles rund um das Stadtmeisterschaftsspiel gegen die Tante aus Charlottenburg. Vom ersten und letzten Stuh... ähhh Toilettengang bis zum Abpfiff und drüber hinaus. Neu in dieser Episode: eine andere Variante der sportlichen Analyse.

This week Craig and Oliver sit down with the ever so talented OIi and Jenna from the band Frequency Within and talk about: Zoom Writing, Formation 2011, New years Bday, Covid Breaks, John the drummer, Elementary school band, PRS, Socal Indie Playlist, Hawaiian Gardens, DIY Merch, Building arcade cabinets, 72 VW buses, and much much more.

Oii, aqui é a Erika Souza, vem respirar comigo alguns minutinhos? Sente-se em uma postura confortável, alinha a coluna e bora lá.

"Oii galera, aqui é o Viola, shhhh, falem baixo porque ninguém sabe que eu tô por aqui... . É isso mesmo, eu vim aqui rapidão e escondido de todo mundo do UmDiaPod pra falar com vocês sobre esse negócio de GEEK, mas não conta pra ninguém, eles não podem saber ainda o que eu DESCOBRI !!! . Eu vou contar aqui pra vocês, nesse episódio de pílula de conhecimento. . O que eu descobri é algo bem interessante e que vai mudar toda a sua visão sobre os nerds e os geeks. . Sabia que não são a mesma coisa? Aliás, são universos beeeeeeem diferentes, mas mesmo assim os dois tem suas semelhanças. Ficou curioso?? . Vem comigo aqui nessa descoberta, mas vem rápido porque acho que o Renan tá chegando... . Conta aqui nos comentários o que você achou da minha descoberta Será que estou certo ou no caminho da verdade?? Qual a sua opinião sobre os mundos nerd e geek?? . Agora eu preciso ir galera, parece que o Renan já descobriu que eu tô aqui e eu preciso ir lá gravar o próximo episódio com ele. . Semana que vem continuamos com essa nossa conversa, fuuuuiiii!!!!"

Oii nesse episódio vou dar algumas dicas de como comprar fidget toys pela Internet! Espero que ajude❤

The internet has blurred the lines between the online and offline workforce. At Avory we calculate that there is roughly $700B in paid workers that could move some or all of their work to online platforms. We brought Fabian Stephany from the Oxford Internet Institute "OII" at the University of Oxford to discuss this revolution. Fabian is working on the iLabour Project at the OII studying the global dynamics of Online Labour Markets. Fabian holds a PhD and degrees in Economics and Social Sciences from different European institutions, including Universitá Bocconi Milan and University of Cambridge. iLabour Website: https://ilabour.oii.ox.ac.uk/online-labour-index Fabians Twitter: https://twitter.com/fabian_stephany --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app