Podcasts about transients

On today's podcast, a Japanese atomic bomb survivors group wins the 2024 Nobel Peace Prize; ways to improve your spelling on Ask a Teacher; what it means when you hear someone say: ‘When in Rome…' followed by 'Transients in Arcadia' by O. Henry on American Stories.

On today's podcast, a Japanese atomic bomb survivors group wins the 2024 Nobel Peace Prize; ways to improve your spelling on Ask a Teacher; what it means when you hear someone say: ‘When in Rome…' followed by 'Transients in Arcadia' by O. Henry on American Stories.

Seit den 1950er Jahren sind mehr als 5000 Sterne verschwunden. Wir wissen nicht, was da passiert ist. Was wir über das Verschwinden der Sterne vermuten, erfahrt ihr in der neuen Folge der Sternengeschichten. Wer den Podcast finanziell unterstützen möchte, kann das hier tun: Mit PayPal (https://www.paypal.me/florianfreistetter), Patreon (https://www.patreon.com/sternengeschichten) oder Steady (https://steadyhq.com/sternengeschichten)

Another Unsolved Mystery of the 50's this week, we take a look at the life of  recently departed Sergio Mendez and I will tell you the story of a moron I met this week.   www.cocktailnation.net   Alien Fashion Show- Rocket 95 Tikiyaki 5-0- The Ipcress File Alika Lyman Group-Theme from Bewitched Stanley Turrentine- Dearly Beloved Serge Gainsbourg- L'Eau A La Bouche  Towner Galaher- Simone Joey Altruda- Mucci's Jag MK. II Stereophonic Space Sound Unlimited- Inspector Cortez Daniel Pemberton- I, Spy Project K /67-Sirocco Sergio Mendez- The Joker Voodoo 5-Trust in Me Andre Basil-Latinova

Today we have a brilliant interview for you as we speak with a fabulous Early Career Researcher, Dr Lauren Rhodes from the University of Oxford. Lauren has just published a paper on the BOAT … the Brightest Object of All Time … a “Once in 10,000 year event” The blast, called GRB 221009A, was over 100 billion times brighter than the sun. Lauren works in powerful collaborations which use a variety of radio interferometers, such as MeerKAT and e-MERLIN to study the radio emissions from explosive celestial events including jets from X-ray binaries and gamma ray bursts. She is using multi wavelength observations of these sources to understand each event's jet physics and its surrounding environment. This stunning episode is available free from Audible Podcasts, Soundcloud, Apple podcasts and Youtube MP3 links and a full transcript for those who may prefer to read our interview, is published on Astrophiz.com

Have you ever wondered what does Enveloper do in Logic Pro or how to use an enveloper? Maybe you're seeking help with the topics: mixing drums in Logic Pro X,  essential drum mixing plugins, drum mixing tips, Logic Pro transient shaper, or maybe just overlooked Logic Pro tips and tricks. Then check out EP 145 of the Inside The Mix podcast.How can you transform a lifeless snare into a punchy element that drives your track forward? In this episode of Inside the Mix, I promise to guide you through the process of enhancing your snare drum's attack using tools like Logic's Enveloper transient shaper plugin. Expect practical, step-by-step techniques to manipulate transients and add that crucial snap, making your mix truly stand out.In this episode, I'll share essential tips on setting the threshold, look-ahead, and gain to achieve the best results. Hear the dramatic differences that different attack times and gain levels can make as we experiment live. Whether you're fine-tuning a snare, strings, or plucky instruments, this episode will equip you with the skills to bring initial transients to life and elevate your entire production. Don't miss out on these invaluable insights to transform your tracks.Send me a MessageSupport the Show.► ► ► WAYS TO CONNECT ► ► ► Grab your FREE Producer Growth Scorecard TODAY!✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸Are you READY to take on the 28-day challenge and release more music? Bag your FREE Producer Growth Scorecard at Synth Music Mastering: https://www.synthmusicmastering.com/scorecardBuy me a COFFEE✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸✸If you like what I do, buy me a coffee so I can create more amazing content for you: https://www.buymeacoffee.com/marcjmatthewsSend a DM through IG @insidethemicpodcastEmail me at marc@synthmusicmastering.comThanks for listening & happy producing!

Are you ready to uncover the mind-bending secrets of our universe? Join us as we reveal the unexpected truth about the formation of habitable planets and the potential for multiple habitable worlds within a single solar system. You won't believe how many habitable planets could exist in the perfect cosmic sweet spot. And as we delve deeper into this cosmic mystery, prepare to be amazed by the surprising possibility of habitable moons orbiting gas giants. The answer lies in the unexplored realms of our vast universe, waiting to be unraveled. Stay tuned for an eye-opening journey through the cosmos that will challenge everything you thought you knew about planetary systems and cosmological potential. Get ready to expand your understanding of the universe in ways you never imagined. In this episode, you will be able to: · Explore the mysteries of fast blue transient explosions and their impact on our understanding of the universe. · Discover the fascinating Glass Z 12 high-redshift galaxy, offering insights into the early universe and cosmic evolution. · Grasp the uncertainties in astronomy research and how they drive innovation and breakthrough discoveries. · Uncover the complexity of the early universe and gain a deeper appreciation for its profound impact on cosmic evolution. The bottom line is Dave's right to question this, because we can't guarantee what the universe is going to do. We don't have any sort of control over that. All we can do is observe what it's doing now, and through the magic of the fact that we can look back in time, we get a good idea of what it's done in the past. - Fred Watson Glass Z 12 High-Redshift Galaxy Glass Z 12 is a high-redshift galaxy, noted for its advanced state of maturity shortly after the Big Bang. Its study, largely facilitated by the GrISM lens Amplified Survey from Space (GLASS) using the James Webb Space Telescope, sheds light on the early universe's formation and evolution. Despite the advanced observational technology, the nature of such galaxies holds persisting enigmas, stimulating ongoing research and debates in the astronomical community. The resources mentioned in this episode are: · Visit spacenutspodcast.com to send in your text or audio questions for the show. · Subscribe to the Space Nuts podcast on Apple Podcasts, Spotify, iHeartRadio, or your favorite podcast player. · Stream on demand at bytes.com to listen to the latest episodes of Space Nuts. · Check out the Space Nuts YouTube channel and subscribe for more space-related content. · Explore the Space Nuts website for more information and to send voice messages to the hosts. Timestamped summary of this episode:00:00:00 - Introduction and Overview Andrew Dunkley introduces the episode as an all-audience questions episode. He mentions the topics to be discussed, including fast blue transients, ghost galaxies, and the heaviest isotopes in planet formation.00:02:23 - Fast Blue Transients and Galaxy Development Derek asks about the cause of fast blue optical transient explosions, referencing the unusual shape of the explosion. Fred Watson discusses the mysterious nature of fast blue optical transients and the potential reasons behind their unique properties.00:09:44 - Early Universe and Galaxy Evolution Renny inquires about the development of mature galaxies like glass z 13 in the early aftermath of the Big Bang. Fred Watson explains the significance of glass z 12 as an early galaxy and addresses the possibility of wormholes and membrane theory in relation to galaxy evolution.00:17:08 - Expansion of the Universe and Dark Energy Dave from Calgary asks about the expansion of the universe and its acceleration. He questions whether the universe will ever slow down due to dark energy. Fred Watson discusses the concept of dark energy and explains why the universe's expansion is unlikely to slow down.00:18:05 - Comparing Bullet Firing with Universe Expansion Discusses the analogy between bullet firing and universe expansion, highlighting the differences due to space conditions. Emphasizes the uncertainty of the universe's future.00:23:16 - Universe at Room Temperature Explores the time when the universe was at room temperature, highlighting the challenges in observing this period due to cosmic microwave background radiation.00:28:18 - Destruction of Black Holes Examines the possibility of black hole destruction, explaining the slow evaporation process through Hawking radiation and the extreme conditions required for their destruction.00:31:45 - Ghost Galaxies and Dark Matter Considers the relationship between normal matter in ghost galaxies and the existence of dark matter, emphasizing the minor impact on our understanding of dark matter in the universe.00:34:59 - Formation of Black Holes and Gravitons Discusses the theoretical concept of gravitons and their inability to clump together to form black holes, highlighting the distinction between force carrier bosons and matter particles.00:36:45 - Garrett's Question on Proto Earth Formation Garrett asks about the differentiation phase of proto-Earth's formation and why heavier isotopes did not sink to the center. Fred discusses nuclear fission on Earth and how it impacts the planet's activity and warmth.00:41:35 - Martin's Question on Habitability of Planets Martin asks about the maximum number of habitable planets in a solar system and the possibility of habitable moons orbiting a gas giant. Fred discusses the potential for multiple habitable planets and moons within a star's habitable zone.00:43:22 - Possibility of Multiple Habitable Planets Andrew and Fred explore the physics behind the number of habitable planets in a solar system and the potential for multiple habitable objects sharing the same orbit. They also touch on the definition of habitability and life.00:48:22 - Call for Questions and Social Media Engagement Andrew encourages listeners to send in their questions for future episodes and highlights the importance of social media engagement. Fred expresses enthusiasm for diverse and unexpected questions.00:49:34 - Conclusion and Farewell Andrew thanks Fred and Hugh, the studio engineer, for their participation in the episode. He wraps up the show and invites listeners to tune in for the next episode of Space Nuts.Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.

In Isaiah 43, God promises to walk with us through water and fire. In today's episode we will join Israel as we see firsthand, the power of God to not only go with Israel, but to guide them through difficulties into the Promised Land.

Rep David Martin is an American Republican politician from Michigan. He was elected to the Michigan House of Representatives from the 48th district in 2020, defeating incumbent representative Sheryl Kennedy. Prior to his role as state representative, Martin served on the Davison City Council. Update on Greyhound bus issue.

Get the links to each show here: http://JustinBarclay.com Get a free special report on the coming global financial reset and find out how to protect yourself and your family. http://JustinBarclay.com/GoldTry Cue Streaming for just $2 / day and help support the good guys https://justinbarclay.com/cueUp to 80% OFF! Use promo code JUSTIN http://MyPillow.com/Justin Patriots are making the Switch! What if we could start voting with our dollars too? http://SwitchWithJustin.com Grab gear in Justin's store http://JustinBarclay.com/store No matter what's coming, you can be ready for your family and others. http://PrepareWithJustin.com #ad Find Justin.. Podcast: https://www.iheart.com/podcast/53-westmichiganlivewith-28276509/?keyid%5B0%5D=West%20Michigan%20Live%20with%20Justin%20Barclay&pname=podcast_profile&sc=widget_share Rumble: https://rumble.com/c/JustinBarclay LOCALS: https://justinbarclay.locals.com Facebook: https://www.facebook.com/MrJustinBarclay Twitter: https://twitter.com/mrjustinbarclay Gettr: https://gettr.com/user/mrjustinbarclay Truth: https://truthsocial.com/@mrjustinbarclay Instagram: https://www.instagram.com/mrjustinbarclay Twitch: https://www.twitch.tv/mrjustinbarclay Gab: https://gab.com/MrJustinBarclay Tiktok: https://www.tiktok.com/@mrjustinbarclay Bitchute: https://www.bitchute.com/channel/OvxYfTftZdRk/ Brighteon: https://www.brighteon.com/channels/mrjustinbarclay Clouthub: https://app.clouthub.com/#/onboarding/?redirect=%2Fusers%2Fu%2Fmrjustinbarclay%2Fposts Substack: https://substack.com/profile/41993224-justin-barclay

Link to bioRxiv paper: http://biorxiv.org/cgi/content/short/2023.07.07.548109v1?rss=1 Authors: Parise, C. V., Ernst, M. Abstract: Audiovisual information reaches the brain via both sustained and transient input channels, representing signals' intensity over time or changes thereof, respectively. To date, it is unclear to what extent transient and sustained input channels contribute to the combined percept obtained through multisensory integration. Based on the results of two novel psychophysical experiments, here we demonstrate the importance of the transient (instead of the sustained) channel for the integration of audiovisual signals. To account for the present results, we developed a biologically-inspired, general-purpose model for multisensory integration, the Multisensory Correlation Detectors, which combines correlated input from unimodal transient channels. Besides accounting for the results of our psychophysical experiments, this model could quantitatively replicate several recent findings in multisensory research, as tested against a large collection of published datasets. In particular, the model could simultaneously account for the perceived timing of audiovisual events, multisensory facilitation in detection tasks, causality judgments, and optimal integration. All-in-all, this study demonstrates that several phenomena in multisensory research that were previously considered unrelated, all stem from the integration of correlated input from unimodal transient channels. Copy rights belong to original authors. Visit the link for more info Podcast created by Paper Player, LLC

On today's podcast you will hear about the growing popularity of food from Asia and Latin America; learn about the difference between 'finish' and 'complete' in a conversation and Ask A Teacher; then listen to American story 'Transients in Arcadia by O. Henry.

In 2020 astronomers spotted an object slowly getting brighter, but it wasn't until 2021 tha they quite understood how unusual it was. In 2021, they studied it in more detail, and found that it was something we don't think has ever been seen before. It was also the most energetic single event ever witnessed. Going by the catchy name of AT2021lwx, or simply "lwx" to its friends, this month we learn more about it. Dr Phil Wiseman, from University of Southampton, and Dr Cosimo Inserra, from Cardiff University, explain more. Elsewhere in the news, Chris North and Edward Gomez discuss how the JUICE mission has been jolting one of its antennas, the retirement of NASA's long-serving astronaut Peggy Whitson, and of course more from JWST.

0:00 -- Intro.1:51 -- Start of interview.2:44 -- On Larry's move from academia to private practice as Special Counsel in Mayer Brown's New York office. His writings in Mayer Brown's Across the Board's blog.4:58 -- His message at the 37th Annual Francis G. Pileggi Distinguished Lecture in Law at Delaware Law School to the state's corporate bench and bar. 9:02 --  Shareholder Typologies and demographics (long/short term, low/high conviction): Indexers, Transients, Activists and Quality Shareholders.14:51 -- Attributes of directors: #1 requirement is business savvy, per Warren Buffett. | Pat formulas in corporate governance, ie. check-the-box approach "mandated by central command": why they should be viewed with great skepticism.18:59 -- On the politicization of ESG, and Delaware's approach: "directors' fiduciary duties run to shareholders, but they may promote the interests of others when those are rationally related to shareholder interests.” Delaware VC Laster's opinion in McDonalds II (dismissing all shareholder claims that directors violated their oversight duties amid a toxic corporate culture.) 25:00 -- Some reasons for increase in ESG debate: 1) Declining trust in government, 2) Rising concern about climate change, 3) Powerful social movements, and 4) Powerful institutional asset managers leaning on ESG.  But Delaware remains a shareholder primacy state, "and that's a good thing", per former Chancellor of the Delaware Court of Chancery Andre Bouchard, now a partner at Paul Weiss partner, cited from a speech at a Directors' & Board event.27:00 -- Directors' personal values "don't matter at all" when it comes to fiduciary duties, "what matters is only what is best for the company [corporate interests]."30:58 -- On the SVB collapse, and the ongoing financial crisis (Silvergate, Signature, FRB, CS, etc). Larry's advice for boards who have been or could be affected, on the fundamentals of governance amid this heightened uncertainty. His firm's client alert: Maintaining Perspective: Governance and Disclosure Reminders for Public Companies. In the Vicinity of Insolvency: "When a company is insolvent, creditors may obtain standing to bring a derivative action on behalf of the company for breach of fiduciary duties. Although the fiduciary duties of care and loyalty to the company remain the same, the beneficiaries of those duties shift. Since it can be hard to tell in real time when a company becomes insolvent, directors of a company in the vicinity of insolvency should view their duties through the lens of the different beneficiaries of those fiduciary duties."36:07 -- The case of Credit Suisse's acquisition by UBS. The precedence of the US Government taking over AIG.40:11 -- On his article: "Share Buybacks, Directors Should Stick with Economics, Avoid Politics."46:32 -- On Warren Buffett, and whether the White House and/or bankers will seek him out for advise and/or dealmaking in this financial crisis: "He's waiting for the phone to ring with an attractive offer on the other end of the line."50:27 -- Final words of advice for directors: "Directors of public companies are stewards of a business and they need to act with business judgement and not on personal preferences, political and social issues of the day."Lawrence A. Cunningham is Special Counsel in Mayer Brown's New York office. Larry is a member of the firm's Capital Markets and Public Companies & Corporate Governance practices. Recognized as an authority on corporate governance and corporate law, Larry advises public companies and boards of directors in those areas and advises investment managers and shareholders on investor relations.If you like this show, please consider subscribing, leaving a review or sharing this podcast on social media. __ You can follow Larry on social media at:Twitter: @CunninghamProfLinkedIn: https://www.linkedin.com/in/lawrence-cunningham-68b7574b/__ You can follow Evan on social media at:Twitter: @evanepsteinLinkedIn: https://www.linkedin.com/in/epsteinevan/ Substack: https://evanepstein.substack.com/__Music/Soundtrack (found via Free Music Archive): Seeing The Future by Dexter Britain is licensed under a Attribution-Noncommercial-Share Alike 3.0 United States License

Link to bioRxiv paper: http://biorxiv.org/cgi/content/short/2023.02.01.526734v1?rss=1 Authors: Watabe, T., Yamahira, S., Takakura, K., Thumkeo, D., Narumiya, S., Matsuda, M., Terai, K. Abstract: Prostaglandin E2 (PGE2) is a key player in a plethora of physiological and pathological events. Nevertheless, little is known about the dynamics of PGE2 secretion from a single cell and its effect on the neighboring cells. Here, by observing confluent Madin-Darby canine kidney (MDCK) epithelial cells expressing fluorescent biosensors we demonstrate that calcium transients in a single cell cause PGE2-mediated radial spread of PKA activation (RSPA) in neighboring cells. By in vivo imaging, RSPA was also observed in the basal layer of the mouse epidermis. Experiments with an optogenetic tool revealed a switch-like PGE2 discharge in response to the increasing cytoplasmic Ca2+ concentrations. The cell density of MDCK cells correlated with the frequencies of calcium transients and the following RSPA. The ERK MAP kinase activation also enhanced the frequency of RSPA in MDCK and in vivo. Thus, the PGE2 discharge is regulated temporally by calcium transients and ERK activity. Copy rights belong to original authors. Visit the link for more info Podcast created by Paper Player, LLC

Guests Matt Hodson (MATTHS) artist, performer, educator Jamie Morden - Geosynths.com - patch designer, performer Video version on youtube: https://youtu.be/Ge81iGprXd0 For preshow and Ad free version and much more: Patreon.com/sonicstate The Future of Mastering is Ozone 10 - Master Assistant - match your mix to a reference file, Stabilizer - clarity with intelligent adaptive mastering EQ, Impact Module - micro dynamics adjustments to enhance the rhythmic content   Head over to iZotope.com  now to get a 7-day free trial and save with the code SONIC10   Babyaudio.com  - save 15% on any purchases of their range of creative effect plugins, designed to add color and depth to your mixes. When checking out, use the code ST15 00:00:00 SHOW START 00:09:37 Live Event 11th March - come along 00:10:33 SPL Transient Designer 4 MK2 00:17:34 AD: Baby Audio - Save 15% With ST15 Code 00:17:49 AD: Baby Audio - Save 15% With ST15 Code 00:18:47 Erica Synths takes on some Hex Inverters 00:37:41 AD: iZotope OZone 10 00:38:35 Importing Gear From Japan 00:53:16 JHVE asks via - [irc] - QQ Does that DX 7 MKII have stereo out? 00:55:12 McGurren asks via - Youtube -QQ what's your best synth / audio bargain? I once got a Yamaha CS40M for £60 and an SCI Pro One for £450 with a Juno 106 thrown in. 01:01:03 Nick Howes asks via - Youtube - QQ Now that both Korg and Arturia have released VST versions of current production hardware are the floodgates opening for more of the same Where to Watch/Listen - We now stream the live show to Youtube Live,  Facebook Live as well as at  Sonicstate.com/live every Weds at 4pm UK time- please do join in. Preshow available on Twitch. You can also download the audio version from RSS FEED 

The Spectroscopic Classification of Astronomical Transients SCAT Survey: Overview, Pipeline Description, Initial Results, and Future Plans by M. A. Tucker et al. on Wednesday 30 November We present the Spectroscopic Classification of Astronomical Transients (SCAT) survey, which is dedicated to spectrophotometric observations of transient objects such as supernovae and tidal disruption events. SCAT uses the SuperNova Integral-Field Spectrograph (SNIFS) on the University of Hawai'i 2.2-meter (UH2.2m) telescope. SNIFS was designed specifically for accurate transient spectrophotometry, including absolute flux calibration and host-galaxy removal. We describe the data reduction and calibration pipeline including spectral extraction, telluric correction, atmospheric characterization, nightly photometricity, and spectrophotometric precision. We achieve $lesssim 5%$ spectrophotometry across the full optical wavelength range ($3500-9000~r{A}$) under photometric conditions. The inclusion of photometry from the SNIFS multi-filter mosaic imager allows for decent spectrophotometric calibration ($10-20%$) even under unfavorable weather/atmospheric conditions. SCAT obtained $approx 640$ spectra of transients over the first 3 years of operations, including supernovae of all types, active galactic nuclei, cataclysmic variables, and rare transients such as superluminous supernovae and tidal disruption events. These observations will provide the community with benchmark spectrophotometry to constrain the next generation of hydrodynamic and radiative transfer models. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09322v2

GECAM Localization of High Energy Transients and the Systematic Error by Yi Zhao et al. on Wednesday 30 November Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a pair of microsatellites (i.e. GECAM-A and GECAM-B) dedicated to monitoring gamma-ray transients including gravitational waves high-energy electromagnetic counterparts, Gamma-ray Bursts, Soft Gamma-ray Repeaters, Solar Flares and Terrestrial Gamma-ray Flashes. Since launch in December 2020, GECAM-B has detected hundreds of astronomical and terrestrial events. For these bursts, localization is the key for burst identification and classification as well as follow-up observations in multi-wavelength. Here, we propose a Bayesian localization method with Poisson data with Gaussian background profile likelihood to localize GECAM bursts based on the burst counts distribution in detectors with different orientations. We demonstrate that this method can work well for all kinds of bursts, especially for extremely short ones. In addition, we propose a new method to estimate the systematic error of localization based on a confidence level test, which can overcome some problems of the existing method in literature. We validate this method by Monte Carlo simulations, and then apply it to a burst sample with accurate location and find that the mean value of the systematic error of GECAM-B localization is $sim 2.5^{circ}$. By considering this systematic error, we can obtain a reliable localization probability map for GECAM bursts. Our methods can be applied to other gamma-ray monitors. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15570v1

GECAM Localization of High Energy Transients and the Systematic Error by Yi Zhao et al. on Tuesday 29 November Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a pair of microsatellites (i.e. GECAM-A and GECAM-B) dedicated to monitoring gamma-ray transients including gravitational waves high-energy electromagnetic counterparts, Gamma-ray Bursts, Soft Gamma-ray Repeaters, Solar Flares and Terrestrial Gamma-ray Flashes. Since launch in December 2020, GECAM-B has detected hundreds of astronomical and terrestrial events. For these bursts, localization is the key for burst identification and classification as well as follow-up observations in multi-wavelength. Here, we propose a Bayesian localization method with Poisson data with Gaussian background profile likelihood to localize GECAM bursts based on the burst counts distribution in detectors with different orientations. We demonstrate that this method can work well for all kinds of bursts, especially for extremely short ones. In addition, we propose a new method to estimate the systematic error of localization based on a confidence level test, which can overcome some problems of the existing method in literature. We validate this method by Monte Carlo simulations, and then apply it to a burst sample with accurate location and find that the mean value of the systematic error of GECAM-B localization is $sim 2.5^{circ}$. By considering this systematic error, we can obtain a reliable localization probability map for GECAM bursts. Our methods can be applied to other gamma-ray monitors. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15570v1

The Spectroscopic Classification of Astronomical Transients SCAT Survey: Overview, Pipeline Description, Initial Results, and Future Plans by M. A. Tucker et al. on Tuesday 29 November We present the Spectroscopic Classification of Astronomical Transients (SCAT) survey, which is dedicated to spectrophotometric observations of transient objects such as supernovae and tidal disruption events. SCAT uses the SuperNova Integral-Field Spectrograph (SNIFS) on the University of Hawai'i 2.2-meter (UH2.2m) telescope. SNIFS was designed specifically for accurate transient spectrophotometry, including absolute flux calibration and host-galaxy removal. We describe the data reduction and calibration pipeline including spectral extraction, telluric correction, atmospheric characterization, nightly photometricity, and spectrophotometric precision. We achieve $lesssim 5%$ spectrophotometry across the full optical wavelength range ($3500-9000~r{A}$) under photometric conditions. The inclusion of photometry from the SNIFS multi-filter mosaic imager allows for decent spectrophotometric calibration ($10-20%$) even under unfavorable weather/atmospheric conditions. SCAT obtained $approx 640$ spectra of transients over the first 3 years of operations, including supernovae of all types, active galactic nuclei, cataclysmic variables, and rare transients such as superluminous supernovae and tidal disruption events. These observations will provide the community with benchmark spectrophotometry to constrain the next generation of hydrodynamic and radiative transfer models. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09322v2

GECAM Localization of High Energy Transients and the Systematic Error by Yi Zhao et al. on Tuesday 29 November Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a pair of microsatellites (i.e. GECAM-A and GECAM-B) dedicated to monitoring gamma-ray transients including gravitational waves high-energy electromagnetic counterparts, Gamma-ray Bursts, Soft Gamma-ray Repeaters, Solar Flares and Terrestrial Gamma-ray Flashes. Since launch in December 2020, GECAM-B has detected hundreds of astronomical and terrestrial events. For these bursts, localization is the key for burst identification and classification as well as follow-up observations in multi-wavelength. Here, we propose a Bayesian localization method with Poisson data with Gaussian background profile likelihood to localize GECAM bursts based on the burst counts distribution in detectors with different orientations. We demonstrate that this method can work well for all kinds of bursts, especially for extremely short ones. In addition, we propose a new method to estimate the systematic error of localization based on a confidence level test, which can overcome some problems of the existing method in literature. We validate this method by Monte Carlo simulations, and then apply it to a burst sample with accurate location and find that the mean value of the systematic error of GECAM-B localization is $sim 2.5^{circ}$. By considering this systematic error, we can obtain a reliable localization probability map for GECAM bursts. Our methods can be applied to other gamma-ray monitors. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15570v1

High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium by Zi-Hang Zhou et al. on Monday 28 November Various supernovae (SN), compact object coalescences, and tidal disruption events are widely believed to occur embedded in active galactic nuclei (AGN) accretion disks and generate detectable electromagnetic (EM) signals. We collectively refer to them as emph{AGN disk transients}. The inelastic hadronuclear ($pp$) interactions between shock-accelerated cosmic rays and AGN disk materials shortly after the ejecta shock breaks out of the disk can produce high-energy neutrinos. However, the expected efficiency of neutrino production would decay rapidly by adopting a pure Gaussian density atmosphere profile applicable for stable gas-dominated disks. On the other hand, AGN outflows and disk winds are commonly found around AGN accretion disks. In this paper, we present that the circum-disk medium would further consume the shock kinetic energy to more efficiently produce high-energy neutrinos, especially for $sim$,TeV$-$PeV neutrinos that IceCube is interested in. Thanks to the existence of the circum-disk medium, we find that the neutrino production will be enhanced significantly and make a much higher contribution to the diffuse neutrino background. Optimistically, $sim20%$ diffuse neutrino background can be contributed from AGN disk transients. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.13953v1

High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium by Zi-Hang Zhou et al. on Sunday 27 November Various supernovae (SN), compact object coalescences, and tidal disruption events are widely believed to occur embedded in active galactic nuclei (AGN) accretion disks and generate detectable electromagnetic (EM) signals. We collectively refer to them as emph{AGN disk transients}. The inelastic hadronuclear ($pp$) interactions between shock-accelerated cosmic rays and AGN disk materials shortly after the ejecta shock breaks out of the disk can produce high-energy neutrinos. However, the expected efficiency of neutrino production would decay rapidly by adopting a pure Gaussian density atmosphere profile applicable for stable gas-dominated disks. On the other hand, AGN outflows and disk winds are commonly found around AGN accretion disks. In this paper, we present that the circum-disk medium would further consume the shock kinetic energy to more efficiently produce high-energy neutrinos, especially for $sim$,TeV$-$PeV neutrinos that IceCube is interested in. Thanks to the existence of the circum-disk medium, we find that the neutrino production will be enhanced significantly and make a much higher contribution to the diffuse neutrino background. Optimistically, $sim20%$ diffuse neutrino background can be contributed from AGN disk transients. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.13953v1

Daksha: On Alert for High Energy Transients by Varun Bhalerao et al. on Wednesday 23 November We present Daksha, a proposed high energy transients mission for the study of electromagnetic counterparts of gravitational wave sources, and gamma ray bursts. Daksha will comprise of two satellites in low earth equatorial orbits, on opposite sides of earth. Each satellite will carry three types of detectors to cover the entire sky in an energy range from 1 keV to >1 MeV. Any transients detected on-board will be announced publicly within minutes of discovery. All photon data will be downloaded in ground station passes to obtain source positions, spectra, and light curves. In addition, Daksha will address a wide range of science cases including monitoring X-ray pulsars, studies of magnetars, solar flares, searches for fast radio burst counterparts, routine monitoring of bright persistent high energy sources, terrestrial gamma-ray flashes, and probing primordial black hole abundances through lensing. In this paper, we discuss the technical capabilities of Daksha, while the detailed science case is discussed in a separate paper. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12055v1

Science with the Daksha High Energy Transients Mission by Varun Bhalerao et al. on Wednesday 23 November We present the science case for the proposed Daksha high energy transients mission. Daksha will comprise of two satellites covering the entire sky from 1~keV to $>1$~MeV. The primary objectives of the mission are to discover and characterize electromagnetic counterparts to gravitational wave source; and to study Gamma Ray Bursts (GRBs). Daksha is a versatile all-sky monitor that can address a wide variety of science cases. With its broadband spectral response, high sensitivity, and continuous all-sky coverage, it will discover fainter and rarer sources than any other existing or proposed mission. Daksha can make key strides in GRB research with polarization studies, prompt soft spectroscopy, and fine time-resolved spectral studies. Daksha will provide continuous monitoring of X-ray pulsars. It will detect magnetar outbursts and high energy counterparts to Fast Radio Bursts. Using Earth occultation to measure source fluxes, the two satellites together will obtain daily flux measurements of bright hard X-ray sources including active galactic nuclei, X-ray binaries, and slow transients like Novae. Correlation studies between the two satellites can be used to probe primordial black holes through lensing. Daksha will have a set of detectors continuously pointing towards the Sun, providing excellent hard X-ray monitoring data. Closer to home, the high sensitivity and time resolution of Daksha can be leveraged for the characterization of Terrestrial Gamma-ray Flashes. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12052v1

Daksha: On Alert for High Energy Transients by Varun Bhalerao et al. on Tuesday 22 November We present Daksha, a proposed high energy transients mission for the study of electromagnetic counterparts of gravitational wave sources, and gamma ray bursts. Daksha will comprise of two satellites in low earth equatorial orbits, on opposite sides of earth. Each satellite will carry three types of detectors to cover the entire sky in an energy range from 1 keV to >1 MeV. Any transients detected on-board will be announced publicly within minutes of discovery. All photon data will be downloaded in ground station passes to obtain source positions, spectra, and light curves. In addition, Daksha will address a wide range of science cases including monitoring X-ray pulsars, studies of magnetars, solar flares, searches for fast radio burst counterparts, routine monitoring of bright persistent high energy sources, terrestrial gamma-ray flashes, and probing primordial black hole abundances through lensing. In this paper, we discuss the technical capabilities of Daksha, while the detailed science case is discussed in a separate paper. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12055v1

Science with the Daksha High Energy Transients Mission by Varun Bhalerao et al. on Tuesday 22 November We present the science case for the proposed Daksha high energy transients mission. Daksha will comprise of two satellites covering the entire sky from 1~keV to $>1$~MeV. The primary objectives of the mission are to discover and characterize electromagnetic counterparts to gravitational wave source; and to study Gamma Ray Bursts (GRBs). Daksha is a versatile all-sky monitor that can address a wide variety of science cases. With its broadband spectral response, high sensitivity, and continuous all-sky coverage, it will discover fainter and rarer sources than any other existing or proposed mission. Daksha can make key strides in GRB research with polarization studies, prompt soft spectroscopy, and fine time-resolved spectral studies. Daksha will provide continuous monitoring of X-ray pulsars. It will detect magnetar outbursts and high energy counterparts to Fast Radio Bursts. Using Earth occultation to measure source fluxes, the two satellites together will obtain daily flux measurements of bright hard X-ray sources including active galactic nuclei, X-ray binaries, and slow transients like Novae. Correlation studies between the two satellites can be used to probe primordial black holes through lensing. Daksha will have a set of detectors continuously pointing towards the Sun, providing excellent hard X-ray monitoring data. Closer to home, the high sensitivity and time resolution of Daksha can be leveraged for the characterization of Terrestrial Gamma-ray Flashes. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12052v1

Glasses Malone joined by Aja and Britt discuss the issue of transients and some of the root causes of this ongoing crisis which compromise quality of life. Rate, subscribe, comment and share. Follow NC on IG @GlassesLoc @AjaTheRedHead @RealBritneyMichelleSee omnystudio.com/listener for privacy information.

The second set of pulsar discoveries by CHIME FRB Pulsar: 14 Rotating Radio Transients and 7 pulsars by Fengqiu Adam Dong et al. on Tuesday 18 October The Canadian Hydrogen Mapping Experiment (CHIME) is a radio telescope located in British Columbia, Canada. The large field of view (FOV) of $sim$ 200 square degrees has enabled the CHIME/FRB instrument to produce the largest FRB catalog to date. The large FOV also allows CHIME/FRB to be an exceptional pulsar and Rotating Radio Transient (RRAT) finding machine, despite saving only the metadata information of incoming Galactic events. We have developed a pipeline to search for pulsars/RRATs using DBSCAN, a clustering algorithm. Output clusters are then inspected by a human for pulsar/RRAT candidates and follow-up observations are scheduled with the more sensitive CHIME/Pulsar instrument. The CHIME/Pulsar instrument is capable of a near-daily search mode observation cadence. We have thus developed the CHIME/Pulsar Single Pulse Pipeline to automate the processing of CHIME/Pulsar search mode data. We report the discovery of 21 new Galactic sources, with 14 RRATs, 6 regular slow pulsars and 1 binary system. Owing to CHIME/Pulsar's daily observations we have obtained timing solutions for 8 of the 14 RRATs along with all the regular pulsars. This demonstrates CHIME/Pulsar's ability at finding timing solutions for transient sources. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09172v1

The Spectroscopic Classification of Astronomical Transients SCAT Survey: Overview, Pipeline Description, Initial Results, and Future Plans by M. A. Tucker et al. on Tuesday 18 October We present the Spectroscopic Classification of Astronomical Transients (SCAT) survey, which is dedicated to spectrophotometric observations of transient objects such as supernovae and tidal disruption events. SCAT uses the SuperNova Integral-Field Spectrograph (SNIFS) on the University of Hawai'i 2.2-meter (UH2.2m) telescope. SNIFS was designed specifically for accurate transient spectrophotometry, including absolute flux calibration and host-galaxy removal. We describe the data reduction and calibration pipeline including spectral extraction, telluric correction, atmospheric characterization, nightly photometricity, and spectrophotometric precision. We achieve $lesssim 5%$ spectrophotometry across the full optical wavelength range ($3500-9000~r{A}$) under photometric conditions. The inclusion of photometry from the SNIFS multi-filter mosaic imager allows for decent spectrophotometric calibration ($10-20%$) even under unfavorable weather/atmospheric conditions. SCAT obtained $approx 650$ spectra of transients over the first 3 years of operations, including supernovae of all types, active galactic nuclei, cataclysmic variables, and rare transients such as superluminous supernovae and tidal disruption events. These observations will provide the community with benchmark spectrophotometry to constrain the next generation of hydrodynamic and radiative transfer models. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09322v1

The second set of pulsar discoveries by CHIME FRB Pulsar: 14 Rotating Radio Transients and 7 pulsars by Fengqiu Adam Dong et al. on Tuesday 18 October The Canadian Hydrogen Mapping Experiment (CHIME) is a radio telescope located in British Columbia, Canada. The large field of view (FOV) of $sim$ 200 square degrees has enabled the CHIME/FRB instrument to produce the largest FRB catalog to date. The large FOV also allows CHIME/FRB to be an exceptional pulsar and Rotating Radio Transient (RRAT) finding machine, despite saving only the metadata information of incoming Galactic events. We have developed a pipeline to search for pulsars/RRATs using DBSCAN, a clustering algorithm. Output clusters are then inspected by a human for pulsar/RRAT candidates and follow-up observations are scheduled with the more sensitive CHIME/Pulsar instrument. The CHIME/Pulsar instrument is capable of a near-daily search mode observation cadence. We have thus developed the CHIME/Pulsar Single Pulse Pipeline to automate the processing of CHIME/Pulsar search mode data. We report the discovery of 21 new Galactic sources, with 14 RRATs, 6 regular slow pulsars and 1 binary system. Owing to CHIME/Pulsar's daily observations we have obtained timing solutions for 8 of the 14 RRATs along with all the regular pulsars. This demonstrates CHIME/Pulsar's ability at finding timing solutions for transient sources. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09172v1

Sam Harris talks about his thoughts on grass, transients and mongrels.

It was an interesting week for both Marshall and Aaron. Aaron finally gets in some story telling time and the transient that came to his house spurred the first topic for this week's discussion. We know its a long one but its worth the listen as Marshall and Aaron discuss one of their favorite versus.  We finally are working with an amazing song artist ZAK TINDAL and featuring his music at the end of the podcast. Make sure to follow the link below and show him some LOVE as he definitely deserves it. We here at Undaunted Pursuit want to extend a huge THANK YOU for his support!  https://linktr.ee/zaktindal @Zaktindal | Linktree

A young woman of obvious class is enjoying a week's stay and an escape from the summer heat at a posh New York City Hotel when she meets a debonair young man who has similar interests. NEW) 1001 Stories From The Old West (Spotify)- https://open.spotify.com/show/0c2fc0cGwJBcPfyC8NWNTw 1001 Stories from Roy's Diner on Player.fm: Follow Us https://player.fm/series/1001-stories-network 1001 Radio Days right here at Google Podcasts FREE: https://podcasts.google.com/search/1001%20radio%20days 1001 Classic Short Stories & Tales at Google Podcasts https://podcasts.google.com/feed/aHR0cHM6Ly9mZWVkcy5tZWdhcGhvbmUuZm0vQURMNzU3MzM0Mjg0NQ== 1001 Heroes, Legends, Histories & Mysteries at Google Podcasts: https://podcasts.google.com/search/1001%20heroes 1001 Sherlock Holmes Stories (& Tales from Arthur Conan Doyle) https://podcasts.google.com/search/1001%20sherlock%20holmes 1001 Ghost Stories & Tales of the Macabre on Spotify: https://podcasts.google.com/search/1001%20ghost%20stories 1001 Stories for the Road on Google Podcasts https://podcasts.google.com/search/1001%20stories%20for%20the%20road Enjoy 1001 Greatest Love Stories on Google Podcasts https://podcasts.google.com/search/1001%20greatest%20love%20stories 1001 History's Best Storytellers: (author interviews) on Stitcher https://www.stitcher.com/show/1001-historys-best-storytellers APPLE USERS (NEW) 1001 Stories From The Old West- https://podcasts.apple.com/us/podcast/1001-stories-from-the-old-west/id1613213865 1001 Stories From Roy's Diner at Apple Podcasts https://podcasts.apple.com/fi/podcast/1001-stories-from-roys-diner/id1594740377 Catch 1001 Heroes on any Apple Device here (Free): https://podcasts.apple.com/us/podcast/1001-heroes-legends-histories-mysteries-podcast/id956154836?mt=2  Catch 1001 CLASSIC SHORT STORIES at Apple Podcast App Now: https://podcasts.apple.com/us/podcast/1001-classic-short-stories-tales/id1078098622 Catch 1001 Stories for the Road at Apple Podcast now:  https://podcasts.apple.com/us/podcast/1001-stories-for-the-road/id1227478901 NEW Enjoy 1001 Greatest Love Stories on Apple Devices here: https://podcasts.apple.com/us/podcast/1001-greatest-love-stories/id1485751552 Catch 1001 RADIO DAYS now at Apple iTunes!  https://itunes.apple.com/us/podcast/1001-radio-days/id1405045413?mt=2 NEW 1001 Ghost Stories & Tales of the Macabre is now playing at Apple Podcasts! https://podcasts.apple.com/us/podcast/1001-ghost-stories-tales-of-the-macabre/id1516332327 NEW Enjoy 1001 History's Best Storytellers (Interviews) on Apple Devices here: https://podcasts.apple.com/us/podcast/1001-historys-best-storytellers/id1483649026 NEW Enjoy 1001 Sherlock Holmes Stories and The Best of Arthur Conan Doyle https://podcasts.apple.com/us/podcast/1001-sherlock-holmes-stories-best-sir-arthur-conan/id1534427618 Get all of our shows at one website: https://.1001storiespodcast.com REVIEWS NEEDED . My email works as well for comments: 1001storiespodcast@gmail.com SUPPORT OUR SHOW BY BECOMING A PATRON! https://.patreon.com/1001storiesnetwork. Its time I started asking for support! Thank you. Its a few dollars a month OR a one time. (Any amount is appreciated). YOUR REVIEWS AND SUBSCRIPTIONS AT APPLE/ITUNES AND ALL ANDROID HOSTS ARE NEEDED AND APPRECIATED! LINKS BELOW. Learn more about your ad choices. Visit podcastchoices.com/adchoices

Joining us as our guest this week is Monika Wieland Shields, co-founder and director of Orca Behavior Institute. In addition to talking with Monika about OBI's field research, we spoke about the two different ecotypes of killer whales we see in the waters around the San Juan Islands, the endangered fish-eating Southern Residents and the thriving marine mammal eating Bigg's (formerly known as Transients). We discussed the changing trends in sightings of each population in the area and what is driving these changes.  Monika also shared some information about OBI's new study about killer whales and vessels in the Salish Sea, offering a new perspective on factors influencing incident rates.  As we do on each episode we got into recent whale sightings around the San Juan Islands, including the fascinating, ongoing saga of young Bigg's killer whale T34A1 switching families.  Our next episode will drop on May 30th. If you would like to submit feedback or questions to us we might read a few submissions on the next episode. Email us at afterthebreachpodcast@gmail.com or message us on Instagram.   Links mentioned in this episode: Orca Behavior Institute Website Instagram Facebook YouTube SoundCloud Souhaut, Marie, and Monika W. Shields. 2021. “Stereotyped whistles in Southern Resident killer whales.” PeerJ 9:e12085 Killer whales and vessels in the Salish Sea: A new perspective on factors influencing incident rates Photos mentioned in this episode: Average days per month SRKWs and Bigg's killer whales are in the Salish Sea. Data compiled by the Orca Behavior Institute.   T34 matriline   T34A1 last sighting with family, August 22, 2021. Photo by Sara Hysong Shimazu, Maya's Legacy Whale Watching.   T34A1 with T36 and T36Bs, September 2021. Photo by Sara Hysong Shimazu, Maya's Legacy Whale Watching.     SRKW J41 as a calf 2005. Photo by Monika Wieland Shields.   SRKW J53 as a calf 2015. Photo by Jeff Friedman, Maya's Legacy Whale Watching. New SRKW calf J59, 2022. Photo by Sara Hysong Shimazu, Maya's Legacy Whale Watching.

AEON (the Astronomical Event Observatory Network) will be a collection of world-class telescope facilities which can be accessed on demand, at the touch of a button.  At the heart of the network, LCO is joining forces with the NOIRLab CSDC and the SOAR 4.1m and Gemini 8m telescopes to build a network for the LSST era.   BIO:  Rachel joined Las Cumbres Observatory (LCO) as a post-doctoral scholar in 2007, and has since become a Staff Scientist. She specializes in the detection and characterization of exoplanets, initially as a founder member of the SuperWASP transit survey, for which she received the RAS Group Achievement Award.    Since joining LCO, she began to study exoplanets via the transient phenomena of microlensing, and now leads the microlensing group there. In the course of this research, she developed automated Target and Observation Management software (TOMs) to make observations through the LCO Network. This motivated her to lead the TOM Toolkit project and to contribute to the development of the Astronomical Event Observatories Network (AEON), to make these powerful observing tools available to the community as part of the ecosystem of software needed to respond to modern survey discoveries.    Rachel was elected as co-chair of the Transients and Variable Stars Science Collaboration (one of the Rubin Observatory's Science Collaborations) in 2017.     Links: AEON: Tracking Things That Go Bump In The Night: https://noirlab.edu/public/bl LCO's AEON website: https://lco.global/aeon/ NOIRLab's website: https://noirlab.edu/public/projects/aeon/ SOAR's website: http://www.ctio.noirlab.edu/soar/content/soar-aeon-home-page   We've added a new way to donate to 365 Days of Astronomy to support editing, hosting, and production costs.  Just visit: https://www.patreon.com/365DaysOfAstronomy and donate as much as you can! Share the podcast with your friends and send the Patreon link to them too!  Every bit helps! Thank you! ------------------------------------ Do go visit http://www.redbubble.com/people/CosmoQuestX/shop for cool Astronomy Cast and CosmoQuest t-shirts, coffee mugs and other awesomeness! http://cosmoquest.org/Donate This show is made possible through your donations.  Thank you! (Haven't donated? It's not too late! Just click!) ------------------------------------ The 365 Days of Astronomy Podcast is produced by the Planetary Science Institute. http://www.psi.edu Visit us on the web at 365DaysOfAstronomy.org or email us at info@365DaysOfAstronomy.org.

The Grand Junction Daily Sentinel's biggest headlines quickly dispensed.  The perfect OTC for people on the go! For the subscription-strength version, sign up for Your Daily Dose newsletter.   For more on these and other stories, visit our official website. TODAY'S TOP NEWS STORIES: PARKS AND WRECK BOTTOM OF THE 9TH.  BASES IMPLODED. PROPER SENTENCE STRUCTURE WORTH ITS WEIGHT IN GOLD

On this episode - We dive into the growing issue of the transient population in northern Colorado and take a look at how quiet our elected officials are with the problems. When will we get answers, and what plans are being proposed. An update on the DPS Tay Anderson situation, walk outs and frustration grows from students, parents, and staff. 50 Billion dollars has been put into the 3.5 Trillion dollar reconciliation bill from Rep. Neguse for forest service and climate change. Beer of the week! - Mash lab brewing/Windsor, CO - and - Prost/Fort Collins, CO - Rugby is back in northern Colorado! - Northern CO Flamingos This Saturday, September 25th, Satori Tattoo - Sexual assault survivor tattoo event to benefit the Avery Center 116 E 4th St. Loveland, CO 80537 theNative.theTransplant@gmail.com --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app Support this podcast: https://anchor.fm/native--transplant/support

We are just trying to make it as transients on a journey, moving towards our future...

Movement of planets September 2021 --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app

Taryn is pretty cool. After being accepted and preforming in one of Canadas largest Orchestras she has found herself in Vancouver, BC working with the MMRU at the University of British Columbia. AND she catches drones, for anyone who needs a drone catcher. In this podcast, we talk about her journey to her current postgrad degree and dive into different questions being asked in one of the most cutting edge marine mammal research groups in the PNW. ━━━━━━━━━━━━━ Taryn Scarff Taryn Scarff is a Masters Candidate at the University of British Columbia in the Marine Mammal Research Unit studying Transient orca prevalence in the Salish Sea. UBC Marine Mammal Research Unit https://mmru.ubc.ca/personnel/taryn-scarff/ Insta @tarynscarff https://www.instagram.com/tarynscarff/ Twitter @taryn_scarff https://twitter.com/taryn_scarff ━━━━━━━━━━━━━ ⏰TIMESTAMPS⏰ 0:00 Marine Mammal Rescue and Tofino 8:56 Undergrad Research 13:27 Road to UBC, Drumming 23:01 Research Vessel 29:28 Filming Orcas: drones and suction cups 36:15 Transients vs Resident Orcas 38:31 Determining Research Question 46:17 Masters Work 49:09 1 month, 1 boat, 1 washing machine, 9 people 57:07 Odd But Useful Skills 1:01:31 Understanding Transients and Populations 1:07:57 Closing out ━━━━━━━━━━━━━ Mentions UBC Marine Mammal Research Unit https://mmru.ubc.ca/ Insta @ubcmarinemammal https://www.instagram.com/ubcmarinemammal/ Marine Mammal Rescue https://mmrpatients.org/ Insta: @marinemammalrescue https://www.instagram.com/marinemammalrescue/ Hakai Institute https://www.hakai.org/ Andrew Trites https://mmru.ubc.ca/personnel/trites/

Veronica German, Louisiana Creole Black Woman Professional Psychic, November 2020 Transients

Veronica German, Louisiana Creole Black Woman Professional Psychic October Episode 2020 --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app

Louisiana Creole Black Woman Professional Psychic, Veronica German USA describes the planetary movement for September 2020. Saturn will depart Capricorn December 17, 2020. Saturn will return to Capricorn January 25, 2047

Join Pacific Mammal Research (PacMam) scientists to learn about different marine mammals each episode! We discuss a little about the biology, behavior and fun facts about each species. Have fun and learn about marine mammals with PacMam! This week: Orcas: Residents, transients and offshores, oh my! Presenters: Cindy Elliser, Katrina MacIver, Trevor Derie --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app Support this podcast: https://anchor.fm/pacific-mammal-research/support

Louisiana Creole Black Woman Professional Psychic leaving a message for August 2020

Planetary movement that we see, feel and observe in behavior on our planet,

Many planetary retrogrades May 2020