Podcasts about Nuv

Today's episode is about the 7 wonders of Banská Štiavnica. In the Slovak lesson, you will learn some new words from my article. You will also learn how to say “Discover magical wonders” in Slovak. At the end you will find my article about the 7 wonders of Banská Štiavnica in Slovak.Episode notesIn today's episode, I'm talking about the 7 wonders of Banská Štiavnica. In the Slovak lesson, you will learn some new words from my article. You will also learn how to say “Discover magical wonders” in Slovak. At the end you will find my article about the 7 wonders of Banská Štiavnica in Slovak.Slovak lesson1. zvláštnosť (oddity)2. koza (goat)3. komín (chimney)4. strecha (roof)5. býk (bull)6. šachta (mine shaft)7. most (bridge)8. akvadukt (aqueduct)9. potok (stream)10. radnica (town hall)11. hodiny (clock)12. ručička (clock hand (minute/hour hand))13. stráž (guard)14. roh (horn (musical instrument))15. turecká hrozba (Turkish threat)16. div / divy (wonder / wonders)17.  Objavte čarovné divy (Discover magical wonders)7 divov Banskej Štiavnice: Mesto plné prekvapeníBanská Štiavnica nie je len historické banské mesto, ale miesto plné zvláštností a kurióznych príbehov. Objavte jej 7 divov, ktoré vás pobavia a očaria!1. Koza priviazaná ku komínuVďaka strmému terénu tu záhrady často susedia s komínmi. Niekedy to vyzeralo, akoby koza bola priviazaná priamo ku komínu – kuriózny pohľad, ktorý ste inde nevideli!2. Domy so zmeneným vchodomVstúpite na „prízemie“, no ocitnete sa na poschodí. Typická zvláštnosť, ktorá môže nových návštevníkov poriadne zmiasť!3. Býk v komíneBýk raz spadol do banskej vetracej šachty, ktorú miestni volali „komín“. Záchrana trvala hodiny, no býk prežil bez ujmy – príbeh, ktorý si mesto pamätá dodnes.4. Most, po ktorom tiekla vodaNa rozdiel od bežných mostov, tu voda tiekla po moste a ľudia prechádzali pod ním. Tento unikátny akvadukt je svedectvom baníckej technickej geniality.5. Sneh na sviatok sv. Petra a PavlaHovorí sa, že na ich sviatok (29. júna) vždy sneží. V skutočnosti sneh pokrýva ich sochy na kostole až v zime, no vtip zostáva živý.6. Hodiny s opačnými ručičkamiVežové hodiny majú prehodené hodinovú a minútovú ručičku. Chyba? Tradícia? Nech je to akokoľvek, čítanie času v Štiavnici je malá výzva.7. Živé hodiny Nového zámkuStrážcovia kedysi trúbili každých 15 minút na znak bezpečia. Dnes sa táto tradícia pripomína počas letných mesiacov – skvelý zážitok pre návštevníkov!Banská Štiavnica je mesto plné histórie, vynaliezavosti a humoru. Príďte a objavte jej čarovné divy sami!Timestamps00:34 Introduction02:26 About 7 wonders03:39 Fun fact11:46 Slovak lesson16:56 About 7 wonders in Slovak19:54 About 7 wonders (English translation)25:25 Final thoughtsIf you have any questions, send it to my email hello@bozenasslovak.com. Check my Instagram https://www.instagram.com/bozenasslovak/ where I am posting the pictures of what I am talking about on my podcast. Also, check my website https://www.bozenasslovak.com © All copywrites reserved to Bozena O Hilko LLC

Apple melder sig omsider ind i AI-kampen med en AI-pakke, de kalder Apple Intelligence. Det betyder, at din telefon snart vil få massevis af AI-funktioner - hvis du da har en af de nye, dyre telefoner. Vi diskuterer, om Apple Intelligence kan give AI det folkelige gennembrud. Nuværende og tidligere ansatte hos OpenAI revser virksomheden og Sam Altman, som beskyldes for at skabe en usund kultur med løgne og psykisk vold. Samtidig frygter de tidligere ansatte, at OpenAI ikke gør nok for at sikre os mod den kunstig intelligens' udvikling, der ifølge dem risikerer at ødelægge vores liv og samfund. Vi ringer til vores husven Fred Benenson, der har arbejdet med Sam Altman, for at forstå, hvad der er på spil. Og så går Meta snart i gang med at træne deres AI på dine billeder, kommentarer og posts - medmindre du gør indsigelse. Vi fortæller dig hvordan. Værter: Marcel Mirzaei-Fard, tech-analytiker og Henrik Moltke, tech-korrespondent.

Welcome to The Nonlinear Library, where we use Text-to-Speech software to convert the best writing from the Rationalist and EA communities into audio. This is: Increasing IQ by 10 Points is Possible, published by George3d6 on March 19, 2024 on LessWrong. A while ago I wrote how I managed to add 13 points to my IQ (as measured by the mean between 4 different tests). I had 3 "self-experimenters" follow my instructions in San Francisco. One of them dropped off, since, surprise surprise, the intervention is hard. The other two had an increase of 11 and 10 points in IQ respectively (using the "fluid" components of each test) and an increase of 9 and 7 respectively if we include verbal IQ. A total of 7 people acted as a control and were given advantages on the test compared to the intervention group to exacerbate the effects of memory and motivation, only 1 scored on par with the intervention group. We get a very good p-value, considering the small n, both when comparing the % change in control vs intervention (0.04) and the before/after intervention values (0.006) Working Hypothesis My working hypothesis for this was simple: If I can increase blood flow to the brain in a safe way (e.g. via specific exercises, specific supplements, and photostimulation in the NUV and NIR range) And I can make people think "out of the box" (e.g. via specific games, specific "supplements", specific meditations) And prod people to think about how they can improve in whatever areas they want (e.g. via journaling, talking, and meditating) Then you get this amazing cocktail of spare cognitive capacity suddenly getting used. As per the last article, I can't exactly have a step-by-step guide for how to do this, given that a lot of this is quite specific. I was rather lucky that 2 of my subjects were very athletic and "got it" quite fast in terms of the exercises they had to be doing. The Rub At this point, I'm confident all the "common sense" distillation on what people were experimenting with has been done, and the intervention takes quite a while. Dedicating 4 hours a day to something for 2 weeks is one thing, but given that we're engaging in a form of training for the mind, the participants need not only be present, but actively engaged. A core component of my approach is the idea that people can (often non-conceptually) reason through their shortcomings if given enough spare capacity, and reach a more holistic form of thinking. I'm hardly the first to propose or observe this, though I do want to think my approach is more well-proven, entirely secular, and faster. Still, the main bottleneck remains convincing people to spend the time on it. What's next My goal when I started thinking about this was to prove to myself that the brain and the mind are more malleable than we think, that relatively silly and easy things, to the tune of: A few supplements and 3-4 hours of effort a day for 2 weeks, can change things that degrade with aging and are taken as impossible to reverse Over the last two months, I became quite convinced there is something here… I don't quite understand its shape yet, but I want to pursue it. At present, I am considering putting together a team of specialists (which is to say neuroscientists and "bodyworkers"), refining this intervention with them, and selling it to people as a 2-week retreat. But there's also a bunch of cool hardware that's coming out of doing this As well as a much better understanding of the way some drugs and supplements work… and understanding I could package together with the insanely long test-and-iterate decision tree to use these substances optimally (more on this soon). There was some discussion and interested expressed by the Lighthaven team in the previous comment section to replicate, and now that I have data from more people I hope that follows through, I'd be high-quality data from a trustworthy first party, and I'm well aware at this point this should still hit the "quack" meter for most people. I'm al...

Link to original articleWelcome to The Nonlinear Library, where we use Text-to-Speech software to convert the best writing from the Rationalist and EA communities into audio. This is: Increasing IQ by 10 Points is Possible, published by George3d6 on March 19, 2024 on LessWrong. A while ago I wrote how I managed to add 13 points to my IQ (as measured by the mean between 4 different tests). I had 3 "self-experimenters" follow my instructions in San Francisco. One of them dropped off, since, surprise surprise, the intervention is hard. The other two had an increase of 11 and 10 points in IQ respectively (using the "fluid" components of each test) and an increase of 9 and 7 respectively if we include verbal IQ. A total of 7 people acted as a control and were given advantages on the test compared to the intervention group to exacerbate the effects of memory and motivation, only 1 scored on par with the intervention group. We get a very good p-value, considering the small n, both when comparing the % change in control vs intervention (0.04) and the before/after intervention values (0.006) Working Hypothesis My working hypothesis for this was simple: If I can increase blood flow to the brain in a safe way (e.g. via specific exercises, specific supplements, and photostimulation in the NUV and NIR range) And I can make people think "out of the box" (e.g. via specific games, specific "supplements", specific meditations) And prod people to think about how they can improve in whatever areas they want (e.g. via journaling, talking, and meditating) Then you get this amazing cocktail of spare cognitive capacity suddenly getting used. As per the last article, I can't exactly have a step-by-step guide for how to do this, given that a lot of this is quite specific. I was rather lucky that 2 of my subjects were very athletic and "got it" quite fast in terms of the exercises they had to be doing. The Rub At this point, I'm confident all the "common sense" distillation on what people were experimenting with has been done, and the intervention takes quite a while. Dedicating 4 hours a day to something for 2 weeks is one thing, but given that we're engaging in a form of training for the mind, the participants need not only be present, but actively engaged. A core component of my approach is the idea that people can (often non-conceptually) reason through their shortcomings if given enough spare capacity, and reach a more holistic form of thinking. I'm hardly the first to propose or observe this, though I do want to think my approach is more well-proven, entirely secular, and faster. Still, the main bottleneck remains convincing people to spend the time on it. What's next My goal when I started thinking about this was to prove to myself that the brain and the mind are more malleable than we think, that relatively silly and easy things, to the tune of: A few supplements and 3-4 hours of effort a day for 2 weeks, can change things that degrade with aging and are taken as impossible to reverse Over the last two months, I became quite convinced there is something here… I don't quite understand its shape yet, but I want to pursue it. At present, I am considering putting together a team of specialists (which is to say neuroscientists and "bodyworkers"), refining this intervention with them, and selling it to people as a 2-week retreat. But there's also a bunch of cool hardware that's coming out of doing this As well as a much better understanding of the way some drugs and supplements work… and understanding I could package together with the insanely long test-and-iterate decision tree to use these substances optimally (more on this soon). There was some discussion and interested expressed by the Lighthaven team in the previous comment section to replicate, and now that I have data from more people I hope that follows through, I'd be high-quality data from a trustworthy first party, and I'm well aware at this point this should still hit the "quack" meter for most people. I'm al...

The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog by Chayan Mondal et al. on Wednesday 30 November We present deep UV imaging observations of the Great Observatories Origins Survey Northern (GOODS-N) field with AstroSat/UVIT (AstroSat UV Deep Field north - AUDFn), using one far-UV (F154W, 34.0 kilosec) and two near-UV filters (N242W, 19.2 kilosec; N245M, 15.5 kilosec). The nature of the UV sky background was explored across the UVIT field and a global mean and rms was estimated for each filter. We reach 3$sigma$ detection limits of $m_{rm AB}$ $sim$ 27.35 mag, 27.28 mag and 27.02 mag for a point source in the F154W, N242W and N245M bands respectively. The 50% completeness limits of the FUV and NUV images are $m_{rm AB}=$ 26.40 mag and 27.05 mag respectively. We constructed PSFs for each band and estimated their FWHM, which were found to be almost the same: 1.18" in F154W, 1.11" in N242W, and 1.24" in N245M. We used SExtractor to separately identify sources in the FUV and NUV filters and produce the UV source catalog of the entire AUDFn field. The source count slope estimated in FUV and NUV is 0.57 dex mag$^{-1}$ (between 19 - 25 mag) and 0.44 dex mag$^{-1}$ (between 18 - 25 mag), respectively. The catalog contains 6839 and 16171 sources (brighter than the 50% completeness limit) in the FUV and NUV, respectively. Our FUV and NUV flux measurements of the identified sources complement existing multi-band data in the GOODS-N field, and enable us to probe rest-frame FUV properties of galaxies at redshift $z < 1$ and search for candidate Lyman continuum leakers at redshift $z > 0.97$. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.16923v1

The Complex Structure of the Bulge of M31 by Denis Leahy et al. on Wednesday 30 November The bulge of M31 is of interest in the context of the nature of galactic bulges and how their structure relates to bulge formation mechanisms and their subsequent evolution. With the UVIT instrument on AstroSat, we have observed the bulge of M31 in five far ultraviolet (FUV) and near ultraviolet (NUV) filters at 1" spatial resolution. Models for the luminosity distribution of the bulge are constructed using the UVIT data and the galaxy image-fitting algorithm GALFIT. We fit the bulge without nuclear region with a Sersic function the five images and find Sersic indices ($simeq2.1$ to 2.5) similar to previous studies but smaller $R_e$ values ($simeq0.5$ to 0.6 kpc). When the images include the nuclear region, a multicomponent model is used to find the best-fit. We use an 8-component fit for the FUV 148nm image, which has the highest sensitivity. The other images (169 to 279 nm) are fit with 4-component models. The dust lanes in the bulge region are recovered in the residual image after subtraction of the bright bulge light using the multicomponent model. The dust lanes show that M31's nuclear spiral is visible in absorption at NUV and FUV wavelengths. The bulge images show boxy contours in all five UVIT wavebands, which is confirmed by fitting using GALFIT. The Sersic indices of $sim$2.1-2.5 are intermediate between expected values for a classical bulge and for a pseudobulge. The boxiness of the bulge provides further evidence that M31's bulge has contributions from a classical bulge and a pseudobulge. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.16311v1

The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog by Chayan Mondal et al. on Wednesday 30 November We present deep UV imaging observations of the Great Observatories Origins Survey Northern (GOODS-N) field with AstroSat/UVIT (AstroSat UV Deep Field north - AUDFn), using one far-UV (F154W, 34.0 kilosec) and two near-UV filters (N242W, 19.2 kilosec; N245M, 15.5 kilosec). The nature of the UV sky background was explored across the UVIT field and a global mean and rms was estimated for each filter. We reach 3$sigma$ detection limits of $m_{rm AB}$ $sim$ 27.35 mag, 27.28 mag and 27.02 mag for a point source in the F154W, N242W and N245M bands respectively. The 50% completeness limits of the FUV and NUV images are $m_{rm AB}=$ 26.40 mag and 27.05 mag respectively. We constructed PSFs for each band and estimated their FWHM, which were found to be almost the same: 1.18" in F154W, 1.11" in N242W, and 1.24" in N245M. We used SExtractor to separately identify sources in the FUV and NUV filters and produce the UV source catalog of the entire AUDFn field. The source count slope estimated in FUV and NUV is 0.57 dex mag$^{-1}$ (between 19 - 25 mag) and 0.44 dex mag$^{-1}$ (between 18 - 25 mag), respectively. The catalog contains 6839 and 16171 sources (brighter than the 50% completeness limit) in the FUV and NUV, respectively. Our FUV and NUV flux measurements of the identified sources complement existing multi-band data in the GOODS-N field, and enable us to probe rest-frame FUV properties of galaxies at redshift $z < 1$ and search for candidate Lyman continuum leakers at redshift $z > 0.97$. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.16923v1

The Complex Structure of the Bulge of M31 by Denis Leahy et al. on Wednesday 30 November The bulge of M31 is of interest in the context of the nature of galactic bulges and how their structure relates to bulge formation mechanisms and their subsequent evolution. With the UVIT instrument on AstroSat, we have observed the bulge of M31 in five far ultraviolet (FUV) and near ultraviolet (NUV) filters at 1" spatial resolution. Models for the luminosity distribution of the bulge are constructed using the UVIT data and the galaxy image-fitting algorithm GALFIT. We fit the bulge without nuclear region with a Sersic function the five images and find Sersic indices ($simeq2.1$ to 2.5) similar to previous studies but smaller $R_e$ values ($simeq0.5$ to 0.6 kpc). When the images include the nuclear region, a multicomponent model is used to find the best-fit. We use an 8-component fit for the FUV 148nm image, which has the highest sensitivity. The other images (169 to 279 nm) are fit with 4-component models. The dust lanes in the bulge region are recovered in the residual image after subtraction of the bright bulge light using the multicomponent model. The dust lanes show that M31's nuclear spiral is visible in absorption at NUV and FUV wavelengths. The bulge images show boxy contours in all five UVIT wavebands, which is confirmed by fitting using GALFIT. The Sersic indices of $sim$2.1-2.5 are intermediate between expected values for a classical bulge and for a pseudobulge. The boxiness of the bulge provides further evidence that M31's bulge has contributions from a classical bulge and a pseudobulge. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.16311v1

The Complex Structure of the Bulge of M31 by Denis Leahy et al. on Wednesday 30 November The bulge of M31 is of interest in the context of the nature of galactic bulges and how their structure relates to bulge formation mechanisms and their subsequent evolution. With the UVIT instrument on AstroSat, we have observed the bulge of M31 in five far ultraviolet (FUV) and near ultraviolet (NUV) filters at 1" spatial resolution. Models for the luminosity distribution of the bulge are constructed using the UVIT data and the galaxy image-fitting algorithm GALFIT. We fit the bulge without nuclear region with a Sersic function the five images and find Sersic indices ($simeq2.1$ to 2.5) similar to previous studies but smaller $R_e$ values ($simeq0.5$ to 0.6 kpc). When the images include the nuclear region, a multicomponent model is used to find the best-fit. We use an 8-component fit for the FUV 148nm image, which has the highest sensitivity. The other images (169 to 279 nm) are fit with 4-component models. The dust lanes in the bulge region are recovered in the residual image after subtraction of the bright bulge light using the multicomponent model. The dust lanes show that M31's nuclear spiral is visible in absorption at NUV and FUV wavelengths. The bulge images show boxy contours in all five UVIT wavebands, which is confirmed by fitting using GALFIT. The Sersic indices of $sim$2.1-2.5 are intermediate between expected values for a classical bulge and for a pseudobulge. The boxiness of the bulge provides further evidence that M31's bulge has contributions from a classical bulge and a pseudobulge. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.16311v1

A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A by Maude Gull et al. on Tuesday 29 November We characterize massive stars (M>8 M_sun) in the nearby (D~0.8 Mpc) extremely metal-poor (Z~5% Z_sun) galaxy Leo A using Hubble Space Telescope ultra-violet (UV), optical, and near-infrared (NIR) imaging along with Keck/LRIS and MMT/Binospec optical spectroscopy for 18 main sequence OB stars. We find that: (a) 12 of our 18 stars show emission lines, despite not being associated with an H II region, suggestive of stellar activity (e.g., mass loss, accretion, binary star interaction), which is consistent with previous predictions of enhanced activity at low metallicity; (b) 6 are Be stars, which are the first to be spectroscopically studied at such low metallicity -- these Be stars have unusual panchromatic SEDs; (c) for stars well-fit by the TLUSTY non-local thermodynamic equilibrium (non-LTE) models, the photometric and spectroscopic values of T_eff and log(g) agree to within ~0.01 dex and ~0.18 dex, respectively, indicating that NUV/optical/NIR imaging can be used to reliably characterize massive (M ~ 8-30 M_sun) main sequence star properties relative to optical spectroscopy; (d) the properties of the most massive stars in H II regions are consistent with constraints from previous nebular emission line studies; and (e) 13 stars with M>8 M_sun are >40 pc from a known star cluster or H II region. Our sample comprises ~50% of all known massive stars at Z < 10% Z_sun with derived stellar parameters, high-quality optical spectra, and panchromatic photometry. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.14349v1

A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A by Maude Gull et al. on Monday 28 November We characterize massive stars (M>8 M_sun) in the nearby (D~0.8 Mpc) extremely metal-poor (Z~5% Z_sun) galaxy Leo A using Hubble Space Telescope ultra-violet (UV), optical, and near-infrared (NIR) imaging along with Keck/LRIS and MMT/Binospec optical spectroscopy for 18 main sequence OB stars. We find that: (a) 12 of our 18 stars show emission lines, despite not being associated with an H II region, suggestive of stellar activity (e.g., mass loss, accretion, binary star interaction), which is consistent with previous predictions of enhanced activity at low metallicity; (b) 6 are Be stars, which are the first to be spectroscopically studied at such low metallicity -- these Be stars have unusual panchromatic SEDs; (c) for stars well-fit by the TLUSTY non-local thermodynamic equilibrium (non-LTE) models, the photometric and spectroscopic values of T_eff and log(g) agree to within ~0.01 dex and ~0.18 dex, respectively, indicating that NUV/optical/NIR imaging can be used to reliably characterize massive (M ~ 8-30 M_sun) main sequence star properties relative to optical spectroscopy; (d) the properties of the most massive stars in H II regions are consistent with constraints from previous nebular emission line studies; and (e) 13 stars with M>8 M_sun are >40 pc from a known star cluster or H II region. Our sample comprises ~50% of all known massive stars at Z < 10% Z_sun with derived stellar parameters, high-quality optical spectra, and panchromatic photometry. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.14349v1

Timescale-dependent X-ray to UV time lags of NGC 4593 using high-intensity XMM-Newton observations with Swift and AstroSat by Max W. J. Beard et al. on Monday 21 November We present a 140ks observation of NGC 4593 with XMM-Newton providing simultaneous and continuous PN X-ray and OM UV (UVW1 2910AA) lightcurves which sample short-timescale variations better than previous observations. These observations were simultaneous with 22d of Swift X-ray and UV/optical monitoring, reported previously, and 4d of AstroSat X-ray (SXT), far (FUV 1541AA), and near (NUV 2632AA) UV allowing lag measurements between them and the highly-sampled XMM. From the XMM we find that UVW1 lags behind the X-rays by 29.5$pm$1.3ks, $sim$half the lag previously determined from the Swift monitoring. Re-examination of the textit{Swift} data reveals a bimodal lag distribution, with evidence for both the long and short lags. However if we detrend the Swift lightcurves by LOWESS filtering with a 5d width, only the shorter lag (23.8$pm$21.2ks) remains. The NUV observations, compared to PN and SXT, confirm the $sim$30ks lag found by XMM and, after 4d filtering is applied to remove the long-timescale component, the FUV shows a lag of $sim$23ks. The resultant new UVW1, FUV, and NUV lag spectrum extends to the X-ray band without requiring additional X-ray to UV lag offset, which if the UV arises from reprocessing of X-rays, implies direct illumination of the reprocessor. By referencing previous Swift and HST lag measurements, we obtain an X-ray to optical lag spectrum which agrees with a model using the KYNreverb disc-reprocessing code, assuming the accepted mass of $7.63times10^{6}M_{odot}$ and a spin approaching maximum. Previously noted lag contribution from the BLR in the Balmer and Paschen continua are still prominent. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.10229v1

Flere stemmer i dansk landbrug frygter en smal rød regering efter folketingsvalg, der mundede ud i rødt flertal. Tidligere L&F-viceformand og griselandmand kommer i Folketinget. Nuværende L&F-viceformand har ingen plan b, hvis han ikke bliver valgt til L&F-bestyrelse.

Deep Investigation of Neutral Gas Origins DINGO : HI stacking experiments with early science data by Jonghwan Rhee et al. on Tuesday 18 October We present early science results from Deep Investigation of Neutral Gas Origins (DINGO), an HI survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP sub-arrays available during its commissioning phase, DINGO early science data were taken over $sim$ 60 deg$^{2}$ of the Galaxy And Mass Assembly (GAMA) 23 h region with 35.5 hr integration time. We make direct detections of six known and one new sources at $z < 0.01$. Using HI spectral stacking, we investigate the HI gas content of galaxies at $0.04 < z< 0.09$ for different galaxy colours. The results show that galaxy morphology based on optical colour is strongly linked to HI gas properties. To examine environmental impacts on the HI gas content of galaxies, three sub-samples are made based on the GAMA group catalogue. The average HI mass of group central galaxies is larger than those of satellite and isolated galaxies, but with a lower HI gas fraction. We derive a variety of HI scaling relations for physical properties of our sample, including stellar mass, stellar mass surface density, $NUV-r$ colour, specific star formation rate, and halo mass. We find that the derived HI scaling relations are comparable to other published results, with consistent trends also observed to $sim$0.5 dex lower limits in stellar mass and stellar surface density. The cosmic HI densities derived from our data are consistent with other published values at similar redshifts. DINGO early science highlights the power of HI spectral stacking techniques with ASKAP. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.09697v1

Aging of galaxies along the morphological sequence, marked by bulge growth and disk quenching by Louis Quilley et al. on Tuesday 18 October We revisit the color bimodality of galaxies using the extensive EFIGI morphological classification of nearby galaxies. The galaxy SDSS images in the g, r and i bands are decomposed as bulge+disk using SourceXtractor++. The spectral energy distributions made of our gri photometry complemented with GALEX NUV are fitted with ZPEG in order to estimate the stellar masses and specific star formations rates (sSFR) of whole galaxies as well as their bulge and disk components. The absolute NUV-r color versus stellar mass diagram shows a continuous relationship between the present sSFR of galaxies and their stellar mass, that spans all morphological types of the Hubble sequence. Irregular galaxies to Sab spirals make up the Blue Cloud, the Green Plain (formerly Valley) is made up of early-type spirals (S0a-Sa) while the Red Sequence contains all lenticular and elliptical galaxies, with systematically higher masses for the ellipticals. Galaxies across the Green Plain undergo a marked growth by a factor 2 to 3 in their bulge-to-total mass ratio and a systematic profile change from pseudo to classical bulges, as well as a significant reddening interpreted as star formation fading in their disks. Therefore, the Green Plain is a transition region, and we exclude a predominantly quick transit due to rapid quenching. We suggest that tracers of increased star formation (bright HII regions, spiral arms, flocculence) determine the limited scatter of the Main Sequence of star-forming galaxies. The high frequency of bars for all spirals as well as the stronger spiral arms and flocculence in the knee of the Green Plain suggest that internal dynamics, likely triggered by flybys or mergers, may be the key to the bulge growth of massive disk galaxies, marker of the aging of galaxies from star forming to quiescence. The Hubble sequence can then be considered as an inverse sequence of galaxy physical evolution. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2206.04707v2

Discovery of a probable very fast extragalactic nova in a symbiotic binary by David Modiano et al. on Wednesday 12 October Very fast novae are novae which evolve exceptionally quickly (on timescales of only days). Due to their rapid evolution, very fast novae are challenging to detect and study, especially at early times. Here we report the discovery, which was made as part of our Transient UV Objects project, of a probable very fast nova in the nearby spiral galaxy NGC 300. We detected the rise to the peak (which is rarely observed for very fast novae) in the near-ultraviolet (NUV), with the first detection just ~2 hours after the eruption started. The peak and early stages of the decay were also observed in UV and optical bands. The source rapidly decayed by 2 NUV magnitudes within 3.5 days, making it one of the fastest novae known. In addition, a likely quiescent counterpart was found in archival near-infrared Spitzer and VIRCAM images but not in any deep optical and UV observations, indicating a very red spectral shape in quiescence. The outburst and quiescence properties suggest that the system is likely a symbiotic binary. We discuss this new transient in the context of very fast novae in general and specifically as a promising supernova Type Ia progenitor candidate, due to its very high inferred WD mass (~1.35 Ms; determined by comparing this source to other very fast novae). arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2210.06057v1

PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry by Connor Stone et al. on Wednesday 21 September We present the Photometry and Rotation Curve Observations from Extragalactic Surveys (PROBES) compendium of extended rotation curves for 3163 late-type spirals, with matching homogeneous multiband photometry for 1677 of them. PROBES rotation curves originally extracted from Halpha long-slit spectra and aperture synthesis HI (21cm) velocity maps typically extend out to a median 2R_e (or 1R_{23.5, r}). Our uniform photometry takes advantage of GALEX, DESI-LIS, and WISE images and the software AutoProf to yield multiband azimuthally averaged surface brightness profiles that achieve depths greater than 25 mag/arcsec^2 (FUV, NUV), 27 mag/arcsec^2 (g, r), and 26 mag/arcsec^2 (z, W1, W2). With its library of spatially resolved profiles and an extensive table of structural parameters, the versatile PROBES data set will benefit studies of galaxy structure and formation. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.09912v1

AstroSat UVIT Cluster Photometry in the Northern Disk of M31 by Denis Leahy et al. on Wednesday 14 September The Andromeda Galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT FUV and NUV photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 which overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicities and extinctions for 170 clusters. The ages show a narrow peak at $sim$4 Myr and a broad peak around 100 Myr. log(Z/Z$_{odot}$) values are mostly between $-0.3$ and $+0.3$. The 7 clusters in the bulge are low metallicity and high mass. Most clusters are in the spiral arms and have metallicities in the range noted above. The youngest clusters are mostly high metallicity and are concentrated along the brightest parts of the spiral arms. The UVIT FUV and NUV data are sensitive to young stars and detect a new metal rich peak in star formation in the disk at age $sim4$ Myr. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.03842v2

AstroSat UVIT Cluster Photometry in the Northern Disk of M31 by Denis Leahy et al. on Wednesday 14 September The Andromeda Galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT FUV and NUV photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 which overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicities and extinctions for 170 clusters. The ages show a narrow peak at $sim$4 Myr and a broad peak around 100 Myr. log(Z/Z$_{odot}$) values are mostly between $-0.3$ and $+0.3$. The 7 clusters in the bulge are low metallicity and high mass. Most clusters are in the spiral arms and have metallicities in the range noted above. The youngest clusters are mostly high metallicity and are concentrated along the brightest parts of the spiral arms. The UVIT FUV and NUV data are sensitive to young stars and detect a new metal rich peak in star formation in the disk at age $sim4$ Myr. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.03842v2

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

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

AstroSat UVIT Cluster Photometry in the Northern Disk of M3 by Denis Leahy et al. on Sunday 11 September The Andromeda Galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT FUV and NUV photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 which overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicities and extinctions for 170 clusters. The ages show a narrow peak at $sim$4 Myr and a broad peak around 100 Myr. log(Z/Z$_{odot}$) values are mostly between $-0.3$ and $+0.3$. The 7 clusters in the bulge are low metallicity and high mass. Most clusters are in the spiral arms and have metallicities in the range noted above. The youngest clusters are mostly high metallicity and are concentrated along the brightest parts of the spiral arms. The UVIT FUV and NUV data are sensitive to young stars and detect a new metal rich peak in star formation in the disk at age $sim4$ Myr. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.03842v1

AstroSat UVIT Cluster Photometry in the Northern Disk of M3 by Denis Leahy et al. on Sunday 11 September The Andromeda Galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT FUV and NUV photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 which overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicities and extinctions for 170 clusters. The ages show a narrow peak at $sim$4 Myr and a broad peak around 100 Myr. log(Z/Z$_{odot}$) values are mostly between $-0.3$ and $+0.3$. The 7 clusters in the bulge are low metallicity and high mass. Most clusters are in the spiral arms and have metallicities in the range noted above. The youngest clusters are mostly high metallicity and are concentrated along the brightest parts of the spiral arms. The UVIT FUV and NUV data are sensitive to young stars and detect a new metal rich peak in star formation in the disk at age $sim4$ Myr. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.03842v1

SDSS J1058+5443: A blue quasar does not have optical NUV broad emission lines by Xue-Guang Zhang et al. on Tuesday 06 September In the manuscript, the blue quasar SDSS J105816.19+544310.2 (=SDSS J1058+5443) at redshift 0.479 is reported as so-far the best candidate of true type-2 quasar with disappearance of central BLRs. There are so-far no definite conclusions on the very existence of true type-2 AGN, mainly due to detected optical broad emission lines in high quality spectra of some previously classified candidates of true type-2 AGN. Here, not similar as previous reported candidates for true type-2 AGN among narrow emission-line galaxies with weak AGN activities but strong stellar lights, the definite blue quasar SDSS J1058+5443 can be well confirmed as a true type-2 quasar due to apparent quasar-shape blue continuum emissions but apparent loss of both the optical broad Balmer emission lines and the NUV broad Mg~{sc ii} emission line. Based on different model functions and F-test statistical technique, after considering blue-shifted optical and UV Fe~{sc ii} emissions, there are no apparent broad optical Balmer emission lines and/or broad NUV Mg~{sc ii} line, and the confidence level is smaller than 1sigma to support broad optical and NUV emission lines. Moreover, assumed the Virialization assumption to broad line emission clouds, the re-constructed broad emission lines strongly indicate that the probable intrinsic broad emission lines, if there were, cannot be hidden or overwhelmed in the noises of SDSS spectrum of SDSS J1058+5443. Therefore, SDSS J1058+5443, so-far the best and robust candidate of true type-2 quasar, leads to the further clear conclusion on the very existence of true type-2 AGN. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.02164v1

Le soleil est là et bien là !Et il va cogner très fort cette semaine…donc attention de ne pas trop s'exposer et surtout de se protéger.Aujourd'hui, on parle justement de la semaine nationale de dépistage du cancer de la peau, organisée jusqu'à vendredi…Un dermatologue d'Auray dans le Morbihan sera avec nous dans un instant pour nous rappeler quelques conseils de bon sens.L'autre invitée du jour, c'est Claudia Galéana qui a trouvé la parade pour se protéger du soleil : elle a créé « Nuvées », une marque de vêtements anti-UV…

45 anni come il Punk Rock! Tanti Auguri Ciao Como Radio! Noi festeggiamo con i Sex pistols, The Backdoor Society, The Nuv, Clamm, Milt, Faz Waltz, Los Fuocos, Castrol e tanti altri... in fondo Italians do it better!!!!

Nuvidio aproxima marcas e consumidores via videochamadas com apenas um clique Agência de marketing vai processar o Facebook por roubar a sua marca Startup Rivian, de veículos elétricos, pode valer tanto quanto a honda Olist compra duas startups do RS para ampliar serviços a empresas Essas são as manchetes de hoje, Quarta-feira dia 3 de novembro de 2021. E você está no RC NEWS. Notícias para empreendedores. E hoje está no programa o Janu Queiroz cofundadora e COO da Nuvídeo, que vai bater um papo com a gente daqui a pouco. Nosso programa é multiplataforma e estamos ao vivo no Youtube, Facebook, Linkedin, Twitter e Twitch do ResumoCast. As edições ficam gravadas nas plataformas podendo ser acessadas a qualquer hora do dia. Se você tem um site e não teve resultados com ele, ou tem vontade de ter um, convido a conversar sem compromisso com meu amigo Eduardo da agência Kryzalis.  Apoiadores já há anos do ResumoCast, possuem 14 anos de experiência já com mkt digital e tem as soluções pra você Micro e Pequeno Empreendedor - ouvinte do RCNews. Bata um papo com o Eduardo ou Everton da Kryzalis pelo endereço:  https://www.resumocast.com.br/resultadonainternet   Whatsapp (14) 99629-6537 E você pode enviar mensagens pelas redes sociais e quando acompanha ao vivo de Segunda à Sexta às 7h da manhã. Curadoria atualizada sobre Startups, negócios inovadores e tendências de mercado. Youtube do ResumoCast : https://youtube.com/playlist?list=PL2wFLSmdA7Zcbre3E2f9AA8KankrxceMu Youtube do Resumo Radio Cast : https://www.youtube.com/channel/UCvnH_YA25EKlEdfu8jVUpRA Facebook : https://www.facebook.com/resumocast/videos https://www.facebook.com/resumocastnews/videos https://www.facebook.com/groups/resumocast/ Linkedin : https://www.linkedin.com/company/resumocast/ Twitte : https://twitter.com/resumocast Twitch : https://www.twitch.tv/resumocast Spotify : https://open.spotify.com/show/3sEG6rOLvz6bLrMxEIcKRq Apple Podcasts : https://podcasts.apple.com/br/podcast/resumocast-news/id1505825539 Visite https://www.resumocast.com.br/news para ler as notícias e se inscrever na listra de transmissão do Telegram

Dilemmaet i supermarkedet er en podcastserie om bæredygtig kost. I podcastseriens fire episoder har vi forskellige forskere i studiet, som gør os klogere på vores nuværende fødevaresystemer, og hvorfor de ikke er bæredygtige.  Serien skal give dig som forbruger gode tips og tricks til at spise mere bæredygtigt. Ordet bæredygtighed er blevet hverdagskost, ikke mindst når vi handler ind. Men hvad betyder det egentlig? Det fortæller professor Michael Hauschild fra DTU om i denne podcast. Første gang ordet bæredygtighed blev defineret var af FN i den såkaldt Brundtlandrapport fra 1987. Her defineres bæredygtighed sådan her: “Nuværende generationer skal opfylde deres behov på en måde så fremtidige generationers mulighed for at opfylde deres behov ikke sættes over styr.” I Michael Hauschilds øjne handler bæredygtig kost derfor om, at vi producerer vores fødevarer på en måde, så vi ikke overskrider plantens grænser for, hvad den kan klare og på den måde sætter klimaet og miljøet over styr. For hvis klimasystemet bringes ud af kontrol, kan fremtidige generationer med stor sikkerhed ikke opfylde deres behov på samme måde, som vi kan i dag. Men i forhold til lige præcis vores kost er, der måske også nogle andre parametre, der er vigtige. FN's landbrugsorganisation FAO definerer en bæredygtig kost, som at kosten skal være økonomisk tilgængelig, ernæringsmæssigt tilstrækkelig, kulturelt acceptabel og produceret så den skåner miljøet. Hvis bliver bedt om at spise noget, som ikke er kulturelt acceptabelt i Danmark - for eksempel græshopper - så er det ikke bæredygtigt, for så vil vi formentlig ikke spise det. Men hvad vil det sige, at en kost er kulturelt acceptabel. Det fortæller ph.d. og madkulturforsker Jonatan Leer fra Professionshøjskolen Absalon. Og han punkterer også myten om, at det er en særlig dansk madkultur at spise masser af kød. Lyt med og bliv klogere på, hvad bæredygtighed faktisk betyder, og hvad du selv kan gøre, for at spise lidt mere bæredygtigt. Dilemmaet i supermarkedet er sponsoreret af og lavet i samarbejde med Landbrug & Fødevarer og Mejeriforeningen. Medvirkende:  Michael Zwicky Hauschild, professor, DTU Jonatan Leer,  ph.d. og madkulturforsker, Professionshøjskolen Absalon Vært, tilrettelæggelse og research: Marie Barse Teknik: Kristian Højgaard Nielsen Musik: Jais Baggestrøm Koch

Hugo tuvo una larga carrera en el mundo corporativo, con posiciones gerenciales en Nuvó Cosméticos en Uruguay, y luego expandiendo sus operaciones en Argentina, y Brasil. Pero llegando a los 50 años decide emprender, de forma de tener independencia financiera y prosperidad económica. La transición fue paulatina, primero fue consultor internacional y docente. Esta experiencia le sirvió de alguna manera para hacer una investigación de mercado preliminar, acercarse a varias empresas, y poder evaluar su potencial posible inversión. En 2011 funda el fondo IBF Negocios, que invierte en empresas de capital privado. Su exito radica en hacer crecer a las empresas, profesionalizando su operativa, y creando sinergias con otras empresas del grupo. IBF invierte en empresas que ya están en marcha, tienen buen potencial de crecimiento y facturan más de 5 millones de dólares. Desde el 2012 a la fecha han invertido 45 millones de dólares y cuentan con inversiones en farmacias, empresas de alimentos, productos veterinarios, repuestos de automóviles, entre otros. Su rendimiento promedio anual neto para sus inversores supera el 10%.Escuchá la charla para conocer cuál es su metodología de inversión, qué es lo que buscan en un emprendimiento, y cuáles son sus consejos a futuros emprendedores. 

Nan u Mast dgel Pael u Nuveen #1 We are happy to announce that we have a new segment on the Newave Podcast called “Nan u Mast”. Nan u Mast is an imaginary show that we have on a Duhok radio station for 15-20 minutes once a week to fit into your morning routine. ( Nan u Mast) di gel Pêl u Nuvîn. Em wek podcast a Newave di xuš halîn bi ragehandina gušeya me ya nuyî bi navê “Nan u Mast”. Nan u Mast, bernamekê heftîtaneye ku em xeyal dikeyîn li ser radîyo eka devera Duhok ê bi hête pexiškirin li berên sipêda. Em di bernamê Nan u Mast de dê li ser rotîna xiwe ya sipêdehîya axivîn u behsa serhatîyên xiwe u guhdara keyîn. Me divêt demekê sivik u xiweš bi keyîne mêhvan li sipêdeya guhdara damê di čine ser rojanên xiwe. Music Credit: Eyaz Yosif Follow us on our Socials! instagram: @newavepodcast @paellos @fufucreations @nuveenbarwari Twitter: @nuveenbarwari @paellos96 @newavepodcast --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app Support this podcast: https://anchor.fm/newave/support

Kan du ikke få nok af bruset fra instrumenternes dronning, så er det her lige noget for dig! Nuværende og tidligere professorer ved DKDM sidder på orgelbænken i musik af bl.a. Messiaen, Bach og 150-årsjubilaren Louis Viernes. Sidst på aftenen smelter orgel, klaver, klassisk og jazz sammen i improvisioner med Monica Melcova og Jacob Anderskov. Bine Bryndorf, Hans Davidson, Hans Fagius, Monica Melcova, orgel. Jacob Anderskov, klaver. (Koncertsalen, DKDM 5. november). Vært: Anne Bro. www.dr.dk/p2koncerten

Statsminister Mette Frederiksen holder klokken 14 pressemøde om Corona-situationen i Danmark. I løbet af den sidste uges tid er smittetrykket blevet øget navnlig i hovedstadsregionen. Vi rapporterer og analyserer dagens pressemøde med vores egen Corona-medarbejder Christian Brandt Petersen. Gennem mange år har Danmark plæderet for at vi bedst hjælper flygtninge i deres nærområder - men hvordan definerer vi nærområder? Nuværende udviklingsminister Rasmus Prehn mener, at Lesbos sagtens kan være en del af det område, som EU agerer indenfor. Nej, siger den svenske EU migrationskommissær Ylva Johansson til, at Europa ikke hører til de nærområder, som EU arbejder i. I dagens Orientering spørger vi, hvorfor Danmark fortsat presser på for de såkaldte nærområder, når succesraten ikke er særlig stor. Plug -in hybrid -bilen kombinerer i reklamerne det bedste af to verdener: en slags elbil, der også har trygheden ved at have en brændstofmotor. Men nu viser en ny britisk undersøgelse, at plug-in-hybridbilerne i kørsel udleder op til to en halv gang mere CO2 end de officielle laboratorie-tests viser. "Ulve i fåreklæder" lød overskriften på britiske BBC forleden. I dagens Orientering kigger vi nærmere på hvad hybridbilerne kan og spørger, om de blot er et overgangsfænomen indtil vi har den perfekte El-bil? Karen Hjulmand og Mathias Bay Lynggaard er dagens værter. Erik Weir redigerer. www.dr.dk/orientering

For et par år siden opdagede erhvervsnetværksforeningen Expand Business i Esbjerg, at der havde været begået underslæb - og der manglede næsten et par hundrede tusinde i den fælles kasse... Nuværende formand Jacob Grumsen fortæller om chokket, skuffelsen - og hvordan foreningen med et godt sammenhold, er kommet på fode igen.

Den respekterede fotoskole Fatamorgana er endt i sit livs stormvejr. Nuværende og tidligere elever på skolen har stået frem og fortalt om et undervisningsmiljø præget af systematisk chikane. De anklager skolens leder og stifter, Morten Bo, for at mobbe, nedværdige og udefryse elever. Men hvorfor er det en stor historie, at en lille skole har et usundt undervisningsmiljø?

Niek (NUV) is piraat in hart en nieren. Hij was actief bij verschillende stations in de omgeving van Vroomshoop in Twente. Onder andere Station Super Tukker, de Condor Sekte, De Zwarte Pannenkoeken Parade, Station Nuv en Muv en Club Snorkels. In deze podcast vertelt Niek over zijn hobby als piraat en zijn vinyl verslaving. 

"Art Talk on the Levee" is part of our video podcast series called Hybrid Diaries. We talk about different techniques of our art process from concept to completion . We will be Inviting artists/musicians/filmmakers from all over the world to share their techniques/struggles and help upcoming artists everywhere. *We made sure of keeping "social distancing parameters" in place while filming this episode.All the links we talked during the show:Colombia TrilogyCuidad - https://www.youtube.com/watch?v=f5Qoy...Bantu- https://www.youtube.com/watch?v=7wv4K...Montaña-https://www.youtube.com/watch?v=5_NuV...Dead White Zombies Holy Bone Full Show- https://vimeo.com/channels/525833/242...Check out other shows at:https://www.deadwhitezombies.comNight Contemplations:Episode 1 - "Downward Spiral"- https://www.youtube.com/watch?v=pBzmN...Episode 2 - "Reflections of the soul"- https://www.youtube.com/watch?v=EB9MI...Episode 3 - "Anxiety"- https://www.youtube.com/watch?v=0ZKHN...Travel Logs Playlist:https://www.youtube.com/playlist?list...Vincent Martin Frequencies:(Download for Root Chakra Composition for Transcendental Meditation)https://www.vincentmartinmusic.com/my...ArtDallas ArtDallas ArtistsVideo PodcastArt philosophyArt processMusiciansArt/spiritualityArt talk

Ivriga och med SPÄNST tar vi oss an veckans avsnitt. Vi hamnar snabbt i ett märkligt sidospår om Peter Settman och Casper the friendly ghost, tar oss vidare förbi Nicholas Cage och hur man inte FÅR uttala Martin Luther King fel p g a respektlöst, ställer oss frågan om ifall Familjepizza är det roligaste OCH sorgligaste på samma gång (hur det nu går ihop) och gör en lång utvikning kring ett handskrivet begravningstal och prasslande papper med fnas. Först DÄREFTER dyker vi in i själva historien med Peter som var älskad av alla – eller var det bara av en endaste? – innan vi till sist tar det i så kallat mål med Jonas kanske sämsta ordvits någonsin. Och inte, som man brukar säga, ”nog” med ”det”, för vi snackar också om andra kul grejer så lyssna NUV!PATREON:www.patreon.com/rattuppiverkligheten See acast.com/privacy for privacy and opt-out information.

Mads Burnell. Straight outta´Husum, på podcastet Version 2.0.  Mads er tidligere UFC fighter. Nuværende CageWarriors Champ og på vej mod de store kampe - måske i UFC igen.  Jeg vil lade Mads fortælle dig historien selv. Vi havde en fed snak og jeg gør det med glæde igen.       

Cogu e Nuvô pegam um dos jogos mais polêmicos da história dos videogames para consertar! Será que fica bom?

Det siges at dem, der er skøre nok til at forestille sig at de kan ændre verden, er dem der rent faktisk er i stand til det. Der er tale om det danske non-profit Constructive Institute, der ledes af den tidligere chef for DR nyheder, Ulrik Haagerup, som er på en vild mission. Missionen er at forandre den globale nyhedskultur på bare fem år ved at gøre nyheder mere troværdige og meningsfulde, og dermed bekæmpe troværdighedsnedbruddet i medierne og demokratiet. Nuværende og fremtidige journalister skal lære, at den gode historie, ikke nødvendigvis behøver at være en dårlig historie. Journalistik skal derimod være fair, balanceret og inspirerende samtidig med at det skal beskæftige sig med morgendagens potentielle løsninger til vores udfordringer i samfundet. I et partnerskab med de Forenede Nationer, Google, globale medie organisationer såsom INMA, WAN-Ifra, European Broadcasting Union og journalistik uddannelser rundt omkring i Europa, har de en påstand om, at det virkelige pr

2018/7/1 Pastor Richard Welsh 韋日卓牧師 Categories: Video: https://hongkong.mylifehouse.com/tv/message/theres-a-whole-lot-of-joy-in-gods-kingdom The fruit of the spirit 聖靈的果子 (Galatians 5:22-23 NKJV) But the fruit of the Spirit is love, joy, peace, longsuffering, kindness, goodness, faithfulness, (23) gentleness, self-control. Against such there is no law. 加拉太書 5章22-23節 (CUV) 聖靈所結的果子、就是仁愛、喜樂、和平、忍耐、恩慈、良善、信實、 溫柔、節制．這樣的事、沒有律法禁止。 The disciples had joy 門徒有喜樂 (Luke 10:17-20 NKJV) Then the seventy returned with joy, saying, “Lord, even the demons are subject to us in Your name.” (18) And He said to them, “I saw Satan fall like lightning from heaven. (19) Behold, I give you the authority to trample on serpents and scorpions, and over all the power of the enemy, and nothing shall by any means hurt you. (20) Nevertheless do not rejoice in this, that the spirits are subject to you, but rather rejoice because your names are written in heaven.” 路加福音 10章17-20節 （NUV) 那七十二個人歡歡喜喜地回來，說：“主啊，因你的名，連鬼也服了我們。”耶穌說：“我看見撒但，像閃電一樣從天墜落。我已經給你們權柄，去踐踏蛇和蠍子，勝過仇敵的一切能力。絕對沒有甚麼能傷害你們了。然而不要因為鬼服了你們就歡喜，卻要因為你們的名字記錄在天上而歡喜。” Jesus had joy 耶穌有喜樂 （Luke 10:21 NKJV) In that hour Jesus rejoiced in the Spirit and said, “I thank You, Father, Lord of heaven and earth, that You have hidden these things from the wise and prudent and revealed them to babes. Even so, Father, for so it seemed good in Your sight. 路加福音10章21節 （NUV) 就在這時候，耶穌因聖靈而歡樂，說：“父啊，天地的主，我讚美你，因為你把這些事向智慧和聰明的人隱藏起來，卻向嬰孩顯明。父啊，是的，這就是你的美意。 (Psalm 100:2 NKJV) Serve the Lord with gladness; Come before His presence with singing. 詩篇 100章2節（NUV) 應當歡歡喜喜事奉耶和華，歡唱著來到他的面前。 (Psalm 118:24 NKJV) This is the day the Lord has made; We will rejoice and be glad in it. 詩篇 118章24節（NUV) 這是耶和華所定的日子，我們要在這一日歡喜快樂。 (Psalm 126:5-6 NKJV) Those who sow in tears Shall reap in joy. (6) He who continually goes forth weeping, Bearing seed for sowing, Shall doubtless come again with rejoicing, Bringing his sheaves with him. 詩篇 126章5-6節（NUV) 那些流淚撒種的，必歡呼收割。那帶著種子流著淚出去撒種的，必帶著禾捆歡呼快樂地回來

"En profil med billede ses 11 gange så ofte som en profil uden" I denne episode: Guldkorn til din LinkedIn profil Morten Vium giver tips og tricks til din karriererstrategi som du kan bruge i din jobsøgning. 1,8 mill danskere har en profil på LinkedIn - altså et godt sted at skabe netværk med andre.   De 3 vigtigste ting når du udfylder din profil på LinkedIn: At dit CV er komplet At du har et godt og professionelt billede du behøver ikke få det taget af en professionel fotograf, men det skal være pænt og præsentabelt = ingen ferie billeder En profil med billede ses 11 gange så ofte som en profil uden billede Din overskrift skal være god Hvad er det, der adskiller dig fra alle de andre? Udnyt de 120 tegn for at fange læserens opmærksomhed Dit summery Brug summary (kort beskrivelse) til at præsentere og sælge dig selv. Vis personlighed og hvad du brænder for. Få evt. hjælp fra venner og familie til at "sætte ord på dig". Eksempler på succeshistorier - hvad har du opnået karrierermæssigt. Det er også her du skal se fremad, fortæl hvad du kan hjælpe en fremtidig arbejdsgiver med. Beskrivelsen af dine tidligere jobs er et tilbageblik, altså viser hvad du har arbejdet med, og hvad du kan. Nuværende stilling som jobsøgende For at linkedIn skal se din profil som komplet (og dermed komme højere op i søgeresultaterne) skal 'Nuværende stilling' være udfyldt. Et tip kan være at du skriver: Jobsøgende Pædagog, Jobsøgende Ingeniør eller andet med relevans for din uddannelse. Profil fokus Din profil skal hjælpe arbejdsgiverne (din målgruppe) med en beskrivelse af hvad det er DU kan. Ikke med fokus på at du er jobsøgende. LinkedIn vs. Facebook Du skal være opmærksom på at arbejdsgiverne tjekker din Facebook profil og søger efter dig på Google, når du søger arbejde hos dem. Facebook = personligt netværk (bruges ikke til at rekruttere nye medarbejdere) LinkedIn = professionelt netværk (bruges til at rekruttere nye medarbejdere) Morten anbefaler Når de 3 basis ting er på plads, udfyldt CV, billede og overskrift, samt at du har skrevet et godt summery er det tid til at kigge på at gøre profilen mere fuldstændig. Det kan du gøre ved at udfylde flere dele og skabe aktivitet på og med din profil:   Hent anbefalinger fra tidligere arbejdsgivere - det skaber troværdighed. Udfylde din profil med: Projekter, udgivelser, frivilligt arbejde, organisationer du er en del af. Bruge søgefunktionen aktivt. Kender du nogen der kender nogen der er connected med en, for dig, interessant person. Herefter sende en mail til vedkommende og præsenter dig. Hvis du kigger på folks profiler kan det betyde at de "kigger tilbage" på din. Dette betyder at du viser interesse i dem og kan gøre dem nysgerrige efter at vide mere om dig.   Statusopdatering og grupper:  VÆR AKTIV - der sker ikke noget før du selv gør noget ~ vær proaktiv   Kender du nogen i dit netværk, der kender vedkommende du gerne vil i kontakt med så, skriv til dem og spørg efter råd til hvordan du kan komme i kontakt med vedkommende. Det virker MEGET bedre end en statusopdatering som: "Jeg er jobsøgende, hjælp mig!"   Brug dine statusopdateringer til at gøre dig selv til "ekspert" inden for dit område. Herved giver du dit netværk mulighed for at like det og sende det ud i deres netværk. Det skaber synlighed omkring DIG.   Skab synlighed om dig selv ved at skrive i din blog på LinkedIn om ting, der skaber værdi for andre.   Vil du connecte med folk du ikke kender personligt på LinkedIn så skriv en personlig hilsen.   Ellers kan du risikere at blive anmeldt for spam og du vil få svært ved at skabe relationer på LinkedIn uden at kende folks mailadresse efterfølgende   Hvis du modtager en invitation fra en du ikke kender så skriv tilbage og sig tak (og fortæl evt lidt om dig selv)   Du kan finde Morten på http://mortenvium.dk/   Lyt til episoden for at finde ud af hvordan du kan vinde Morten's kursus - Strategisk networking på LinkedIn, den digitale vej til nye kunder og nye relationer. Du kan også finde det første modul af kurset gratis på hans website. Du er velkommen til at komme med kommentarer og ideer til fremtidige episoder ved at skrive en mail til mig på info@jobeksperten.dk Go' jobjagt

Galaxies have been found to divide into two families: one dominated by late-type, star forming, blue objects, which are rich in cold gas and have a low stellar mass surface density (mu*); the other is made of early-type, red and passive galaxies with higher mu* and on average low gas content. The physical mechanisms responsible for the galaxy transition between the active and passive regime are still debated. In the high mass range, mechanisms proposed to quench the star formation (SF) through cold gas heating or depletion are not efficient enough to reproduce the correct red sequence of passive systems, when implemented in models of galaxy evolution. Input for a better understanding of the physics of quenching mechanisms, and of their relative importance and efficiency, can come from a comparison of the cold atomic neutral hydrogen (HI) content and SF for a statistically significant sample of massive systems where quenching is at work. However, existing surveys do not sample this high mass, gas poor regime well enough. In this work, we study the HI properties of a volume-limited sample of ~5000 nearby galaxies with stellar mass M*>10^10 Msun, selected from the state-of-the-art blind HI survey ALFALFA to have optical and ultraviolet data so that star formation and galaxy properties can be derived. As ALFALFA does not sample with sufficient sensitivity the high mass, gas poorest range, we developed a software tool to co-add its data, in order to obtain average gas properties of galaxy classes which individually may be largely undetected. Using this technique, we study three types of quenching processes, namely the presence of a bulge component, feedback from an active galactic nucleus (AGN), and environmental mechanisms acting on the interstellar medium. Simulations of early-type galaxies with non star-forming HI disks have suggested that the presence of a bulge can stabilize the gas, thus preventing star formation, but on average we do not observe this. We find that, once mu* and NUV-r colours are fixed, the HI gas fraction in massive bulge- and disk-dominated galaxies is the same. A similar negative result is obtained if we compare M_HI/M* of AGN hosts and control galaxies, despite simulations that invoke feedback from AGN to heat or deplete cold gas in massive systems. The relation we observe between the cold gas content and the accretion rate in the red population actually points towards a co-evolution of SF and AGN activity, both driven by the amount of gas available. The last class of quenching mechanisms studied in this work includes environmental processes, which are known to affect the SF properties of galaxies and, at least in rich clusters, their cold gas content. For the first time, though, we study the effect of the environment on the HI content as a continuous function of local density, comparing it with global and inner specific star formation rate. The gradual increase in the suppression of SF from the inner to the outer regions that we observe, and the even stronger HI deficiency as a function of increasing local density, can be explained by a mechanism acting on the disk from the outside-in, like ram-pressure stripping of the HI. A comparison with mock catalogs from models, which include only removal of the hot gas, shows how models underestimate environmental effects, especially on the cold gas component of galaxies. We therefore suggest that, in order to improve our understanding of the galaxy bimodality in the local Universe, observations and models should particularly focus on environmental mechanisms acting on the cold interstellar medium. These processes are efficient over a broader range of local densities than previously thought, and could solve parts of the puzzle in the formation of massive and passive systems.