Podcasts about candels

Welcome to Cyrus Says! 00:00 - SUBSCRIBE NOW! 01:01 - PYAAR TOH HONA HI THA! 05:42 - AYESHA LOOKS HAPPY :) 16:41 - LET THE FIGHT BEGIN! 24:08 - FOOD DATE without CANDELS! 32:40 - AMA X FANS XD 42:45 - PRODUCER GOING ALL OUT! Cyrus and Ayesha bring the ultimate mix of fun, sarcasm, and marriage truths in this special episode! From celebrating Ayesha’s big win at Ironman Goa (and scoring a Scott Sports bicycle as a gift) to binge-watching The Fabulous Lives of Bollywood Wives and attending Vijay 69 with Anupam Kher—this episode is packed with hilarious moments! Who said “I love you” first? Who’s more likely to survive in the wild without the internet? Would Ayesha rather never argue again or never hear Cyrus talk again? And why isn’t marriage banned in 193 countries yet? Fans take over in the AMA session, asking when Ayesha will finally record a gym video of Cyrus, what a podcast designed purely to trouble him would look like, and whether we’ll ever see the couple painting, weightlifting, or even doing a triathlon together. Plus, we keep the cameras rolling during brunch, capturing those raw, unfiltered rants for marketing gold! Don’t miss this episode filled with laughs, chaos, and classic Cyrus madness! Kripya subscribe to the channel: https://www.youtube.com/c/CyrusSays Listen to the full audio episodes at: Amazon Music Exclusive https://music.amazon.in/podcasts/4d52847d-6dbd-46b1-8219-34792a987d09/cyrus-says---amazon-music-exclusive Email your AMA questions to us at whatcyrussays@gmail.com Don’t forget to follow Cyrus Says’ official Instagram handle at @‌whatcyrussays [https://www.instagram.com/whatcyrussays/] Connect with Cyrus on socials: Instagram: https://www.instagram.com/cyrus_broacha/ Twitter: https://twitter.com/Broacha_Cyrus Aur like, share, comment karna na bhule!See omnystudio.com/listener for privacy information.

Deep Learning-based galaxy image deconvolution by Utsav Akhaury et al. on Monday 21 November With the onset of large-scale astronomical surveys capturing millions of images, there is an increasing need to develop fast and accurate deconvolution algorithms that generalize well to different images. A powerful and accessible deconvolution method would allow for the reconstruction of a cleaner estimation of the sky. The deconvolved images would be helpful to perform photometric measurements to help make progress in the fields of galaxy formation and evolution. We propose a new deconvolution method based on the Learnlet transform. Eventually, we investigate and compare the performance of different Unet architectures and Learnlet for image deconvolution in the astrophysical domain by following a two-step approach: a Tikhonov deconvolution with a closed-form solution, followed by post-processing with a neural network. To generate our training dataset, we extract HST cutouts from the CANDELS survey in the F606W filter (V-band) and corrupt these images to simulate their blurred-noisy versions. Our numerical results based on these simulations show a detailed comparison between the considered methods for different noise levels. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.09597v1

The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3 by P. Santini et al. on Sunday 25 September Despite significant efforts in the recent years, the physical processes responsible for the formation of passive galaxies through cosmic time remain unclear. The shape and evolution of the Stellar Mass Function (SMF) give an insight into these mechanisms. Taking advantage from the CANDELS and the deep Hubble Frontier Fields (HFF) programs, we estimated the SMF of total, star-forming and passive galaxies from z=0.25 to z=2.75 to unprecedented depth, and focus on the latter population. The density of passive galaxies underwent a significant evolution over the last 11 Gyr. They account for 60% of the total mass in the nearby Universe against ~20% observed at z~2.5. The inclusion of the HFF program allows us to detect, for the first time at z>1.5, the characteristic upturn in the SMF of passive galaxies at low masses, usually associated with environmental quenching. We observe two separate populations of passive galaxies evolving on different timescales: roughly half of the high mass systems were already quenched at high redshift, while low mass passive galaxies are gradually building-up over the redshift range probed. In the framework of environmental-quenching at low masses, we interpret this finding as evidence of an increasing role of the environment in the build-up of passive galaxies as a function of time. Finally, we compared our findings with a set of theoretical predictions. Despite good agreement in some redshift and mass intervals, none of the models are able to fully reproduce the observations. This calls for further investigation into the involved physical mechanisms, both theoretically and observationally, especially with the brand new JWST data. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.11250v1

Luke 2:11 says, "For unto you is born this day in the city of David a Savior, who is Christ the Lord." Bethlehem was not your typical destination city.  So why would a king chose this place to be born?  Today, let us go into the text and discover the meaning of our second candle: The Bethlehem Candle.

Bruma perpetua es una aventura de género noir que ha sido adaptada por nuestro máster de cabecera Adrián para ser jugada en el juego de rol Ten Candles, un fantástico juego indie de aventuras de terror de una sola sesión. Sirve también esta aventura como previa de una futura campaña de City of Mist dirigida por Adrián que pronto llevaremos a mesa. Jack en el papel de Mr. Brown Iván en el papel de Joseph John en el papel de Luca Merch

Of Dresses and Candels - part 116 Theo takes Prince Rugh-Malan on a tour of the pubs and taverns, while the girls check out a new candel factory. And Duilintrast has issues with some of the house servents who seem to always ignore him.

Ianthe Mauro is a momprenuer that has cascades light and turned it into a glowing business as a candle creator with a booming product line. Her candle have graces some of Hollywood greatest swag bags. And.. Speaking of Hollywood don't let me forget that she is an actress herself.    

In this special podcast from the National Astronomy Meeting in Llandudno, we hear how twisted sunspots cause solar flares, how 17th century poetry can put a date on a supernova, and why some pulsars are part-timers. We'll find out how CANDELS and LOFAR can probe the early universe, while DEBRIS looks for dusty disks around stars. Plus, we shed light on your solar science questions! Like this podcast? Please help us by supporting the Naked Scientists

In this special podcast from the National Astronomy Meeting in Llandudno, we hear how twisted sunspots cause solar flares, how 17th century poetry can put a date on a supernova, and why some pulsars are part-timers. We'll find out how CANDELS and LOFAR can probe the early universe, while DEBRIS looks for dusty disks around stars. Plus, we shed light on your solar science questions! Like this podcast? Please help us by supporting the Naked Scientists

The universe is big – really big.* Galaxies, for instance, are often large enough to hold a trillion stars. But how did these heavenly heavyweights come to be? Hear how still-mysterious dark matter is implicated in the birth of galaxies. Also, gamma ray bursts - explosions more energetic than anything since the Big Bang - take place somewhere in the visible universe every day. What are they, and could they obliterate life on Earth? And, the biggest cosmic mystery de jour: dark energy. Why new, super-size telescopes may finally reveal just what it is. We're living large on “Big, Really Big.” *appreciative nod to Douglas Adams Guests: George Djorgovski - Astronomer, California Institute of Technology Sandra Faber - Astronomer and Chair of Astronomy and Astrophysics, University of California at Santa Cruz; leads the CANDELS survey that uses the Hubble Space Telescope to image more than 250,000 distant galaxies Daniel Perley - Astronomer, University of California at Berkeley Ed Stone - Former director of the Jet Propulsion Laboratory, and physicist at the California Institute of Technology Richard Panek - Author of The 4 Percent Universe: Dark Matter, Dark Energy, and the Race to Discover the Rest of Reality Descripción en español Learn more about your ad choices. Visit megaphone.fm/adchoices

The universe is big – really big.* Galaxies, for instance, are often large enough to hold a trillion stars. But how did these heavenly heavyweights come to be? Hear how still-mysterious dark matter is implicated in the birth of galaxies. Also, gamma ray bursts - explosions more energetic than anything since the Big Bang - take place somewhere in the visible universe every day. What are they, and could they obliterate life on Earth? And, the biggest cosmic mystery de jour: dark energy. Why new, super-size telescopes may finally reveal just what it is. We’re living large on “Big, Really Big.” *appreciative nod to Douglas Adams Guests: George Djorgovski - Astronomer, California Institute of Technology Sandra Faber - Astronomer and Chair of Astronomy and Astrophysics, University of California at Santa Cruz; leads the CANDELS survey that uses the Hubble Space Telescope to image more than 250,000 distant galaxies Daniel Perley - Astronomer, University of California at Berkeley Ed Stone - Former director of the Jet Propulsion Laboratory, and physicist at the California Institute of Technology Richard Panek - Author of The 4 Percent Universe: Dark Matter, Dark Energy, and the Race to Discover the Rest of Reality Descripción en español

We met someone with a bumper sticker this morning. Your job, imagine "16 Candles" with Pelicans. Good. Now that you've done that, imagine who is bailing out Steve Baldwin now. Hint: it might be God. One final imagine. Imagine, if you will, the next step in cellular technology. Forget Apple Phones, Google Phones, and Yahoo Phones. The future my friends is the Ask Jeeves Steamer Trunk. Imagine that! Phew, by now I imagine your imaginations is all tuckered out. Why don't you give that old brain box a rest and join us for some laughs. Go ahead, LISTEN. Yup, now is fine. Go ahead. Seriously, why are you still reading.