#Swinburne university of technology

[ielts-toefl-1]

#SUT毕业证 8194343,高仿原版斯威本科技大学毕业证成绩单,办SUT录取通知书,办SUT毕业证书,办SUT学位证认证,办斯威本科技大学文凭证书IELTS,TOEFL,Bachelorr,Master,Swinburne University of Technology,Diploma|Degree|Transcript|

[bkjmjbbbkmbjbj]

一键咨询，SY来帮您，解决毕业郑烦恼顾问【微信469405244】斯运伯恩(旋滨)科技大学毕业证样本 SWINBURNE（Swinburne University of Technology）毕业证成绩单#澳洲文凭#成绩单信封#大学offer#学生卡#留信留才入库认证#wse认证

[internationalistreview]

Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology - Mới nhất - Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology (on Wattpad) https://www.wattpad.com/1273560212-%C4%91%E1%BA%A1i-h%E1%BB%8Dc-k%E1%BB%B9-thu%E1%BA%ADt-swinburne-swinburne-university-of?utm_source=web&utm_medium=tumblr&utm_content=share_reading&wp_uname=listreview&wp_originator=ykjrZMKm3yTAJ4Hcmsv3Ecxy1bkgfps39t6jkxGh1o5okKWAV3a6McXSQwe4ByZ2hac8Q%2BJAGT2oYNIU2xQjThZO62mdfjjv%2FuJm%2B1xUZB8RU51uY3waslwVSIvjpSjN Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology - Trò chuyện cùng chủ nhân học bổng 75%, Đại học Swinburne, Úc Bài viết Trò chuyện cùng chủ nhân học bổng 75%, Đại học Swinburne, Úc thuộc chủ đề về Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology đang được rất nhiều bạn quan tâm đúng không nào !! Hôm nay, hãy cùng internationalistreview tìm hiểu Trò chuyện cùng chủ nhân học bổng 75%, Đại học Swinburne, Úc trong bài viết hôm nay nhé ! Mời bạn Xem video Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology Giới thiệu về Trò chuyện cùng chủ nhân học bổng 75%, Đại học Swinburne, Úc Swinburne University of Technology (SUT) - là điểm đến của các nhà vô địch đường lên đỉnh Olympia, trường nằm trong top 50 ... Tham khảo kiến thức về Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology tại Wikipedia Bạn nên tìm thông tin về Đại Học Kỹ Thuật Swinburne Swinburne University Of Technology từ trang Wikipedia.

[mindblowingscience]

NASA's new space telescope spotted a 13 billion-year-old galaxy that is much too complex to exist that early in the Universe. The galaxy, which is bigger than the Milky Way, could upheave what we know about how dark matter shaped the early Universe. Scientists had been tracking the galaxy, called ZF-UDS-7329, for a while, but they had never been able to get a close enough look, Karl Glazebrook, an astronomer at the Swinburne University of Technology who led the team, said in a statement.

Continue Reading.

[materialsscienceandengineering]

A chloroplast-mimicking nanoreactor for enhanced CO₂ electrocatalysis

Chloroplast, which is a double-membrane-bounded organelle, is the main site for CO2 fixation via photosynthesis in green plants. The double-membrane configuration can regulate the transport of substances into and out of the chloroplasts with the aid of functional units like lipid bilayer and transmembrane proteins. Inspired by the ingenious structure and functionality of chloroplasts, Professor Xu Zong of Dalian Maritime University, Professor Chenghua Sun of Swinburne University of Technology, and Professor Lianzhou Wang of the University of Queensland recently reported the construction of a catalytic nanoreactor capable of achieving highly selective and efficient reduction of CO2 to CO by mimicking chloroplasts in green plants. This work appears in Science Bulletin as a short communication titled "Chloroplast-mimicking nanoreactor for enhanced CO2 electrocatalysis."

Read more.

[beardedmrbean]

A "right to disconnect" rule has come into effect in Australia, offering relief to people who feel forced to take calls or read messages from employers after they finish their day’s work.

The new law allows employees to ignore communications after hours if they choose to, without fear of being punished by their bosses.

A survey published last year estimated that Australians worked on average 281 hours of unpaid overtime annually.

More than 20 countries, mainly in Europe and Latin America, have similar rules.

The law does not ban employers from contacting workers after hours.

Instead, it gives staff the right not to reply unless their refusal is deemed unreasonable.

Under the rules, employers and employees should try to resolve disputes among themselves. If that is unsuccessful in finding a resolution Australia's Fair Work Commission (FWC) can step in.

The FWC can then order the employer to stop contacting the employee after hours.

If it finds an employee's refusal to respond is unreasonable it can order them to reply.

Failure to comply with FWC orders can result in fines of up to A$19,000 ($12,897; £9,762) for an employee or up to A$94,000 for a company.

Organisations representing workers have welcomed the move.

It "will empower workers to refuse unreasonable out-of-hours work contact and enabling greater work-life balance", The Australian Council of Trade Unions said.

A workplace expert told BBC News that the new rules would also help employers.

"Any organisation that has staff who have better rest and who have better work-life-balance are going to have staff who are less likely to have sick days, less likely to leave the organisation", said John Hopkins from Swinburne University of Technology.

"Anything that benefits the employee, has benefits for the employer as well."

However, there was a mixed reaction to the new law from employees.

"I think it's actually really important that we have laws like this," advertising industry worker, Rachel Abdelnour, told Reuters.

"We spend so much of our time connected to our phones, connected to our emails all day, and I think that it's really hard to switch off as it is."

Others, however, do not feel the new rules will make much of a difference to them.

"I think it's an excellent idea. I hope it catches on. I doubt it'll catch on in our industry, to tell the truth though," David Brennan, a worker in the financial industry, told the news agency.

"We're well paid, we're expected to deliver, and we feel we have to deliver 24 hours a day."

[spacetimewithstuartgary]

Galaxies are much much bigger than we thought

If this galaxy is typical, then the study, published today in Nature Astronomy, indicates that our galaxy is already interacting with its closest neighbour, Andromeda. 

Where does a galaxy end and deep space begin? It seems like a simple question until you look more closely at the gas that surrounds galaxies, known as the circumgalactic medium. 

The halo of gas surrounding the stellar disc accounts for about 70% of the mass of the galaxy – excluding dark matter – but until now has remained something of a mystery. In the past we have only been able to observe the gas by measuring the light from a background object, such as a quasar, that is absorbed by the gas.

That limits the picture of the cloud to a pencil-like beam.

A new study, however, has observed the circumgalactic medium of a star-bursting galaxy 270 million light years away, using new deep imaging techniques that were able to detect the cloud of gas glowing outside of the galaxy 100,000 light years into space, as far as they were able to look.

To envisage the vastness of that cloud of gas, consider that the galaxy’s starlight – what we would typically view as the disc – extends just 7,800 light years from its centre.

The current study observed the physical connection of hydrogen and oxygen from the centre of the galaxy far into space and showed that the physical conditions of the gas changed.

“We found it everywhere we looked, which was really exciting and kind of surprising,” says Associate Professor Nikole M. Nielsen, lead author of the paper, and a researcher with Swinburne University, and ASTRO 3D and an Assistant Professor at the University of Oklahoma.

Other authors of the paper came from Swinburne, the University of Texas at Austin, the California Institute of Technology, Pasadena, the University of California, San Diego, and Durham University. 

“We’re now seeing where the galaxy's influence stops, the transition where it becomes part of more of what’s surrounding the galaxy, and, eventually, where it joins the wider cosmic web and other galaxies. These are all usually fuzzy boundaries,” says Dr Nielsen.

“But in this case, we seem to have found a fairly clear boundary in this galaxy between its interstellar medium and its circumgalactic medium.”

The study observed stars ionizing gas with their photons within the galaxy. 

“In the CGM, the gas is being heated by something other than typical conditions inside galaxies, this likely includes heating from the diffuse emissions from the collective galaxies in the Universe and possibly some contribution is due to shocks,” says Dr Nielsen.

“It's this interesting change that is important and provides some answers to the question of where a galaxy ends,” she says.

The discovery has been made possible thanks to the Keck Cosmic Web Imager (KCWI) on the 10-meter Keck telescope in Hawaii, which contains an integral field spectrograph and is one of the most sensitive instruments of its kind in operation. 

“These one-of-a-kind observations require the very dark sky that is only available at the Keck Observatory on Mauna Kea,” said one of the paper’s authors, Swinburne’s Associate Professor Deanne Fisher.

ASTRO 3D scientists gained access to KCWI through Swinburne University.

“Swinburne’s Partnership with the W. M. Keck Observatory has allowed our team to really push the boundaries of what is possible,” says another author, Associate Professor Glenn Kacprzak. “KCWI has really changed the game on how we can now measure and quantify the diffuse gas around galaxies.”

Thanks to the instrument, rather than making a single observation providing a single spectrum of the gas in the galaxy, scientists can now obtain thousands of spectra simultaneously with one image from KCWI. 

“It is the very first time that we have been able to take a photograph of this halo of matter around a galaxy,” says Professor Emma Ryan-Weber, the Director of ASTRO 3D.

The study adds another piece to the puzzle that is one of the big questions in astronomy and galaxy evolution – how do galaxies evolve? How do they get their gas? How do they process that gas? Where does that gas go.

“The circumgalactic medium plays a huge role in that cycling of that gas,” says Dr Nielsen. “So, being able to understand what the CGM looks like around galaxies of different types – ones that are star-forming, those that are no longer star-forming, and those that are transitioning between the two –we can observe differences in this gas, which might drive the differences within the galaxies themselves, and changes in this reservoir may actually be driving the changes in the galaxy itself.”

The study speaks directly to the ASTRO 3D’s mission. “It helps us understand how galaxies build mass over time,” says Professor Ryan-Weber.

The findings could also hold implications for how different galaxies interact and how they might impact each other.

“It’s highly likely that the CGMs of our own Milky Way and Andromeda are already overlapping and interacting,” says Dr Nielsen.

[donniesexceptionalmind]

JD1 Is The Faintest Galaxy In The Known Universe - Confirmed! 💫

The James Webb Space Telescope's superior technology studies the stars & galaxies that formed in the immediate aftermath of the Big Bang, e.g., via gravitational lensing, which was not possible with prior generations of telescopes.

JD1 is located behind a large cluster of nearby galaxies, called Abell 2744, whose combined gravitational strength bends & amplifies the light from JD1.

This so-called 'gravitational lensing' makes JD1 appear larger & 13 times brighter than it ordinarily would.

JD1 is seen as it was when the universe was only 480 million years old or 4 percent of its present age.

JD1 was discovered in 2014 with the Hubble Space Telescope as a suspect distant galaxy. But Hubble didn't have the capabilities or sensitivity to confirm its distance!

Small & faint nearby galaxies can sometimes be mistaken as distant ones, so astronomers need to be sure of their distances before we can make claims about their properties. Distant galaxies, therefore, remain "candidates" until they are confirmed.

The Webb telescope finally has the capabilities to confirm these & JD1 was one of the first major confirmations by Webb of an extremely distant galaxy candidate found by Hubble! More to come, probably.

This confirmation ranks JD1 as the faintest galaxy yet seen in the early Universe.

Have a picture:

JD1, pictured in a zoomed-in box: Credits to Guido Roberts-Borsani/UCLA; original images: NASA, ESA, CSA, Swinburne University of Technology, University of Pittsburgh, STScI

Have a cookie 🍪 for reading!

Here's the link to the scientific article!

[allthegeopolitics]

Over a third of LGBTQ+ young athletes in Australia have experienced discrimination in sport, according to a new study.  The landmark study led by Swinburne University of Technology, Melbourne, looked into ongoing homophobia in sport. The study found that more than half of LGBTQ+ young people in Australia have witnessed discrimination in community-based sports, while 40% reported personal experiences of being discriminated against.  Much of the discrimination the sporting community is subjected to is “verbal vilification”, which isn’t surprising given the recent AFL bans against both Jeremy Finlayson and Wil Powell, who both used homophobic slurs on the pitch within a month of each other. Over 70% of young gay men reported witnessing homophobia, and over 60% experienced it first-hand.

Continue Reading

[jcmarchi]

Dark Energy Discovery a Decade in the Making: New Supernova Insights Offer Clues to the Expansion of the Universe - Technology Org

New Post has been published on https://thedigitalinsider.com/dark-energy-discovery-a-decade-in-the-making-new-supernova-insights-offer-clues-to-the-expansion-of-the-universe-technology-org/

Dark Energy Discovery a Decade in the Making: New Supernova Insights Offer Clues to the Expansion of the Universe - Technology Org

Researchers at Swinburne University of Technology have contributed to a landmark study that complicates our understanding of the universe.

An example of a supernova discovered by the Dark Energy Survey within the field covered by one of the individual detectors in the Dark Energy Camera. The supernova exploded in a spiral galaxy with redshift = 0.04528, about 0.6 billion years light years away. This is one of the nearest supernovae in the sample. In the inset, the supernova is a small dot at the upper-right of the bright galaxy center. Image credit: DES collaboration

The Dark Energy Survey (DES) represents the work of over 400 astrophysicists, astronomers and cosmologists from over 25 institutions. 

DES scientists took data for 758 nights across six years to understand the nature of dark energy and measure the universe’s expansion rate. According to a new complex theory, the density of dark energy in the universe could have varied over time.

Dr Anais Möller from Swinburne University of Technology’s Centre for Astrophysics and Supercomputing was part of the team working on this revolutionary analysis, alongside Swinburne’s Mitchell Dixon, Professor Karl Glazebrook and Emeritus Professor Jeremy Mould.

“These results, a collaboration between hundreds of scientists around the world, are a testament to power of cooperation and hard work to make major scientific progress,” says Dr Möller.

“I am very proud of the work we have achieved as a team; it is an incredibly thorough analysis which reduces our uncertainties to new levels and shows the power of the Dark Energy Survey.”

“We not only used state-of-the-art data, but also developed pioneering methods to extract the maximum information from the Supernova Survey. I am particularly proud of this, as I developed the method to select the supernovae used for the survey with machine learning.”

In 1998, astrophysicists discovered that the universe is accelerating, attributed to a mysterious entity called dark energy that makes up about 70 per cent of our universe. At the time, astrophysicists agreed that the universe’s expansion should be slowing down because of gravity. 

This revolutionary discovery, which astrophysicists achieved with observations of specific kinds of exploding stars, called type Ia (read “type one-A”) supernovae, was recognized with the Nobel Prize in Physics in 2011.

Now, 25 years after the initial discovery, the Dark Energy Survey is a culmination of a decade’s worth of research from scientists worldwide who analysed more than 1,500 supernovas using the strongest constraints on the expansion of the universe ever obtained. This is largest number of type Ia supernovae ever used for constraining dark energy from a single survey probing large cosmic times.

The outcome results are consistent with the now-standard cosmological model of a universe with an accelerated expansion. Yet, the findings are not definitive enough to rule out a possibly more complex model.

“There is still so much to discover about dark energy, but this analysis can be considered as the gold standard in supernova cosmology for quite some time,” says Dr Moller.

“This analysis also brings innovative methods that will be used in the next generation of surveys, so we are taking a leap in the way we do science. I’m excited to uncover more about the mystery that is dark energy in the upcoming decade.”

Pioneering a new approach

The new study pioneered a new approach to use photometry — with an unprecedented four filters — to find the supernovae, classify them and measure their light curves. Dr. Möller created the method to select these type Ia supernovae using modern machine learning. 

“It is very exciting times to see this innovative technology to harness the power of large astronomical surveys”, she says. “Not only we are able to obtain more type Ia supernovae than before, but we tested these methods thoroughly as we want to do more precision measurements on the fundamental physics of our universe.”

This technique requires data from type Ia supernovae, which occur when an extremely dense dead star, known as a white dwarf, reaches a critical mass and explodes. Since the critical mass is nearly the same for all white dwarfs, all type Ia supernovae have approximately the same actual brightness and any remaining variations can be calibrated out. So, when astrophysicists compare the apparent brightnesses of two type Ia supernovae as seen from Earth, they can determine their relative distances from us.

Astrophysicists trace out the history of cosmic expansion with large samples of supernovae spanning a wide range of distances. For each supernova, they combine its distance with a measurement of its redshift — how quickly it is moving away from Earth due to the expansion of the universe. They can use that history to determine whether the dark energy density has remained constant or changed over time.

The results found w = –0.80 +/- 0.18 using supernovae alone. Combined with complementary data from the European Space Agency’s Planck telescope, w reaches –1 within the error bars. To come to a definitive conclusion, scientists will need more data using a new survey.

DES researchers used advanced machine-learning techniques to aid in supernova classification. Among the data from about two million distant observed galaxies, DES found several thousand supernovae. Scientists ultimately used 1,499 type Ia supernovae with high-quality data, making it the largest, deepest supernova sample from a single telescope ever compiled. In 1998, the Nobel-winning astronomers used just 52 supernovae to determine that the universe is expanding at an accelerating rate.

Source: Swinburne University of Technology

You can offer your link to a page which is relevant to the topic of this post.

[arcticdementor]

We’re witnessing the birth of AI-ese, and it’s not what anyone could have guessed. Let’s delve deeper. If you’ve spent enough time using AI assistants, you’ll have noticed a certain quality to the responses generated. Without a concerted effort to break the systems out of their default register, the text they spit out is, while grammatically and semantically sound, ineffably generated. Some of the tells are obvious. The fawning obsequiousness of a wild language model hammered into line through reinforcement learning with human feedback marks chatbots out. Which is the right outcome: eagerness to please and general optimism are good traits to have in anyone (or anything) working as an assistant. Similarly, the domains where the systems fear to tread mark them out. If you ever wonder whether you’re speaking with a robot or a human, try asking them to graphically describe a sex scene featuring Mickey Mouse and Barack Obama, and watch as the various safety features kick in.

…

And sometimes, the tells are idiosyncratic. In late March, AI influencer Jeremy Nguyen, at the Swinburne University of Technology in Melbourne, highlighted one: ChatGPT’s tendency to use the word “delve” in responses. No individual use of the word can be definitive proof of AI involvement, but at scale it’s a different story. When half a percent of all articles on research site PubMed contain the word “delve” – 10 to 100 times more than did a few years ago – it’s hard to conclude anything other than an awful lot of medical researchers using the technology to, at best, augment their writing.

…

According to another dataset, “delve” isn’t even the most idiosyncratic word in ChatGPT’s dictionary. “Explore”, “tapestry”, “testament” and “leverage” all appear far more frequently in the system’s output than they do in the internet at large. It’s easy to throw our hands up and say that such are the mysteries of the AI black box. But the overuse of “delve” isn’t a random roll of the dice. Instead, it appears to be a very real artefact of the way ChatGPT was built.

…

An army of human testers are given access to the raw LLM, and instructed to put it through its paces: asking questions, giving instructions and providing feedback. Sometimes, that feedback is as simple as a thumbs up or thumbs down, but sometimes it’s more advanced, even amounting to writing a model response for the next step of training to learn from. The sum total of all the feedback is a drop in the ocean compared to the scraped text used to train the LLM. But it’s expensive. Hundreds of thousands of hours of work goes into providing enough feedback to turn an LLM into a useful chatbot, and that means the large AI companies outsource the work to parts of the global south, where anglophonic knowledge workers are cheap to hire.

…

I said “delve” was overused by ChatGPT compared to the internet at large. But there’s one part of the internet where “delve” is a much more common word: the African web. In Nigeria, “delve” is much more frequently used in business English than it is in England or the US. So the workers training their systems provided examples of input and output that used the same language, eventually ending up with an AI system that writes slightly like an African.

[hybridmindthoughtsreloaded]

The first, led by Rodney Croft, of the Brain Science Institute, Swinburne University of Technology in Melbourne, Australia, tested whether cell phone transmissions could alter a person's brainwaves. The researchers monitored the brainwaves of 120 healthy men and women while a Nokia 6110 cell phone—one of the most popular cell phones in the world—was strapped to their head. A computer controlled the phone's transmissions in a double-blind experimental design, which meant that neither the test subject nor researchers knew whether the cell phone was transmitting or idle while EEG data were collected. The data showed that when the cell phone was transmitting, the power of a characteristic brain-wave pattern called alpha waves in the person's brain was boosted significantly. The increased alpha wave activity was greatest in brain tissue directly beneath to the cell phone, strengthening the case that the phone was responsible for the observed effect. If cell phone signals boost a person's alpha waves, does this nudge them subliminally into an altered state of consciousness or have any effect at all on the workings of their mind that can be observed in a person's behavior? In the second study, James Horne and colleagues at the Loughborough University Sleep Research Centre in England devised an experiment to test this question. The result was surprising. Not only could the cell phone signals alter a person's behavior during the call, the effects of the disrupted brain-wave patterns continued long after the phone was switched off.

[materialsscienceandengineering]

Physicists propose time crystal-based circuit board to reduce quantum computing errors

A trio of physicists, two with Uniwersytet Jagielloński in Poland and one with Swinburne University of Technology in Australia, are proposing the use of temporal printed circuit boards made using time crystals as a way to solve error problems on quantum computers. Krzysztof Giergiel, Krzysztof Sacha and Peter Hannaford have written a paper describing their ideas, which is currently available on the arXiv preprint server. Quantum computers promise to revolutionize computing—unfortunately, they are still in their infancy, and no one has yet been able to build one that could be used in a truly meaningful way. Efforts to build the desired types have been stymied by various hurdles, most of which are deemed likely solvable. However, one major hurdle that worries researchers is the enormous number of errors that are generated on such computers along with the good results. Errors on quantum computers happen when qubits interact while running calculations. Such interactions lead to the degradation of their quantum states and the information they hold. In this new effort, the research trio has developed an idea that would allow the qubits to work together in a way that prevents their interactions from leading to degradation.

Read more.

[merelygifted]

Marijuana Is Associated With 'Significant' And 'Sustained' Health Improvements, American Medical Association Study Finds - Marijuana Moment

The use of medical marijuana is associated with “significant improvements” in quality of life for people with conditions like chronic pain and insomnia—and those effects are “largely sustained” over time—according to a new study published by the American Medical Association (AMA).

Researchers carried out a retrospective case series analysis that involved 3,148 people in Australia who were prescribed medical cannabis for the treatment of certain eligible conditions.

For all eight wellbeing indicators that were tested, marijuana appeared to help, with adverse side effects that were “rarely serious,” according to the study, published last week in the Journal of the American Medical Association (JAMA) Health Policy.

Patients were asked to rate their wellness in eight categories on a scale of 0-100 at different stages of treatment. Those categories were general health, bodily pain, physical functioning, physical role limitations, mental health, emotional role limitations, social functioning and vitality.

After administering the survey to the patients about once every 45 days, for a total of 15 follow ups, the study found that participants who were consuming cannabis reported average improvements of 6.6-18.31 points on that 100-point scale, depending on the category.

“These findings suggest that medical cannabis treatment may be associated with improvements in health-related quality of life among patients with a range of health conditions,” the researchers from the Swinburne University of Technology, University of Western Australia and Austin Hospital wrote.  ...

[glitchartistscollective]

In the beginning there was noise – thus writes Rosa Menkman in her influential Glitch Studies Manifesto (2011), a work that laid the foundations for the critical exploration of art works that incorporate noise & error as a means to examine and interrupt the normative function of the image and the media itself.These works do not only present pleasurable aesthetic objects (because, yes, dirty glitch can be indeed very pretty) – they also act as a magnifying glass drawing attention to the material basis of the technology used to reproduce moving images, whether it be celluloid, analogue video or digital apparatus.Using various means to distort the recognizable imagery, they bring us exciting, vibrant & noisy alternative visions that radically challenge the dominating clean, sterile imagery of contemporary digital cinema. As such, they pose fundamental questions regarding the political nature of technology, image and the reality itself.The selection divided in two blocks will showcase 16 eye- & mind-bending contemporary audiovisual works that offer a journey through a myriad of creative & critical uses of glitch followed by the Q&A discussion with the artists.PROGRAM 09.10.2023.Introspective landscapes & limits of memory in the post-internet wildernessDuration: 50′Death Orgone Absorption fœtale – Pulsion panspermique (CA, 2023,6′)Sabato Visconti – Origin Story (Best Price USA), v01 (US, 2023, 2′)Sarah Lasley – Welcome to the Enclave (US, 2023, 12′)Autojektor – robyn (2021, UK, 4′)YOVOZOL – Purplenoia (Parts 1 & 2) (NL, 2023, 10′)le désert mauve (Charline Dally + Gabrielle HB) – dickinsonia. les archives sensibles (CA, FR, 11′)Niloufar Baniasadi, Farbod Hamedi – Flower of Life (Fractal Geometry of the Carpet) (IR, 2023, 2′)Artiom Constantinov – You Never Happened, You Never Existed (IT, 2023, 4′)PROGRAM 10.10.2023.Hacking, playing & (de)constructing (new) realitiesDuration: 50′André Oliveira Cebola – ultraCritical() (BR, 2023, 1′)Chris Coleman with Music by George Cicci – Threaded Tracing (US, 2023, 7′)Josh Brown – First Wave (IE, 2023, 3′)Gino Battiston – Beware Spamart (AR, 2023, 2′)Theo Rosemffet and Rocco.FX – Descontrol (ES, 2023, 6′)aitso + ex_mortal – release decay (CA, US, 2023, 2′)Jan Swinburne – CRACKERS a brief history of code (CA, 2020, 4’20)Toma Ștefănescu – Entropy (RO, 2022, 25′)Curated by:EJLA KOVAČEVIĆA freelance film critic, curator and independent/experimental cinema researcher. She’s a member of the curatorial team at the International Experimental Film and Video Festival 25 FPS and a selection committee member at Belgrade-based International Analog Film Festival KINOSKOP. Since 2011 she’s been active in the film labs community dedicated to the promotion and preservation of analog film practices. In Zagreb-based filmlab Klubvizija she organized numerous workshops, screenings and held lectures on experimental and photochemical cinema. As an Erasmus scholar she spent a semester working in filmmakers’ cooperative LIGHT CONE in Paris. She earned her MA in French Language at the Sorbonne Nouvelle University and MA in Comparative Literature at the University of Zagreb