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  • Fernandez shows off jump rope wizardry in warm-ups

    Fernandez shows off jump rope wizardry in warm-ups

    We’ve all seen Leylah Fernandez’s skills on the tennis court, but have you seen how she handles a jump rope?

    Look at that wizardry, just like a heavyweight fighter before a title bout.

    The Canadian showed off her rope excellence before her doubles quarterfinal match at the US Open, where she — alongside her new partner and pal, Venus Williams — fell 6-1, 6-2 to the top-seeded team of Taylor Townsend and Katerina Siniakova.

    Despite the defeat, it was a memorable week for the 22-year-old, whose run with Williams became one of the stories of the tournament after they accepted a wild card into the draw. The pair won three straight-set matches — including upsets of a pair of seeded teams — before running into the top two doubles players in the world.

    Reflecting on their run, the former US Open singles finalist said she learned so much from her brief partnership with the 45-year-old icon. But perhaps more than anything, she was inspired by the joy that Williams plays with after all these years.

    “It’s just been an incredible week and a half being here and learning so much from Venus,” Fernandez said. “I’m just kind of like a sponge, so I’m just kind of sucking everything in and learning and just trying to improve my tennis game. Today didn’t go our way, but there’s definitely a lot of positives for myself going forward, and seeing Venus playing on court for joy just kind of brought me back as to why I started playing tennis.

    “It’s probably the most important thing, is that I started playing tennis for the love of the game, and for bringing joy on court — not only for myself, but also for the fans.”

    It was positively joyful in Louis Armstrong Stadium for their four matches, with the crowd backing them from first ball to last. They complemented each other beautifully on court, and adorably played to the fans, with Venus twirling after victories and encouraging Fernandez to follow suit.

    Their chemistry was obvious, so much so that Venus said Fernandez is her favorite doubles partner ever outside of her sister, Serena. (High praise considering the Williams sisters won 14 doubles majors together.)

    On the singles side, Fernandez won her first two matches — against Rebecca Marino and Elsa Jacquemot — before falling to top-seeded Aryna Sabalenka in straight sets in the third round.

     

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    September 3, 2025
  • First JWST Thermal Phase Curves Of Temperate Terrestrial Exoplanets Reveal No Thick Atmosphere Around TRAPPIST-1 b and c

    First JWST Thermal Phase Curves Of Temperate Terrestrial Exoplanets Reveal No Thick Atmosphere Around TRAPPIST-1 b and c

    Range of best-fit phase curve and eclipse models for TRAPPIST-1 b and c. The detrended data are shown with gray dots and binned data with black dots. Red curves show the light curve model for each JWST program that observed TRAPPIST-1 b and c at 15µm using MIRI F1500W; the shading spans the range of models drawn from the posterior distribution of the day flux, night flux and phase offset for planets b and c from Analysis # 1 at 2-σ. The top panel shows the phase curve from GO 3077; the second row displays the five visits from GO 1177 (PI: Greene); and the third row presents the four visits from GO 2304 (PI: Kreidberg), along with a zoom-in on the double occultation observed in GO 3077. The expected transit and eclipse timings for each planet from [19] are shown in vertical dashed and plain lines respectively (purple for b, orange for c, and green for g). — astro-ph.EP

    We report JWST/MIRI 15 μm phase curves of TRAPPIST-1 b and c, revealing thermal emission consistent with their irradiation levels, assuming no efficient heat redistribution.

    We find that TRAPPIST-1 b shows a high dayside brightness temperature (490 ± 17 K), no significantly detectable nightside emission (Fb,Night,max = 39+55−27 ppm), and no phase offset — features consistent with a low-albedo, airless ultramafic rocky surface.

    TRAPPIST-1 c exhibits a lower dayside brightness temperature (369 ± 23 K), and a nightside flux statistically indistinguishable from that of TRAPPIST-1 b (Fc,Night,max = 62+60−43 ppm).

    Atmosphere models with surface pressures ≥1 bar and efficient greenhouse effects are strongly disfavoured for both planets. TRAPPIST-1 b is unlikely to possess any substantial atmosphere, while TRAPPIST-1 c may retain a tenuous, greenhouse-poor O2-dominated atmosphere or be similarly airless with a more reflective surface.

    These results suggest divergent evolutionary pathways or atmospheric loss processes, despite similar compositions. These measurements tightly constrain atmosphere retention in the inner TRAPPIST-1 system.

    Michaël Gillon, Elsa Ducrot, Taylor J. Bell, Ziyu Huang, Andrew Lincowski, Xintong Lyu, Alice Maurel, Alexandre Revol, Eric Agol, Emeline Bolmont, Chuanfei Dong, Thomas J. Fauchez, Daniel D.B. Koll, Jérémy Leconte, Victoria S. Meadows, Franck Selsis, Martin Turbet, Benjamin Charnay, Laetita Delre, Brice-Olivier Demory, Aaron Householder, Sebastian Zieba, David Berardo, Achrène Dyrek, Billy Edwards, Julien de Wit, Thomas P. Greene, Renyu Hu, Nicolas Iro, Laura Kreidberg, Pierre-Olivier Lagage, Jacob Lustig-Yaeger, Aishwarya Iyer

    Comments: 72 pages, 4 main text Figures, 20 Extended Data Figures, 6 Supplementary Figures. Accepted for publication in Nature Astronomy
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2509.02128 [astro-ph.EP] (or arXiv:2509.02128v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2509.02128
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    Submission history
    From: Elsa Ducrot
    [v1] Tue, 2 Sep 2025 09:23:03 UTC (12,845 KB)
    https://arxiv.org/abs/2509.02128
    Astrobiology,

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    September 3, 2025
  • Detecting Water Ice And Vapor Disks Originating From Icy Planetary Bodies Around White Dwarfs With Future PRIMA Observations

    Detecting Water Ice And Vapor Disks Originating From Icy Planetary Bodies Around White Dwarfs With Future PRIMA Observations

    Schematic showing the distribution of the modeled volatile gas (e.g., water vapor) disk and water ice disk around a WD. The rocky dust disk and their observationally inferred properties are also summarized. — astro-ph.EP

    Observations of atmospheres of polluted white dwarfs provide insights into the elemental composition of accreted exoplanets and exo-asteroids.

    However, they poorly constrain the abundance of ice-forming volatile elements due to the properties of white dwarf atmospheres. Instead of focusing solely on atmospheric observations, we propose observing circumstellar water ice and vapor disks formed by the tidal disruption of icy bodies using the future PRobe far-Infrared Mission for Astrophysics (PRIMA) far-infrared enhanced survey spectrometer.

    PRIMA has the potential to measure volatile abundances in colder circumstellar regions inaccessible by shorter-wavelength observations. We employ a simple disk emission model with disk parameter ranges inferred from previous observations and disk evolution simulations. We find the 44-μm water ice feature promising for observing icy disks.

    For white dwarfs within 60 pc, 1-hour PRIMA observations could detect water ice with a mass above 1020 g, representing a potential lower limit of circumstellar disk mass. Water vapor rotational lines also abundantly emerge within the PRIMA wavelength coverage, and 5-hour observations for white dwarfs within 20 pc could detect water vapor with a total disk mass ≳1020 g, depending on the H2/H2O ratio. 19 metal polluted white dwarfs within 20 pc and 210 within 60 pc could be optimal targets for water vapor and ice observations, respectively.

    Ayaka Okuya, Hideko Nomura

    Comments: 19 pages, 7 figures, published in JATIS. This paper is part of the JATIS special issue focused on the PRobe Infrared Mission for Astrophysics (PRIMA) probe mission concept. The issue is edited by Matt Griffin and Naseem Rangwala (JATIS VOL. 11, NO. 3 | July 2025)
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2509.01697 [astro-ph.EP] (or arXiv:2509.01697v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2509.01697
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    Journal reference: J. Astron. Telesc. Instrum. Syst. 11(3), 031607 (2025)
    Related DOI:
    https://doi.org/10.1117/1.JATIS.11.3.031607
    Focus to learn more
    Submission history
    From: Ayaka Okuya
    [v1] Mon, 1 Sep 2025 18:17:26 UTC (957 KB)
    https://arxiv.org/abs/2509.01697
    Astrobiology,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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    September 3, 2025
  • Hacking group linked to M&S breach claim responsibility for Jaguar Land Rover cyber-attack | Jaguar Land Rover

    Hacking group linked to M&S breach claim responsibility for Jaguar Land Rover cyber-attack | Jaguar Land Rover

    A group of English-speaking hackers linked to the Marks & Spencer cyber-attack has claimed responsibility for an attack on Jaguar Land Rover.

    A channel on the Telegram platform posted a screenshot of what appeared to be the car maker’s internal IT systems, as well as a news article detailing the hack.

    The name of the Telegram channel is a combination of three English language speaking, or western-based, hacking groups known as Scattered Spider, Lapsus$ and ShinyHunters.

    Scattered Spider, a collective of teenage and twentysomething hackers, has been blamed for attacks this year on British retailers M&S, Co-op and Harrods. Four people including three teenagers were arrested at UK addresses in July as part of an investigation into the retail cyber-attacks.

    Britain’s biggest car maker halted production at key sites on Monday after admitting its manufacturing and retailing activities had been “severely disrupted” by a cyber incident. It said there was no evidence that any customer data had been taken but had “proactively” shut down its systems and taken “immediate action to mitigate” the impact.

    JLR did not give more details about who was behind the cyber incident, when it was discovered or how long it would take to recover from it.

    Car industry sources said the incident had severely affected its suppliers, which normally make regular deliveries of parts to its factories. These suppliers could lose tens of millions of pounds in sales because of the halt in production, they added.

    Aiden Sinnott, a security researcher at UK cybersecurity firm, said one of the personas on the Telegram group, Rey, shared the same name as a member of Hellcat, the ransomware gang that claimed to have extracted data from JLR earlier this year. Sinnott said Hellcat fitted the same mould as Scattered Spider and ShinyHunters.

    “They speak English and they are keen on using social media channels,” he said, adding that Lapsus$ shared similar tactics and demographics as the Scattered Spider collective.

    The cyber-attack at JLR comes amid disruption from the impact of US tariffs and declining sales.

    The car maker reported that underlying pre-tax profits fell by 49% to £351m in the three months to June, which included a period when the company temporarily paused exports to the US.

    In 2023 an 18-year-old from Oxford and part of the Lapsus$ hacking group, Arion Kurtaj, who is autistic, was sentenced to an indefinite hospital order after stealing 90 clips of the unreleased Grand Theft Auto 6 game as part of a hacking spree.

    Describing ShinyHunters and Scattered Spider, Sinnott said: “Consolidating them into a group is difficult because they are essentially individuals operating online, communicating via platforms like Telegram, who might sometimes work together.”

    Sinnott said Scattered Spider was an “umbrella term for a kind of demographic” of hackers in their late teens or early 20s who are native English speaking and “don’t really fit into a box as a structure hierarchy”. Traditionally, groups that deploy ransomware – malicious software that locks up a target’s IT systems – are linked to eastern Europe and former Soviet Union countries including Russia.

    The ShinyHunters group also has French links. Sebastien Raoult, a Frenchman in his early 20s, was sentenced to three years in prison in the US last year for his activities as a ShinyHunters member.

    The Telegraph first reported the activity on the Scattered Lapsus$ Hunters group.

    A spokesperson for the National Crime Agency said: “We are aware of an incident impacting Jaguar Land Rover and are working with partners to better understand its impact.”

    The car maker, which is headquartered in Coventry, employs 32,800 people in the UK across 17 different sites.

    JLR has been contacted for comment.

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    September 3, 2025
  • ‘Ketamine Queen’ pleads guilty in Matthew Perry overdose case

    ‘Ketamine Queen’ pleads guilty in Matthew Perry overdose case

    Reuters Image shows Matthew PerryReuters

    Perry was found dead in a jacuzzi at his Los Angeles home in October 2023

    A woman dubbed the “Ketamine Queen” has pleaded guilty to selling the drugs that ultimately killed Friends actor Matthew Perry.

    Jasveen Sangha, 42, pleaded guilty to five charges in Los Angeles on Wednesday, including one count of distributing ketamine resulting in death or bodily injury.

    The American-British dual-national originally faced nine criminal counts. Federal prosecutors called her Los Angeles home a “drug-selling emporium” and found dozens of vials of ketamine during a raid.

    Perry was found dead in a jacuzzi at his Los Angeles home in October 2023, with an examination finding his death was caused by the acute effects of ketamine.

    A sentencing hearing for Sangha, who is being held in federal custody, has been set for 10 December in Los Angeles.

    Sangha initially denied the charges but agreed to change her plea in August, just weeks before she had been due to stand trial.

    She is one of five people – including medical doctors and the actor’s assistant – who US officials say supplied ketamine to Perry, exploiting his drug addiction for profit, and leading to his overdose death.

    They include: Dr Salvador Plasencia and Dr Mark Chavez, two doctors who sold ketamine; Kenneth Iwamasa, who worked as Perry’s live-in assistant and both helped purchase and inject the actor with ketamine; and Eric Fleming, who sold ketamine he’d gotten from Sangha to Perry.

    The four others have also agreed to plead guilty to charges in the case. They will be sentenced at different times in November and December.

    Sangha faces a maximum sentence of 65 years in federal prison, according to the justice department.

    Ketamine is a dissociative anaesthetic that has some hallucinogenic effects, according to the US Drug Enforcement Administration (DEA). It can distort perception of sight and sound and makes the user feel disconnected and not in control.

    It is used as an injectable anaesthetic for humans and animals because it makes patients feel detached from their pain and environment.

    The substance is supposed to be administered only by a physician, officials say, and patients who have taken the drug should be monitored by a professional because of its possible harmful effects.

    Jasveen Sangha's social media Image shows Jasveen SanghaJasveen Sangha’s social media

    Sangha is said to have mixed with celebrities socially, with one of her friends telling the Daily Mail she attended the Oscars

    Perry’s death and the investigation into how he obtained so much of the drug over multiple years offered a glimpse into Hollywood’s ketamine drug network, which one doctor called the “wild west” in an interview with the BBC.

    As part of her plea agreement, Sangha also pleaded guilty to selling ketamine to a man named Cody McLaury in August 2019, who died hours after the purchase from a drug overdose, according to the justice department.

    Federal authorities accused Sangha of supplying ketamine from her “stash house” in North Hollywood since at least 2019, alleging in an indictment that she worked with celebrities and high-end clients.

    More than 80 vials of ketamine were found there in a search before her arrest in March 2024, along with thousands of pills that included methamphetamine, cocaine and Xanax.

    Sangha is said to have mixed with celebrities socially, with one of her friends telling the Daily Mail she attended the Golden Globes and the Oscars.

    Her social media presence depicted an extravagant lifestyle, including parties and trips to Japan and Mexico.

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    September 3, 2025
  • GENIUS Act Stablecoin Regulation: Federal vs. State Divide

    GENIUS Act Stablecoin Regulation: Federal vs. State Divide


    LawFlash




    September 03, 2025

    As the stablecoin market continues to evolve at lightning speed, regulation of these innovative financial products has strived to keep apace. While the GENIUS Act in the United States has created a robust regulatory framework, there remains fragmentation due to the regulatory approaches taken by different states. However, several recent federal legislative actions provide some clarity and predictability to this rapidly changing space—but it is still unclear how successful these efforts will be.

    A key feature of the GENIUS Act is its approach to harmonizing federal and state stablecoin[1] regulatory frameworks, particularly through the establishment of the Stablecoin Certification Review Committee (SCRC), which will be chaired by the secretary of the US Department of the Treasury and include the chair of the Federal Reserve and chair of the Federal Deposit Insurance Corporation.[2]

    In sum, the GENIUS Act provides a regulatory framework for payment stablecoins in the United States and provides for the SCRC to be responsible for determining whether a particular state’s stablecoin regulatory framework is “substantially similar” to the required federal framework.

    Accordingly, the SCRC will wield considerable influence over state-level stablecoin regulatory regimes and in doing so will seek to provide private stablecoin issuers with consistent standards designed to prevent fraud and ensure consumer protection throughout the US market. However, with state-issued stablecoins exempt, questions remain as to the extent to which the GENIUS Act can successfully create regulatory consistency.[3]

    FEDERAL AND STATE REGULATORY DIVIDE

    The GENIUS Act delineates a clear federal framework for the regulation of private payment stablecoins while also allowing states to promulgate their own state-level private payment stablecoin regulatory regimes.[4]

    Under the GENIUS Act, state-qualified payment stablecoin issuers with a consolidated total outstanding issuance of not more than $10 billion may elect to be regulated under a state-level regime provided that the state stablecoin regime is substantially similar to the federal framework.[5] This provision aims to streamline the regulatory landscape for privately issued stablecoins and reduce the complexity of navigating disparate state regulations.

    The SCRC will play a deciding role in this process by determining whether state regulatory frameworks are “substantially similar” to the federal regime. SCRC decisions to approve state stablecoin regulatory frameworks must be unanimous,[6] which effectively ensures that each state’s regulation of privately issued stablecoins will align closely with federal standards, promoting consistency across jurisdictions and preventing states from creating a stablecoin regulatory framework that is either too stringent or too permissive.

    Nevertheless, the SCRC’s role will be limited to the oversight of a state’s regulation of privately issued stablecoins and will not extend to state-issued stablecoins themselves.

    STABLECOIN CERTIFICATION REVIEW COMMITTEE

    The SCRC will be responsible for reviewing and certifying state regulatory regimes to ensure they meet the standards set forth in the GENIUS Act. This process will involve an initial certification by state regulators, to be submitted to the SCRC by July 18, 2026, which will then be followed by a review and potential recertification by the SCRC.[7] The SCRC’s role will extend beyond the initial certification and involve ongoing oversight and the ability to deny or revoke a certification if a state’s stablecoin regulatory regime fails to maintain required standards.[8]

    This oversight function will be crucial in maintaining the integrity and safety of the stablecoin overall market in the United States, effectively ensuring that all private stablecoin issuers operate under similar regulatory frameworks. While each state’s regulatory regime for privately issued stablecoins must be substantially similar to the federal standards, the SCRC’s authority does not extend to state-issued stablecoins, which are not covered by the GENIUS Act.

    STATE GOVERNMENT–ISSUED STABLECOINS

    The exemption from the GENIUS Act for state-issued stablecoins has not gone unnoticed by several states. Wyoming has emerged as an early mover in the state-issued stablecoin arena, launching the Frontier Stable Token (FRNT) on August 20, which is backed by US dollars and short-term Treasuries. Since 2016, Wyoming has passed more than 45 pieces of crypto-linked legislation, and the state’s special purpose depository institution banking charter further provides a framework for custody services and other crypto-related products.

    The rapid launch of the FRNT after the passage of the GENIUS Act is part of Wyoming’s push to attract digital asset businesses and promote digital asset innovation in the state. Its neighbor to the east, Nebraska, has also obtained legislative approval for a state-issued stablecoin and will likely follow in Wyoming’s footsteps. More states are expected to follow.

    NEXT STEPS TO EXPECT

    The present parallel systems between state-issued stablecoins and privately issued stablecoins present both opportunities and challenges for private stablecoin issuers, particularly as more states explore the potential of state-issued stablecoins. Federalism disputes could arise as regulators seek to balance federally mandated consistency for private issuers with a state’s ability to launch and operate stablecoins under its own standards, without federal preemption or approval.

    The federal government is left with only indirect levers, such as Financial Stability Oversight Council designations, if a state’s stablecoin scheme threatened the monetary system or violated federal law. Accordingly, stakeholders should remain engaged with regulatory developments to ensure compliance and capitalize on opportunities presented by an evolving landscape.

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    September 3, 2025
  • An Analysis Of The Radius Gap In A Sample Of Kepler, K2 And TESS Exoplanets Orbiting M Dwarf Stars

    An Analysis Of The Radius Gap In A Sample Of Kepler, K2 And TESS Exoplanets Orbiting M Dwarf Stars

    Distribution of the derived planetary radii as a function of insolation, along with the associated KDE. — astro-ph.EP

    Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars. Stellar radii are based on an analysis of APOGEE high-resolution near-IR spectra for a subsample of the M-dwarfs; these results are used to define a stellar radius-MKs calibration that is applied to the sample of M-dwarf planet hosts.

    The planetary radius distribution displays a gap over Rp∼1.6-2.0 R⊕, bordered by two peaks at Rp∼1.2-1.6 R⊕ (super-Earths) and 2.0-2.4 R⊕ (sub-Neptunes). The radius gap is nearly constant with exoplanetary orbital period (a power-law slope of m=+0.01+0.03−0.04), which is different (2-3σ) from m∼−0.10 found previously for FGK dwarfs.

    This flat slope agrees with pebble accretion models, which include photoevaporation and inward orbital migration. The radius gap as a function of insolation is approximately constant over the range of Sp∼20-250 S⊕. The Rp-Porb plane exhibits a sub-Neptune desert for Porb<2d, that appears at Sp>120 S⊕, being significantly smaller than Sp>650 S⊕ found in the FGK planet-hosts, indicating that the appearance of the sub-Neptune desert is a function of host-star mass.

    Published masses for 51 exoplanets are combined with our radii to determine densities, which exhibit a gap at ρp∼0.9ρ⊕, separating rocky exoplanets from sub-Neptunes. The density distribution within the sub-Neptune family itself reveals two peaks, at ρp∼0.4ρ⊕ and ∼0.7ρ⊕. Comparisons to planetary models find that the low-density group are gas-rich sub-Neptunes, while the group at ρp∼0.7ρ⊕ likely consists of volatile-rich water worlds.

    Fábio Wanderley, Katia Cunha, Verne V. Smith, Diogo Souto, Ilaria Pascucci, Aida Behmard, Carlos Allende Prieto, Rachael L. Beaton, Dmitry Bizyaev, Simone Daflon, Sten Hasselquist, Steve Howell, Steven R. Majewski, Marc Pinsonneault

    Comments: Submitted to ApJ
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2509.01930 [astro-ph.EP] (or arXiv:2509.01930v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2509.01930
    Focus to learn more
    Submission history
    From: Fábio Carneiro Wanderley
    [v1] Tue, 2 Sep 2025 03:56:15 UTC (13,697 KB)
    https://arxiv.org/abs/2509.01930
    Astrobiology,

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    September 3, 2025
  • Julian Schnabel defends Gal Gadot, Gerard Butler at Venice

    Julian Schnabel defends Gal Gadot, Gerard Butler at Venice | The Jerusalem Post

    Jerusalem Post/Diaspora

    US director Julian Schnabel defended Gal Gadot and Gerard Butler after activists urged the Venice Film Festival to exclude them over their support for Israel.

    Julian Schnabel poses during a photocall for the movie "In the Hand of Dante" out of competition, at the 82nd Venice Film Festival, Venice, Italy, September 3, 2025.
    Julian Schnabel poses during a photocall for the movie “In the Hand of Dante” out of competition, at the 82nd Venice Film Festival, Venice, Italy, September 3, 2025.
    (photo credit: REUTERS/YARA NARDI)
    ByREUTERS
    SEPTEMBER 3, 2025 20:02



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    September 3, 2025
  • American Cinematographer Earns 7 Folio: Eddie & Ozzie Noms

    American Cinematographer Earns 7 Folio: Eddie & Ozzie Noms

    American Cinematographer has earned nominations for seven 2025 Folio: Eddie and Ozzie Awards. The awards program is the most prestigious in the publishing community, recognizing business-to-business, regional, association and consumer publications.

    AC was nominated for Best Full Issue in the category of “Association/Nonprofit, Professional Membership Association — Arts, Lifestyle & Specialized Markets” for the December 2024 issue, which features a cover story on Joker: Folie à Deux, shot by Lawrence Sher, ASC; and for the January 2025 issue, which features a cover story on Wicked, shot by Alice Brooks, ASC.

    For Best Single Article in the category of “Association/Nonprofit, Professional/Membership Association — Cultural, Scientific & Public Engagement,” AC received three nominations: “Furiosa: Raising Hell Down Under,” written by AC web editor Max Weinstein; “The Jazz of Joker: Folie à Deux,” written by AC managing editor Andrew Fish; and “Nosferatu Exhumes a Vampire Classic,” written by AC editor-in-chief Stephen Pizzello.

    “Furiosa: Raising Hell Down Under” — which was the cover story of the September 2024 issue — explores ASC member Simon Duggan’s cinematography for writer-director George Miller’s action epic Furiosa: A Mad Max Saga. “The Jazz of Joker: Folie à Deux” details Sher’s approach to Todd Phillips’ twisted jukebox-musical sequel to Joker. “Nosferatu Exhumes a Vampire Classic” — featured in the January 2025 issue — unpacks cinematographer Jarin Blaschke’s process on Nosferatu, writer-director Robert Eggers’ adaptation of the classic vampire tale.

    For Best Profile or Q&A in the category of “Association/Nonprofit,” AC received a nomination for “John Simmons, ASC: Commitment to Artistic Voice,” written by AC contributing writer Sarah Fensom. The piece — featured in the March 2025 issue — considers the storied career of ASC member John Simmons, who reflects on his creative achievements and impact on the greater cinematography community.

    For Best Instructional/How-To in the category of “Service Journalism,” AC was nominated for Shot Craft, the magazine’s monthly column written by AC technical editor Jay Holben that provides lessons, tips and techniques for aspiring and working cinematographers.

    Winners in all categories will be announced Monday, October 6 from 4:30-7:30 pm est at Second in New York City.

    Read the full list of nominations here.

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    September 3, 2025
  • The ‘Man’s Best Friend’ Album Cover Was Kind Of An Accident

    The ‘Man’s Best Friend’ Album Cover Was Kind Of An Accident

    Let the cover for Sabrina Carpenter’s Man’s Best Friend be a lesson for us all: Nothing is ever as it seems. Months after receiving major backlash for the cheeky album art, the pop star is giving fans a peek behind the curtain and sharing the inspiration behind the imagery.

    In case you need a refresher, the visuals feature a shot of Carpenter on her hands and knees as a man stands above her pulling her hair — or so you thought. In a new interview with Zane Lowe, the singer revealed that the hair pull was never the goal, it was (seemingly) an accident. “I wanted a man playing with my hair and I actually used maybe five different men to take that photo because none of them could play with my hair,” she tells the Apple Music host. “They were all pulling it … the grip looked like they were yanking it.”

    The original intention behind the photo was much more lighthearted than the internet would have you think. In Carpenter’s words, she wanted to express a feeling of, “I got myself here, here I am, this is someone I love but also someone that emotionally can be doing a lot with my heart and doing a lot with my emotions.” Her friends and family all agreed the photo was “perfect,” so when the controversy began swirling online, the 26-year-old chalked it up to a lack of context and kept it moving.

    The concept may not have been well received by all, but Carpenter is standing by the artwork regardless. “The photo we landed on was so special,” she tells Lowe, explaining how it was the only pic caught on film that featured her desired lighting and a facial expression that conveyed control “even though I’m on all fours.”

    The full interview is out now on Apple Music 1.

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    September 3, 2025
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