Synthèse sonore d'ambiances urbaines pour les applications vidéoludiques

In video gaming and interactive media, the making of complex sound ambiences relies heavily on the allowed memory and computational resources. So a compromise solution is necessary regarding the choice of audio material and its treatment in order to reach immersive and credible real-time ambiences. Alternatively, the use of procedural audio techniques, i.e. the generation of audio content relatively to the data provided by the virtual scene, has increased in recent years. Procedural methodologies seem appropriate to sonify complex environments such as virtual cities.In this thesis we specifically focus on the creation of interactive urban sound ambiences. Our analysis of these ambiences is based on the Soundscape theory and on a state of art on game oriented urban interactive applications. We infer that the virtual urban soundscape is made of several perceptive auditory grounds including a background. As a first contribution we define the morphological and narrative properties of such a background. We then consider the urban background sound as a texture and propose, as a second contribution, to pinpoint, specify and prototype a granular synthesis tool dedicated to interactive urban sound backgrounds.The synthesizer prototype is created using the visual programming language Pure Data. On the basis of our state of the art, we include an urban ambiences recording methodology to feed the granular synthesis. Finally, two validation steps regarding the prototype are described: the integration to the virtual city simulation Terra Dynamica on the one side and a perceptive listening comparison test on the other.Suite à un état de l'art détaillant la création et l'utilisation de l'espace sonore dans divers environnements urbains virtuels (soundmaps, jeux vidéo, réalité augmentée), il s'agira de déterminer une méthodologie et des techniques de conception pour les espaces sonores urbains virtuels du point de vue de l'immersion, de l'interface et de la dramaturgie.ces développements se feront dans le cadre du projet terra dynamica, tendant vers une utilisation plurielle de la ville virtuelle (sécurité et sureté, transports de surface, aménagement de l'urbanisme, services de proximité et citoyens, jeux). le principal objectif du doctorat sera de déterminer des réponses informatiques concrètes à la problématique suivante : comment, en fonction de leur utilisation anticipée, les espaces sonores urbains virtuels doivent-ils être structurés et avec quels contenus?la formalisation informatique des solutions étayées au fil du doctorat et la création du contenu sonore illustrant le projet seront basés sur l'analyse de données scientifiques provenant de domaines variés tels que la psychologie de la perception, l'architecture et l'urbanisme, l'acoustique, la recherche esthétique (musicale) ainsi que sur l'observation et le recueil de données audio-visuelles du territoire urbain, de manière à rendre compte tant de la richesse du concept d'espace sonore que de la multiplicité de ses déclinaisons dans le cadre de la ville virtuelle

JWST/NIRCam probes young star clusters in the reionization era sunrise arc

This work is based on observations made with the NASA/ ESA/CSA James Webb Space Telescope (JWST) and Hubble Space Telescope (HST). These observations are associated with JWST GO program 2282 and HST GO programs 14096, 15842, and 16668. The data (doi:10.17909/cqfq-5n80) were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contractNAS 5-03127 for JWST. We acknowledge financial support from NASA through grant JWST-GO-02282. We thank the anonymous referee for the constructive comments. A.A. acknowledges support from the Swedish Research Council (Vetenskapsrådet project grant 2021-05559). A.A. and A.C. thank M. Messa for sharing an earlier version of his software. E.V. acknowledges financial support through grants PRIN-MIUR 2017WSCC32 and 2020SKSTHZ and INAF “main-stream” grants 1.05.01.86.20 and 1.05.01.86.31. We acknowledge support from INAF GO grant 2022, “The revolution is around the corner: JWST will probe globular cluster precursors and Population III stellar clusters at cosmic dawn” (PI: Vanzella). J.M.D. acknowledges the support of projects PGC2018-101814-B-100 and MDM-2017-0765. M.B. acknowledges support from the Slovenian national research agency ARRS through grant N1-0238. P.D. acknowledges support from NWO grant 016.VIDI.189.162 (“ODIN”) and the European Commission’s and University of Groningen’s COFUND Rosalind Franklin program. M.O. acknowledges support from JSPS KAKENHI grant Nos. JP22H01260, JP20H05856, and JP20H00181. S.F. acknowledges support from NASA through NASA Hubble Fellowship grant HSTHF2-51505.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. B.W. acknowledges support from NASA under award No. 80GSFC21M0002. L.J.F. and A.Z. acknowledge support by grant No. 2020750 from the United States–Israel Binational Science Foundation (BSF), grant No. 2109066 from the United States National Science Foundation (NSF), and the Ministry of Science & Technology, Israel. E.V. thanks the colleague Antonio Sollima for inspiring discussions on local stellar clusters; Antonio, unfortunately, passed away prematurely at the age of 43, during the acceptance of this work

High-redshift Galaxy Candidates at z = 9-10 as Revealed by JWST Observations of WHL0137-08

We report the discovery of four galaxy candidates observed 450–600 Myr after the Big Bang with photometric redshifts between z ∼ 8.3 and 10.2 measured using James Webb Space Telescope (JWST) NIRCam imaging of the galaxy cluster WHL0137−08 observed in eight filters spanning 0.8–5.0 μm, plus nine Hubble Space Telescope filters spanning 0.4–1.7 μm. One candidate is gravitationally lensed with a magnification of μ ∼ 8, while the other three are located in a nearby NIRCam module with expected magnifications of μ 1.1. Using SED fitting, we estimate the stellar masses of these galaxies are typically in the range log M M = 8.3–8.7. All appear young, with mass-weighted ages < 0.15 mag, and specific star formation rates sSFR ∼0.25–10 Gyr−1 for most. One z ∼ 9 candidate is consistent with an ageBased on observations with the NASA/ESA/CSA James Webb Space Telescope obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy (AURA), Incorpo rated, under NASA contract NAS5-03127. Support for Program number JWST-GO-02282 was provided through a grant from the STScI under NASA contract NAS5-03127. The data described here may be obtained from the MAST archive at doi:10.17909/cqfq-5n80. Also based on observations made with the NASA/ESA Hubble Space Telescope, obtained at STScI, which is operated by AURA under NASA contract NAS5-26555. The HST observations are associated with programs HST-GO-14096, HST-GO-15842, and HST-GO 16668. Cloud-based data processing and file storage for this work is provided by the AWS Cloud Credits for Research program. The Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF) under grant #140. A.Z. and L.F. acknowledge support by grant No. 2020750 from the United States–Israel Binational Science Foundation (BSF) and grant No. 2109066 from the United States National Science Foundation (NSF), and by the Ministry of Science & Technology, Israel

High-Redshift Galaxy Candidates at z=9−13z = 9-13 as Revealed by JWST Observations of WHL0137-08

JWST was designed to peer into the distant universe and study galaxies nearer the beginning of time than previously. Here we report the discovery of 12 galaxy candidates observed 300-600 Myr after the Big Bang with photometric redshifts between z ~ 8.5-13 measured using JWST NIRCam imaging of the galaxy cluster WHL0137 observed in 8 filters spanning 0.8-5.0 $\mu$m, plus 9 HST filters spanning 0.4-1.7 $\mu$m. Three of these candidates are gravitationally lensed by the foreground galaxy cluster and have magnifications of $\mu \sim 3 - 8$. The remaining nine candidates are located in a second JWST NIRCam module, centered ~29' from the cluster center, with expected magnifications of $\mu$ <~ 1.1. Our sample of high-redshift candidates have observed F200W AB magnitudes between 25.9 and 28.1 mag and intrinsic F200W AB magnitudes between 26.4 and 29.7 mag ($M_{UV}$ = -22.5 to -17). We find the stellar masses of these galaxies are in the range $\log M_{*}/M_{\odot}$ = 8 - 9, and down to 7.5 for the lensed galaxies. All are young with mass-weighted ages < 100 Myr, low dust content $A_V$ < 0.15 mag, and high specific star formation rates sSFR ~10-50 Gyr$^{-1}$ for most. One z ~ 9 candidate is consistent with an age < 5 Myr and a sSFR ~250 Gyr$^{-1}$, as inferred from a strong F444W excess, implying [OIII]+H-beta rest-frame equivalent width ~2000 Angstrom, although an older and redder z~ 10 object is also allowed. Another z~9 candidate ID9356 is lensed into an arc 2.6" long by the effects of strong gravitational lensing ($\mu$~8), and has at least two bright knots of unevenly distributed star formation. This arc is the most spatially-resolved galaxy at z~9 known to date, revealing structures ~30 pc across. Follow-up spectroscopy of WHL0137 with JWST/NIRSpec is planned for later this year, which will validate some of these candidates and study their physical properties in more detail.Comment: submitted to Ap

Two lensed star candidates at z≃4.8z\simeq4.8 behind the galaxy cluster MACS J0647.7+7015

We report the discovery of two extremely magnified lensed star candidates behind the galaxy cluster MACS J0647.7+7015, in recent multi-band James Webb Space Telescope (JWST) NIRCam observations. The candidates are seen in a previously known, $z_{phot}\simeq4.8$ dropout giant arc that straddles the critical curve. The candidates lie near the expected critical curve position but lack clear counter images on the other side of it, suggesting these are possibly stars undergoing caustic crossings. We present revised lensing models for the cluster, including multiply imaged galaxies newly identified in the JWST data, and use them to estimate a background macro-magnification of at least $\gtrsim90$ and $\gtrsim50$ at the positions of the two candidates, respectively. With these values, we expect effective, caustic-crossing magnifications of $10^4-10^5$ for the two star candidates. The Spectral Energy Distributions (SEDs) of the two candidates match well spectra of B-type stars with best-fit surface temperatures of $\sim10,000$ K, and $\sim12,000$ K, respectively, and we show that such stars with masses $\gtrsim20$ M$_{\odot}$ and $\gtrsim50$ M$_{\odot}$, respectively, can become sufficiently magnified to be observed. We briefly discuss other alternative explanations and conclude these are likely lensed stars, but also acknowledge that the less magnified candidate may instead be or reside in a star cluster. These star candidates constitute the second highest-redshift examples to date after Earendel at $z_{phot}\simeq6.2$, establishing further the potential of studying extremely magnified stars to high redshifts with the JWST. Planned visits including NIRSpec observations will enable a more detailed view of the candidates already in the near future.Comment: 12 pages, 5 figures, 2 tables. Fixed Fig 3. comments are welcom

Reaching for the stars – JWST/NIRSpec spectroscopy of a lensed star candidate at z = 4.76

We present JWST/NIRSpec observations of a highly magnified star candidate at a photometric redshift of zphot ≃ 4.8, previously detected in JWST/NIRCam imaging of the strong lensing (SL) cluster MACS J0647+7015 (z = 0.591). The spectroscopic observation allows us to precisely measure the redshift of the host arc at zspec = 4.758 ± 0.004, and the star’s spectrum displays clear Lyman- and Balmer-breaks commensurate with this redshift. A fit to the spectrum suggests a B-type super-giant star of surface temperature  K with either a redder F-type companion (⁠ K) or significant dust attenuation (AV ≃ 0.82) along the line of sight. We also investigate the possibility that this object is a magnified young globular cluster rather than a single star. We show that the spectrum is in principle consistent with a star cluster, which could also accommodate the lack of flux variability between the two epochs. However, the lack of a counter image and the strong upper limit on the size of the object from lensing symmetry, r ≲ 0.5 pc, could indicate that this scenario is somewhat less likely – albeit not completely ruled out by the current data. The presented spectrum seen at a time when the Universe was only ∼1.2 Gyr old showcases the ability of JWST to study early stars through extreme lensing

Reaching for the stars -- JWST/NIRSpec spectroscopy of a lensed star candidate at z=4.76z=4.76

We present JWST/NIRSpec observations of a highly magnified star candidate at a photometric redshift of $z_{\mathrm{phot}}\simeq4.8$, previously detected in JWST/NIRCam imaging of the strong lensing (SL) cluster MACS J0647+7015 ($z=0.591$). The spectroscopic observation allows us to precisely measure the redshift of the host arc at $z_{\mathrm{spec}}=4.758\pm0.004$, and the star's spectrum displays clear Lyman- and Balmer-breaks commensurate with this redshift. A fit to the spectrum suggests a B-type super-giant star of surface temperature $T_{\mathrm{eff,B}}\simeq15000$ K with either a redder F-type companion ($T_{\mathrm{eff,F}}\simeq6250$K) or significant dust attenuation ($A_V\simeq0.82$) along the line of sight. We also investigate the possibility that this object is a magnified young globular cluster rather than a single star. We show that the spectrum is in principle consistent with a star cluster, which could also accommodate the lack of flux variability between the two epochs. However, the lack of a counter image and the strong upper limit on the size of the object from lensing symmetry, $r\lesssim0.5$ pc, could indicate that this scenario is somewhat less likely -- albeit not completely ruled out by the current data. The presented spectrum seen at a time when the Universe was only $\sim1.2$ Gyr old showcases the ability of JWST to study early stars through extreme lensing.Comment: Accepted for publication in MNRAS letters. v2 updated to match the published versio

JWST reveals a possible z∼11z \sim 11 galaxy merger in triply-lensed MACS0647−-JD

MACS0647$-$JD is a triply-lensed $z\sim11$ galaxy originally discovered with the Hubble Space Telescope. Here we report new JWST imaging, which clearly resolves MACS0647$-$JD as having two components that are either merging galaxies or stellar complexes within a single galaxy. Both are very small, with stellar masses $\sim10^8\,M_\odot$ and radii $r<100\,\rm pc$. The brighter larger component "A" is intrinsically very blue ($\beta\sim-2.6$), likely due to very recent star formation and no dust, and is spatially extended with an effective radius $\sim70\,\rm pc$. The smaller component "B" appears redder ($\beta\sim-2$), likely because it is older ($100-200\,\rm Myr$) with mild dust extinction ($A_V\sim0.1\,\rm mag$), and a smaller radius $\sim20\,\rm pc$. We identify galaxies with similar colors in a high-redshift simulation, finding their star formation histories to be out of phase. With an estimated stellar mass ratio of roughly 2:1 and physical projected separation $\sim400\,\rm pc$, we may be witnessing a galaxy merger 400 million years after the Big Bang. We also identify a candidate companion galaxy C $\sim3\,{\rm kpc}$ away, likely destined to merge with galaxies A and B. The combined light from galaxies A+B is magnified by factors of $\sim$8, 5, and 2 in three lensed images JD1, 2, and 3 with F356W fluxes $\sim322$, $203$, $86\,\rm nJy$ (AB mag 25.1, 25.6, 26.6). MACS0647$-$JD is significantly brighter than other galaxies recently discovered at similar redshifts with JWST. Without magnification, it would have AB mag 27.3 ($M_{UV}=-20.4$). With a high confidence level, we obtain a photometric redshift of $z=10.6\pm0.3$ based on photometry measured in 6 NIRCam filters spanning $1-5\rm\mu m$, out to $4300\,\r{A}$ rest-frame. JWST NIRSpec observations planned for January 2023 will deliver a spectroscopic redshift and a more detailed study of the physical properties of MACS0647$-$JD.Comment: 27 pages, 14 figures, submitted to Natur

Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang

The Cosmic Gems arc is among the brightest and highly magnified galaxies observed at redshift z ≈ 10.2 (ref. 1). However, it is an intrinsically ultraviolet faint galaxy, in the range of those now thought to drive the reionization of the Universe2–4. Hitherto the smallest features resolved in a galaxy at a comparable redshift are between a few hundreds and a few tens of parsecs (pc)5, 6. Here we report JWST observations of the Cosmic Gems. The light of the galaxy is resolved into five star clusters located in a region smaller than 70 pc. They exhibit minimal dust attenuation and low metallicity, ages younger than 50 Myr and intrinsic masses of about 106M⊙. Their lensing-corrected sizes are approximately 1 pc, resulting in stellar surface densities near 105M⊙ pc−2, three orders of magnitude higher than typical young star clusters in the local Universe7. Despite the uncertainties inherent to the lensing model, they are consistent with being gravitationally bound stellar systems, that is, proto-globular clusters. We conclude that star cluster formation and feedback likely contributed to shaping the properties of galaxies during the epoch of reionization

Sound synthesis of urban ambiences for video gaming applications

Suite à un état de l'art détaillant la création et l'utilisation de l'espace sonore dans divers environnements urbains virtuels (soundmaps, jeux vidéo, réalité augmentée), il s'agira de déterminer une méthodologie et des techniques de conception pour les espaces sonores urbains virtuels du point de vue de l'immersion, de l'interface et de la dramaturgie.ces développements se feront dans le cadre du projet terra dynamica, tendant vers une utilisation plurielle de la ville virtuelle (sécurité et sureté, transports de surface, aménagement de l'urbanisme, services de proximité et citoyens, jeux). le principal objectif du doctorat sera de déterminer des réponses informatiques concrètes à la problématique suivante : comment, en fonction de leur utilisation anticipée, les espaces sonores urbains virtuels doivent-ils être structurés et avec quels contenus?la formalisation informatique des solutions étayées au fil du doctorat et la création du contenu sonore illustrant le projet seront basés sur l'analyse de données scientifiques provenant de domaines variés tels que la psychologie de la perception, l'architecture et l'urbanisme, l'acoustique, la recherche esthétique (musicale) ainsi que sur l'observation et le recueil de données audio-visuelles du territoire urbain, de manière à rendre compte tant de la richesse du concept d'espace sonore que de la multiplicité de ses déclinaisons dans le cadre de la ville virtuelle.In video gaming and interactive media, the making of complex sound ambiences relies heavily on the allowed memory and computational resources. So a compromise solution is necessary regarding the choice of audio material and its treatment in order to reach immersive and credible real-time ambiences. Alternatively, the use of procedural audio techniques, i.e. the generation of audio content relatively to the data provided by the virtual scene, has increased in recent years. Procedural methodologies seem appropriate to sonify complex environments such as virtual cities.In this thesis we specifically focus on the creation of interactive urban sound ambiences. Our analysis of these ambiences is based on the Soundscape theory and on a state of art on game oriented urban interactive applications. We infer that the virtual urban soundscape is made of several perceptive auditory grounds including a background. As a first contribution we define the morphological and narrative properties of such a background. We then consider the urban background sound as a texture and propose, as a second contribution, to pinpoint, specify and prototype a granular synthesis tool dedicated to interactive urban sound backgrounds.The synthesizer prototype is created using the visual programming language Pure Data. On the basis of our state of the art, we include an urban ambiences recording methodology to feed the granular synthesis. Finally, two validation steps regarding the prototype are described: the integration to the virtual city simulation Terra Dynamica on the one side and a perceptive listening comparison test on the other