Prof. Michaela Hirschmann
Journal Articles
2025
The Cosmic Evolution Early Release Science Survey (CEERS)
Astrophysical Journal Letters. 2025. Vol. 983, num. 1, p. L4. DOI : 10.3847/2041-8213/adbbd3.RUBIES Reveals a Massive Quiescent Galaxy at z=7.3
ASTROPHYSICAL JOURNAL. 2025. Vol. 983, num. 1. DOI : 10.3847/1538-4357/adab7a.RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at z ∼ 2
ASTROPHYSICAL JOURNAL. 2025. Vol. 982, num. 2. DOI : 10.3847/1538-4357/adb8e1.You Shall Not Pass! The Propagation of Low-/Moderate-powered Jets Through a Turbulent Interstellar Medium
ASTROPHYSICAL JOURNAL. 2025. Vol. 981, num. 2. DOI : 10.3847/1538-4357/adb016.[Erratum] Study of backward Brillouin scattering in gas-filled anti-resonant fibers (vol 8, 086104, 2023)
APL PHOTONICS. 2025. Vol. 10, num. 3. DOI : 10.1063/5.0263994.Molecular gas and dust properties in z > 7 quasar hosts
ASTRONOMY & ASTROPHYSICS. 2025. Vol. 695. DOI : 10.1051/0004-6361/202453226.COSMOS-Web: The Role of Galaxy Interactions and Disk Instabilities in Producing Starbursts at z < 4
Astrophysical Journal. 2025. Vol. 980, num. 2, p. 204. DOI : 10.3847/1538-4357/ada566.The MBH–M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images
The Astrophysical Journal. 2025. Vol. 979, num. 2, p. 215. DOI : 10.3847/1538-4357/ad9d0a.SCUBADive. I. JWST plus ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web
The Astrophysical Journal. 2025. Vol. 979, num. 2, p. 229. DOI : 10.3847/1538-4357/ada357.The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2025. Vol. 537, num. 2, p. 956 – 977. DOI : 10.1093/mnras/staf002.Unveiling the Dark Side of Ultraviolet/Optical Bright Galaxies: Optically Thick Dust Absorption
The Astrophysical Journal. 2025. Vol. 979, num. 1, p. 71. DOI : 10.3847/1538-4357/ad9909.Clumps as multiscale structures in cosmic noon galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2025. num. 3, p. 3090 – 3111. DOI : 10.1093/mnras/stae2781.Do stars still form in molecular gas within CO-dark dwarf galaxies?
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2025. num. 3, p. 2936 – 2955. DOI : 10.1093/mnras/stae2759.2024
The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2024. num. 3, p. 2324 – 2354. DOI : 10.1093/mnras/stae2626.Testing kinematic distances under a realistic Galactic potential Investigating systematic errors in the kinematic distance method arising from a non-axisymmetric potential
ASTRONOMY & ASTROPHYSICS. 2024. Vol. 692. DOI : 10.1051/0004-6361/202450000.MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4
The Astrophysical Journal. 2024. num. 1, p. 51. DOI : 10.3847/1538-4357/ad8b1c.The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2024. Vol. 536, num. 1, p. 851 – 870. DOI : 10.1093/mnras/stae2663.Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
ASTRONOMY & ASTROPHYSICS. 2024. DOI : 10.1051/0004-6361/202450035.ASTRODEEP-JWST: NIRCam-HST multi-band photometry and redshifts for half a million sources in six extragalactic deep fields
ASTRONOMY & ASTROPHYSICS. 2024. Vol. 691. DOI : 10.1051/0004-6361/202451409.Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z =4.91
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. 2024. Vol. 76, num. 6, p. 1323 – 1335. DOI : 10.1093/pasj/psae091.On the origin of star formation quenching in massive galaxies at z ≳ 3 in the cosmological simulations Illustris TNG
Monthly Notices of the Royal Astronomical Society. 2024. Vol. 534, num. 4, p. 3974 – 3988. DOI : 10.1093/mnras/stae2297.Physical properties of extreme emission-line galaxies at z~4-9 from the JWST CEERS survey
Astronomy & Astrophysics. 2024. Vol. 691, p. A59. DOI : 10.1051/0004-6361/202449904.What Are the Pillars of Reionization? Revising the AGN Luminosity Function at z ∼ 5
The Astrophysical Journal. 2024. Vol. 974, num. 1, p. 84. DOI : 10.3847/1538-4357/ad6980.Evolution of the star formation rate and ΣSFR of galaxies at cosmic morning (4 < z < 10)
Astronomy & Astrophysics. 2024. Vol. 690, p. A290. DOI : 10.1051/0004-6361/202449768. A Census from JWST of Extreme Emission-line Galaxies Spanning the Epoch of Reionization in CEERS
The Astrophysical Journal. 2024. Vol. 974, num. 1, p. 42. DOI : 10.3847/1538-4357/ad6865.Unveiling the Distant Universe: Characterizing z ≥ 9 Galaxies in the First Epoch of COSMOS-Web
The Astrophysical Journal. 2024. Vol. 973, num. 1, p. 23. DOI : 10.3847/1538-4357/ad5e6a.Lyα Emission Line Profiles of Extreme [O iii]- emitting Galaxies at z ≳ 2: Implications for Lyα Visibility in the Reionization Era
The Astrophysical Journal. 2024. Vol. 972, num. 1, p. 56. DOI : 10.3847/1538-4357/ad5ae0.Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4-8 from CEERS
Astronomical Journal. 2024. Vol. 168, num. 3, p. 113. DOI : 10.3847/1538-3881/ad57c1.Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
Astronomy & Astrophysics. 2024. Vol. 689, p. A276. DOI : 10.1051/0004-6361/202449500.Not-so-little Red Dots: Two Massive and Dusty Starbursts at z ∼ 5-7 Pushing the Limits of Star Formation Discovered by JWST in the COSMOS-Web Survey
The Astrophysical Journal Letters. 2024. Vol. 973, num. 1, p. L2. DOI : 10.3847/2041-8213/ad738a.Characterizing the Average Interstellar Medium Conditions of Galaxies at z ∼ 5.6-9 with Ultraviolet and Optical Nebular Lines
The Astrophysical Journal. 2024. Vol. 971, num. 1, p. 21. DOI : 10.3847/1538-4357/ad5015.BEAGLE-AGN I: simultaneous constraints on the properties of gas in star-forming and AGN narrow-line regions in galaxies
Monthly Notices Of The Royal Astronomical Society. 2024. Vol. 527, num. 3, p. 7217 – 7241. DOI : 10.1093/mnras/stad3252.The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5-14.5
The Astrophysical Journal Letters. 2024. Vol. 969, num. 1, p. L2. DOI : 10.3847/2041-8213/ad4495.pyC 2 Ray: A flexible and GPU-accelerated radiative transfer framework for simulating the cosmic epoch of reionization
Astronomy and Computing. 2024. Vol. 48, p. 100861. DOI : 10.1016/j.ascom.2024.100861.Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS
The Astrophysical Journal. 2024. Vol. 970, num. 1, p. 68. DOI : 10.3847/1538-4357/ad4cea.Tracing the quenching journey across cosmic time
Astronomy & Astrophysics. 2024. Vol. 687, p. 1 – 17. DOI : 10.1051/0004-6361/202349045.Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351
The Astrophysical Journal. 2024. Vol. 967, num. 2, p. 133. DOI : 10.3847/1538-4357/ad3de6.The First Quenched Galaxies: When and How?
The Astrophysical Journal Letters. 2024. Vol. 966, num. 1, p. L2. DOI : 10.3847/2041-8213/ad380a.CEERS: Diversity of Lyα Emitters during the Epoch of Reionization
The Astrophysical Journal. 2024. Vol. 967, num. 1, p. 73. DOI : 10.3847/1538-4357/ad3913.Tracing the rise of supermassive black holes A panchromatic search for faint, unobscured quasars at z ≥ 6 with COSMOS-Web and other surveys
Astronomy & Astrophysics. 2024. Vol. 685, p. A25. DOI : 10.1051/0004-6361/202349025.New insight on the nature of cosmic reionizers from the CEERS survey
Astronomy & Astrophysics. 2024. Vol. 685, p. A3. DOI : 10.1051/0004-6361/202347884.On the origin of globular clusters in a hierarchical universe
Monthly Notices Of The Royal Astronomical Society. 2024. Vol. 530, num. 3, p. 2760 – 2777. DOI : 10.1093/mnras/stae1006.The effect of cosmic rays on the observational properties of the CGM
Monthly Notices Of The Royal Astronomical Society. 2024. Vol. 530, num. 1, p. 52 – 65. DOI : 10.1093/mnras/stae837.COSMOS-Web: Intrinsically Luminous z ≳ 10 Galaxy Candidates Test Early Stellar Mass Assembly
The Astrophysical Journal. 2024. Vol. 965, num. 1, p. 98. DOI : 10.3847/1538-4357/ad2075.Extremely Red Galaxies at z=5-9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
The Astrophysical Journal. 2024. Vol. 963, num. 2, p. 128. DOI : 10.3847/1538-4357/ad167e.The Origins of Gas Accreted by Supermassive Black Holes: The Importance of Recycled Gas
The Astrophysical Journal. 2024. Vol. 964, num. 1, p. 54. DOI : 10.3847/1538-4357/ad245a.CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2
The Astrophysical Journal. 2024. Vol. 962, num. 2, p. 195. DOI : 10.3847/1538-4357/ad1520.CLASSY. VIII. Exploring the Source of Ionization with UV Interstellar Medium Diagnostics in Local High-z Analogs
The Astrophysical Journal. 2024. Vol. 962, num. 1, p. 95. DOI : 10.3847/1538-4357/ad1033.Evolution of the Size-Mass Relation of Star-forming Galaxies Since z=5.5 Revealed by CEERS
The Astrophysical Journal. 2024. Vol. 962, num. 2, p. 176. DOI : 10.3847/1538-4357/ad20ed.Environmental effects on satellite galaxies from the perspective of cold gas
Monthly Notices Of The Royal Astronomical Society. 2024. Vol. 528, num. 2, p. 2451 – 2463. DOI : 10.1093/mnras/stae162.A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]
Nature Astronomy. 2024. DOI : 10.1038/s41550-024-02397-3.Uncovering a Massive z ∼ 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
The Astrophysical Journal Letters. 2024. Vol. 961, num. 1, p. L25. DOI : 10.3847/2041-8213/ad11ee.2023
Probing the roles of orientation and multiscale gas distributions in shaping the obscuration of active galactic nuclei through cosmic time
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 527, num. 4, p. 10878 – 10896. DOI : 10.1093/mnras/stad3265.Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST
The Astrophysical Journal. 2023. Vol. 958, num. 2, p. 141. DOI : 10.3847/1538-4357/acfed4.CEERS Key Paper. VII. JWST/MIRI Reveals a Faint Population of Galaxies at Cosmic Noon Unseen by Spitzer
The Astrophysical Journal Letters. 2023. Vol. 959, num. 1, p. L7. DOI : 10.3847/2041-8213/ad0b14.The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 527, num. 3, p. 8598 – 8617. DOI : 10.1093/mnras/stad3751.The connection between mergers and AGN activity in simulated and observed massive galaxies
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 527, num. 3, p. 9461 – 9479. DOI : 10.1093/mnras/stad3836.Near-infrared emission line diagnostics for AGN from the local Universe to z ∼ 3
Astronomy & Astrophysics. 2023. Vol. 679, p. A80. DOI : 10.1051/0004-6361/202347190.MOSEL Survey: JWST Reveals Major Mergers/strong Interactions Drive the Extreme Emission Lines in the Early Universe
The Astrophysical Journal Letters. 2023. Vol. 957, num. 2, p. L35. DOI : 10.3847/2041-8213/ad0788.Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 526, num. 3, p. 3610 – 3636. DOI : 10.1093/mnras/stad2955.High-redshift metallicity calibrations for JWST spectra: insights from line emission in cosmological simulations
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 526, num. 3, p. 3504 – 3518. DOI : 10.1093/mnras/stad2745.Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST
The Astrophysical Journal. 2023. Vol. 956, num. 1, p. 61. DOI : 10.3847/1538-4357/acef21.COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
The Astrophysical Journal. 2023. Vol. 954, num. 1, p. 31. DOI : 10.3847/1538-4357/acc2bc.The filament determination depends on the tracer: comparing filaments based on dark matter particles and galaxies in the GAEA semi-analytical model
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 525, num. 3, p. 4079 – 4092. DOI : 10.1093/mnras/stad2562.The Pandora project – I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 525, num. 3, p. 3806 – 3830. DOI : 10.1093/mnras/stad2559.Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z> 5 with CEERS
The Astrophysical Journal Letters. 2023. Vol. 954, num. 1. DOI : 10.3847/2041-8213/ace5a0.Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 525, num. 1, p. 962 – 968. DOI : 10.1093/mnras/stad2344.Euclid preparation XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys
Astronomy & Astrophysics. 2023. Vol. 676, p. A34. DOI : 10.1051/0004-6361/202346177.On the distribution of the cold neutral medium in galaxy discs
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 524, num. 1, p. 873 – 885. DOI : 10.1093/mnras/stad1537.Optical and mid-infrared line emission in nearby Seyfert galaxies
Astronomy & Astrophysics. 2023. Vol. 675, p. A74. DOI : 10.1051/0004-6361/202245516.Resolving Galactic-scale Obscuration of X-Ray AGNs at z & GSIM; 1 with COSMOS-Web
The Astrophysical Journal Letters. 2023. Vol. 951, num. 2, p. L41. DOI : 10.3847/2041-8213/acdef4.Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z similar or equal to 8-10
The Astrophysical Journal Letters. 2023. Vol. 951, num. 1, p. L22. DOI : 10.3847/2041-8213/acdd54.CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts
The Astrophysical Journal Letters. 2023. Vol. 950, num. 1, p. L5. DOI : 10.3847/2041-8213/acd639.Fuelling the nuclear ring of NGC 1097
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 523, num. 2, p. 2918 – 2927. DOI : 10.1093/mnras/stad1554.An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
The Astrophysical Journal. 2023. Vol. 947, num. 1, p. 20. DOI : 10.3847/1538-4357/acbefa.Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko
Journal Of Geophysical Research-Space Physics. 2023. Vol. 128, num. 4, p. e2022JA031249. DOI : 10.1029/2022JA031249.CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results
The Astrophysical Journal Letters. 2023. Vol. 946, num. 1, p. L12. DOI : 10.3847/2041-8213/acbb08.The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
The Astrophysical Journal. 2023. Vol. 945, num. 1, p. 35. DOI : 10.3847/1538-4357/acba8a.CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST
The Astrophysical Journal Letters. 2023. Vol. 946, num. 1, p. L13. DOI : 10.3847/2041-8213/acade4.The star formation history and the nature of the mass-metallicity relation of passive galaxies at 1.0 < z < 1.4 from VANDELS
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 520, num. 2, p. 3027 – 3048. DOI : 10.1093/mnras/stad241.Semi-analytic forecasts for Roman – the beginning of a new era of deep-wide galaxy surveys
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 519, num. 1, p. 1578 – 1600. DOI : 10.1093/mnras/stac3595.PHANGS-JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC 1365
The Astrophysical Journal Letters. 2023. Vol. 944, num. 2, p. L15. DOI : 10.3847/2041-8213/acac9e.PHANGS-JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628
The Astrophysical Journal Letters. 2023. Vol. 944, num. 2, p. L22. DOI : 10.3847/2041-8213/aca7b9.Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 520, num. 1, p. 89 – 106. DOI : 10.1093/mnras/stad105.Study of backward Brillouin scattering in gas-filled anti-resonant fibers
APL Photonics. 2023. Vol. 8, num. 8, p. 086104. DOI : 10.1063/5.0151018.2022
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z similar to 12 Galaxy in Early JWST CEERS Imaging
The Astrophysical Journal Letters. 2022. Vol. 940, num. 2, p. L55. DOI : 10.3847/2041-8213/ac966e.From starburst to quenching: merger-driven evolution of the star formation regimes in a shell galaxy
Monthly Notices Of The Royal Astronomical Society. 2022. Vol. 518, num. 3, p. 3261 – 3273. DOI : 10.1093/mnras/stac3136.Enhanced Signal-Associated Noise in a φ-OTDR System
IEEE Access. 2022. Vol. 10, p. 44974 – 44981. DOI : 10.1109/ACCESS.2022.3170243.The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
The Astrophysical Journal. 2022. Vol. 929, num. 2, p. 113. DOI : 10.3847/1538-4357/ac5d47.2021
On the Measurement Accuracy of Coherent Rayleigh-based Distributed Sensors
Optics Express. 2021. Vol. 29, num. 26, p. 42538 – 42552. DOI : 10.1364/OE.442790.2020
Distributed and dynamic strain sensing with high spatial resolution and large measurable strain range
Optics Letters. 2020. Vol. 45, num. 18, p. 5020 – 5023. DOI : 10.1364/OL.395922.Conference Papers
2024
Investigations on assembly and coverage for modular focal planes of multiplexed telescopes
2024. 10 Ground-Based and Airborne Instrumentation for Astronomy, Yokohama, Japan, 2024-06-16 – 2024-06-21. DOI : 10.1117/12.3018315.2023
New Avenues in Optical Fiber Sensing Using Gas
2023. 28th International Conference on Optical Fiber Sensors, Hamamatsu, Japan, November 20-24, 2023. DOI : 10.1364/OFS.2023.W5.1.Study on the possibility of Φ-OTDR sensing in hollow-core fibres
2023. European Workshop on Optical Fibre Sensors (EWOFS 2023), Mons, Belgium, May 23-26, 2023. DOI : 10.1117/12.2679743.2022
Analytical prediction of the final error due to noise in a ϕ-OTDR system
2022. 27th International Conference on Optical Fiber Sensors, Alexandria, Virginia, USA, 29 August–2 September 2022. DOI : 10.1364/OFS.2022.Th4.60.Distributed Temperature Sensing Using Gas-filled Conjoined-tube Anti-resonant Fiber
2022. 27th International Conference on Optical Fiber Sensors, Alexandria, Virginia, USA, 29 August–2 September 2022. DOI : 10.1364/OFS.2022.Tu2.3.2021
Determination of the Measurement Accuracy of a Phase-sensitive OTDR
2021. OSA Optical Sensors and Sensing Congress 2021 (AIS, FTS, HISE, SENSORS, ES), Washington, DC United States, July 19-23, 2021. DOI : 10.1364/SENSORS.2021.SM5A.5.Distributed Temperature Sensing Based on φ-OTDR Using Back-reflection-enhanced Fiber
2021. CLEO: Science and Innovations 2021Conference on Lasers and Electro-Optics, San Jose, California, United States, May 9-17, 2021. DOI : 10.1364/CLEO_SI.2021.STu1A.3.Theses
2022
Investigating Novel Optical Fibres for More Advanced Distributed Optical Fibre Sensing
Lausanne, EPFL, 2022.Talks
2021
Spontaneous Brillouin Scattering in Gas-filled Anti-resonant Fibre
Frontiers in Optics + Laser Science 2021, Online, November 1–4, 2021.Dr. Robin Tress
Journal Articles
2025
Do stars still form in molecular gas within CO-dark dwarf galaxies?
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2025. num. 3, p. 2936 – 2955. DOI : 10.1093/mnras/stae2759.2024
Testing kinematic distances under a realistic Galactic potential Investigating systematic errors in the kinematic distance method arising from a non-axisymmetric potential
ASTRONOMY & ASTROPHYSICS. 2024. Vol. 692. DOI : 10.1051/0004-6361/202450000.Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351
The Astrophysical Journal. 2024. Vol. 967, num. 2, p. 133. DOI : 10.3847/1538-4357/ad3de6.2023
Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 525, num. 1, p. 962 – 968. DOI : 10.1093/mnras/stad2344.On the distribution of the cold neutral medium in galaxy discs
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 524, num. 1, p. 873 – 885. DOI : 10.1093/mnras/stad1537.Fuelling the nuclear ring of NGC 1097
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 523, num. 2, p. 2918 – 2927. DOI : 10.1093/mnras/stad1554.PHANGS-JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC 1365
The Astrophysical Journal Letters. 2023. Vol. 944, num. 2, p. L15. DOI : 10.3847/2041-8213/acac9e.PHANGS-JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628
The Astrophysical Journal Letters. 2023. Vol. 944, num. 2, p. L22. DOI : 10.3847/2041-8213/aca7b9.The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS
The Astrophysical Journal Letters. 2023. Vol. 944, num. 2, p. L17. DOI : 10.3847/2041-8213/acaaae.Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 520, num. 1, p. 89 – 106. DOI : 10.1093/mnras/stad105.Dr. Farcy Marion
Journal Articles
2025
You Shall Not Pass! The Propagation of Low-/Moderate-powered Jets Through a Turbulent Interstellar Medium
ASTROPHYSICAL JOURNAL. 2025. Vol. 981, num. 2. DOI : 10.3847/1538-4357/adb016.2024
On the origin of star formation quenching in massive galaxies at z ≳ 3 in the cosmological simulations Illustris TNG
Monthly Notices of the Royal Astronomical Society. 2024. Vol. 534, num. 4, p. 3974 – 3988. DOI : 10.1093/mnras/stae2297.The effect of cosmic rays on the observational properties of the CGM
Monthly Notices Of The Royal Astronomical Society. 2024. Vol. 530, num. 1, p. 52 – 65. DOI : 10.1093/mnras/stae837.2023
The Pandora project – I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 525, num. 3, p. 3806 – 3830. DOI : 10.1093/mnras/stad2559.Dr. Adèle Plat
Journal Articles
2024
Lyα Emission Line Profiles of Extreme [O iii]- emitting Galaxies at z ≳ 2: Implications for Lyα Visibility in the Reionization Era
The Astrophysical Journal. 2024. Vol. 972, num. 1, p. 56. DOI : 10.3847/1538-4357/ad5ae0.CLASSY. VIII. Exploring the Source of Ionization with UV Interstellar Medium Diagnostics in Local High-z Analogs
The Astrophysical Journal. 2024. Vol. 962, num. 1, p. 95. DOI : 10.3847/1538-4357/ad1033.2023
Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST
Monthly Notices Of The Royal Astronomical Society. 2023. Vol. 526, num. 3, p. 3610 – 3636. DOI : 10.1093/mnras/stad2955.Jonathan Petersson
Journal Articles
2025
The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2025. Vol. 537, num. 2, p. 956 – 977. DOI : 10.1093/mnras/staf002.2022
From starburst to quenching: merger-driven evolution of the star formation regimes in a shell galaxy
Monthly Notices Of The Royal Astronomical Society. 2022. Vol. 518, num. 3, p. 3261 – 3273. DOI : 10.1093/mnras/stac3136.Lucie Scharré
Journal Articles
2023
Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko
Journal Of Geophysical Research-Space Physics. 2023. Vol. 128, num. 4, p. e2022JA031249. DOI : 10.1029/2022JA031249.Dr. Malak Galal
Journal Articles
2025
[Erratum] Study of backward Brillouin scattering in gas-filled anti-resonant fibers (vol 8, 086104, 2023)
APL PHOTONICS. 2025. Vol. 10, num. 3. DOI : 10.1063/5.0263994.2023
Study of backward Brillouin scattering in gas-filled anti-resonant fibers
APL Photonics. 2023. Vol. 8, num. 8, p. 086104. DOI : 10.1063/5.0151018.2022
Enhanced Signal-Associated Noise in a φ-OTDR System
IEEE Access. 2022. Vol. 10, p. 44974 – 44981. DOI : 10.1109/ACCESS.2022.3170243.2021
On the Measurement Accuracy of Coherent Rayleigh-based Distributed Sensors
Optics Express. 2021. Vol. 29, num. 26, p. 42538 – 42552. DOI : 10.1364/OE.442790.2020
Distributed and dynamic strain sensing with high spatial resolution and large measurable strain range
Optics Letters. 2020. Vol. 45, num. 18, p. 5020 – 5023. DOI : 10.1364/OL.395922.Conference Papers
2024
Investigations on assembly and coverage for modular focal planes of multiplexed telescopes
2024. 10 Ground-Based and Airborne Instrumentation for Astronomy, Yokohama, Japan, 2024-06-16 – 2024-06-21. DOI : 10.1117/12.3018315.2023
Novel low-temperature fiber sensing technique using Brillouin scattering in gas
2023. 28th International Conference on Optical Fiber Sensors (OFS-28), Hamamatsu, Japan, November 20-24, 2023. DOI : 10.1364/OFS.2023.F2.3.New Avenues in Optical Fiber Sensing Using Gas
2023. 28th International Conference on Optical Fiber Sensors, Hamamatsu, Japan, November 20-24, 2023. DOI : 10.1364/OFS.2023.W5.1.Study on the possibility of Φ-OTDR sensing in hollow-core fibres
2023. European Workshop on Optical Fibre Sensors (EWOFS 2023), Mons, Belgium, May 23-26, 2023. DOI : 10.1117/12.2679743.2022
Analytical prediction of the final error due to noise in a ϕ-OTDR system
2022. 27th International Conference on Optical Fiber Sensors, Alexandria, Virginia, USA, 29 August–2 September 2022. DOI : 10.1364/OFS.2022.Th4.60.Distributed Temperature Sensing Using Gas-filled Conjoined-tube Anti-resonant Fiber
2022. 27th International Conference on Optical Fiber Sensors, Alexandria, Virginia, USA, 29 August–2 September 2022. DOI : 10.1364/OFS.2022.Tu2.3.2021
Determination of the Measurement Accuracy of a Phase-sensitive OTDR
2021. OSA Optical Sensors and Sensing Congress 2021 (AIS, FTS, HISE, SENSORS, ES), Washington, DC United States, July 19-23, 2021. DOI : 10.1364/SENSORS.2021.SM5A.5.Distributed Temperature Sensing Based on φ-OTDR Using Back-reflection-enhanced Fiber
2021. CLEO: Science and Innovations 2021Conference on Lasers and Electro-Optics, San Jose, California, United States, May 9-17, 2021. DOI : 10.1364/CLEO_SI.2021.STu1A.3.Theses
2022
Investigating Novel Optical Fibres for More Advanced Distributed Optical Fibre Sensing
Lausanne, EPFL, 2022.2018
Distributed analyses using distinct classes of Brillouin scatterings in optical fibres
Lausanne, EPFL, 2018.Talks
2021
Spontaneous Brillouin Scattering in Gas-filled Anti-resonant Fibre
Frontiers in Optics + Laser Science 2021, Online, November 1–4, 2021.
- Prof. Michaela Hirschmann’s publication list (PDF)
- Prof. Michaela Hirschmann’s full publication list on ADS
- Dr. Marion Farcy’s full publication list on ADS
- Dr. Robin Tress’ full publication list on ADS
- Dr. Adèle Plat’s full publication list on ADS
- Dr. Salvatore Taibi’s full publication list on ADS
- Lucie Scharré’s full publication list on ADS
- Jonathan Petersson’s full publication list on ADS
- Patrick Hirling’s full publication list on ADS