Search Results - "Bardeau, Sebastien"
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Combining Strong and Weak Gravitational Lensing in Abell 1689
Published in The Astrophysical journal (20-10-2007)“…We present a reconstruction of the mass distribution of galaxy cluster Abell 1689 at z = 0.18 using detected strong lensing features from deep ACS observations…”
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Journal Article -
2
Learning from model grids: Tracers of the ionization fraction in the ISM
Published in EPJ Web of Conferences (2022)“…The ionization fraction in neutral interstellar clouds is a key physical parameter controlling multiple physical and chemical processes, and varying by orders…”
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Journal Article Conference Proceeding -
3
Revealing which Combinations of Molecular Lines are Sensitive to the Gas Physical Parameters of Molecular Clouds
Published in EPJ Web of Conferences (01-01-2022)“…Atoms and molecules have long been thought to be versatile tracers of the cold neutral gas in the universe, from high-redshift galaxies to star forming regions…”
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Conference Proceeding Journal Article -
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A Fully Bayesian Approach For Inferring Physical Properties With Credibility Intervals From Noisy Astronomical Data
Published in 10th Workshop on Hyperspectral Imaging and Signal Processing: Evolution in Remote Sensing (WHISPERS), Amsterdam, Netherlands (01-09-2019)“…The atoms and molecules of interstellar clouds emit photons when passing from an excited state to a lower energy state. The resulting emission lines can be…”
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Conference Proceeding -
5
Solving the Abell 1689 puzzle: A combined strong and weak gravitational lensing analysis
Published in The Astrophysical journal (2007)“…We present a reconstruction of the mass distribution of galaxy cluster Abell 1689 at z = 0.18 using detected strong lensing features from deep HST/ACS…”
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Journal Article -
6
Bias versus variance when fitting multi-species molecular lines with a non-LTE radiative transfer model
Published 29-03-2024“…Robust radiative transfer techniques are requisite for efficiently extracting the physical and chemical information from molecular rotational lines.We study…”
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Journal Article -
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Revealing which Combinations of Molecular Lines are Sensitive to the Gas Physical Parameters of Molecular Clouds: Astrophysics Meet Data Science towards the Orion B Cloud
Published in EPJ Web of conferences (2022)“…Atoms and molecules have long been thought to be versatile tracers of the cold neutral gas in the universe, from high-redshift galaxies to star forming regions…”
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Journal Article -
8
C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud: An analysis of the precision achievable when modeling spectral line within the Local Thermodynamic Equilibrium approximation
Published 17-05-2020“…A&A 645, A26 (2021) CO isotopologue transitions are routinely observed in molecular clouds to probe the column density of the gas, the elemental ratios of…”
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Journal Article -
9
The Most Massive Clusters in the Universe
Published 23-11-2002“…Clusters of galaxies need to be investigated using complementary approaches combining all currently available observational techniques (X-ray, gravitational…”
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Journal Article -
10
Toward a robust physical and chemical characterization of heterogeneous lines of sight: The case of the Horsehead nebula
Published 30-09-2024“…Dense cold molecular cores/filaments are surrounded by an envelope of translucent gas. Some of the low-J emission lines of CO and HCO$^+$ isotopologues are…”
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Journal Article -
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Quantifying the informativity of emission lines to infer physical conditions in giant molecular clouds. I. Application to model predictions
Published 21-09-2024“…A&A 691, A109 (2024) Observations of ionic, atomic, or molecular lines are performed to improve our understanding of the interstellar medium (ISM). However,…”
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12
Neural network-based emulation of interstellar medium models
Published 04-09-2023“…A&A 678, A198 (2023) The interpretation of observations of atomic and molecular tracers in the galactic and extragalactic interstellar medium (ISM) requires…”
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Journal Article -
13
Deep learning denoising by dimension reduction: Application to the ORION-B line cubes
Published 24-07-2023“…A&A 677, A158 (2023) Context. The availability of large bandwidth receivers for millimeter radio telescopes allows the acquisition of…”
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Journal Article -
14
Gas kinematics around filamentary structures in the Orion B cloud
Published 25-11-2022“…A&A 670, A59 (2023) Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational…”
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Journal Article -
15
Quantitative inference of the $H_2$ column densities from 3 mm molecular emission: A case study towards Orion B
Published 31-08-2020“…A&A 645, A27 (2021) Molecular hydrogen being unobservable in cold molecular clouds, the column density measurements of molecular gas currently rely either on…”
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Journal Article -
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Tracers of the ionization fraction in dense and translucent gas: I. Automated exploitation of massive astrochemical model grids
Published 27-07-2020“…A&A 645, A28 (2021) The ionization fraction plays a key role in the physics and chemistry of the neutral interstellar medium, from controlling the coupling of…”
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Journal Article -
17
A dynamically young, gravitationally stable network of filaments in Orion B
Published 11-03-2019“…A&A 624, A113 (2019) Filaments are a key step on the path that leads from molecular clouds to star formation. However, their characteristics are heavily…”
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Journal Article -
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Clustering the Orion B giant molecular cloud based on its molecular emission
Published 19-10-2017“…A&A 610, A12 (2018) Previous attempts at segmenting molecular line maps of molecular clouds have focused on using position-position-velocity data cubes of a…”
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Journal Article -
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Dissecting the molecular structure of the Orion B cloud: Insight from Principal Component Analysis
Published 16-01-2017“…A&A 599, A100 (2017) Context. The combination of wideband receivers and spectrometers currently available in (sub-)millimeter observatories deliver wide- field…”
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Journal Article -
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Turbulence and star formation efficiency in molecular clouds: solenoidal versus compressive motions in Orion B
Published 04-01-2017“…A&A 599, A99 (2017) The nature of turbulence in molecular clouds is one of the key parameters that control star formation efficiency: compressive motions, as…”
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Journal Article