Calibration of Star Formation Rate Indicators and Spectral Diagnostics
Evaluating star formation rates at z = 5
Ismail, D., Kraljic, K., Béthermin, M., Kapoor, A. U. et al.
This study utilizes synthetic observations to evaluate the [CII]-SFR relation at z=5, identifying dependencies on gas density and metallicity that align with your research on metallicity-dependent conversion factors and carbon tracers in high-redshift environments.
First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars
Gong, Yan, Zhong, Jiaqiang, Ren, Yuan, Zhang, Yilong et al.
This study maps the full carbon cycle ([CII], [CI], CO) and attributes elevated C0/CO ratios to radiation penetration in a clumpy ISM, offering observational data that aligns with your 3D-PDR modeling of carbon phase transitions and fractal cloud structures.
PDRs4All: XVII. Formation and excitation of HD in photodissociation regions: Application to the Orion Bar
Zannese, Marion, Le Bourlot, Jacques, Roueff, Evelyne, Bron, Emeric et al.
This study analyzes JWST NIRSpec observations of HD formation and excitation using the Meudon PDR code, providing a direct comparative framework for your own 3D-PDR synthetic observations and modeling of molecular tracers in irradiated environments.
The Calibration of Short-wavelength Polycyclic Aromatic Hydrocarbon Emission as Star Formation Rate Indicators with JWST
Gregg, Benjamin, Calzetti, Daniela, Adamo, Angela, Pedrini, Alex et al.
This study utilizes JWST to calibrate PAH emission as a star formation tracer, presenting findings on metallicity-dependent variations and grain destruction that complement your recent work on environmental impacts in PDRs and metallicity-dependent conversion factors.
SPARCS– combining radiation hydrodynamics with non-equilibrium metal chemistry in the SWIFT astrophysical code
Chan, Tsang Keung, Richings, Alexander J., Theuns, Tom, Liu, Yuankang et al.
This paper presents SPARCS, an SPH-based code coupling radiation hydrodynamics with non-equilibrium chemistry and cosmic ray ionization, which parallels your development of 3D-PDR and use of RADMC-3D for generating synthetic observations of ISM structures.
Calibrating Mid-Infrared Emission Features As Diagnostics of Star Formation in Infrared-Luminous Galaxies via Radiative Transfer Modeling
Robinson, L., Farrah, D., Efstathiou, A., Engholm, A. et al.
This study employs radiative transfer modeling to calibrate mid-infrared star formation tracers for JWST, relevant to your focus on synthetic observations and disentangling AGN versus star-formation contributions in high-redshift environments.
Active Galactic Nuclei (AGN) Feedback and Outflows
Evidence of Feedback Effects in Low-luminosity Active Galactic Nuclei Revealed by JWST Spectroscopy
Zhang, Lulu, Packham, Chris, Hicks, Erin K. S., Davies, Ric I. et al.
This study utilizes JWST MIRI and NIRSpec spectroscopy to analyze non-thermalized H2 transitions and shock excitation, directly relating to your recent work on modeling molecular gas heating and distinguishing mechanical feedback from radiative processes.
Blowing Star Formation Away in AGN Hosts (BAH). IV. Feeding and Feedback in 3C 293 Observed with JWST NIRSpec
de Mellos, Maitê S. Z., Riffel, Rogemar A., Souza-Oliveira, Gabriel L., Zakamska, Nadia L. et al.
The analysis of H2 2.12 μm emission and extinction maps using JWST NIRSpec directly parallels your recent work on characterizing warm molecular gas reservoirs and feedback mechanisms in AGN hosts like MACS 1931-26.
Strong Evidence for Cosmic-Ray-supported ∼L* Galaxy Halos via X-Ray and tSZ Constraints
Ponnada, Sam B., Hopkins, Philip F., Lu, Yue Samuel, Silich, Emily M. et al.
This study presents observational constraints identifying Cosmic Rays as a dominant source of non-thermal pressure in galaxy halos, complementing your research on Cosmic Ray interactions and their role in regulating the interstellar medium.
Measurement of the gas consumption history of a massive quiescent galaxy
Scholtz, Jan, D'Eugenio, Francesco, Maiolino, Roberto, Pérez-González, Pablo G. et al.
This study combines ALMA CO and JWST data to constrain gas reservoirs and AGN-driven outflows in a z ≈ 3 galaxy, overlapping with your research on high-redshift gas dynamics and the reliability of molecular tracers in feedback-dominated environments.
Interstellar Medium and Abundances in the Galactic Center
A survey of molecular clouds in the Galactic center's outflow
Di Teodoro, Enrico M., Heyer, Mark, Krumholz, Mark R., Armillotta, Lucia et al.
This study presents APEX observations of molecular-to-atomic gas phase transitions in galactic outflows, analyzing virial parameters and CO dissociation timescales that align with your research on the dynamical evolution and chemical cycling of the ISM.
New Estimate for the Cosmic Ray-Induced H₂ Photodissociation Rate in the Interstellar Medium
Sipilä, O., Caselli, P., Padovani, M., Galli, D. et al.
This study derives a revised rate coefficient for cosmic ray-induced H₂ dissociation, which directly impacts the chemical networks used in your 3D-PDR code and aligns with your recent work on cosmic ray excitation with co-author M. Padovani.
VizieR Online Data Catalog: ISM phases and abundances in the central parsec (Vermot+, 2025)
Vermot, P., Ciurlo, A., Rouan, D., Morris, M. R. et al.
This catalog provides JWST/MIRI-MRS phase maps and spectra of the Galactic Center's ISM, offering high-resolution mid-infrared benchmarks for your research on modeling thermodynamics and generating synthetic observations in extreme environments.
Nonthermal Pressures: Key to Energy Balance and Structure Formation near Sgr A* in the Milky Way
Mazoochi, Farideh, Tabatabaei, Fatemeh S., Barnes, Ashley T., Colzi, Laura et al.
This study quantifies the balance between cosmic ray, magnetic, and molecular gas pressures near Sgr A*, concluding that magnetic fields stabilize clouds against collapse, which parallels your recent research on sub-virial, magnetically supported gas and cosmic ray regulation of the ISM.
Widespread Hot Molecular Gas Heated by Shear-induced Turbulence in the Galactic Center
Li, Juan, Wang, Junzhi, Shen, Zhiqiang, Vidal-García, Alba et al.
This study features your frequent collaborator Di Li and identifies shear-induced turbulence as the dominant heating mechanism for molecular gas, paralleling your recent analysis of kinetic energy dissipation in cluster cores.
Interstellar medium phases and abundances in the central parsec: A JWST MIRI/MRS view of the Galactic center
Vermot, P., Ciurlo, A., Rouan, D., Morris, M. R. et al.
This study employs JWST MIRI/MRS observations and synthetic spectral modeling to constrain multiphase ISM abundances—specifically Fe depletion and α-enhancement—which directly parallels your recent research on metallicity-dependent chemical tracers and α-enhanced astrochemistry.
Star Formation, Magnetic Fields, and Molecular Cloud Dynamics
Collision between molecular clouds IV: The role of feedback and magnetic field in head on collisions
Tanvir, Tabassum S., Grudić, Michael Y.
This study simulates cloud-cloud collisions with radiative feedback and varying magnetic field orientations, offering dynamical insights relevant to your work on [CII] collision diagnostics and magnetic support in molecular clouds.
The Column Density Probability Density Function of Cygnus-X
Xing, Yuchen, Qiu, Keping
This study analyzes the Column Density Probability Density Function (N-PDF) in Cygnus-X, providing observational constraints on density structures that align with your development of the PDFchem code, which utilizes such statistical distributions to model ISM chemistry.
The influence of magnetic fields in Cloud-Cloud Collisions
Georgatos, Theotokis, Whitworth, Anthony P.
Co-authored by your mentor Anthony Whitworth, this SPH study examines how magnetic fields regulate morphology in cloud-cloud collisions, complementing your research on [CII] collision diagnostics and magnetic support in molecular clouds.
A High-resolution Study of the Cold Neutral Medium in and around 30 Doradus
Park, Gyueun, Lee, Min-Young, Dickey, John M., Pingel, Nick M. et al.
This study characterizes the Cold Neutral Medium and H I shielding layers in 30 Doradus, providing observational constraints on the atomic-to-molecular transition and gas dynamics in a low-metallicity starburst environment relevant to your PDR modeling.
A Pan-galaxy Study of Synthetic Giant Molecular Filaments: A Turbulence-dominated Life Cycle
Hu, Zipeng, Wang, Ke, Krumholz, Mark R., Su, Keyun
This study utilizes synthetic CO emission maps from MHD simulations to analyze the role of magnetized turbulence in supporting molecular filaments, directly paralleling your work on synthetic observations and the balance between turbulence and magnetic fields in cloud dynamics.
The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-luminosity Protostars
Sequeira-Murillo, Francisco, Rosero, Viviana, Marvil, Joshua, Tan, Jonathan C. et al.
This paper presents results from the SOMA survey, a collaboration you actively contribute to, and analyzes ionization mechanisms in massive protostars that complement your research on star formation feedback and H II region expansion.
GMCs and Star Formation in Galaxies. I. Mass Loss from a GMC Induced by an H II Region
Hollenbach, David, Parravano, Antonio, McKee, Christopher F.
This theoretical study on H II region expansion and the formation of cometary cloud structures directly parallels your research on Radiatively Driven Implosion (RDI) and the dynamical benchmarking of ionization fronts within the STARBENCH project.
Time-dependent chemical evolution during cloud formation: H₂-regulated chemistry in diffuse molecular cloud
Komichi, Yuto, Aikawa, Yuri, Iwasaki, Kazunari, Furuya, Kenji
This study uses 3D MHD simulations coupled with chemical post-processing to investigate the "CO-poor" gas phase and derive analytic abundance solutions, directly paralleling your research on CO-dark gas and the calibration of alternative molecular tracers relative to H2.
A bottleneck for star formation: the importance of magnetic fields during the formation of cold gas in galaxies
McGuiness, Ryan, Smith, Rowan J., Whitworth, David
This study quantifies the energetic dominance of magnetic fields in the cold neutral medium and CO-dark gas of dwarf galaxies, directly aligning with your recent findings on magnetic support in sub-virial, low-metallicity clouds.
The Influential Roles of Gravity, Turbulence, and Magnetic Fields in Shaping the Physical Evolution of Dense Massive Clumps
Asogwa, Moses Onyemaechi, Negu, Seblu Humne, Kumssa, Gemechu Muleta, Eya, Innocent Okwudili
This study analyzes virial parameters and velocity dispersion relations in APEX-identified clumps to argue that turbulence is insufficient to balance gravity, paralleling your recent work on sub-virial states and magnetic support in low-metallicity environments.
High-Redshift Galaxy Evolution and ISM Properties
Breathless BEARS: [OIII] 88μm Emission of Dusty Star-Forming Galaxies at z = 3–4
Bakx, T. J. L. C., Algera, Hiddo S. B., Prajapati, Prachi, Bendo, George et al.
This paper analyzes [O III] and [C II] line ratios in z=3–4 dusty star-forming galaxies, providing observational constraints on metallicity and ionization fields relevant to your PDR modeling of high-redshift ISM, and is co-authored by your frequent collaborator Kevin Harrington.
One cloud is not enough: extreme conditions bias chemical abundances in high-redshift galaxies
Moreschini, Bianca, Belfiore, Francesco, Marconi, Alessandro, Cataldi, Elisa et al.
The study demonstrates how unresolved density clumps bias chemical diagnostics in high-redshift galaxies observed by JWST, directly relating to your research on quantifying the impact of ISM inhomogeneity on molecular tracers and metallicity estimates using 3D-PDR and PDFchem.
On the dusty proximate damped Lyman-α system toward Q 2310−3358 at z = 2.40
Han, S., Krogager, J.-K., Ledoux, C., Ma, G. et al.
This study employs Atomic Carbon ([CI]) fine-structure lines to constrain gas density and UV radiation fields in a z=2.4 system, providing observational data that directly relates to your theoretical modeling of PDR chemistry and [CI] as a molecular gas tracer.