Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

Abstract

The Binary Population and Spectral Synthesis (BPASS) suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby. We present a new version 2.1 data release of these models, detailing the methodology by which BPASS incorporates binary mass transfer and its effect on stellar evolution pathways, as well as the construction of simple stellar populations. We demonstrate key tests of the latest BPASS model suite demonstrating its ability to reproduce the colours and derived properties of resolved stellar populations, including well- constrained eclipsing binaries. We consider observational constraints on the ratio of massive star types and the distribution of stellar remnant masses. We describe the identification of supernova progenitors in our models, and demonstrate a good agreement to the properties of observed progenitors. We also test our models against photometric and spectroscopic observations of unresolved stellar populations, both in the local and distant Universe, finding that binary models provide a self-consistent explanation for observed galaxy properties across a broad redshift range. Finally, we carefully describe the limitations of our models, and areas where we expect to see significant improvement in future versions.

69 pages, 45 figures. Accepted for publication in PASA. Accompanied by a full, documented data release at http://bpass.auckland.ac.nz and http://warwick.ac.uk/bpass

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• On the nature and physical conditions of the luminous Lya emitter CR7 and its rest-frame UV components
• The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning $0.2\lesssim z\lesssim 15$
• Neutron Star Kicks II: Revision and further testing of the conservation of momentum "kick" model
• Pégase.3: A code for modeling the UV-to-IR/submm spectral and chemical evolution of galaxies with dust
• The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3
• You Can't Always Get What You Want: The Impact of Prior Assumptions on Interpreting GW190412
• Ionization correction factors and dust depletion patterns in giant HII regions
• Ultraviolet Detection of the Binary Companion to the Type IIb SN 2001ig
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• Gravitational Wave Astronomy With TianQin
• The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?
• Hoki: Making BPASS accessible through Python
• Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground
• High Equivalent Width of Hα+[N II] Emission in z~8 Lyman-break Galaxies from IRAC 5.8μm Observations: Evidence for Efficient Lyman-continuum Photon production in the Epoch of Re-ionization
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Very massive stars and Nitrogen emitting galaxies
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• A two-stage formalism for common-envelope phases of massive stars
• Binary population synthesis models for core-collapse gamma-ray burst progenitors
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Paschen-line Constraints on Dust Attenuation and Star Formation at z~1-3 with JWST/NIRSpec
• The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5
• Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
• Extreme Emission-Line Galaxies in SDSS. I. Empirical and model-based calibrations of chemical abundances
• J1234+3901: an extremely metal-deficient compact star-forming dwarf galaxy at redshift 0.133
• Semi-analytic forecasts for JWST -- III. Intrinsic production efficiency of Lyman-continuum radiation
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• SPISEA: A Python-Based Simple Stellar Population Synthesis Code for Star Clusters
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Mass loss and the Eddington parameter: a new mass-loss recipe for hot and massive stars
• Weighing in on black hole binaries with BPASS: LB-1 does not contain a 70M${}_{\odot }$ black hole
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at $z=4.5-11.5$
• The Pre-Explosion Mass Distribution of Hydrogen-Poor Superluminous Supernova Progenitors and New Evidence for a Mass-Spin Correlation
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• A Potential Progenitor for the Type Ic Supernova 2017ein
• The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming Galaxies
• Recalibrating the Cosmic Star Formation History
• Lyman-alpha opacities at z=4-6 require low mass, radiatively-suppressed galaxies to drive cosmic reionization
• Star Formation Stochasticity Measured from the Distribution of Burst Indicators
• Photometric properties of reionization-epoch galaxies in the Simba simulations
• EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with $\sim 1.0$ (Fe/O)${}_{\odot }$ and $0.02$ (O/H)${}_{\odot }$ : Possible Traces of Super Massive ($>300M_{\odot }$) Stars in Early Galaxies
• The MOSDEF Survey: Implications of the Lack of Evolution in the Dust Attenuation-Mass Relation to z~2
• Early results from GLASS-JWST XVI: Discovering a bluer z~4-7 Universe through UV slopes
• The stellar mass versus stellar metallicity relation of star-forming galaxies at $1.6\le z\le 3.0$ and implications for the evolution of the $\alpha$-enhancement
• Chemodynamics of Green Pea galaxies -- I. Outflows and turbulence driving the escape of ionising photons and chemical enrichment
• Can nebular HeII emission be explained by ultra-luminous X-ray sources?
• The Ionizing Photon Production Efficiency (${\xi }_{ion}$) Of Lensed Dwarf Galaxies At $z\sim 2$
• Neutral Gas Properties and Ly$\alpha$ Escape in Extreme Green Pea Galaxies
• Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations
• Tracing Lyman-alpha and Lyman Continuum Escape in Galaxies with Mg II Emission
• Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
• Characterizing Extreme Emission Line Galaxies II: A Self-Consistent Model of Their Ionizing Spectrum
• Spectroscopic evolution of very massive stars at Z = 1/2.5 Zsun
• Large Binocular Telescope observations of new six compact star-forming galaxies with [NeV] 3426A emission
• The mass-metallicity relation at z~1-2 and its dependence on star formation rate
• MIRI/JWST observations reveal an extremely obscured starburst in the z=6.9 system SPT0311-58
• Nebular emission from young stellar populations including binary stars
• Clues on the presence and segregation of very massive stars in the Sunburst Lyman-continuum cluster at z=2.37
• A Blast from the Pasture: Studying the environment of AT 2018cow with MUSE
• The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
• The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova
• The Luminosity Function of Red Supergiants in M31
• A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. I. The northern WC sequence
• Revisiting the Impact of Dust Production from Carbon-Rich Wolf-Rayet Binaries
• The Red Supergiant Content of M31 and M33
• The DUVET Survey: Direct $T_e$-based metallicity mapping of metal-enriched outflows and metal-poor inflows in Mrk 1486
• Nebular Line Emission During the Epoch of Reionization
• Star formation in the outskirts of DDO 154: A top-light IMF in a nearly dormant disc
• JADES: Primaeval Lyman-$\alpha$ emitting galaxies reveal early sites of reionisation out to redshift $z\sim 9$
• The orbit and stellar masses of the archetype colliding-wind binary WR 140
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• The Sunburst Arc with JWST: I. Detection of Wolf-Rayet stars injecting nitrogen into a low-metallicity, $z=2.37$ proto-globular cluster leaking ionizing photons
• Weak Evolution of the Mass-metallicity Relation at Cosmic Dawn in the FirstLight Simulations
• Prospects for LISA to detect a gravitational-wave background from first order phase transitions
• Measuring the properties of active galactic nuclei disks with gravitational waves
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties
• Numerical experiments to help understand cause and effect in massive star evolution
• Spatially resolved evidence of the impact of quasar driven outflows on recent star formation : The case of Mrk 34
• Physical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy
• Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions
• Galaxy Size and Mass Build-up in the First 2 Gyrs of Cosmic History from Multi-Wavelength JWST NIRCam Imaging
• The Dusty and Extremely Red Progenitor of the Type II Supernova 2023ixf in Messier 101
• The Semi-forbidden CIII]$\lambda$1909Å~ Emission in the Rest-Ultraviolet Spectra of Green Pea Galaxies
• Simultaneous Constraints on the Star Formation History and Nucleosynthesis of Sculptor dSph
• Observability of inflated companion stars after supernovae in massive binaries
• An Early-Time Optical and Ultraviolet Excess in the type-Ic SN 2020oi
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• FirstLight III: Rest-frame UV-optical spectral energy distributions of simulated galaxies at cosmic dawn
• Explaining the differences in massive star models from various simulations
• Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies
• Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation
• Progenitor candidate for the type II-P supernova SN 2018aoq in NGC 4151
• The VANDELS survey: A strong correlation between Ly$\alpha$ equivalent width and stellar metallicity at $3\le \mathbf{z}\le 5$
• An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion
• A candidate runaway supermassive black hole identified by shocks and star formation in its wake
• The host galaxies of double compact objects across cosmic time
• Photometric identification and MMT spectroscopy of new extremely metal-poor galaxies: towards a better understanding of young stellar populations at low metallicity
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3
• Stars and gas in the most metal-poor galaxies I: COS and MUSE observations of SBS 0335-052E
• MESA models with magnetic braking
• The Circumstellar Environments of Double-Peaked, Calcium-strong Supernovae 2021gno and 2021inl
• Properties of five z~0.3-0.4 confirmed LyC leakers: VLT/XShooter observations
• A Short Introduction to Reionization Physics
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• The Impact of Star-Formation-Rate Surface Density on the Electron Density and Ionization Parameter of High-Redshift Galaxies
• WO-Type Wolf-Rayet Stars: the Last Hurrah of Massive Star Evolution
• X-ray binary accretion states in Active Galactic Nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines
• Observable and ionizing properties of star-forming galaxies with very massive stars and different IMFs
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• Gravitational Potential and Surface Density Drive Stellar Populations -- II. Star-Forming Galaxies
• The diversity of supernovae and impostors shortly after explosion
• The Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system
• Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
• Modeling Kepler Eclipsing Binaries: Homogeneous Inference of Orbital & Stellar Properties
• The changing-type SN 2014C may come from an 11-$M_{\odot }$ star stripped by binary interaction and violent eruption
• Astraeus II: Quantifying the impact of cosmic variance during the Epoch of Reionization
• An Hα Impression of Lyα Galaxies at $z\simeq 6$ with Deep JWST/NIRCam Imaging
• The connection between the escape of ionizing radiation and galaxy properties at z~3 in the Keck Lyman Continuum Spectroscopic Survey
• SuperBoRG: Exploration of point sources at $z\sim 8$ in HST parallel fields
• The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift
• The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup medium
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• Direct Constraints on the Extremely Metal-Poor Massive Stars Underlying Nebular C IV Emission from Ultra-Deep HST/COS Ultraviolet Spectroscopy
• EMPRESS. VII. Ionizing Spectrum Shapes of Extremely Metal-Poor Galaxies: Uncovering the Origins of Strong HeII and the Impact on Cosmic Reionization
• The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift
• A comparison of UV and optical metallicities in star-forming galaxies
• Broad-band selection, spectroscopic identification, and physical properties of a population of extreme emission line galaxies at 3<z<3.7
• The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
• The distance, supernova rate and supernova progenitors of NGC 6946
• Line Luminosities of Galactic and Magellanic Cloud Wolf-Rayet stars
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• The disappearances of six supernova progenitors
• Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)
• Spatially-resolved H$\alpha$ and ionizing photon production efficiency in the lensed galaxy MACS1149-JD1 at a redshift of 9.11
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• Inferring the presence of very massive stars in local star-forming regions
• Evidence for Very Massive Stars in extremely UV-bright star-forming galaxies at $z\sim 2.2-3.6$
• Elevated Hot Gas and High-Mass X-ray Binary Emission in Low Metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• X-ray properties of He II 1640 emitting galaxies in VANDELS
• The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-ray Source at z = 10.145
• Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
• Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• A hot and luminous source at the site of the fast transient AT2018cow at 2-3 years after its explosion
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Supernova lightCURVE POPulation Synthesis II: Validation against supernovae with an observed progenitor
• CECILIA: The Faint Emission Line Spectrum of z~2-3 Star-forming Galaxies
• Anatomy of a z=6 Lyman-α emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters
• Improving Star Cluster Age Estimates in PHANGS-HST Galaxies and the Impact on Cluster Demographics in NGC 628
• Nothing to see here: Failed supernovae are faint or rare
• The origin of the late-time luminosity of supernova 2011dh
• Binary evolution pathways of Blue Large-Amplitude Pulsators
• Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at $1.5<z<6.4$
• Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Physics of Prodigious Lyman Continuum Leakers
• The Faint Host Galaxies of C IV Absorbers at z > 5
• Reconstructing the observed ionizing photon production efficiency at z~2 using stellar population models
• Young massive clusters in the interacting LIRG Arp 299: evidence for the dependence of star cluster formation and evolution on environment
• Observations of the luminous red nova AT 2021biy in the nearby galaxy NGC 4631
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Dynamical formation of the GW190814 merger
• Gravitational Lensing of Gravitational Waves: Probability of Microlensing in Galaxy-Scale Lens Population
• Evaluating the impact of binary parameter uncertainty on stellar population properties
• Search Instructions for Globular Clusters in Formation at High Redshifts
• Phase-dependent study of near-infrared disk emission lines in LB-1
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• The IACOB project VIII. Searching for empirical signatures of binarity in fast-rotating O-type stars
• An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
• Extreme broad He\2 emission at high and low redshifts: the dominant role of VMS in NGC 3125-A1 and CDFS131717
• Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)
• IGM Transmission Bias for $z$ $\ge$ 2.9 Lyman Continuum Detected Galaxies
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• LIMFAST. II. Line Intensity Mapping as a Probe of High-Redshift Galaxy Formation
• On the contribution of the X-ray source to the extended nebular HeII emission in IZw18
• Where are the magnetar binary companions? Candidates from a comparison with binary population synthesis predictions
• Identifying the SN 2022acko progenitor with JWST
• Polarimetry of Hydrogen-Poor Superluminous Supernovae
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Supernovae Producing Unbound Binaries and Triples
• Haro 11 -- Untying the knots of the nuclear starburst
• A machine-learning photometric classifier for massive stars in nearby galaxies I. The method
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• The Detection of Intergalactic Halpha Emission from the Slug Nebula at z~2.3
• A high fraction of close massive binary stars at low metallicity
• Updated Photometry of the Yellow Supergiant Progenitor and Late-time Observations of the Type IIb Supernova 2016gkg
• Exploring the impact of IMF and binary parameter stochasticity with a binary population synthesis code
• Bridging Optical and Far-Infrared Emission-Line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 $\mu \mathrm{m}$/SFR at $z>6$
• The First Dynamical Mass Determination of a Nitrogen-rich Wolf-Rayet Star using a Combined Visual and Spectroscopic Orbit
• Lyman Continuum Galaxy Candidates in COSMOS
• Type II-P Supernova Progenitor Star Initial Masses and SN 2020jfo: Direct Detection, Light Curve Properties, Nebular Spectroscopy, and Local Environment
• Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
• Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars
• The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies
• Optimal neighbourhood to nurture giants: a fundamental link between star forming galaxies and direct collapse black holes
• ArtPop: A Stellar Population and Image Simulation Python Package
• JWST's PEARLS: TN J1338-1942 -- I. Extreme jet triggered star-formation in a $z=4.11$ luminous radio galaxy
• The density-bounded twilight of starbursts in the early Universe
• Observational properties of a general relativistic instability supernova from a primordial supermassive star
• Remnant masses from 1D+ core-collapse supernovae simulations: bimodal neutron star mass distribution and black holes in the low-mass gap
• Stellar Population Diagnostics of the Massive Star Binary Fraction
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations
• The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars
• Detection of He++ ion in the star-forming ring of the Cartwheel using MUSE data and ionizing mechanisms
• Binary black holes mergers from hierarchical triples in open clusters
• Balmer breaks in simulated galaxies at z>6
• Observational signature of circumstellar interaction and ${}^{56}$Ni-mixing in the Type II Supernova 2016gfy
• Delayed Photons from Binary Evolution Help Reionize the Universe
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• The "Giraffe": Discovery of a stripped red giant in an interacting binary with a $\sim 2M_{\odot }$ lower giant
• DSPS: Differentiable Stellar Population Synthesis
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• Astraeus VI: Hierarchical assembly of AGN and their large-scale effect during the Epoch of Reionization
• A tiny host galaxy for the first giant black hole: $z=7.5$ quasar in BlueTides
• Spatially-resolved chemodynamics of the starburst dwarf galaxy CGCG 007-025: Evidence for recent accretion of metal-poor gas
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• On the impact of spectral template uncertainties in synthetic stellar populations
• Lyman-Alpha Escape from Low-Mass, Compact, High-Redshift Galaxies
• A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE: I. Sample selection, analysis of local environments, and correlations with light curve properties
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Red Supergiant Mass Loss and Mass-Loss Rates
• Systematic uncertainties in models of the cosmic dawn
• Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova
• Wolf-Rayet galaxies in SDSS-IV MaNGA. I. Catalog construction and sample properties
• The 50-100pc scale parent stellar populations of type II supernovae and limitations of single star evolution models
• The possible disappearance of a massive star in the low metallicity galaxy PHL 293B
• The OmegaWhite Survey for Short-Period Variable Stars VII: High amplitude, short period blue variables
• Statistical Microlensing Toward Magnified High-Redshift Star Clusters
• Constraining Type Iax Supernova Progenitor Systems with Stellar Population Aging
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• Insights into the reionization epoch from cosmic-noon-CIV emitters in the VANDELS survey
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions
• A Comparison of Rotating and Binary Stellar Evolution Models: Effects on Massive Star Populations
• Photon leaking or very hard ionizing radiation? Unveiling the nature of heII-emitters using the softness diagram
• Late-time Hubble Space Telescope Observations of AT 2018cow. II. Evolution of a UV bright Underlying Source 2--4 Yr Post-discovery
• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
• Hitting the slopes: A spectroscopic view of UV continuum slopes of galaxies reveals a reddening at z > 9.5
• The impostor revealed: SN 2016jbu was a terminal explosion
• First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
• QSOFEED: The relationship between star formation and AGN Feedback
• Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE
• A Mixture of LBG Overdensities in the Fields of Three $6<z<7$ Quasars: Implications for the Robustness of Photometric Selection
• Signatures of inflowing gas in red geyser galaxies hosting radio-AGN
• SOFIA FIFI-LS Observations of Sgr B1: Ionization Structure and Sources of Excitation
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• Stellar populations and physical properties of starbursts in the Antennae galaxy from self-consistent modelling of MUSE spectra
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• Synthetic photometry of OB star clusters with stochastically sampled IMFs: analysis of models and HST observations
• Mergers of neutron stars and black holes with cores of giant stars: a population synthesis study
• Exploring Active Galactic Nuclei and Little Red Dots with the Obelisk simulation
• MEGARA-IFU detection of extended HeII4686 nebular emission in the central region of NGC1569 and its ionization budget
• Unveiling the Nature of SN 2011fh: a Young and Massive Star Gives Rise to a Luminous SN 2009ip-like Event
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• End-to-end study of the home and genealogy of the first binary neutron star merger
• Binary Fraction Indicators in Resolved Stellar Populations and Supernova Type Ratios
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• Ultra wide black-hole - neutron star binaries as a possible source for gravitational waves and short gamma ray bursts
• Scrutiny of a very young, metal-poor star-forming Lyα-emitter at z ~ 3.7
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• Panchromatic evolution of three luminous red novae: Forbidden hugs in pandemic times -- IV
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The White Dwarfs of the Old, Solar Metallicity Open Star Cluster Messier 67: Properties and Progenitors
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors
• The ionizing and heating power of ultraluminous X-ray sources under the geometrical beaming model
• The contribution of globular clusters to cosmic reionization
• The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
• A Nitrogen-Enhanced Metal-Poor star discovered in the globular cluster ESO280-SC06
• Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies
• The effects of binary stars on galaxies and metal-enriched gas during reionization
• A metallicity dependence on the occurrence of core-collapse supernovae
• Revisiting the progenitor of the low-luminosity type II-plateau supernova, SN 2008bk
• Extended high-ionization [MgIV] emission tracing widespread shocks in starbursts seen by JWST /NIRSpec
• Investigating the physical properties of galaxies in the Epoch of Reionization with MIRI/JWST spectroscopy
• A Study of Wolf-Rayet stars Formed via Chemically Homogeneous Evolution
• Dust attenuation in galaxies at cosmic dawn from the FirstLight simulations
• Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
• Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of Evolution
• SN 2024abfo: a partially stripped SN II from a yellow supergiant
• The mass distribution of stars stripped in binaries: The effect of metallicity
• The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
• Towards an understanding of long gamma-ray burst environments through circumstellar medium population synthesis predictions
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• FirstLight IV: Diversity in sub-L${}_{\ast }$ galaxies at cosmic dawn
• Wolf-Rayet galaxies in SDSS-IV MaNGA. II. Metallicity dependence of the high-mass slope of the stellar initial mass function
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• A systematic aging method I: HII regions D118 and D119 in NGC 300
• To be or not to be a black hole: detailed binary population models as a sanity check
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Impact of binary interaction on the evolution of blue supergiants
• Subaru narrow-band imaging search for Lyman continuum from galaxies at z>3 in the GOODS-N field
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• Observations and Spectral Modelling of the Narrow-Lined Type Ic SN 2017ein
• The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
• Sagittarius B1 -- A Patchwork of H II Regions and PhotoDissociation Regions
• An Orientation Bias in Observations of Submillimetre Galaxies
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Multi-wavelength observations of the Luminous Fast Blue Optical Transient AT2023fhn
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Photometric Classifications of Evolved Massive Stars: Preparing for the Era of Webb and Roman with Machine Learning
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Searching for the connection between ionizing-photon escape and the surface density of star formation at z~3
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations I: Unique Galaxy Morphologies in Imaging
• Unveiling the stellar origin of the Wolf-Rayet nebula NGC6888 through infrared observations
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Red Supergiants in the JWST Era. I: Near-IR Photometric Diagnostics
• Wolf-Rayet stars in the Antennae unveiled by MUSE
• New calibrations for estimating the N/O ratio in HII regions
• Ionising Feedback Effects on Star Formation in Globular Clusters with Multiple Stellar Populations
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• Wolf-Rayet stars in M81 using GTC/OSIRIS: 7 new detections, analysis and classification of the full sample
• pySTARBURST99: The Next Generation of STARBURST99
• On aging star clusters using red supergiants independent of the fraction of interacting binary stars
• HETDEX Public Source Catalog 1 -- Stacking 50K Lyman Alpha Emitters
• Newly Discovered Wolf-Rayet Stars in M31
• Extreme mass ratios and fast rotation in three massive binaries
• Stellar population synthesis models with a physically varying IMF
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• Phase-locked polarization by photospheric reflection in the semidetached eclipsing binary ${\mu }^1$ Sco
• Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
• SN 2020pvb: a Type IIn-P supernova with a precursor outburst
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• Physical Properties of the Host Galaxies of Ca-rich Transients
• New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Strong nebular HeII emission induced by He${}^{+}$ ionizing photons escaping through the clumpy winds of massive stars
• Ages and Masses of Star Clusters in M33: a Multi-wavelength Study
• JWST spectroscopic confirmation of the Cosmic Gems arc at z=9.625 -- Insights into the small scale structure of a post-burst system
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
• Peculiar Supernovae
• The Star-Forming Interstellar Medium of Lyman Break Galaxy Analogs
• Correlation of the rate of Type Ia supernovae with the parent galaxy properties: Light and shadows
• Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE. The diverse ionization mechanisms acting in low-mass starbursts
• Analytic approximations for massive close post-mass transfer binary systems
• BAT99-9 -- a WC4 Wolf-Rayet star with nitrogen emission: Evidence for binary evolution?
• A study of the F-giant star $\theta$ Scorpii A: a post-merger rapid rotator?
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• What can Gaussian Processes really tell us about supernova lightcurves? Consequences for Type II(b) morphologies and genealogies
• Gravitational wave spectral synthesis
• Surface chemical composition of single WNh stars
• Physical properties of strong 1 < z < 3 Balmer and Paschen lines emitters observed with JWST
• The Progenitor of the Vela Pulsar
• Applications of Stellar Population Synthesis in the Distant Universe
• Riroriro: Simulating gravitational waves and evaluating their detectability in Python
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• Exploring the mysterious high-ionization source powering [Ne V] in high-z analog SBS0335-052 E with JWST/MIRI
• Resolved galactic superwinds reconstructed around their host galaxies at z>3
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• A Runaway Giant in the Galactic Halo
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• A Cautionary Tale of LyC Escape Fraction Estimates from High Redshift Galaxies
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• VFTS 243 as predicted by the BPASS fiducial models
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Physical Origins of Outflowing Cold Clouds in Local Star-forming Dwarf Galaxies
• Dust Eddington Ratios for Star-Forming Galaxy Subregions
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• The softness diagram for MaNGA star-forming regions: diffuse ionized gas contamination or local HOLMES predominance?
• Don't believe the hype(r): The Yellow Supergiants of Westerlund 1
• He II Emission from Wolf-Rayet Stars as a Tool for Measuring Dust Reddening
• The fate of rotating massive stars across cosmic times
• On the star formation efficiencies and evolution of multiple stellar generations in Globular Clusters
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Observational Signatures of Carbon-Oxygen White Dwarf Merger Remnants
• Inferring the Distribution of the Ionising Photon Escape Fraction
• Unveiling the Cosmic Gems Arc at $z\sim 10$ with JWST NIRCam
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• The origins of low-luminosity supernovae: the case of SN 2016bkv
• Very massive stars at low metallicity: evolution, synthetic spectroscopy, and impact on the integrated light of starbursts
• NIHAO XXVII: Crossing the green valley
• New Methods of Identifying AGN in the Early Universe using Spectroscopy and Photometry in the JWST Era
• Observations of Ly$\alpha$ Emitters at High Redshift
• Lyman continuum leakage versus quenching with the James Webb Space Telescope: The spectral signatures of quenched star formation activity in reionization-epoch galaxies
• The infrared counterpart and proper motion of magnetar SGR0501+4516
• Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging
• Looking for nebular He II emission south of the multiple-massive star system, HD 5980
• Cosmic Variance and the Inhomogeneous UV Luminosity Function of Galaxies During Reionization
• Modelling the escape of Lyman Continuum photons from galaxies in the Epoch of Reionization
• Identifying type II quasars at intermediate redshift with few-shot learning photometric classification
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Flashlights: Prospects for constraining the Initial Mass Function around cosmic noon with caustic-crossing events
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
• GRB 241105A: A test case for GRB classification and rapid r-process nucleosynthesis channels
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• Massive stars dying alone: the remote environment of SN 2010jp and its associated late-time source
• New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling
• Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Everything that glitters is not gold: V1315 Cas is not a dormant black hole
• A Global Census of Metals in the Universe
• The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
• Radiation-driven dusty outflows from early galaxies
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• Star formation history of the post-collisional Cartwheel galaxy using Astrosat/UVIT FUV images
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• The role of triple evolution in the formation of LISA double white dwarfs
• The Epoch of Reionization in Warm Dark Matter Scenarios
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Addressing the [O III]/H\b{eta} Offset of Dwarf Galaxies in the RESOLVE Survey
• Modelling LAEs in the Epoch of Reionization with OBELISK
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a $z=3.6$ star-forming galaxy lensed into a near-Einstein Ring by a $z=1.258$ massive elliptical galaxy
• Gas excitation in galaxies and active galactic nuclei with He IIλ4686 and X-ray emission
• HeII emitters at cosmic noon and beyond. Characterising the HeII λ1640 emission with MUSE and JWST/NIRSpec
• Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• High-redshift AGN population in radiation-hydrodynamics simulations
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• Reconstructing EUV spectrum of star forming regions from millimeter recombination lines of HI, HeI, and HeII
• Probing the heating of the neutral atomic interstellar medium in the Dwarf Galaxy Survey through infrared cooling lines
• Binary neutron star merger offsets from their host galaxies II. Short-duration gamma-ray bursts
• Dust-UV offsets in high-redshift galaxies in the Cosmic Dawn III simulation
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Counting stars from the integrated spectra of galaxies
• Thorne-Żytkow Objects
• Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
• Distinguishing ram pressure from gravitational interactions: Applying the Size-Shape Difference method to real galaxies
• Galactic chimney sweeping: the effect of 'gradual' stellar feedback mechanisms on the evolution of dwarf galaxies
• On the Binary Nature of the Progenitor of SN2015ap: Insights from Its Light Curve and Spectral Evolution
• Extended Enriched Gas in a Multi-Galaxy Merger at Redshift 6.7
• Relation between spectral indices and binary fractions in GCs
• Gamma-Ray Absorption By The Cosmic Lyman Continuum From Star-forming Galaxies
• Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
• The THESAN project: environmental drivers of Local Group reionization
• Sengi: a small, fast, interactive viewer for spectral outputs from stellar population synthesis models
• REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization
• A Multiwavelength Classification and Study of Red Supergiant Candidates in NGC 6946
• MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z$\sim$2
• Stellar evolution through the Red Supergiant phase
• Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy formation and reionization
• MUSE IFU observations of galaxies hosting Tidal Disruption Events
• oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
• Comparing population synthesis models of compact double white dwarfs to electromagnetic observations
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
• Population Synthesis of Gravitational Wave Sources
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Investigation of [KSF2015] 1381-19L, a WC9-type star in the high extinction Galactic region
• Constraints on the galaxy formation models during epoch of reionization with high redshift observations
• Discovery of a 310-day Period from the Enshrouded Massive System NaSt1 (WR 122)
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• Interpreting Galaxy Properties with Improved Modelling
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~0 ECO volume-limited star-forming galaxy sample
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• Gravitational wave energy spectral density properties from BPASS Galactic binary population in the Milky Way galaxy
• Mass Transfer as an Explanation for the Lifetime-Travel Time Discrepancy in IT Librae
• On the Origins of "Hostless'' Supernovae: Testing the Faint-end Galaxy Luminosity Function and Supernova Progenitors with Events in Dwarf Galaxies
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Mapping the z>=5 SiIV Column Density Distribution onto the Galaxy Stellar Mass Function Using the Cumulative Absorption Cross Section
• POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization
• The Age of the R127 & R128 Clusters: Implications for the LBV
• Infrared view of the multiphase ISM in NGC 253 II. Modelling the ionised and neutral atomic gas
• Estimating Transient Rates from Cosmological Simulations and BPASS
• From simulations to observations. Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS
• Supernovae in colliding-wind binaries: observational signatures in the first year
• The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants
• Gravitational lensing of fast radio bursts: prospects for probing microlens populations in lensing galaxies
• Intergalactic Medium Tomography with the Sunburst Arc
• Locating Red Supergiants in the Galaxy NGC 6822
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Nebular abundance gradient in the Cartwheel galaxy using MUSE data
• Resolving white dwarf binaries within globular clusters with LISA
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• SN 2024hpj: A perspective on SN 2009ip-like events
• When Stars Mimic Monsters: Spectral Evidence for an $\eta$ Carinae-like Giant Eruption in SBS 0335$-$052 E
• Topological models to infer multiphase interstellar medium properties
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
• Implications of the cosmological 21-cm absorption profile for high-redshift star formation and deep JWST surveys
• Quantifying Systematic Age Discrepancies in Very Young Star Clusters
• Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons