177 citations · 265 across the 10 of their papers we have counts for
12 papers
The Equivalent Width as an Ionization-Parameter Diagnostic Across Cosmic Time
Dian P. Triani, Lisa J. Kewley
Nebular emission lines and stellar continua probe the conditions of regions. The optical emission line is important because it is observab…
KiDS-DR5: Exploring dust transport in dark matter halos of galaxies
Eray Genc, Angus H. Wright, Hendrik Hildebrandt +12
We analyse a well-defined sample of galaxies from the final data release of the Kilo-Degree Survey (KiDS-DR5), selected using magnitude, photometric redshift, and stellar mass cuts…
Interplay of Compaction, Quenching, and Black Hole Growth in the Most Massive Galaxies since : Insights from JWST and Chandra Data
Novan Saputra Haryana, Masayuki Akiyama, Abdurro'uf +16
The buildup of dense stellar cores is expected to mark an important transition in the star-formation and black-hole growth of massive galaxies. Using spatially resolved spectral en…
The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe
A. Mailvaganam, T. Zafar, P. Corcho-Caballero +39
We study the spatially resolved relation between dust attenuation () and star formation rate surface density () in galaxies from the MAGPI survey ($0.25 < z…
The significant contribution of supersoft X-ray Sources to the nebular HeII line emission
Dian P. Triani, Rosanne Di Stefano, Tiger Yu-yang Hsiao +1
Nebular spectral lines provide insight into the properties of the interstellar medium (ISM) and the ionizing radiation within galaxies. The presence of high-energy ionization lines…
Observational Signatures of AGN Feedback in the Morphology and the Ionization States of Milky Way-like Galaxies
Nadia Qutob, Razieh Emami, Kung-Yi Su +24
We make an in-depth analysis of different AGN jet models' signatures, inducing quiescence in galaxies with a halo mass of . Three jet models, including cosmic ray-…
Dust contribution to the panchromatic galaxy emission
Dian P. Triani, Darren J. Croton, Manodeep Sinha +3
We have developed a pipeline called \mentari to generate the far-ultraviolet to far-infrared spectral energy distribution (SED) of galaxies from the \dustysage semi-analytic galaxy…
The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher +52
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy…
Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
Geray S. Karademir, Edward N. Taylor, Chris Blake +3
We develop a framework for using clustering-based redshift inference (cluster-) to measure the evolving galaxy luminosity function (GLF) and galaxy stellar mass function (GSMF)…
Exploring the relation between dust mass and galaxy properties using Dusty SAGE
Dian P. Triani, Manodeep Sinha, Darren J. Croton +2
We explore the relation between dust and several fundamental properties of simulated galaxies using the Dusty SAGE semi-analytic model. In addition to tracing the standard galaxy p…
Mentari: A pipeline to model the galaxy SED using semi analytic models
Dian Triani, Darren Croton, Manodeep Sinha
We build a theoretical picture of how the light from galaxies evolves across cosmic time. In particular, we predict the evolution of the galaxy spectral energy distribution (SED) b…
The origin of dust in galaxies across cosmic time
Dian P. Triani, Manodeep Sinha, Darren J. Croton +2
We study the dust evolution in galaxies by implementing a detailed dust prescription in the SAGE semi-analytical model for galaxy formation. The new model, called Dusty SAGE, follo…