Short-Author Papers
31.07.25: Hierarchical Triples vs. Globular Clusters: Binary black hole merger eccentricity distributions compete and evolve with redshift - A. Dorozsmai, I. M. Romero-Shaw, A. Vijaykumar, S. Toonen, F. Antonini, K. Kremer, M. Zevin, E. Grishin, submitted to MNRAS
25.07.25: Rapid stellar and binary population synthesis with COMPAS: methods paper II - I. Mandel et al. incl. I. M. Romero-Shaw, accepted for publication in ApJS
20.06.25: GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications - I. Romero-Shaw, J. Stegmann, H. Tagawa, D. Gerosa, J. Samsing, N. Gupte, S. R. Green, submitted to PRD
10.06.25: Inferring the pair-instability mass gap from gravitational wave data using flexible models - F. Antonini, T. Callister, F. Dosopoulou, I. M. Romero-Shaw, D. Chattopadhyay, submitted to PRD
19.05.25: Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements - J. Stegmann, D. Gerosa, I. M. Romero-Shaw, G. Fumagalli, H. Tagawa, L. Zwick, submitted to ApJL
29.04.25: Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope - F. Santoliquido et al. incl. I. M. Romero-Shaw, submitted to PRD
07.01.25: A Star Cluster Population of High Mass Black Hole Mergers in Gravitational Wave Data - F. Antonini, I. M. Romero-Shaw, T. Callister, published in PRL
09.09.24: Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes - G. Fumagalli, I. M. Romero-Shaw, D. Gerosa, V. De Renzis, K. Kritos, A. Olejak, published in PRD
03.09.24: Eccentric Signatures of Stellar-Mass Binary Black Holes with Circumbinary Disks in LISA - I. M. Romero-Shaw, S. Goorachurn, M. Siwek, C. J. Moore, published in MNRAS Letters.
14.08.24: Detecting gravitational-wave bursts from black hole binaries in the Galactic Center with LISA - A. Knee, J. McIver, S. Naoz, I. M. Romero-Shaw, B-M. Hoang, published in ApJL
24.07.24: Gravitational-wave data analysis with high-precision numerical relativity simulations of boson star mergers - T. Evstafyeva, U. Sperhake, I. M. Romero-Shaw, M. Agathos, accepted for publication in PRL
22.04.24: Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA - N. Gupte, A. Ramos-Buades, A. Buonanno, J. Gair, M. C. Miller, M. Dax, S. R. Green, M. Pürrer, J. Wildberger, J. Macke, I. M. Romero-Shaw, B. Schölkopf, submitted to ApJ
21.02.24: Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes - Divyajyoti, S. Kumar, S. Tibrewal, I. M. Romero-Shaw, C. K. Mishra, published in PRD
06.10.23: Binary black hole mergers in nuclear star clusters: eccentricities, spins, masses, and the growth of massive seeds -D. Chattopadhyay, J. Stegmann, F. Antonini, J. Barber, I. M. Romero-Shaw, published in MNRAS
05.07.23: Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution - I. M. Romero-Shaw, R. Hirai, A. Bahramian, R. Willcox, I.Mandel, published in MNRAS
08.06.23: Inferring Interference: Identifying a Perturbing Tertiary with Eccentric Gravitational Wave Burst Timing - I. M. Romero-Shaw, N. Loutrel, M. Zevin, published in PRD
11.01.23: Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data - I. M. Romero-Shaw, D. Gerosa, N. Loutrel, published in MNRAS
13.09.22: A Rosetta Stone for eccentric gravitational waveform models - A. M. Knee, I. M. Romero-Shaw, P. D. Lasky, J. McIver, E. Thrane, published in ApJ
07.07.22: Subtracting glitches from gravitational-wave detector data during the third observing run - D. Davis, T. B. Littenberg, I. M. Romero-Shaw, M. Millhouse, J. McIver, F. Di Renzo, G. Ashton, published in Classical and Quantum Gravity
29.06.22: Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically - I. M. Romero-Shaw, P. D. Lasky, E. Thrane, published in ApJ
28.06.22: Gravitational-wave inference for eccentric binaries: the argument of periapsis - T. A. Clarke, I. M. Romero-Shaw, P. D. Lasky, E. Thrane, published in MNRAS
08.06.22: When models fail: an introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy - I. M. Romero-Shaw, E. Thrane, P. Lasky. Published in PASA
05.11.21: Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes - I. M. Romero-Shaw, P. Lasky, E. Thrane, published in ApJ Letters
11.11.21: Implications of Eccentric Observations on Binary Black Hole Formation Channels - M. Zevin, I. M. Romero-Shaw, K. Kremer, E. Thrane, P. Lasky, published in ApJ Letters
02.07.21: Gravitational Waves as a Probe of Globular Cluster Formation and Evolution - I. M. Romero-Shaw, K. Kremer, P. D. Lasky, E. Thrane, J. Samsing, published in MNRAS
23.10.20: GW190521: Orbital Eccentricity and Signatures of Dynamical Formation in a Binary Black Hole Merger Signal - I. M. Romero-Shaw, P. D. Lasky, E. Thrane, J. Calderon Bustillo, published in ApJ Letters
21.09.20: Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO-Virgo gravitational-wave transient catalogue - I. M. Romero-Shaw, C. Talbot, S. Biscoveanu, V. D'Emilio, G. Ashton et al., published in MNRAS
11.05.20: On the Origin of GW190425 - I. M. Romero-Shaw, N. Farrow, S. Stevenson, E. Thrane, X-J. Zhu, published in MNRAS Letters
12.09.19: Searching for Eccentricity: Signatures of Dynamical Formation in the First Gravitational-Wave Transient Catalogue of LIGO and Virgo - I. M. Romero-Shaw, P. D. Lasky, E. Thrane, published in MNRAS
Posts
Research outline
I am a Postdoctoral Research Fellow at the University of Bristol. Previously, I was the Herchel Smith Fellow at the Department of Applied Mathematics and Theoretical Physics at the University of Cambridge. I'm interested in things that go bump in the fabric of space-time (aka, black holes crashing together). I am working to answer the question of how black holes and neutron stars find each other and collide, producing the space-time ripples that we observe with detectors like LIGO and Virgo. I did my PhD at Monash University in Melbourne, Australia. My PhD supervisors were Associate Professor Paul Lasky and Professor Eric Thrane. I'm an alumnus of the OzGrav organisation and a member of the LIGO Scientific Collaboration.
In both my PhD thesis and my current work, I focus primarily on things to do with the dynamical assembly of binary black hole systems. I am particularly interested in different dynamical formation environments, such as globular clusters, AGN disks, and nuclear clusters.
The parameters of a binary leave an imprint on their gravitational-wave signal, and these can give us clues to how the binary formed. Sometimes, in dynamical environments, binaries can retain significant orbital eccentricity just before they merge; this leaves its mark on the gravitational-wave signal that we detect. Along with component masses, spins and redshift evolution, eccentricity can tell us about the way that a compact object binary formed. This video is a great illustration of a three-body interaction causing a highly eccentric binary.
I was involved in developing bilby, a modular Python library facilitating Bayesian inference, optimised for gravitational wave science.
I completed my MSci in Physics at Birmingham University in the UK. I did my Master's project with Professor Andreas Freise, using Python code to model the noise at gravitational wave detectors. I helped to develop Space Py Quest, a Python code that lets you simulate your own gravitational wave detections! Its more glamorous older sister is Space Time Quest, a game with lovely graphics that lets you build and run your own detector without touching the code.
During my time at the University of Birmingham, I worked with Professor Ilya Mandel as a summer student. I worked on comparing different methods of evolving virtual stars within COMPAS, a code that simulates and analyses stellar evolution in order to work out how LIGO’s observed binaries formed. Recently, I worked with Ilya and the COMPAS team to answer another formation mystery: how X-ray binaries are made.
If you’d like to have a chat about any of the above, please get in touch!