Grant number: 109266 | Funding period: 2024 - 2031
Active
M Curyło, A Zic, S Wang, E Thrane, PD Lasky, JC Tremblay, ZC Chen, S Dai, VD Marco, G Hobbs, A Kapur, W Ling, ME Lower, RF Mandow, S Mishra, DJ Reardon, CJ Russell, RM Shannon, XJ Zhu
2026-07-01
Pulsar timing is used for a variety of applications including tests of fundamental physics, probing the structure of neutron stars..
Xiao-Song Hu, Siyuan Chen, Kuo Liu, Xingjiang Zhu, Shi-Yi Zhao, Wu Jiang, John Antoniadis, ND Ramesh Bhat, Amodio Carleo, Shi Dai, Valentina Di Marco, Huanchen Hu, Wenhua Ling, Yang Liu, Saurav Mishra, Christopher J Russell, Ryan M Shannon, Clemente Smarra, Jingbo Wang, Lin Wang
2026-06-08
The cold dark matter model successfully describes the Universe on large scales, yet faces challenges at subgalactic scales. Ultral..
R Brunet, A Melatos, PHB Rossetto
2026-05-01
Hydromagnetic instabilities modify the structure of a magnetically confined mountain on an accreting neutron star, once the accret..
D Farias, C Gall, VA Villar, K Auchettl, KM de Soto, A Gagliano, WB Hoogendam, G Narayan, A Sedgewick, SK Yadavalli, Y Zenati, CR Angus, KW Davis, J Hjorth, WV Jacobson-Galán, DO Jones, CD Kilpatrick, MJ Bustamante Rosell, DA Coulter, G Dimitriadis
2026-04-01
<jats:p> <jats:italic>Context</jats:italic> . Type Ibn supernovae (SNe) are characterized ..
N Van Bemmel, J Zhang, J Cooke, A Möller, AW Shafter, I Andreoni, K Auchettl, D Buckley, J Carney, D Dobie, J Freeburn, B Gendre, V Kansal, I Monageng, A Rau, N Rawat, M Suhr, EN Taylor
2026-03-01
In the first observational run of the Kilonova and Transients Programme (KNTraP), a rapidly evolving optical transient, KNTraP2022..
J Cardinal Tremblay, B Goncharov, R Van Haasteren, NDR Bhat, ZC Chen, V Di Marco, S Iguchi, A Kapur, W Ling, R Mandow, S Mishra, DJ Reardon, RM Shannon, H Sudou, J Wang, SY Zhao, XJ Zhu, A Zic
2026-02-20
A subparsec supermassive black hole binary (SMBHB) at the center of the galaxy 3C 66B is a promising candidate for continuous grav..
G Teixeira, CD Kilpatrick, CR Bom, A Santos, P Darc, K Auchettl, Á Álvarez-Candal, RJ Foley, PK Humire, AL Piro, C Rojas-Bravo, C Mendes de Oliveira, A Kanaan, T Ribeiro, W Schoenell
2026-02-10
<jats:title>Abstract</jats:title> <jats:p> We present ultraviolet, optical, and infrared obs..
W Dong, A Melatos, NJ O'Neill, PM Meyers, DK Boek
2026-02-01
Crust-superfluid coupling plays an important role in neutron star rotation, particularly with respect to timing noise and glitches..
JH Gillanders, ME Huber, M Nicholl, SJ Smartt, KW Smith, KC Chambers, DR Young, JW Tweddle, S Srivastav, MD Fulton, F Stoppa, GSH Paek, A Aamer, MR Alarcon, A Andersson, A Aryan, K Auchettl, TW Chen, T de Boer, AKH Kong
2025-12-10
Kilonovae are the scientifically rich—but observationally elusive—optical transient phenomena associated with compact binary merge..
WV Jacobson-Galán, L Dessart, CD Kilpatrick, PJ Patel, K Auchettl, S Tinyanont, R Margutti, VV Dwarkadas, KA Bostroem, R Chornock, RJ Foley, H Abunemeh, T Ahumada, P Arunachalam, MJ Bustamante-Rosell, DA Coulter, C Gall, H Gao, X Guo, DO Jones
2025-11-20
We present multiwavelength observations of the Type II supernova (SN II) 2023ixf during its first 2 yr of evolution. We combine gr..
T Cheunchitra, A Melatos, RL Webster
The luminosity distance–redshift (D <inf>L</inf>–z) relation derived from Type Ia supernovae (SNe Ia) yields evidence for a nonzer..
K Medler, C Ashall, P Hoeflich, E Baron, JM DerKacy, M Shahbandeh, T Mera, CM Pfeffer, WB Hoogendam, DO Jones, S Shiber, E Fereidouni, OD Fox, J Jencson, L Galbany, JT Hinkle, MA Tucker, BJ Shappee, ME Huber, K Auchettl
2025-11-10
We present the nebular phase spectroscopic and photometric observations of the nearby hydrogen-rich core-collapse supernova (CCSN)..
YSC Lee, MJ Szczepańczyk, T Mishra, M Millhouse, A Melatos
2025-10-30
Gravitational-wave (GW) emissions from core-collapse supernovae (CCSNe) provide insights into the internal processes leading up to..
SY Zhao, ZC Chen, JC Tremblay, B Goncharov, XJ Zhu, NDR Bhat, M Curyło, S Dai, V Di Marco, H Ding, G Hobbs, A Kapur, W Ling, T Liu, R Mandow, S Mishra, DJ Reardon, CJ Russell, RM Shannon, S Wang
2025-10-20
We present results from an all-sky search for continuous gravitational waves from individual supermassive binary black holes using..
Y Bu, A Melatos, R Evans
2025-10-01
The rising use of educational tools controlled by artificial intelligence (AI) has provoked a debate about their proficiency. Whil..
B Larsen, CMF Mingarelli, PT Baker, JS Hazboun, S Chen, L Schult, SR Taylor, J Simon, J Antoniadis, J Baier, RN Caballero, A Chalumeau, Z Chen, I Cognard, D Deb, V Di Marco, T Dolch, IO Eya, EC Ferrara, KA Gersbach
The International Pulsar Timing Array (IPTA)'s second data release (IPTA DR2) combines decades of observations of 65 millisecond p..
V Di Marco, A Zic, RM Shannon, E Thrane, AD Kulkarni
2025-09-01
Accurately estimating the parameters of the nanohertz gravitational-wave background is essential for understanding its origin. The..
J Horstman, A Melatos, F Farokhi
An individual's opinion concerning political bias in the media is shaped by exogenous factors (independent analysis of media outpu..
A Gagliano, VA Villar, T Matsumoto, DO Jones, CL Ransome, AE Nugent, D Hiramatsu, K Auchettl, D Tsuna, Y Dong, S Gomez, PD Aleo, CR Angus, T de Boer, KA Bostroem, KC Chambers, DA Coulter, KW Davis, JR Fairlamb, J Farah
2025-08-20
We present ultraviolet to infrared observations of the extraordinary Type IIn supernova 2023zkd (SN 2023zkd). Photometrically, it ..
L Dunn, C Flynn, M Bailes, YSC Lee, G Howitt, A Melatos, V Gupta, A Mandlik, A Deller
2025-08-01
The UTMOST-NS pulsar timing programme operated at the Molonglo Observatory Synthesis Telescope from 2021 April to 2023 June, obser..
N Rehemtulla, WV Jacobson-Galán, A Singh, AA Miller, CD Kilpatrick, KR Hinds, C Liu, S Schulze, J Sollerman, T Jegou du Laz, T Ahumada, K Auchettl, SJ Brennan, MW Coughlin, C Fremling, A Gangopadhyay, DA Perley, NZ Prusinski, J Purdum, YJ Qin
2025-06-01
We present observations of the Type IIP supernova (SN) SN 2024jlf, including spectroscopy beginning just 0.7 days (∼17 hr) after f..
L Dunn, A Melatos, P Clearwater, S Suvorova, L Sun, W Moran, RJ Evans
2025-04-15
A search is performed for continuous gravitational waves emitted by unknown neutron stars in five nearby globular clusters using d..
YSC Lee, S Doshi, M Millhouse, A Melatos
2025-04-01
Einstein's theory of general relativity predicts that gravitational waves (GWs) are tensor-polarized, with two modes of polarizati..
N Van Bemmel, J Zhang, J Cooke, A Rest, A Möller, I Andreoni, K Auchettl, D Dobie, B Gendre, S Goode, J Freeburn, DO Jones, CD Kilpatrick, A Lien, A Rau, L Spitler, M Suhr, F Valdes
2025-03-01
Compact binary mergers detectable in gravitational waves can be accompanied by a kilonova, an electromagnetic transient powered by..
Y Xia, J Wang, S Kuroyanagi, W Yan, Y Wen, A Kapur, J Zou, Y Feng, V Di Marco, S Mishra, CJ Russell, S Wang, D Zhao, X Zhu
Pulsar timing arrays (PTAs) are designed to detect nanohertz-frequency gravitational waves (GWs). Since GWs are anticipated from c..
W Dong, A Melatos
2025-02-01
r-mode oscillations in rotating neutron stars are a source of continuous gravitational radiation. We investigate the excitation of..
J Freeburn, B O’Connor, J Cooke, D Dobie, A Möller, N Tejos, J Zhang, P Beniamini, K Auchettl, J DeLaunay, S Dichiara, WF Fong, S Goode, A Gordon, CD Kilpatrick, A Lien, C Mihalenko, G Ryan, K Siellez, M Suhr
GRB 220831A is a gamma-ray burst (GRB) with a duration and spectral peak energy that places it at the interface between the distri..
D Dobie, A Zic, LS Oswald, J Pritchard, ME Lower, Z Wang, H Qiu, N Hurley-Walker, Y Wang, E Lenc, DL Kaplan, A Anumarlapudi, K Auchettl, M Bailes, AD Cameron, J Cooke, A Deller, LN Driessen, J Freeburn, T Murphy
2024-11-01
Several sources of repeating coherent bursts of radio emission with periods of many minutes have now been reported in the literatu..