SIGNAL ACTIVE · ASTRON · NANOHERTZ GW PROGRAMME · ONLINE
MJD —
Aditya Parthasarathy Staff Scientist · ASTRON

Hearing the universe in the
quiet ticking of distant stars.

I lead a research group at ASTRON, the Netherlands Institute for Radio Astronomy. We work on nanohertz gravitational wave science, design the next generation of radio‑astronomy instruments, and build the pipelines that turn petabytes of telescope data into physics. Pulsars sit at the centre of all of it, as the most precise clocks in the Universe.

Peer-reviewed
82papers
Total citations
~12kADS
Group funding
€2MERC + Veni
First GWB evidence
2023EPTA DR2
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§ 01 / About

A research programme at ASTRON.

Nanohertz gravitational waves, the instruments that detect them, and the algorithms and pipelines that make sense of the data in between.

I lead the only research group in the Netherlands working on nanohertz gravitational wave astrophysics, based at ASTRON. The programme is supported by over €2M in competitive funding from a European Research Council Starting Grant (project GIGA) together with an NWO-I Veni fellowship.

Our work rests on two main pillars. The first is gravitational wave science. I co-led the European PTA noise analysis that contributed to the first compelling evidence for the gravitational wave background in 2023, work that was recognised with the Frontiers of Science Award and the RAS Group Achievement Award. Research in our group also includes EPTA noise modelling, Gamma-ray PTA methodologies and science, young pulsar timing and ISM modelling.

The second pillar is algorithms and instrumentation. I commissioned MeerKAT’s pulsar timing backend in South Africa and co-founded the Gamma-ray Pulsar Timing Array with M. Kerr, which remains the only independent path to the gravitational wave background outside of radio. I also co-lead a novel phased-array feed design in collaboration with Breakthrough Listen, and a proposal to upgrade the Westerbork dishes into a national radio astronomy facility.

Read more about the programme on the GIGA group page or see the full CV.

§ 02 / Group

The GIGA group at ASTRON.

Gravitational-wave Inference from Gamma-rays and the Array.

We lead research at the frontier of nanohertz gravitational wave science, combining PTA noise modelling , young pulsar timing, and ISM modelling to push the sensitivity of pulsar timing arrays. The group is supported by the GIGA compute cluster at ASTRON, dedicated to large-scale pulsar timing inference.

2 + 2 + 2
postdocs · PhDs · MSc
€2M+
ERC Starting Grant + Veni
5M+
SURF compute hours (2y)
Visit the GIGA group page
§ 03 / Recent

Recent news.

Selected milestones, awards, and new programmes from the last few years.
2026
Organising a Lorentz Center workshop on pulsar science with modern interferometers. Fully funded, international.
2025 · May
RAS Group Achievement Award to the EPTA for the first evidence of the nanohertz gravitational wave background.
2025
Invited talks at Beyond the Earth and CASPER 2025 on a prototype phased-array feed built with Breakthrough Listen and ASTRON.
2025
Co-leading an infrastructure proposal to upgrade the Westerbork dishes into a national radio astronomy facility.
2024 · Oct
Frontiers of Science Award for the EPTA DR2 series on the gravitational wave background.
2024
Elected to the EPTA Steering Committee (5 members), youngest to represent the IPTA SC for Europe.
2024
Awarded a Dutch Supercomputing (SURF) grant providing more than 5M compute hours over two years.
2023 · Sep
Joined ASTRON as Staff Scientist on a permanent contract. Also awarded the €1.7M ERC Starting Grant (GIGA) to establish the group.
2023 · Jul
EPTA reports the first compelling evidence of the nanohertz gravitational wave background. I co-led the noise analysis underpinning the result.
2022 · Jun
Science paper on the Gamma-ray Pulsar Timing Array, co-founded with M. Kerr. It remains the only independent path to the gravitational wave background outside of radio.
2022
Awarded the NWO-I Veni Fellowship (€300k) on pulsar timing methods.
§ 04 / Signature

The Nanohertz Sky.

A placeholder for more context on the Hellings–Downs curve and what the spectrum of the gravitational wave background tells us. More coming soon.
HELLINGS–DOWNS · PTA CORRELATION
90° 180° PULSAR PAIR SEPARATION +0.5 0 −0.25

A fingerprint in the sky.

Gravitational waves passing through the galaxy leave a very specific pattern in pulsar timing data: pairs of pulsars close together in the sky are correlated, pairs ninety degrees apart are anti-correlated, and opposite pairs are correlated again.

This shape — the Hellings–Downs curve — cannot be faked by noise, solar-system uncertainties, or interstellar scattering. Finding it in our data is how we know the signal is real.

The points above are sketched from the EPTA DR2 analysis; error bars are illustrative.

§ 05 / Catalogue

Selected publications.

82 peer-reviewed papers across MNRAS, A&A, Science, Nature Astronomy, ApJ, ApJL, Phys. Rev. D, Phys. Rev. Lett., and PASA, published between 2017 and 2026.
82
peer-reviewed papers
~12k
total citations
2,400+
citations, EPTA DR2 II alone
20
additional Astronomer's Telegrams
2017–'26
publication span

Highlighted

07 narrative papers · first-author · co-led · collaboration-led
H/01
The second data release from the European Pulsar Timing Array. II. Customised pulsar noise models for spatially correlated gravitational waves
EPTA Collaboration, InPTA Collaboration · A. Parthasarathy co-led the noise-analysis team (~30 researchers) · A&A 678, A49 (2023)
This paper lays out the noise-modelling framework that underpins the entire EPTA DR2 series, which together presented the first compelling evidence for the nanohertz gravitational wave background. It has accumulated over 2,400 citations and was recognised with the Frontiers of Science Award (2024/25) and the RAS Group Achievement Award (2024/25).
H/02
A gamma-ray pulsar timing array constrains the nanohertz gravitational wave background
Fermi-LAT Collaboration · M. Kerr & A. Parthasarathy as co-founders of the GPTA · Science 376, 521–523 (2022)
This work repurposed NASA's Fermi telescope as the only independent means of characterising the gravitational wave background spectrum outside of radio. Gamma-ray photons sidestep the interstellar medium entirely, and overlapping pulsars in both bands give a unique lever arm for isolating spin noise and the ISM models used by radio PTAs.
H/03
Measurements of pulse jitter and single-pulse variability in millisecond pulsars using MeerKAT
A. Parthasarathy, M. Bailes, R. M. Shannon, W. van Straten, S. Oslowski, et al. · MNRAS 502, 407–422 (2021)
This paper established MeerKAT as a premier pulsar timing instrument. I led the commissioning of the pulsar timing backend and built meerpipe, the primary timing pipeline, which has processed over 30,000 observations of roughly 1,500 pulsars to date. The paper reports high-precision timing for more than 20 millisecond pulsars, including the most precisely timed pulsar ever observed, at better than 5 ns.
H/04
Combining the second data release of the European Pulsar Timing Array with low-frequency pulsar data
F. Iraci, A. Chalumeau … A. Parthasarathy, et al. · A&A 704, A109 (2025)
Co-led by a postdoc in my group, this paper shows that adding LOFAR low-frequency data sharpens dispersion-measure tracking, isolates plasma propagation effects, and exposes solar-wind biases. It provides direct observational evidence that multi-frequency PTAs are more sensitive to the gravitational wave background, and reflects the group's growing leadership on IPTA noise modelling and combined-data analyses.
H/05
Bow shock and Local Bubble plasma unveiled by the scintillating millisecond pulsar J0437−4715
D. J. Reardon, R. Main, S. K. Ocker … A. Parthasarathy, et al. · Nature Astronomy 9, 1053–1063 (2025)
This study resolves 25 distinct plasma structures along the line of sight to PSR J0437−4715 with MeerKAT. It reveals a bow shock within 5,000 AU of the pulsar and unexpectedly turbulent structure inside the Local Bubble. The results directly inform the noise-modelling strategy at the heart of the group's programme.
H/06
The second data release from the European Pulsar Timing Array. I. The dataset and timing analysis
EPTA Collaboration · J. Antoniadis, S. Babak, A.-S. Bak Nielsen, C. G. Bassa, … A. Parthasarathy, et al. · A&A 678, A48 (2023)
Companion paper to H/01. It presents the 24.7-year EPTA DR2 dataset and timing analysis that made the gravitational wave background evidence possible.
H/07
The second data release from the European Pulsar Timing Array. III. Search for gravitational wave signals
EPTA Collaboration, InPTA Collaboration · J. Antoniadis, P. Arumugam, S. Arumugam, … A. Parthasarathy, et al. · A&A 678, A50 (2023)
Companion paper to H/01. It reports the gravitational wave background search itself, with evidence at the 3 to 4 sigma level consistent with a Hellings–Downs correlation.

Full list, chronological

all 82 peer-reviewed papers
Full list on ADS
§ 06 / Hail
If you have a pulsar, a paper, or an idea worth timing, send a signal.
ASTRON · The Netherlands Institute for Radio Astronomy
aparthas3112.github.io