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Events

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European Pulsar Timing Array Wins Two Prestigious Awards

© EPTA

The European Pulsar Timing Array (EPTA) has received two prestigious awards: the 2024 International Congress of Basic Sciences (ICBS) Frontiers of Science Award in China and the 2025 Royal Astronomical Society (RAS) Group Achievement Award in the UK. These honours recognise the team's innovative work in gravitational wave astronomy through pulsar timing. The EPTA is a collaboration between scientists from over ten European institutions, including ASTRON with its Westerbork Synthesis Radio Telescope.

"These awards highlight the dedication of the entire EPTA team. Our work has the potential to transform our understanding of black holes and spacetime, and this recognition motivates us to continue advancing gravitational wave science," says Aditya Parthasarathy, Lead Researcher and EPTA and IPTA Steering Committee member.

The EPTA project, part of the International Pulsar Timing Array (IPTA), uses millisecond pulsars to detect nanoHertz gravitational waves--spacetime ripples caused by massive cosmic events. The ICBS award, shared with other international pulsar timing array collaborations, recognised their pioneering approach to detecting low-frequency gravitational waves that traditional detectors cannot observe.

The RAS Group Achievement Award acknowledged the EPTA's exceptional contributions to pulsar timing and gravitational wave astronomy. "We are excited to continue our work on pulsar timing and gravitational waves and strengthen our first detection," says Gemma Janssen, ASTRON scientist and EPTA steering committee member. ASTRON's contribution to the EPTA was carried out by Gemma Janssen, Aditya Parthasarathy, Emma van der Wateren, Aurélien Chalumeau, and Cees Bassa.

Colloquia

May 1, 2022

The Commensal Radio Astronomy FAST Survey (CRAFTS)

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has released its first call for proposal and will be open to the international community next year. Based on a novel technique of high-cadence CAL injection, we have realized the world's first calibrated commensal survey mode, simultaneously taking data for pulsar search, HI galaxies, HI imaging, and FRBs. I introduce here one of the major survey plans, namely, the Commensal Radio Astronomy FAST Survey (CRAFTS, Li et al. 2018), which has discovered more than 100 new pulsars, including a few dozen MSPs, 5 new FRBs, including one new repeater. I will also briefly describe recent FAST results from CRAFTS and other dedicated programs, including new insights into the characteristic energy of FRBs, the formation process of neutron stars, the evolution of interstellar medium, etc.
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May 14, 2022

Extreme UV Emission: Bridging Galaxy Evolution Across Cosmic Time

In the last few years, our first glimpse of the spectral properties of z∼5−7 galaxies has emerged. Deep UV spectra have revealed prominent high-ionization nebular emission lines (i.e., C IV, He II, C III]) indicating that extreme radiation fields may be characteristic of reionization-era systems. While such strong high-ionization emission lines are atypical of the well-studied z∼0−3 galaxy samples, our recent UV spectral campaigns have revealed several galaxies with analogous emission-line features to reionization-era systems. I will discuss the recent detection of extremely strong UV emission in nearby galaxies and the potential sources of their very hard ionizing radiation fields. Such strong detections of high-ionization emission lines have been linked to the leakage of Lyman continuum (LyC) photons (necessary for reionization) both theoretically and observationally. These extreme UV emission-line dwarf galaxies provide a template for the extreme conditions that are important for reionization, however their features are still poorly understood. In preparation for the coming UV window onto the early universe with the advent of ELTs and JWST, I will introduce the COS Legacy Archival Spectroscopic SurveY - an upcoming large HST program designed to disentangle the stellar and nebular spectral signatures of 45 star-forming galaxies. This program will calibrate new UV diagnostics that will allow us to trace galaxy evolution to the distant universe, unveiling the properties of reionization-era galaxies.
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