News & Events

News

LOFAR Newsletter June 2026
LOFAR Newsletter February 2026
LOFAR Newsletter October 2025
LOFAR Newsletter March 2025
LOFAR Newsletter November 2024
LOFAR Newsletter August 2024

Events

[MEC id="167"]

Daily image

LOFAR2.0: upgrade of the first international station SE607.

© Lofar

The upgrade of SE607 started in April 20 with the decommissioning of LOFAR1 by the team at the Onsala Space Observatory (OSO), see https://www.astron.nl/dailyimage/main.php?date=20260501.

A first team from ASTRON: Steyn Hulshof and Xander Blaak, visited on April 28 to install the LOFAR2.0 station switches (data, network and control). The upgrade to the network connection from Onsala to Groningen to 10Gbs, was prepared in the months before.

On May 18, a second team from ASTRON: Henri Meulman, Sjouke Kuidersma, Ronald Schrik, and Scott Polotto, travelled to complete the station integration.

We were welcomed on the morning of Tuesday 19 by the Onsala colleagues. After and introductory meeting to get to know each other and discuss the plans for the week, and a well deserved coffee, we could start with the hard work. The LOFAR2.0 subracks and power supplies were installed and the installation of the coaxial cables began.

On Wednesday 20, the coaxial cables were finalized and floor panels were placed back into their position.

On Thursday 21, the station integration tests were completed and the installation finalized.

Constant support from the teams in Dwingeloo ensured the swift solution of any issues. Team Ruby, ICT, Observers, and Verification team worked well into the evenings to make sure the station was left in good condition by the end of the week.

Thanks to the good preparations done by the OSO team, the coordination between ASTRON and Onsala, the support from Dwingeloo, and the enthusiasm and commitment from the rollout team, the upgrade happened with no major problems.

Special thanks for the hospitality provided by Roger Hammargren, Henrik Olofsson and colleagues.

Overall, the upgrade of the first station was a good experience that gives further confidence to proceed. The Next station will be PL612.

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.
Speaker
Institute
Host
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.
Speaker
Institute
Host
NEWSLETTER

Subscribe to the LOFAR newsletter:

Subscribe

For previous editions, click here.

To view the current and previous editions of the LOFAR2.0 newsletter, click here.

@astron

SDC Helpdesk