News & Events

News

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

Events

[MEC id="167"]

Daily image

Dwingeloo telescope 70 years

© Nationaal Archief / Tammo Jan Dijkema

"Majesteit, wilt u op deze knop drukken?" "Majesty, would you press this button please?" With these words, Professor Oort asked Her Majesty Queen Juliana to open the Dwingeloo telescope on 17 April 1956, exactly 70 years ago today.

The button that played a central role in the opening ceremony recently returned to the telescope, when a former ASTRON employee brought it back. He had taken it home in the 1990s, when it would otherwise have been discarded during a round of cleaning. The button is now kept in the ‘museum’ of CAMRAS, together with other historical artefacts.

The button bears the name of HEMAF (“Hengelosche Electrische en Mechanische Apparaten Fabriek”), a company from Hengelo that supplied a large part of the electrical installation of the Dwingeloo telescope.

CAMRAS celebrated the 70th anniversary of the telescope and the 75th anniversary of the first detection of the hydrogen line with a seminar on amateur observing of the 21 cm line.

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