News & Events

News

LOFAR Newsletter March 2025
LOFAR Newsletter November 2024
LOFAR Newsletter August 2024
LOFAR Newsletter May 2024
LOFAR Newsletter January 2024
Retirement of Early LOFAR Cycle data (Cycle 0 to Cycle 6)

Events

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Enhancing the Value and Sustainability of LOFAR Science Archive

© LDV team

The LOFAR Data Valorisation (LDV) project aims to give added value to LOFAR archived data in the Long Term Archive (LTA) by offering users well curated, science-ready data. It also paves the way for LOFAR2.0 operations because it streamlines data processing operations at the LTA sites (currently Surf, Juelich and PSNC) and ensure sustainability of science operations by reducing data volume at the LTA, thereby also lowering the operational costs.

LDV is reaching the conclusion of its first phase of operations at Surf. The storage occupancy was reduced by 7.5 PB through resampling of beam formed data, compression of interferometric data and a large data placement action. This gain in storage translates in a saving of about 56 kEuro/yr. Curation of data enabled the removal of duplicates and the addition of quality flags. Currently, preparations are ongoing to perform a major retirement action (~9.5 PB distributed over the three LTA sites) of the early cycles (0-6) archived data with no legacy value.

The next operational aim at Surf is the generation of higher level data products by running the LOFAR Initial Calibration (LINC) pipeline on a significant portion of the archived data. For the first time, calibrated visibilities through the observatory processing framework with latest workflows will be offered to the astronomical community.

Furthermore efforts are ongoing to extend the processing framework infrastructure at the Juelich LTA site, for enabling the next round of data editing operations with an expected duration of 1 year. As a result more than 4 PB of tape storage space will be gained. Looking ahead, the LDV processing infrastructure will be expanded to support the LOFAR2.0 MPS operations, marking a key step toward future-ready science operations.

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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