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Daily image

LOFAR data compression using Sisco

© Creative Commons

LOFAR produces enormous data sets. During calibration, it may be necessary to create several instances of the same data set: these are forward-predicted (model) data that allow direction-dependent calibration.

We've been compressing LOFAR data with Dysco compression to reduce the volume for archive and transfer, but it turns out that Dysco is not efficient for forward-predicted model data. This is because model data has different properties compared to the original data: it is smooth and noiseless. Therefore, we developed a novel compression framework called 'Sisco' (Simulated Signal Compression), that aims to compress model data. Unlike Dysco, compression is lossless, and compression ratios of nearly a factor of 8 can be reached on LOFAR data.

Sisco is somewhat similar to the FLAC compression that is used for compressing music or audio: it tries to estimate the next value based on the previous value, and uses efficient encoding for storing the residual. FLAC does this in one dimension (time), but Sisco extends this to two dimensions (time-frequency). Quite some effort went into applying this on standard measurement set ordering and integrating this into the Casacore I/O library, with the final result that the method can be applied transparently to our data, thereby reducing the intermediate I/O considerably.

The image shows compression results on MeerKAT (left) and LOFAR data (right), using various prediction methods to determine the most efficient ones. The method was accepted for publication in A&A: Offringa & Van Weeren (2026), https://arxiv.org/abs/2512.23490 .

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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Institute
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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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