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Events

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2nd year research practicum at UvA and ASTRON

© Ziggy Pleunis/ASTRON

Last week four 2nd-year University of Amsterdam BSc students in physics & astronomy, Dominique, Dunya, Duran and Jua, visited ASTRON for three days as part of a one-week research project. While at ASTRON, the students enjoyed an engaging tour and observing session with the Dwingeloo Radio Telescope thanks to Tammo Jan Dijkema, a tour of the Westerbork Synthesis Radio Telesope, a wonderful tour of the R&D labs by Mark Ruiter and of course a pannenkoek at the Bospub.

For their project the students measured the spin period of the first pulsar discovered by Jocelyn Bell-Burnell, B1919+21, in LOFAR data. They also analyzed a series of LOFAR observations of pulsar J1810+1744, a source discovered by Jason Hessels, and rediscovered that this pulsar is in an eclipsing binary system. They were able to estimate the mass of the pulsar's binary companion based on the changes in the pulsar spin period over time, from the Doppler shift induced by the binary orbit, and they observed how the free electron density in the line of sight towards the pulsar changes around the eclipse.

The students left with a good understanding of all it takes to design, build and operate a radio telescope and felt the joy of discovery when observations show something unexpected. Thank you to everyone at ASTRON for making the students feel welcome and hopefully we'll see some of them again soon for another research project in radio astronomy!

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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