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European observatories and administrations in dialogue on satellite interference

© Emma van der Wateren

On Friday 23 January, ASTRON hosted a meeting at the Paris Observatory, led by ASTRON Director Jessica Dempsey and organised by Emma van der Wateren, together with the Square Kilometre Array Observatory (SKAO). Representatives from radio astronomy observatories and national administrations from Germany, France, Italy, the Netherlands, and Sweden came together with members of the Committee on Radio Astronomy Frequencies (CRAF) and the SKAO to exchange views on the challenges posed by unintended electromagnetic radiation (UEMR) from Low Earth Orbit (LEO) satellite constellations.

UEMR is understood as radio waves that likely leak from electronics onboard satellites and are at low levels compared to communication signals, yet are sufficiently strong to affect astronomical observations. Participants discussed the significance of radio astronomy and the ways in which UEMR from satellites can affect the highly sensitive astronomical observations as conducted with today's radio telescopes.

Experts from CRAF and the SKAO reported on dedicated measurements of UEMR, which allow the estimation of its potential impact on radio astronomical observations, and summarised the regulatory context. Administrators contributed their perspectives on various regulatory paths, and underlined the importance of collaboration between the scientific community, industry, and administrations. Ongoing discussions between the industry sector and radio astronomy were also highlighted, with efforts to design future satellites and constellations with due consideration for UEMR.

The meeting was regarded as an opportunity to strengthen connections between the stakeholders and to develop a shared understanding of the impact of the increasing interference from satellite constellations on radio astronomy. Participants acknowledged the importance of radio astronomical research and agreed to remain in active contact to work on solutions.

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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