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Events

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Daily image

Dual Channel RF over Fiber

© Lesley Goudbeek

Over the years ASTRON has developed its own RF over Fiber modules. These modules have been used by several institutes around the world, such as MWA (50MHz to 350MHz) and a SKA prototype (50MHZ to 650MHz).

https://www.astron.nl/dailyimage/main.php?date=20170112

A couple of years ago a special module was developed for Ingram Networks, situated in England.

The Ingram module operates from 20kHz to 800MHz (not a typo) and over a hundred optical links have been shipped to Ingram. The modules are destined to be used for a railway project, where base stations connect to moving trains providing wireless internet to the passengers. The RFoF modules provide signal transport between base stations.

A dual channel RFoF module has been suggested and if it is easily achievable. As a Friday afternoon test, a dual channel RFoF module was made using previous developed single channel PCB’s (shown in upper picture). Instead of using a single laser, a dual laser module was used. This dual laser module is connected to 2 separate PCB’s (without any additional modifications). The same is done on the receiver side were a dual channel detector is connected to 2 separate PCB’s. The graph on the left show an old “normal” single channel RFoF module, and the right graph shows the modified dual channel RFoF Frankenstein (shown in the picture), where 2 separate signals are visible. And without any additional modifications, the results are not that far off of the original module. Reducing pin length and removing the unused detectors should improve stability.

This shows that a dual channel RFoF module is quite feasible and existing designs can be used. Plus the costs of a dual channel laser or detector is not significantly higher than 2 separate laser or detector modules. A dual channel can, for example, be used for transmitting both antenna polarizations and reduce the number of fibers needed by half. With a small PCB redesign, the total PCB size used can also be reduced. Sometimes a Friday afternoon can give insight into a lingering question.

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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