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1. An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

   https://doi.org/10.1051/0004-6361/201730443  

   Miettinen, O. ; Novak, M. ; Smolčić, V. ; Delvecchio, I. ; Aravena, M. ; Brisbin, D. ; Karim, A. ; Murphy, E. J. ; Schinnerer, E. ; Albrecht, M. ; et al ( June 2017 , Astronomy & Astrophysics)
2. An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution

   https://doi.org/10.1051/0004-6361/201730558  

   Brisbin, Drew ; Miettinen, Oskari ; Aravena, Manuel ; Smolčić, Vernesa ; Delvecchio, Ivan ; Jiang, Chunyan ; Magnelli, Benjamin ; Albrecht, Marcus ; Arancibia, Alejandra Muñoz ; Aussel, Hervé ; et al ( December 2017 , Astronomy & Astrophysics)
3. An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

   https://doi.org/10.1051/0004-6361/201730762  

   Miettinen, O. ; Delvecchio, I. ; Smolčić, V. ; Aravena, M. ; Brisbin, D. ; Karim, A. ; Magnelli, B. ; Novak, M. ; Schinnerer, E. ; Albrecht, M. ; et al ( October 2017 , Astronomy & Astrophysics)
4. From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars

   https://doi.org/10.1146/annurev-nucl-101917-021141  

   Frebel, Anna ( October 2018 , Annual Review of Nuclear and Particle Science)

   Understanding the origin of the elements has been a decades-long pursuit, with many open questions remaining. Old stars found in the Milky Way and its dwarf satellite galaxies can provide answers because they preserve clean element abundance patterns of the nucleosynthesis processes that operated some 13 billion years ago, enabling reconstruction of the chemical evolution of the elements. This review focuses on the astrophysical signatures of heavy neutron-capture elements made in the s-, i-, and r-processes found in old stars. A highlight is the recently discovered r-process galaxy Reticulum II, which was enriched by a neutron star merger. These resultsmore »show that old stars in dwarf galaxies provide a novel means to constrain the astrophysical site of the r-process, ushering in much-needed progress on this major outstanding question. This nuclear astrophysics research complements the many experimental and theoretical nuclear physics efforts into heavy-element formation, and also aligns with results on the gravitational-wave signature of neutron star mergers.« less
5. Experimentation with Full-Duplex Wireless in the COSMOS Testbed

   https://doi.org/10.1109/ICNP.2019.8888146  

   Chen, Tingjun ; Welles, Jackson ; Kohli, Manav ; Dastjerdi, Mahmood Baraani ; Kolodziejski, Jakub ; Sherman, Michael ; Seskar, Ivan ; Krishnaswamy, Harish ; Zussman, Gil ( October 2019 , Conference: 2019 IEEE 27th International Conference on Network Protocols (ICNP))

   In order to support experimentation with full-duplex (FD) wireless, we integrated the FlexICoN Gen-2 wideband FD radio with the city-scale PAWR COSMOS testbed [1]. In particular, the implemented FD radio consists of an antenna, a customized Gen-2 RF self-interference (SI) canceller box, a USRP software-defined radio (SDR), and a compute node. The RF canceller box includes an RF SI canceller implemented using discrete components on a printed circuit board (PCB), which emulates its RFIC canceller counterpart. The Gen-2 RF SI canceller achieves 50 dB RF SI cancellation across 20 MHz bandwidth using the technique of frequency-domain equalization (FDE) [2]. Inmore »this abstract, we present the design and implementation of the remotely accessible Gen-2 wideband FD radio integrated with the COSMOS sandbox at Columbia University. We also present an example real-time wideband F« less