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This paper examines the impact of a human rights framework in engineering education on students' perceptions of sustainability and human rights. Recently, scholars have emphasised the need to develop a new engineering pedagogy and an ethical framework for the workforce. This emphasis arises from the fact that, as the engineering workforce has become multicultural and globalised, prospective engineers require new ideas, technologies, perspectives and professional ethics to adapt to the changing world. In this context, scholars have primarily focused on creating sustainable approaches that highlight the coexistence between humans and nature, along with equity, diversity and human dignity, while also developing educational strategies to challenge the conventional notion of engineers as problem‐solvers. The University of Connecticut (UConn) has developed a curriculum that equips students with the core concepts and methodological tools essential for understanding the socially and environmentally responsive roles of engineers and their solutions. This paper examines learning outcomes in an existing course within this curriculum, ‘Engineering for Human Rights’, by analysing original, anonymized exit survey data and anonymized SET evaluations from enrolled students. We also assess the instructors' reflections on the class. The findings of our research contribute to broader discussions of innovation in engineering pedagogy. 

Abstract Let $$G$$ be a connected semisimple real algebraic group. For a Zariski dense Anosov subgroup $$\Gamma <G$$, we show that a $$\Gamma $$-conformal measure is supported on the limit set of $$\Gamma $$ if and only if its dimension is $$\Gamma $$-critical. This implies the uniqueness of a $$\Gamma $$-conformal measure for each critical dimension, answering the question posed in our earlier paper with Edwards [13]. We obtain this by proving a higher rank analogue of the Hopf–Tsuji–Sullivan dichotomy for the maximal diagonal action. Other applications include an analogue of the Ahlfors measure conjecture for Anosov subgroups. 

Abstract Let $$\Gamma $$ be a Zariski dense Anosov subgroup of a connected semisimple real algebraic group $$G$$. For a maximal horospherical subgroup $$N$$ of $$G$$, we show that the space of all non-trivial $NM$-invariant ergodic and $$A$$-quasi-invariant Radon measures on $$\Gamma \backslash G$$, up to proportionality, is homeomorphic to $${\mathbb {R}}^{\text {rank}\,G-1}$$, where $$A$$ is a maximal real split torus and $$M$$ is a maximal compact subgroup that normalizes $$N$$. One of the main ingredients is to establish the $NM$-ergodicity of all Burger–Roblin measures. 

ABSTRACT We report the detection of cold dust in an apparently quiescent massive galaxy (log (M⋆/M⊙) ≈ 11) at z ∼ 2 (G4). The source is identified as a serendipitous 2 mm continuum source in a deep ALMA observation within the field of Q2343-BX610, a z = 2.21 massive star-forming disc galaxy. Available multiband photometry of G4 suggests redshift of z ∼ 2 and a low specific star formation rate (sSFR), log (SFR/M⋆)[yr−1] ≈ −10.2, corresponding to ≈1.2 dex below the z = 2 main sequence (MS). G4 appears to be a peculiar dust-rich quiescent galaxy for its stellar mass (log (Mdust/M⋆) = −2.71 ± 0.26), with its estimated mass-weighted age (∼1–2 Gyr). We compile z ≳ 1 quiescent galaxies in the literature and discuss their age–ΔMS and log (Mdust/M⋆)–age relations to investigate passive evolution and dust depletion scale. A long dust depletion time and its morphology suggest morphological quenching along with less efficient feedback that could have acted on G4. The estimated dust yield for G4 further supports this idea, requiring efficient survival of dust and/or grain growth, and rejuvenation (or additional accretion). Follow-up observations probing the stellar light and cold dust peak are necessary to understand the implication of these findings in the broader context of galaxy evolutionary studies and quenching in the early universe. 

Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composition of their chromospheres. Despite the fundamental progress in (sub-)millimeter observations of the Sun, some important aspects require diagnostic capabilities that are not offered by existing observatories. In particular, simultaneously observations of the radiation continuum across an extended frequency range would facilitate the mapping of different layers and thus ultimately the 3D structure of the solar atmosphere. Mapping large regions on the Sun or even the whole solar disk at a very high temporal cadence would be crucial for systematically detecting and following the temporal evolution of flares, while synoptic observations, i.e., daily maps, over periods of years would provide an unprecedented view of the solar activity cycle in this wavelength regime. As our Sun is a fundamental reference for studying the atmospheres of active main sequence stars, observing the Sun and other stars with the same instrument would unlock the enormous diagnostic potential for understanding stellar activity and its impact on exoplanets. The Atacama Large Aperture Submillimeter Telescope (AtLAST), a single-dish telescope with 50m aperture proposed to be built in the Atacama desert in Chile, would be able to provide these observational capabilities. Equipped with a large number of detector elements for probing the radiation continuum across a wide frequency range, AtLAST would address a wide range of scientific topics including the thermal structure and heating of the solar chromosphere, flares and prominences, and the solar activity cycle. In this white paper, the key science cases and their technical requirements for AtLAST are discussed.