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Why do (or do not) people encourage others in their social networks to adopt climate-friendly behaviors? Encouragement like this has been referred to as “relational organizing,” and can help scale up climate action across communities. Since relational organizing is a social behavior, it likely has its own specific barriers and motivations beyond what affects personal climate action. Food is a big part of our day-to-day lives and our relationships with people we care about. It also impacts the climate, ecosystems, animal welfare, and our own health. As such, people’s climate-friendly food choices provide an ideal case study to explore drivers of relational organizing. Using an online survey with two North American samples of motivated audiences (one US-wide animal advocacy community,N = 1166, and one environmentally focused community in Boulder, Colorado,N = 363), we sought to identify and categorize the social–psychological barriers to and drivers of relational organizing for climate-friendly food choices. Using exploratory factor analysis and predictive models, we found that self-efficacy in carrying out the personal behavior, response efficacy beliefs, supportive social norms, and personal aptitude in relational organizing (e.g., personal norms) predicted relational organizing action after the survey. People’s sense of personal obligation to engage in relational organizing (i.e., personal norms), beliefs that would make a difference to important causes (i.e. response efficacy), and social identity beliefs around activism were particularly important. We discuss how these findings can help inform interventions related to climate-friendly diets, and what this means more broadly for how relational organizing can support climate action.

Although neutron star–black hole binaries have been identified through mergers detected in gravitational waves, a pulsar–black hole binary has yet to be detected. While short-period binaries are detectable due to a clear signal in the pulsar’s timing residuals, effects from a long-period binary could be masked by other timing effects, allowing them to go undetected. In particular, a long-period binary measured over a small subset of its orbital period could manifest via time derivatives of the spin frequency incompatible with isolated pulsar properties. We assess the possibility of pulsars having unknown companions in long-period binaries and put constraints on the range of binary properties that may remain undetected in current data, but that may be detectable with further observations. We find that for 35% of canonical pulsars with published higher-order derivatives, the precision of measurements is not enough to confidently reject binarity (period ≳2 kyr), and that a black hole binary companion could not be ruled out for a sample of pulsars without published constraints if the period is >1 kyr. While we find no convincing cases in the literature, we put more stringent limits on orbital period and longitude of periastron for the few pulsars with published higher-order frequency derivatives (n≥ 3). We discuss the detectability of candidates and find that a sample pulsar in a 100 yr orbit could be detectable within 5–10 yr.

Motivating people to take environmentally friendly action, especially collective actions that promote greater social engagement, is important for addressing environmental issues like biodiversity loss. We conducted an online workshop‐based field experiment to target social‐psychological perceptions to motivate people to plant native plants and encourage others to do the same. To shift these perceptions, we added 13 microinterventions to half the workshops, including normative messaging, public commitment‐making, and providing feedback on the impact of reaching out to others. We used a voucher system to track real‐world behavior by partnering with native plant nurseries. Compared to an information‐only control workshop, our intervention workshops initially increased certain social‐psychological perceptions related to encouraging others to plant native plants. However, they did not change behaviors, or many perceptions, compared to control workshops. Additional exploratory analyses revealed differing patterns of behavioral perceptions 2 months after the workshops. Further research is needed that implements experimental methods and real‐world measures of conservation behavior to evaluate the impacts of theory‐based outreach tactics on collective actions.

We present the detection of 661 known pulsars observed with the Australian SKA Pathfinder (ASKAP) telescope at 888 MHz as part of the Rapid ASKAP Continuum Survey (RACS). Detections were made through astrometric coincidence and we estimate the false alarm rate of our sample to be ∼0.5%. Using archival data at 400 and 1400 MHz, we estimate the power-law spectral indices for the pulsars in our sample and find that the mean spectral index is −1.78 ± 0.6. However, we also find that a single power law is inadequate for modeling all the observed spectra. With the addition of flux densities between 150 MHz and 3 GHz from various imaging surveys, we find that up to 40% of our sample show deviations from a simple power-law model. Using StokesVmeasurements from the RACS data, we measured the circular polarization fraction for 9% of our sample and find that the mean polarization fraction is ∼10% (consistent between detections and upper limits). Using the dispersion-measure-derived distance, we estimate the pseudo-luminosity of the pulsars and do not find any strong evidence for a correlation with the pulsars’ intrinsic properties.

As biodiversity loss and climate change accelerate, more people worldwide are engaging in conservation behaviors to “do their part.” Yet, individual behavior change alone is insufficient for the large‐scale, rapid change needed to address these crises. Relational organizing, which involves individuals reaching out to others in their social network, can enhance the speed and scale of conservation behavior change and address the complex, collective action nature of many conservation problems. However, many people practicing conservation behaviors in their own lives do not engage in relational organizing about conservation issues. Here, we suggest this may be the result of specific social‐psychological factors inhibiting people from reaching out to others. We summarize the evidence and offer a research and practice agenda to prioritize (1) understanding the social‐psychological barriers that prevent relational organizing, and (2) addressing these barriers through targeted outreach interventions to help scale and accelerate community action for conservation.

The millisecond pulsar J1713+0747 underwent a sudden and significant pulse shape change between 2021 April 16 and 17 (MJDs 59320 and 59321). Subsequently, the pulse shape gradually recovered over the course of several months. We report the results of continued multifrequency radio observations of the pulsar made using the Canadian Hydrogen Intensity Mapping Experiment and the 100 m Green Bank Telescope in a 3 yr period encompassing the shape change event, between 2020 February and 2023 February. As of 2023 February, the pulse shape had returned to a state similar to that seen before the event, but with measurable changes remaining. The amplitude of the shape change and the accompanying time-of-arrival residuals display a strong nonmonotonic dependence on radio frequency, demonstrating that the event is neither a glitch (the effects of which should be independent of radio frequency,ν) nor a change in dispersion measure alone (which would produce a delay proportional toν⁻²). However, it does bear some resemblance to the two previous “chromatic timing events” observed in J1713+0747, as well as to a similar event observed in PSR J1643−1224 in 2015.