Protected areas are under immense pressure to safeguard much of the remaining global biodiversity and can be strained by unpredicted events such as the Covid-19 pandemic. Understanding the extent of the effects of the pandemic on protected area management and conservation outcomes is critical for recovery and future planning to buffer against these types of events. We used survey and focus group data to measure the perceived impact of the pandemic on protected areas in Mexico and outline the pathways that led to these conservation outcomes. Across 62 protected areas, we found substantial changes in management capacity, monitoring and tourism, and a slight increase in non-compliant activities. Our findings highlight the need to integrate short-term relief plans to support communities dependent on tourism, who were particularly vulnerable during the pandemic, and to increase access to technology and technical capacity to better sustain management activities during future crises.

Anxiety and depression affect a significant number of children and young people (CYP) and can have a far reaching and long-lasting impact. Cognitive behavioural (CB) interventions can be effective for treating anxiety and depression in CYP but are difficult to access. Recent government policy in England seeks to train a non-traditional graduate workforce to deliver a range of CB interventions for mild to moderate anxiety and depression to CYP, in community settings. This practice-based evaluation aimed to estimate the effectiveness of CB interventions delivered by postgraduate trainees undertaking training in a range of CB interventions for mild to moderate anxiety and depression whilst on placement in schools or community Child and Adolescent Mental Health Services (CAMHS). Self- and parent-reported routine outcome measures (ROMS) were completed pre- and post-intervention, including measures of symptom severity, symptom impact and goal achievement. Significant improvements were demonstrated across all self and parent-reported measures post-intervention, with mean scores falling firmly in the non-clinical range, a significant reduction in the proportion of CYP in the clinical range on measures, and predominantly medium to large effect sizes. Results are promising in terms of the capacity to train a graduate workforce to deliver a range of low-intensity CB interventions to CYP experiencing mild to moderate depression or anxiety-based difficulties in either CAMHS or school settings, increasing capacity across the system. The current practice-based evaluation also supports the potential effectiveness of current training models/programmes. Further research is needed in terms of long-term outcomes and to compare outcomes between settings, interventions, and demographic groups.

The Variables and Slow Transients Survey (VAST) on the Australian Square Kilometre Array Pathfinder (ASKAP) is designed to detect highly variable and transient radio sources on timescales from 5 s to $\sim\!5$ yr. In this paper, we present the survey description, observation strategy and initial results from the VAST Phase I Pilot Survey. This pilot survey consists of $\sim\!162$ h of observations conducted at a central frequency of 888 MHz between 2019 August and 2020 August, with a typical rms sensitivity of $0.24\ \mathrm{mJy\ beam}^{-1}$ and angular resolution of $12-20$ arcseconds. There are 113 fields, each of which was observed for 12 min integration time, with between 5 and 13 repeats, with cadences between 1 day and 8 months. The total area of the pilot survey footprint is 5 131 square degrees, covering six distinct regions of the sky. An initial search of two of these regions, totalling 1 646 square degrees, revealed 28 highly variable and/or transient sources. Seven of these are known pulsars, including the millisecond pulsar J2039–5617. Another seven are stars, four of which have no previously reported radio detection (SCR J0533–4257, LEHPM 2-783, UCAC3 89–412162 and 2MASS J22414436–6119311). Of the remaining 14 sources, two are active galactic nuclei, six are associated with galaxies and the other six have no multi-wavelength counterparts and are yet to be identified.