2014 ◽  
Vol 47 (02) ◽  
pp. 485-489 ◽  
Author(s):  
Kate Roll

ABSTRACTThis article highlights the contribution of randomized, quantitative sampling techniques to answeringqualitativequestions posed by the study. In short it asks: what qualitative insights do we derive from quantitative sampling processes? Rather than simply being a means to an end, I argue the sampling process itself generated data. More specifically, seeking out more than 220 geographically dispersed individuals, selected though a randomized cluster sample, resulted in the identification of relationship patterns, highlighted extant resistance-era hierarchies and patronage networks, as well as necessitated deeper, critical engagement with the sampling framework. While this discussion is focused on the study of former resistance members in Timor-Leste, these methodological insights are broadly relevant to researchers using mixed methods to study former combatants or other networked social movements.


The Lancet ◽  
2004 ◽  
Vol 364 (9448) ◽  
pp. 1857-1864 ◽  
Author(s):  
Les Roberts ◽  
Riyadh Lafta ◽  
Richard Garfield ◽  
Jamal Khudhairi ◽  
Gilbert Burnham

2019 ◽  
Vol 486 (4) ◽  
pp. 4863-4879 ◽  
Author(s):  
Ali Takey ◽  
Florence Durret ◽  
Isabel Márquez ◽  
Amael Ellien ◽  
Mona Molham ◽  
...  

ABSTRACT We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey. The sample includes 54 galaxy clusters in the redshift range of 0.05–1.2, with a median redshift of 0.36. We first present the X-ray temperature and luminosity measurements that are used to investigate the X-ray luminosity–temperature relation. The slope and intercept of the relation are consistent with those published in the literature. Then, we investigate the optical properties of the cluster galaxies including their morphological analysis and the galaxy luminosity functions (GLFs). The morphological content of cluster galaxies is investigated as a function of cluster mass and distance from the cluster centre. No strong variation of the fraction of early- and late-type galaxies with cluster mass is observed. The fraction of early-type galaxies as a function of cluster radius varies as expected. The individual GLFs of red sequence galaxies were studied in the five ugriz bands for 48 clusters. The GLFs were then stacked in three mass bins and two redshift bins. Twenty clusters of the present sample are studied for the first time in X-rays, and all are studied for the first time in the optical range. Altogether, our sample appears to have X-ray and optical properties typical of ‘average’ cluster properties.


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