[HTML][HTML] Implementing educational technology in Higher Education Institutions: A review of technologies, stakeholder perceptions, frameworks and metrics
In a world driven by constant change and innovation, Higher Education Institutions (HEIs)
are undergoing a rapid transformation, often driven by external factors such as emerging …
are undergoing a rapid transformation, often driven by external factors such as emerging …
Discovery of a Galaxy Cluster with a Violently Starbursting Core at z= 2.506
…, V Strazzullo, F Valentino, R Van Der Burg… - The Astrophysical …, 2016 - iopscience.iop.org
We report the discovery of a remarkable concentration of massive galaxies with extended X-ray
emission at z spec= 2.506, which contains 11 massive (M*≳ 10 11 M⊙) galaxies in the …
emission at z spec= 2.506, which contains 11 massive (M*≳ 10 11 M⊙) galaxies in the …
The phase space and stellar populations of cluster galaxies at z∼ 1: simultaneous constraints on the location and timescale of satellite quenching
A Muzzin, RFJ Van Der Burg, SL McGee… - The Astrophysical …, 2014 - iopscience.iop.org
… by normalizing each relative to its σ v and R 200 (see van der Burg et al. 2014, Table 1). …
range of combined timescales for quenching at R = 0.25 R 200 and R = 1.0 R 200 ; however, no …
range of combined timescales for quenching at R = 0.25 R 200 and R = 1.0 R 200 ; however, no …
The abundance and spatial distribution of ultra-diffuse galaxies in nearby galaxy clusters
… For g–r colour measurements we use a matched aperture approach in which we take
account of the seeing differences between the two bands (see Appendix A in van der Burg et al. …
account of the seeing differences between the two bands (see Appendix A in van der Burg et al. …
[HTML][HTML] The UV galaxy luminosity function at z= 3–5 from the CFHT Legacy Survey Deep fields
RFJ van der Burg, H Hildebrandt, T Erben - Astronomy & Astrophysics, 2010 - aanda.org
Aims. We measure and study the evolution of the UV galaxy luminosity function (LF) at z = 3−5
from the largest high-redshift survey to date, the Deep part of the CFHT Legacy Survey. …
from the largest high-redshift survey to date, the Deep part of the CFHT Legacy Survey. …
[HTML][HTML] The environmental dependence of the stellar mass function at z~ 1-Comparing cluster and field between the GCLASS and UltraVISTA surveys
… This leads to estimates of R 200 , the radius at which the mean interior density is 200 times
… RFJ van der Burg and H. Hoekstra acknowledge support from the Netherlands Organisation …
… RFJ van der Burg and H. Hoekstra acknowledge support from the Netherlands Organisation …
Evidence for a change in the dominant satellite galaxy quenching mechanism at z = 1
… Stellar masses are computed as described in van der Burg et al… van der Burg et al. (2013)
showed that the stellar masses … stellar mass profiles can be found in van der Burg et al. (2013, …
showed that the stellar masses … stellar mass profiles can be found in van der Burg et al. (2013, …
The massive ancient galaxies at z> 3 NEar-infrared (MAGAZ3NE) survey: Confirmation of extremely rapid star formation and quenching timescales for massive …
…, M Stefanon, RFJ Van der Burg - The Astrophysical …, 2020 - iopscience.iop.org
… Cemile Marsan 2 , Marianna Annunziatella 3,4 , Gillian Wilson 1 , Adam Muzzin 2 , Danilo
Marchesini 3 , MC Cooper 5 , Jeffrey CC Chan 1 , Ian McConachie 1 , Percy Gomez 6 , Erin …
Marchesini 3 , MC Cooper 5 , Jeffrey CC Chan 1 , Ian McConachie 1 , Percy Gomez 6 , Erin …
Reviewing research on teaching writing based on Vygotsky's theories: What we can learn
RM Vanderburg - Reading & Writing Quarterly, 2006 - Taylor & Francis
This review focuses on the development of writing research informed by a Vygotskian
perspective. A methodological environment to aid the instruction of writing is presented. The …
perspective. A methodological environment to aid the instruction of writing is presented. The …
The abundance of ultra-diffuse galaxies from groups to clusters-UDGs are relatively more common in more massive haloes
In recent years, many studies have reported substantial populations of large galaxies with
low surface brightness in local galaxy clusters. Various theories that aim to explain the …
low surface brightness in local galaxy clusters. Various theories that aim to explain the …