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A coincidence of disturbed morphology and blue UV colour: minor‐merger‐driven star formation in early‐type galaxies at z∼ 0.6

[PDF] from arxiv.org…, KM Tan, RS Ellis, J Silk - Monthly Notices of the …, 2011 - Wiley Online Library
ABSTRACT We exploit multiwavelength photometry of early-type galaxies (ETGs) in the Cosmological
Evolution Survey (COSMOS) to demonstrate that the low-level star formation activity in the ETG
population at intermediate redshift is likely to be driven by minor mergers. Splitting the ...
Cited by 16 - Related articles - All 8 versions

The Hubble Space Telescope Wide Field Camera 3 Early Release Science Data: Panchromatic Faint Object Counts for 0.2-2 μm Wavelength

…, F Paresce, A Saha, JI Silk… - The Astrophysical …, 2011 - iopscience.iop.org
We describe the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) Early Release
Science (ERS) observations in the Great Observatories Origins Deep Survey (GOODS) South
field. The new WFC3 ERS data provide calibrated, drizzled mosaics in the UV filters ...
Cited by 33 - Related articles - All 3 versions

Neural systems of threat processing in adolescents: role of pubertal maturation and relation to measures of negative affect

EE Forbes, ML Phillips, JS Silk… - Developmental …, 2011 - Taylor & Francis
Adolescence ushers in dramatic social and affective changes and increased vulnerability for
affective disorders. Yet, little is known about the effects of pubertal maturation on neural systems
of social threat processing. We examined adolescents' brain function to social stimuli in ...
Cited by 2 - Related articles - All 3 versions

Probability of the most massive cluster under non‐Gaussian initial conditions

[PDF] from arxiv.org…, C Gordon, J Silk - Monthly Notices of the Royal …, 2011 - Wiley Online Library
Laura Cayón,1⋆ Christopher Gordon2 and Joseph Silk2 1Department of Physics, Purdue
University, 525 Northwestern Avenue, West Lafayette, IN 47907-2036, USA 2Oxford
Astrophysics, Department of Physics, Denys Wilkinson Building, Keble Road, Oxford OX1 ...
Cited by 24 - Related articles - All 7 versions

Dark Matter Seeding in Neutron Stars

[PDF] from arxiv.orgMA Perez-Garcia, J Silk… - Arxiv preprint arXiv:1108.5206, 2011 - arxiv.org
There is compelling evidence [1] that as much as 90% of the matter in the Universe is under the
form of dark matter (DM). A set of very popular candidates for DM are WIMPs (weakly interacting
massive particles). This mostly follows from what is called the WIMP miracle since ...

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