papers

Publications (10)

astro-ph.GA2016

KROSS: Mapping the Ha emission across the star-formation sequence at z~1

Georgios E. Magdis, M. Bureau, J. P. Stott +7

We present first results from the KMOS Redshift One Spectroscopic Survey (KROSS), an ongoing large kinematical survey of a thousand, z~1 star forming galaxies, with VLT KMOS. Out o…

astro-ph.CO2013

Chronos: A NIR spectroscopic galaxy survey. From the formation of galaxies to the peak of activity

I. Ferreras, R. Sharples, J. S. Dunlop +30

Chronos is our response to ESA's call for white papers to define the science for the future L2, L3 missions. Chronos targets the formation and evolution of galaxies, by collecting…

astro-ph.HE2020

The Chandra Deep Wide-Field Survey: A New Chandra Legacy Survey in the Boötes Field I. X-ray Point Source Catalog, Number Counts and Multi-Wavelength Counterparts

A. Masini, R. C. Hickox, C. M. Carroll +30

We present a new, ambitious survey performed with the Chandra X-ray Observatory of the 9.3 deg Boötes field of the NOAO Deep Wide-Field Survey. The wide field probes a statist…

astro-ph.CO2014

Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high redshift studies

J. Richard, M. Jauzac, M. Limousin +9

Extending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the…

astro-ph2006

Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation

M. Swinbank, R. Bower, G. P. Smith +5

We exploit the gravitational potential of massive cluster lenses to probe the emission line properties of six z=1 galaxies which appear as highly magnified luminous arcs. Using the…

astro-ph2001

Distinguishing Local and Global Influences on Galaxy Morphology: An HST Comparison of High and Low X-ray Luminosity Clusters

Michael Balogh, Ian Smail, R. Bower +6

(Abridged) We present a morphological analysis of 17 X-ray selected clusters at z~0.25, imaged uniformly with HST WFPC2. Eight of these clusters have low X-ray luminosities (<10^{4…