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Low-mass halo perturbations in strong gravitational lenses at redshift z ∼ 0.5 are consistent with CDM

by Ritondale, E, Vegetti, S, Despali, G, Auger, M W, Koopmans, L V E, McKean, J P
Published in Monthly notices of the Royal Astronomical Society (11.05.2019)

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Resolving on 100 pc scales the UV-continuum in Lyman-α emitters between redshift 2 and 3 with gravitational lensing

by Ritondale, E, Auger, M W, Vegetti, S, McKean, J P
Published in Monthly notices of the Royal Astronomical Society (01.02.2019)

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$Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing$

Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing

by Ritondale, E, Auger, M. W, Vegetti, S, McKean, J. P
Year of Publication 08.11.2018

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$Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM$

Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM

by Ritondale, E, Vegetti, S, Despali, G, Auger, M. W, Koopmans, L. V. E, McKean, J. P
Year of Publication 08.11.2018

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$Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing$

Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing

by Ritondale, E, Auger, M W, Vegetti, S, McKean, J P
Published in arXiv.org (08.11.2018)

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$Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM$

Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM

by Ritondale, E, Vegetti, S, Despali, G, Auger, M W, Koopmans, L V E, McKean, J P
Published in arXiv.org (08.11.2018)

Get full text

Paper

Low-mass halo perturbations in strong gravitational lenses at redshift z ∼ 0.5 are consistent with CDM

Resolving on 100 pc scales the UV-continuum in Lyman-α emitters between redshift 2 and 3 with gravitational lensing

Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing

Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM

Resolving on 100 pc scales the UV-continuum in Lyman-\(\alpha\) emitters between redshift 2 to 3 with gravitational lensing

Low-mass halo perturbations in strong gravitational lenses at redshift z\(\sim\)0.5 are consistent with CDM

Low-mass halo perturbations in strong gravitational lenses at redshift z ∼ 0.5 are consistent with CDM

Resolving on 100 pc scales the UV-continuum in Lyman-α emitters between redshift 2 and 3 with gravitational lensing

Resolving on 100 pc scales the UV-continuum in Lyman-$\alpha$ emitters between redshift 2 to 3 with gravitational lensing

Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM

Resolving on 100 pc scales the UV-continuum in Lyman-\(\alpha\) emitters between redshift 2 to 3 with gravitational lensing

Low-mass halo perturbations in strong gravitational lenses at redshift z\(\sim\)0.5 are consistent with CDM

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