📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

The clustering of typical Ly a emitters from z ~ 2.5-6: host halo masses depend on Ly a and UV luminosities (2019)

First Author: Khostovan A

Attributed to: Lancaster University Astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stz2149

Publication URI: http://dx.doi.org/10.1093/mnras/stz2149

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1