69 citations · 145 across the 6 of their papers we have counts for
6 papers
Size-scaling of clump instabilities in turbulent, feedback regulated disks
Kamran Ali, Danail Obreschkow, Liang Wang +5
We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galax…
Cosmological Constraints from Fourier Phase Statistics
Kamran Ali, Danail Obreschkow, Cullan Howlett +4
Most statistical inference from cosmic large-scale structure relies on two-point statistics, i.e.\ on the galaxy-galaxy correlation function (2PCF) or the power spectrum. These sta…
Probing redshift-space distortions with phase correlations
Felipe O. Franco, Camille Bonvin, Danail Obreschkow +2
Redshift-space distortions are a sensitive probe of the growth of large-scale structure. In the linear regime, redshift-space distortions are fully described by the multipoles of t…
Robust Cross-correlation-based Measurement of Clump Sizes in Galaxies
Kamran Ali, Danail Obreschkow, David B. Fisher +4
Stars form in molecular complexes that are visible as giant clouds () in nearby galaxies and as giant clumps () in ga…
A precise deuterium abundance: Re-measurement of the z=3.572 absorption system towards the quasar PKS1937-101
S. Riemer-Sørensen, S. Kotuš, J. K. Webb +4
The primordial deuterium abundance probes fundamental physics during the Big Bang Nucleosynthesis and can be used to infer cosmological parameters. Observationally, the abundance c…
A robust deuterium abundance; Re-measurement of the z=3.256 absorption system towards the quasar PKS1937-1009
S. Riemer-Sørensen, J. K. Webb, N. Crighton +6
The primordial deuterium abundance is an important tracer of the fundamental physics taking place during Big Bang Nucleosynthesis. It can be determined from absorption features alo…