Zobrazeno 1 - 5
of 5
pro vyhledávání: '"J R Whitbourn"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.511(4), pp.5742-5755 [Peer Reviewed Journal]
We investigate the ‘Local Hole’, an anomalous underdensity in the local galaxy environment, by extending our previous galaxy K-band number-redshift and number-magnitude counts to ≈90 per cent of the sky. Our redshift samples are taken from the
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2019, Vol.490(4), pp.4715-4720 [Peer Reviewed Journal]
We revisit our mapping of the `Local Hole', a large underdensity in the local galaxy redshift distribution that extends out to redshift, $z\approx0.05$ and a potential source of outflows that may perturb the global expansion rate and thus help mitiga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6049424b1569ad669b398cc6ee848882
http://arxiv.org/abs/1909.01878
http://arxiv.org/abs/1909.01878
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2013, Vol.437(1), pp.622-640 [Peer Reviewed Journal]
The prime evidence underpinning the standard Λ cold dark matter cosmological model is the cosmic microwave background (CMB) power spectrum as observed by Wilkinson Microwave Anisotropy Probe (WMAP) and other microwave experiments. But Sawangwit and
Autor:
Tom Shanks, J. R. Whitbourn
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2016, Vol.459(1), pp.496-507 [Peer Reviewed Journal]
Whitbourn & Shanks (2014) have reported evidence for a local void underdense by ~15% extending to 150-300h-1Mpc around our position in the Southern Galactic Cap (SGC). Assuming a local luminosity function they modelled K- and r-limited number counts
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b77780f1992ac6a52f7b6041df848332
Autor:
J. R. Whitbourn, Tom Shanks
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2014, Vol.437(3), pp.2146-2162 [Peer Reviewed Journal]
The redshifts of ~250000 galaxies are used to study the Local Hole and its associated peculiar velocities. The sample, compiled from 6dFGS and SDSS provides wide sky coverage to a depth of ~300h-1Mpc. We have therefore examined K and r limited galaxy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae252d2cb698e4a3e59a174113ba3720