Caltech Faint Galaxy Redshift Survey X: A Redshift Survey in the Region of the Hubble Deep Field North

dc.creatorCohen, Judith
dc.creatorHogg, David
dc.creatorBlandford, Roger
dc.creatorCowie, Lennox
dc.creatorHu, Esther
dc.creatorSongaila, Antoinette
dc.creatorShopbell, Patrick
dc.creatorRichberg, Kevin
dc.date1999-12-02
dc.date2000-05-24
dc.date.accessioned2026-07-07T11:08:31Z
dc.date.available2026-07-07T11:08:31Z
dc.descriptionA redshift survey has been carried out in the region of the Hubble Deep Field North using the Low Resolution Imaging Spectrograph at the Keck Observatory. The resulting redshift catalog, which contains 671 entries, is a compendium of our own data together with published LRIS/Keck data. It is more than 92% complete for objects, irrespective of morphology, to $R = 24$ mag in the HDF itself and to $R = 23$ mag in the Flanking Fields within a diameter of 8 arcmin centered on the HDF, an unusually high completion for a magnitude limited survey performed with a large telescope. A median redshift $z = 1.0$ is reached at $R \sim 23.8$. Strong peaks in the redshift distribution, which arise when a group or poor cluster of galaxies intersect the area surveyed, can be identified to $z \sim 1.2$ in this dataset. More than 68% of the galaxies are members of these redshift peaks. In a few cases, closely spaced peaks in $z$ can be resolved into separate groups of galaxies that can be distinguished in both velocity and location on the sky. The radial separation of these peaks in the pencil-beam survey is consistent with a characteristic length scale for the their separation of $\approx$70 Mpc in our adopted cosmology ($h = 0.6, Ω_M = 0.3$, $Λ= 0$). Strong galaxy clustering is in evidence at all epochs back to $z \le 1.1$. (abstract abridged)
dc.descriptionAccepted to the ApJ. This version contains all the figures and tables. 2 minor typos in table 2b corrected
dc.identifierhttps://arxiv.org/abs/astro-ph/9912048
dc.identifierhttp://arxiv.org/abs/astro-ph/9912048
dc.identifierAstrophys.J.538:29-52,2000
dc.identifierdoi:10.1086/309096
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190161
dc.subjectAstrophysics
dc.titleCaltech Faint Galaxy Redshift Survey X: A Redshift Survey in the Region of the Hubble Deep Field North
dc.typetext

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