Results 131 to 140 of about 47,826 (245)

Photometric Redshift Forecast for the 7-Dimensional Sky Survey

open access: yesThe Astrophysical Journal
We investigate the expected accuracy of redshifts that can be obtained using low-resolution spectroscopic (medium-band) data from the 7-Dimensional Sky Survey (7DS). By leveraging 40 densely sampled filters with widths of FWHM = 25 nm, we create 7DS mock
Eunhee Ko   +5 more
doaj   +1 more source

On photometric redshift requirements

open access: yesNew Journal of Physics, 2007
Cosmic shear constrains cosmology by exploiting the apparent alignments of pairs of galaxies due to gravitational lensing by intervening mass clumps. However, galaxies may become (intrinsically) aligned with each other, and with nearby mass clumps, during their formation.
Bridle, Sarah, King, Lindsay
openaire   +1 more source

Photometric Redshifts and Gravitational Telescopes

open access: yes, 2000
We review the use of photometric redshifts in the particular context of Gravitational Telescopes. We discuss on the possible application of such a technique to the study of both the faint population of distant sources and the properties of cluster lenses.
Pello, R.   +10 more
openaire   +2 more sources

The FENIKS Survey: Multiwavelength Photometric Catalog in the UDS Field, and Catalogs of Photometric Redshifts and Stellar Population Properties

open access: yesThe Astrophysical Journal
We present the construction of a deep multiwavelength point-spread-function-matched photometric catalog in the Ultra-Deep Survey (UDS) field following the final UKIDSS UDS release.
Kumail Zaidi   +13 more
doaj   +1 more source

Analytical marginalization over photometric redshift uncertainties in cosmic shear analyses [PDF]

open access: hybrid, 2023
Jaime Ruiz-Zapatero   +5 more
openalex   +1 more source

Photometric Redshifts in the CFDF

open access: yes, 1999
The Canada-France Deep Fields (CFDF) is a large, deep, multi-colour imaging survey undertaken primarily at CFHT. It is about 10 times fainter than the CFRS (Lilly et al 1995a) and contains over 100 times as many galaxies. With three common fields, CFDF redshifts will be estimated photometrically using the CFRS spectroscopic catalogue as a training set.
Brodwin, Mark   +2 more
openaire   +2 more sources

Improving Photometric Redshift Estimates with Training Sample Augmentation

open access: yesThe Astrophysical Journal Letters
Large imaging surveys will rely on photometric redshifts (photo- z 's), which are typically estimated through machine-learning methods. Currently planned spectroscopic surveys will not be deep enough to produce a representative training sample for Legacy
Irene Moskowitz   +6 more
doaj   +1 more source

Astrometric Redshifts of Supernovae

open access: yesThe Astrophysical Journal
Differential Chromatic Refraction (DCR) is caused by the wavelength dependence of our atmosphere’s refractive index, which shifts the apparent positions of stars and galaxies and distorts their shapes depending on their spectral energy distributions ...
Jaemyoung (Jason) Lee   +4 more
doaj   +1 more source

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