Results 71 to 80 of about 245,319 (342)

Redshift Accuracy Requirements for Future Supernova and Number Count Surveys [PDF]

open access: yesAstrophys.J.615:595,2004; Astrophys.J.615:595-602,2004, 2004
We investigate the required redshift accuracy of type Ia supernova and cluster number-count surveys in order for the redshift uncertainties not to contribute appreciably to the dark energy parameter error budget. For the SNAP supernova experiment, we find that, without the assistance of ground-based measurements, individual supernova redshifts would ...
arxiv   +1 more source

An improved redshift indicator for Gamma-Ray Bursts, based on the prompt emission

open access: yes, 2006
We propose an improved version of the redshift indicator developed by Atteia (2003), which gets rid of the dependence on the burst duration and provides better estimates for high-redshift GRBs.
Atteia, Jean-Luc   +4 more
core   +2 more sources

Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory [PDF]

open access: yes, 2010
We present an improved prescription for matter power spectrum in redshift space taking a proper account of both the non-linear gravitational clustering and redshift distortion, which are of particular importance for accurately modeling baryon acoustic ...
A. J. S. Hamilton   +14 more
core   +3 more sources

ASTROMETRIC REDSHIFTS FOR QUASARS [PDF]

open access: yesThe Astronomical Journal, 2009
The wavelength dependence of atmospheric refraction causes differential chromatic refraction (DCR), whereby objects imaged at different optical/UV wavelengths are observed at slightly different positions in the plane of the detector. Strong spectral features induce changes in the effective wavelengths of broad-band filters that are capable of producing
Gordon T. Richards   +3 more
openaire   +3 more sources

Facet‐Junction Induced Strong Metal Support Interaction for Enhanced Alkaline Hydrogen Evolution Reaction

open access: yesAdvanced Functional Materials, EarlyView.
In this study, a novel facet‐junction strategy is proposed to enhance the strong metal‐support interaction (SMSI) between the loaded Ru atoms and the Co3O4 support. The synthesized structure with the incorporation of Ru doping and the (100)/(111) crystal plane junction has a particular influence on the catalyst's hydrogen evolution reaction (HER ...
Wenqian Shen   +6 more
wiley   +1 more source

Fast Radio Burst Energy Function in the Presence of DMhost Variation

open access: yesUniverse
Fast radio bursts (FRBs) have been found in great numbers, but the physical mechanism of these sources is still a mystery. The redshift evolutions of the FRB energy distribution function and the volumetric rate shed light on the origin of FRBs.
Ji-Guo Zhang   +5 more
doaj   +1 more source

The Redshift Distribution of Infrared-Faint Radio Sources [PDF]

open access: yes, 2018
Infrared-Faint Radio Sources (IFRSs) are an important class of high-redshift active galaxy, and potentially important as a means of discovering more high-redshift radio sources, but only 25 IFRSs had redshifts prior to this paper. Here we increase the number of IFRSs with known spectroscopic redshifts by a factor of about 5 to 131, with redshifts up to
arxiv   +1 more source

Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift [PDF]

open access: yesAstrophys.J.651:14-23,2006, 2006
We investigate how well the redshift distributions of galaxies sorted into photometric redshift bins can be determined from the galaxy angular two-point correlation functions. We find that the uncertainty in the reconstructed redshift distributions depends critically on the number of parameters used in each redshift bin and the range of angular scales ...
arxiv   +1 more source

The Angular Diameter-Redshift Test for Large Redshift Quasars [PDF]

open access: yesSymposium - International Astronomical Union, 1977
Complete samples of quasars in the 3CR and 4C catalogues have been observed with a resolution of 2″ arc in RA and 2″ cosecδ in dec with the Cambridge 5-km telescope at 5 GHz (Riley & Pooley 1975; Jenkins et al 1977), from which it has been possible to determine the overall angular sizes of their radio structures (LAS). The angular diameter-redshift
J. M. Riley, A. Hooley, M. S. Longair
openaire   +2 more sources

Perfect Ultraviolet Absorbers via Disordered Polarizonic Metasurfaces for Multiband Camouflage and Stealth Technologies

open access: yesAdvanced Functional Materials, EarlyView.
An ultrathin polarizonic metasurface achieves multiband camouflage and stealth with near‐perfect ultraviolet (UV) absorption, visible light blending, and infrared signature masking. Leveraging earth‐abundant materials, this design creates a reflective color palette through polarizonic effects, integrating transparent and non‐plasmonic materials.
Mhd Adel Assad, Mady Elbahri
wiley   +1 more source

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