Does Amati Relation Depend on Luminosity of GRB's Host Galaxies?
arXiv:0710.5302 · doi:10.1088/1009-9271/8/3/02
Abstract
In order to test systematic of the Amati relation, the 24 long-duration GRBs with firmly determined and are separated into two sub-groups according to B-band luminosity of their host galaxies. The Amati relations in the two subgroups are found to be in agreement with each other within uncertainties. Taking into account of the well established luminosity - metallicity relation of galaxies, no strong evolution of the Amati relation with GRB's environment metallicity is implied in this study.
7 pages, 3 figures and 1 table, accepted by ChJAA
References in corpus (37)
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
- The Supernova -- Gamma-Ray Burst Connection
- Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
- Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir
- Metallicities of 0.3<z<1.0 Galaxies in the GOODS-North Field
- The collimation--corrected GRB energies correlate with the peak energy of their spectrum
- Gamma-Ray Bursts in the Swift Era
- The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation
- Dissipative Photosphere Models of Gamma-ray Bursts and X-ray Flashes
- The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications
- The Hubble Diagram to Redshift >6 from 69 Gamma-Ray Bursts
- An analysis of gamma-ray burst spectral break models
- Are the hosts of Gamma-Ray Bursts sub-luminous and blue galaxies?
- Linear Polarization and Proper Motion in The Afterglow of Beamed GRBs
- Is Thermal Emission in Gamma-Ray Bursts Ubiquitous?
- Physical Parameters for the Afterglows of GRB 980703, 990123, 990510, and 991216 Determined from Modeling of Multi-Frequency Data
- Probing Cosmic Chemical Evolution with Gamma-Ray Bursts: GRB060206 at z=4.048
- Thermalization in Relativistic Outflows and the Correlation between Spectral Hardness and Apparent Luminosity in Gamma-ray Bursts
- Gamma-Ray Burst Hubble Diagram to z=4.5
- The Diversity of Gamma-Ray Bursts and the Surroundings of Massive Stars
- On the nature of nearby GRB/SN host galaxies
- Detection of Wolf-Rayet stars in host galaxies of Gamma-Ray Bursts (GRBs): are GRBs produced by runaway massive stars ejected from high stellar density regions ?
- Deceleration of a Relativistic, Photon-Rich Shell: End of Preacceleration, Damping of MHD Turbulence, and the Emission Mechanism of Gamma-Ray Bursts
- The Luminosity - E_p Relation within Gamma--Ray Bursts and Implications for Fireball Models
- Confirming the gamma-ray burst spectral-energy correlations in the era of multiple time breaks
- Probing the existence of the E_peak-E_iso correlation in long Gamma Ray Bursts
- Jets, Structured Outflows, and Energy Injection in GRB Afterglows: Numerical Modelling
- A Spectacular Radio Flare from XRF 050416a at 40 days and Implications for the Nature of X-ray Flashes
- SDSS 0809+1729: Connections Between Extremely Metal Poor Galaxies and Gamma Ray Burst Hosts
- A Unified Jet Model of X-Ray Flashes and Gamma-Ray Bursts
- Two extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey
- Variation of the Amati Relation with the Cosmological Redshift: a Selection Effect or an Evolution Effect?
- Significant evolution of the stellar mass-metallicity relation since z~0.65
- The host of GRB/XRF 030528 - an actively star forming galaxy at z=0.782
- GRB 050223: A dark GRB in a dusty starburst galaxy
- Intrinsic spectra and energetics of cosmological Gamma-Ray Bursts
Cited by in corpus (3)
- Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
- Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
- Standardizing the GRBs with the Amati Ep,i - Eiso relation: the updated Hubble diagram and implications for cosmography