Except as set forth in the Disclosure Schedule of Pantheon attached hereto as Schedule III (the “Pantheon Disclosure Schedule”), each of the Pantheon Parties, jointly and severally, represents and warrants to the Warrantors and Selling Shareholders as follows: Sample 1Sample 2Sample 3 SaveCopy ...
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We first divided the low-redshift sample of GRBs into two bins and examined the Amati relation and its potential modifications. We found that under both calibrations, the Amati relation did not show evidence of redshift evolution (68% confidence level). For the other two Amati relations that...
The value of the luminosity distance log(dL )and its error σlog(dL )(its redshift range is 0.0331 < z < 1.95) for 48 data points in the sample of Gamma-Ray Burst A118 sample. Next, we reconstruct the relation between the redshift z of type Ia supernovae and the distance modulus...
Using gamma-ray bursts as standard candles for cosmological parameter constraints rely on their empirical luminosity relations and low-redshift calibration. In this paper, we examine the Amati relation and its potential corrections based on the A118 sample of higher-quality gamma-ray bursts, using ...
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The recently released Type Ia supernovae (SNe Ia) sample, Pantheon+, is an updated version of Pantheon and has very important cosmological implications. To explore the origin of the enhanced constraining power and internal correlations of datasets in different redshifts, we perform a comprehensivel...
Very recently, the Pantheon sample consisting of 1048 type Ia supernovae (SNIa) has been released, which is the largest spectroscopically confirmed SNIa sample to date. In the present work, we test the cosmic anisotropy in the Pantheon SNIa sample by using three methods, and hence the ...