English
Related papers

Related papers: Construction and Preliminary Application of the Va…

200 papers

We present a possible Cepheid-like luminosity estimator for the long-duration gamma-ray bursts based on the variability of their light curves.

Astrophysics · Physics 2009-11-06 Daniel E. Reichart , Donald Q. Lamb

We present a possible Cepheid-like luminosity estimator for the long gamma-ray bursts based on the variability of their light curves. To construct the luminosity estimator, we use CGRO/BATSE data for 13 bursts, Wind/KONUS data for 5 bursts,…

We use the possible Cepheid-like luminosity estimator for the long-duration gamma-ray bursts (GRBs) developed by Reichart et al. (2000) to estimate the intrinsic luminosity, and thus the redshift, of 907 long-duration GRBs from the BATSE 4B…

Astrophysics · Physics 2009-11-07 Timothy Donaghy , Donald Q. Lamb , Daniel E. Reichart , Carlo Graziani

We have applied the proposed variability -> luminosity indicator to ten "X-Ray Flashes" (XRFs) observed by the Wide-Field Cameras on BeppoSAX for which BATSE survey data exists. Our results suggest that the variability -> luminosity…

Astrophysics · Physics 2007-05-23 D. E. Reichart , D. Q. Lamb , R. M. Kippen , J. Heise , J. J. M. in't Zand , M. Nysewander

Two different luminosity indicators have been recently proposed for Gamma Ray Bursts that use the lag between light curve peaks with hard and soft photons as well as the variability ('spikiness') of the burst light curve. Schaefer, Deng, &…

Astrophysics · Physics 2007-05-23 Bradley E. Schaefer

At the dawn of the gamma-ray burst (GRB) afterglow era, a Cepheid-like correlation was discovered between time variability V and isotropic-equivalent peak luminosity Liso of the prompt emission of about a dozen long GRBs with measured…

The low energy spectra of some gamma-ray bursts' show excess components beside the power-law dependence. The consequences of such a feature allows to estimate the gamma photometric redshift of the long gamma-ray bursts in the BATSE Catalog.…

Astrophysics · Physics 2007-05-23 Z. Bagoly , I. Csabai , A. Meszaros , P. Meszaros , I. Horvath , L. G. Balazs , R. Vavrek

We show that the time variability of a gamma-ray burst (GRB) appears to be correlated with the absolute luminosity of the burst: smooth bursts are intrinsically less luminous. This Cepheid-like relationship can be used to determine the…

Astrophysics · Physics 2007-05-23 E. E. Fenimore , E. Ramirez-Ruiz

We present results from a detailed analysis of theoretical and observed light curves of classical Cepheid variables in the Galaxy and the Magellanic Clouds. Theoretical light curves of Cepheid variables are based on non-linear convective…

Astrophysics of Galaxies · Physics 2019-09-04 A. Bhardwaj , S. M. Kanbur , M. Marconi , H. P. Singh , M. Rejkuba , C. -C. Ngeow

We have analyzed the 241 bursts for which peak counts $\C$ exist in the publicly available Burst and Transient Source Experiment (BATSE) catalog. Introducing peak counts in 1024 ms as a measure of burst brightness $\B$ and the ratio of peak…

Astrophysics · Physics 2009-10-22 D. Q. Lamb , C. Graziani , I. A. Smith

A new procedure for smoothing a gamma-ray burst (GRB) lightcurve and calculating its variability is presented. Applying the procedure to a sample of 25 long GRBs, we have obtained a very tight correlation between the variability and the…

Astrophysics · Physics 2009-11-13 Li-Xin Li , Bohdan Paczynski

Simple hardness ratios are found to be a good estimator for the spectral peak energy in Gamma-Ray Bursts (GRBs). Specifically, a high correlation strength is found between the $\nu F_{\nu}$ peak in the spectrum of BATSE GRBs, $\epo$, and…

High Energy Astrophysical Phenomena · Physics 2018-02-05 Amir Shahmoradi , Robert J. Nemiroff

Within the framework of the internal shock model, we study the luminosity and the variability in gamma-ray bursts from collimated fireballs. In particular we pay attention to the role of the photosphere due to $e^\pm$ pairs produced by…

Astrophysics · Physics 2009-11-07 Shiho Kobayashi , Felix Ryde , Andrew MacFadyen

We propose a new empirical redshift indicator for gamma-ray bursts. This indicator is easily computed from the gamma-ray burst spectral parameters, and its duration, and it provides ``pseudo-redshifts'' accurate to a factor two. Possible…

Astrophysics · Physics 2009-11-07 J-L Atteia

Gamma-ray bursts of short duration may harbor vital clues to the range of phenomena producing bursts. However, recent progress from the observation of optical counterparts has not benefitted the study of short bursts. We have searched for…

The measure of the distances and luminosities of gamma-ray bursts (GRBs) led to the discovery that many GRB properties are strongly correlated with their intrinsic luminosity, leading to the construction of reliable luminosity indicators.…

Astrophysics · Physics 2010-11-11 J-L. Atteia

A gravitationally lensed gamma-ray burst (GRB) would appear as multiple bursts with identical light curves, separated in time and differing only by the scaling of their amplitudes. However, noise may make them difficult to identify as…

Astrophysics · Physics 2009-10-22 M. A. Nowak , S. A. Grossman

An analysis of the observed characteristics of the Galactic Cepheid variables is carried out in the framework of their period-luminosity relation being used as a standard candle for distance measurement. The variation of the observed number…

Astrophysics · Physics 2007-05-23 Anwesh Mazumdar , D. Narasimha

We are conducting a long-term photometric survey of the nearby galaxy M33 to discover Cepheids, eclipsing binaries, and long-period variables. The dataset combines previously-obtained optical images from the DIRECT project with new…

Solar and Stellar Astrophysics · Physics 2015-05-13 Anne Pellerin , Lucas M. Macri , Andrew K. Bradshaw , Krzysztof Z. Stanek

It is known that the soft tail of the gamma-ray bursts' spectra show excesses from the exact power-law dependence. In this article we show that this departure can be detected in the peak flux ratios of different BATSE DISCSC energy…

Astrophysics · Physics 2009-11-07 Z. Bagoly , I. Csabai , A. Mészáros , P. Mészáros , I. Horváth , L. G. Balázs , R. Vavrek
‹ Prev 1 2 3 10 Next ›