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We present a possible Cepheid-like luminosity estimator for the long-duration gamma-ray bursts based on the variability of their light curves. We also present a preliminary application of this luminosity estimator to 907 long-duration…

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

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

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

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 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

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 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 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

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

I show how an empirical variability - luminosity relationship for prompt gamma-ray bursts, first proposed by Fenimore and Ramirez-Ruiz, can be understood as a special-relativistic beaming effect in the ``cannonball model'' of Dar and De…

Astrophysics · Physics 2009-10-31 R. Plaga

The gamma-ray burst's lightcurves have been analyzed using a special wavelet transformation. The applied wavelet base is based on a typical Fast Rise-Exponential Decay (FRED) pulse. The shape of the wavelet coefficients' total distribution…

Astrophysics · Physics 2010-12-13 Z. Bagoly , I. Horvath , A. Meszaros , L. G. Balazs

Using the Euclidean value of <V/Vmax> as a cosmological distance indicator, we derive the isotropic-equivalent characteristic peak luminosity of gamma-ray bursts both longer and shorter than 2 s. The short bursts have essentially the same…

Astrophysics · Physics 2009-11-07 Maarten Schmidt

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 present a technique for decomposing Cepheid light curves into their fundamental constituent parts; that is, their radius and temperature variations. We demonstrate that any given pair of optical luminosity and color curves can be used to…

Solar and Stellar Astrophysics · Physics 2015-05-19 Wendy L. Freedman , Barry F. Madore

We have investigated the time variations in the light curves from a sample of long and short Fermi/GBM Gamma ray bursts (GRBs) using an impartial wavelet analysis. The results indicate that in the source frame, the variability time scales…

High Energy Astrophysical Phenomena · Physics 2015-06-03 G. A. MacLachlan , A. Shenoy , E. Sonbas , K. S. Dhuga , B. Cobb , T. N. Ukwatta , D. C. Morris , A. Eskandarian , L. C. Maximon , W. C. Parke

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

In almost any scenario for 'cosmological' gamma-ray bursts (and in many models where they originate in our own Galaxy), the initial energy density is so large that the resulting relativistic plasma expands with $v\sim c$ producing a blast…

Astrophysics · Physics 2009-10-22 P. Meszaros , M. J. Rees

We calculate the spectra expected from unsteady relativistic wind models of gamma-ray bursts, suitable for events of arbitrary duration. The spectral energy distribution of the burst is calculated over photon energies spanning from eV to…

Astrophysics · Physics 2009-10-28 Hara Papathanassiou , Peter Meszaros
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