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1. Inflection Points on the Light Curves of Type Ia Supernovae

   While the distribution of supernova absolute magnitudes at peak is often investigated, there was no systematic study of absolute light curve behavior...

   N. N. Pavliouk, D. Yu Tsvetkov in From Twilight to Highlight: The Physics of Supernovae

   Conference paper
   

2. The Nearby Supernova Factory

   The Nearby Supernova Factory is an international project dedicated to the study of the nearby thermonuclear (type Ia) supernovæ. Based upon the NEAT...

   Emmanuel Pécontal, Greg Aldering, ... Michael Wood-Vasey in From Twilight to Highlight: The Physics of Supernovae

   Conference paper
   

3. The HETE Triggering Algorithm

   The High Energy Transient Explorer uses a triggering algorithm for gammaray bursts that can achieve near the statistical limit by fitting to several...

   E. E. Fenimore, M. Galassi in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

4. Progress on MARGIE, a Gamma-Ray Burst Ultra-long Duration Balloon Mission

   We are designing the Minute of Arc Resolution Gamma-ray Imaging Experiment (MARGIE) as a 100 day Ultra Long Duration Balloon (ULDB) mission to: a)...

   D. Band, M. Cherry, ... J. Matteson in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

5. Statistics of Faint Variable Sources for GRB OA Analyses

   In GRB Optical Afterglows analyses, good knowledge and statistics of variable background sources is required. For statistical analyses of faint...

   Jiri Polcar, Rene Hudec, Helmut Meusinger in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

6. Analysis of the BATSE GRB Light Curves

   Different progenitors and physicalpro cesses could be at the origin of GRBs. New information about the properties of the gamma-ray emission can help...

   B. M. Belli in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

7. New Version of Optical Transient Monitor for BOOTES Project

   We present controlling software for two wide field cameras of BOOTES station in this paper. Optical Transient Monitor (OTM) system is prepared for...

   Petr Páta, Martin Bernas, ... René Hudec in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

8. A Gamma-Ray Bursts’ Fluence-Duration Correlation

   We present an analysis indicating that there is a correlation between the fluences and the durations of gamma-ray bursts, and provide arguments that...

   István Horváth, Lajos G. Balázs, ... Attila Mészáros in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

9. The Unique Signature of Shell Curvature in Gamma-Ray Bursts

   As a result of sphericalkinematics, temporalev olution of received gammaray emission should demonstrate signatures of curvature from the emitting...

   Alicia Margarita Soderberg, Edward E. Fenimore in Gamma-Ray Bursts in the Afterglow Era

   Conference paper
   

10. Estimation of Emission Time Parameter for APEX Experiment

    The data on gamma-ray bursts are presented collected by Russian-France APEX experiment on Phobos-2 interplanetary spacecraft. The values of emission...

    Alexandr Kozyrev, Igor Mitrofanov, ... Claude Barat in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

11. Broadband Spectral Deconvolution of GRBs

    Data from GRBs which occurred in the field of view of COMPTEL have been jointly analysed with the corresponding BATSE data using the Band spectral...

    L. Hanlon, D. Kinsella, ... R. Preece in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

12. X-Ray Flashes and X-Ray Rich Gamma Ray Bursts

    X-ray flashes are detected in the Wide Field Cameras on BeppoSAX in the energy range 2-25 keV as bright X-ray sources lasting of the order of...

    John Heise, Jean in ’t. Zand, ... Peter M. Woods in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

13. Hypernovae and Gamma-Ray Bursts

    Recently, there have been a number of candidates for the gamma-ray burst (GRB)/supernova (SN) connection (see Nomoto et al. 2001 for references)....

    P. A. Mazzali, K. Nomoto, ... T. Nakamura in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

14. GRB Optical Afterglows: Correlation between Pair of Parameters

    Parameters of 22 GRBs are analysed. Correlations between energies and luminosities in optical and...

    Corrado Bartolini, Gregory Beskin, ... Aleksej Pozanenko in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

15. Theoretical Implications of the Gamma-Ray Burst-Supernova Connection

    Although observations of circumstellar shock interactions around supernovae are generally consistent with a...

    Roger A. Chevalier in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

16. The Multiband Photometry of GRB Host Galaxies: Comparison with the Spectral Energy Distributions of Nearby Galaxies and Theoretical Modeling

    We present one of the results of BV RI photometry of the hosts of GRB for the host galaxy of GRB 970508 and the theoretical modeling of its continuum...

    V. V. Sokolov, T. A. Fatkhullin, ... V. I. Korchagin in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

17. Early Afterglows as Probes for the Reionization Epoch

    The nature of Gamma-Ray Burst (GRB) progenitors is still a debated issue, but consensus is growing on the association of GRBs with massive stars....

    Davide Lazzati, Gabriele Ghisellini, ... Alberto Fernández-Soto in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

18. Host Galaxies as Gamma-Ray Burst Distance Indicators

    We calculate the distributions of the total burst energy, the peak luminosity and the X-ray afterglow energy using burst observations and distances...

    David Band, Raul Jimenez, Tsvi Piran in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

19. Observational Consequences of $e^\pm$ Pair Creation in $\gamma$ -Ray Bursts

    Physical models for $\gamma$ -ray emission from a relativistic...

    Enrico Ramirez-Ruiz, Piero Madau, ... Christopher Thompson in Gamma-Ray Bursts in the Afterglow Era

    Conference paper
    

20. Interaction between Internal Shocks and the Reverse Shock for a GRB in a Dense Stellar Wind

    In the most popular scenario for GRBs a relativistic shell is produced by a compact central source (collapsar, BH + WD, BH + NS or NS + NS merger)...

    Frédéric Daigne, Robert Mochkovitch in Gamma-Ray Bursts in the Afterglow Era

    Conference paper