Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst

@article{Thone2008PhotometryAS,
  title={Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst},
  author={Christina C. Thone and David Alexander Kann and G. J'ohannesson and Josefine H. Selj and Andreas O. Jaunsen and Johan P. U. Fynbo and Carl W. Akerlof and Kiran S. Baliyan and Corrado Bartolini and Ilfan F. Bikmaev and Joshua S. Bloom and Rodion Burenin and B. E. Cobb and Stefano Covino and Peter A. Curran and H{\aa}kon Dahle and Alejandro Ferrero and Suzanne Foley and James C. French and Andrew S. Fruchter and Shashikiran Ganesh and John F. Graham and Giuseppe Greco and Adriano Guarnieri and Lorraine Hanlon and Jens Hjorth and Mansur A. Ibrahimov and Gian Luca Israel and P. Jakobsson and Martin Jel'inek and Brian L. Jensen and U. G. J{\o}rgensen and Irek M. Khamitov and T. S. Koch and Andrew J. Levan and Daniele B. Malesani and Nicola Masetti and S. Meehan and G. Melady and Domenico Nanni and Jyri Naranen and Erika Pak{\vs}tienė and Mikhail N. Pavlinsky and Daniel A. Perley and Adalberto Piccioni and Graziella Pizzichini and Alexei Pozanenko and P. W. A. Roming and Wiphu Rujopakarn and Vasilij Rumyantsev and Eli S. Rykoff and Dmitriy A. Sharapov and Dan L. Starr and Rashid Sunyaev and Heather Swan and Nial R. Tanvir and F. Terra and Paul M. Vreeswijk and A C Wilson and Scott A. Yost and Fang Yuan},
  journal={Scopus},
  year={2008}
}
Aims. With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at z = 3: 221. Methods. We present one of the largest photometric datasets ever obtained for a GRB afterglow, consisting of multi-color photometric data from the ultraviolet to the near infrared. The data set contains 4 12 data points in total to which we add additional data from the literature. Furthermore, we present low-resolution high signal-to-noise spectra… 

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References

SHOWING 1-10 OF 149 REFERENCES

The host of GRB 060206: kinematics of a distant galaxy

Context. GRB afterglow spectra are sensitive probes of interstellar matter along the line-of-sight in their host galaxies, as well as in intervening galaxies. The rapid fading of GRBs makes it very

Spectroscopy of GRB 050505 at z = 4.275: A log N(H I) = 22.1 DLA Host Galaxy and the Nature of the Progenitor

We present optical spectroscopy of the afterglow of GRB 050505 obtained with the Keck I 10 m telescope. The spectrum exhibits three absorption systems with the highest, at z = 4.2748, arising in the

Optical and X-Ray Observations of GRB 060526: A Complex Afterglow Consistent with an Achromatic Jet Break

We obtained 98 R-band and 18 B, r′, i′ images of the optical afterglow of GRB 060526 (z = 3.21) with the MDM 1.3 m, 2.4 m, and the PROMPT telescopes at CTIO over the five nights following the burst

The Detailed Optical Light Curve of GRB 030329

We present densely sampled BVRI light curves of the optical transient associated with the gamma-ray burst (GRB) 030329, the result of a coordinated observing campaign conducted at five observatories.

High-Precision Photometry of the Gamma-Ray Burst GRB 020813: The Smoothest Afterglow Yet

We report results of our precise reduction of the high signal-to-noise ratio VRI observations of the optical afterglow of the gamma-ray burst GRB 020813 obtained by Gladders & Hall with the Magellan

GRB 060605: multi-wavelength analysis of the first GRB observed using integral field spectroscopy

The long and relatively faint gamma-ray burst GRB 060605 detected by Swift/BAT lasted about 20 sec. Its afterglow could be observed with Swift/XRT for nearly 1 day, while Swift/UVOT could detect the

LOW-RESOLUTION SPECTROSCOPY OF GAMMA-RAY BURST OPTICAL AFTERGLOWS: BIASES IN THE SWIFT SAMPLE AND CHARACTERIZATION OF THE ABSORBERS

We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for which spectroscopic follow-up observations have been secured. Our first objective is to measure the

THE AFTERGLOWS OF SWIFT-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-SWIFT AND SWIFT-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

TLDR
The first indications of a class of long GRBs are presented, which form a bridge between the typical high-luminosity, high-redshift events and nearby low- luminosity events (which are also associated with spectroscopic supernovae) in terms of energetics and observed redshift distribution, indicating a continuous distribution overall.

Revealing the Jet Structure of GRB 030329 with High-Resolution Multicolor Photometry

We present multicolor optical observations of the nearby (z = 0.1685) gamma-ray burst GRB 030329 obtained with the same instrumentation over a time period of 6 hours, for a total of an unprecedented

The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125

We report on multiwavelength observations, ranging from X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the presence of absorption lines
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