Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329

Stanek, K. Z.; Matheson, T.; Garnavich, P.; Martini, Paul; Berlind, P.; Caldwell, Nelson; Challis, Peter; Brown, Warren R.; Schild, Rudolph E.; Krisciunas, K.; Calkins, M.; Lee, Janice; Hathi, N. P.; Jansen, Rolf A.; Windhorst, Rogier A.; Echevarria, L.; Eisenstein, Daniel J.; Pindor, B.; Olszewski, Edward W.; Harding, Paul; Holland, S. T.; Bersier, D.

doi:10.1086/376976

Cited by 1,188 publications

(1,093 citation statements)

References 31 publications

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“…Observationally, all known supernova counterparts of GRBs are Type Ic, with the implication that the dying star lacked an outer hydrogen/helium envelope [16]. The winds of Wolf-Rayet stars, which are typically the cause of the loss of this envelope, are known to increase in strength with stellar metallicity (particularly iron) [44].…”

Section: Metals and The Predicted Grb Ratementioning

confidence: 99%

Enhanced cosmological GRB rates and implications for cosmogenic neutrinos

Yüksel

Kistler

2007

Phys. Rev. D

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Gamma-ray bursts, which are among the most violent events in the Universe, are one of the few viable candidates to produce ultra high-energy cosmic rays. Recently, observations have revealed that GRBs generally originate from metal-poor, low-luminosity galaxies and do not directly trace cosmic star formation, as might have been assumed from their association with core-collapse supernovae. Several implications follow from these findings. The redshift distribution of observed GRBs is expected to peak at higher redshift (compared to cosmic star formation), which is supported by the mean redshift of the Swift GRB sample, hzi 3. If GRBs are, in fact, the source of the observed UHECR, then cosmic-ray production would evolve with redshift in a stronger fashion than has been previously suggested. This necessarily leads, through the GZK process, to an enhancement in the flux of cosmogenic neutrinos, providing a near-term approach for testing the gamma-ray burst-cosmic-ray connection with ongoing and proposed UHE neutrino experiments.

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Section: Metals and The Predicted Grb Ratementioning

confidence: 99%

Enhanced cosmological GRB rates and implications for cosmogenic neutrinos

Yüksel

Kistler

2007

Phys. Rev. D

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“…LGRBs have been associated to supernovae (Galama et al 1999;Stanek et al 2003;Hjorth et al 2003;Matheson et al 2003), all of which lacked any hydrogen or helium lines and so were of the type-Ib/c (e.g., Filippenko 1997). In combination with the fact that any outer hydrogen layer of the star would stop the LGRB escaping (MacFadyen & Woosley 1999), means that the hydrogen envelope of the progenitor has to be lost before it undergoes gravitational collapse.…”

Section: Manymentioning

confidence: 99%

“…The association of LGRBs with the death of massive stars (Galama et al 1999;Stanek et al 2003;Hjorth et al 2003;Matheson et al 2003) facilitates their use as star formation tracers and their naturally luminous nature would complement or even surpass conventional methods at high redshift. However, before this connection can be used routinely and robustly, the way in which they trace one another must be known accurately.…”

Section: Manymentioning

confidence: 99%

The First Billion Years project: gamma-ray bursts at z > 5

Elliott

Khochfar

Greiner

et al. 2014

Monthly Notices of the Royal Astronomical Society

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Long gamma-ray burst's (LGRB's) association to the death of massive stars suggest they could be used to probe the cosmic star formation history (CSFH) with high accuracy, due to their high luminosities. We utilise cosmological simulations from the First Billion Years project to investigate the biases between the CSFH and the LGRB rate at z > 5, assuming various different models and constraints on the progenitors of LGRBs. We populate LGRBs using a selection based on environmental properties and demonstrate that the LGRB rate should trace the CSFH to high redshifts. The measured LGRB rate suggests that LGRBs have opening angles of θ jet = 0.1 • , although the degeneracy with the progenitor model cannot rule out an underlying bias. We demonstrate that proxies that relate the LGRB rate with global LGRB host properties do not reflect the underlying LGRB environment, and are in fact a result of the host galaxy's spatial properties, such that LGRBs can exist in galaxies of solar metallicity. However, we find a class of host galaxies that have low stellar mass and are metal-rich, and that their metallicity dispersions would not allow low-metallicity environments. Detection of hosts with this set of properties would directly reflect the progenitor's environment. We predict that 10% of LGRBs per year are associated with this set of galaxies that would have forbidden line emission that could be detected by instruments on the James Webb Space Telescope. Such a discovery would place strong constraints on the collapsar model and suggest other avenues to be investigated.

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“…Table 1 shows the list of the spectroscopically identified SN-GRB samples in this work. Three GRBs -030329, 060218, and 100316D (bold fonts in the table) -have secure associations with supernovae since a spectral evolution from a non-thermal power-law to a supernova-like thermal feature is clearly seen in the optical spectroscopic observations (e.g., Stanek et al 2003, Hjorth et al 2003 for GRB 030329; e.g., Pian et al 2006 for GRB 060218; e.g., Chornock et al 2011 for GRB 100316D). …”

Section: Introductionmentioning

confidence: 97%

GRB Prompt X-ray Emission

Sakamoto

2011

Proc. IAU

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Abstract. I present the observational properties of the prompt emission of supernova associated GRBs (SN-GRBs) focusing on temporal and spectral characteristics. I compare the properties of SN-GRBs with typical long GRBs to see whether there is a distinct difference or not. Furthermore, I present our attempt to search for hard X-ray emission prior to the discovery date from optically identified type Ibc supernovae using Swift BAT survey data.

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Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329

Cited by 1,188 publications

References 31 publications

Enhanced cosmological GRB rates and implications for cosmogenic neutrinos

Enhanced cosmological GRB rates and implications for cosmogenic neutrinos

The First Billion Years project: gamma-ray bursts at z > 5

GRB Prompt X-ray Emission

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