↓ Skip to main content

No supernovae associated with two long-duration γ-ray bursts

Overview of attention for article published in Nature, December 2006
Altmetric Badge

Mentioned by

wikipedia
3 Wikipedia pages

Citations

dimensions_citation
383 Dimensions

Readers on

mendeley
47 Mendeley
citeulike
1 CiteULike
You are seeing a free-to-access but limited selection of the activity Altmetric has collected about this research output. Click here to find out more.
Title
No supernovae associated with two long-duration γ-ray bursts
Published in
Nature, December 2006
DOI 10.1038/nature05375
Pubmed ID
Authors

Johan P. U. Fynbo, Darach Watson, Christina C. Thöne, Jesper Sollerman, Joshua S. Bloom, Tamara M. Davis, Jens Hjorth, Páll Jakobsson, Uffe G. Jørgensen, John F. Graham, Andrew S. Fruchter, David Bersier, Lisa Kewley, Arnaud Cassan, José María Castro Cerón, Suzanne Foley, Javier Gorosabel, Tobias C. Hinse, Keith D. Horne, Brian L. Jensen, Sylvio Klose, Daniel Kocevski, Jean-Baptiste Marquette, Daniel Perley, Enrico Ramirez-Ruiz, Maximilian D. Stritzinger, Paul M. Vreeswijk, Ralph A. M. Wijers, Kristian G. Woller, Dong Xu, Marta Zub

Abstract

It is now accepted that long-duration gamma-ray bursts (GRBs) are produced during the collapse of a massive star. The standard 'collapsar' model predicts that a broad-lined and luminous type Ic core-collapse supernova accompanies every long-duration GRB. This association has been confirmed in observations of several nearby GRBs. Here we report that GRB 060505 (ref. 10) and GRB 060614 (ref. 11) were not accompanied by supernova emission down to limits hundreds of times fainter than the archetypal supernova SN 1998bw that accompanied GRB 980425, and fainter than any type Ic supernova ever observed. Multi-band observations of the early afterglows, as well as spectroscopy of the host galaxies, exclude the possibility of significant dust obscuration and show that the bursts originated in actively star-forming regions. The absence of a supernova to such deep limits is qualitatively different from all previous nearby long-duration GRBs and suggests a new phenomenological type of massive stellar death.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 47 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United States 2 4%
China 1 2%
Germany 1 2%
Unknown 43 91%

Demographic breakdown

Readers by professional status Count As %
Researcher 18 38%
Student > Ph. D. Student 10 21%
Professor 4 9%
Student > Doctoral Student 2 4%
Student > Bachelor 2 4%
Other 4 9%
Unknown 7 15%
Readers by discipline Count As %
Physics and Astronomy 34 72%
Arts and Humanities 1 2%
Earth and Planetary Sciences 1 2%
Chemistry 1 2%
Unknown 10 21%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 3. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 14 December 2019.
All research outputs
#8,527,033
of 25,378,162 outputs
Outputs from Nature
#70,633
of 97,719 outputs
Outputs of similar age
#44,615
of 168,103 outputs
Outputs of similar age from Nature
#382
of 481 outputs
Altmetric has tracked 25,378,162 research outputs across all sources so far. This one is in the 43rd percentile – i.e., 43% of other outputs scored the same or lower than it.
So far Altmetric has tracked 97,719 research outputs from this source. They typically receive a lot more attention than average, with a mean Attention Score of 102.4. This one is in the 11th percentile – i.e., 11% of its peers scored the same or lower than it.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 168,103 tracked outputs that were published within six weeks on either side of this one in any source. This one is in the 16th percentile – i.e., 16% of its contemporaries scored the same or lower than it.
We're also able to compare this research output to 481 others from the same source and published within six weeks on either side of this one. This one is in the 9th percentile – i.e., 9% of its contemporaries scored the same or lower than it.