| Title |
Accuracy in measuring the neutron star mass in the gravitational wave parameter estimation for black hole-neutron star binaries
|
|---|---|
| Published in |
Journal of the Korean Physical Society, September 2016
|
| DOI | 10.3938/jkps.69.884 |
| Authors |
Hee-Suk Cho |
X Demographics
The data shown below were collected from the profile of 1 X user who shared this research output. Click here to find out more about how the information was compiled.
Geographical breakdown
| Country | Count | As % |
|---|---|---|
| Unknown | 1 | 100% |
Demographic breakdown
| Type | Count | As % |
|---|---|---|
| Members of the public | 1 | 100% |
Attention Score in Context
This research output has an Altmetric Attention Score of 1. 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 26 July 2016.
All research outputs
#20,336,031
of 22,881,154 outputs
Outputs from Journal of the Korean Physical Society
#425
of 562 outputs
Outputs of similar age
#278,671
of 321,036 outputs
Outputs of similar age from Journal of the Korean Physical Society
#13
of 31 outputs
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So far Altmetric has tracked 562 research outputs from this source. They receive a mean Attention Score of 2.3. This one is in the 1st percentile – i.e., 1% of its peers scored the same or lower than it.
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We're also able to compare this research output to 31 others from the same source and published within six weeks on either side of this one. This one is in the 1st percentile – i.e., 1% of its contemporaries scored the same or lower than it.