The First Detection of a Pulsar with ALMA
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00540169" target="_blank" >RIV/67985815:_____/17:00540169 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3847/2041-8213/aa9c3e" target="_blank" >https://doi.org/10.3847/2041-8213/aa9c3e</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/2041-8213/aa9c3e" target="_blank" >10.3847/2041-8213/aa9c3e</a>
Alternative languages
Result language
angličtina
Original language name
The First Detection of a Pulsar with ALMA
Original language description
We used the Atacama Large Millimeter/submillimeter Array (ALMA) to observe the Vela pulsar (PSR B0833-45), one of the very few observed in radio and from the mid-IR up to the very high-energy gamma-rays. We detected Vela at frequencies of 97.5, 145, 233, and 343.5 GHz, which makes it the first pulsar ever detected with ALMA. Its energy density spectrum follows a power law of spectral index alpha = -0.93 +/- 0.16.
Czech name
—
Czech description
—
Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
—
Others
Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal
ISSN
1538-4357
e-ISSN
—
Volume of the periodical
851
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
6
Pages from-to
L10
UT code for WoS article
000417542100010
EID of the result in the Scopus database
2-s2.0-85039148552