Example of Frontiers in Astronomy and Space Sciences format
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Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format Example of Frontiers in Astronomy and Space Sciences format
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open access Open Access

Frontiers in Astronomy and Space Sciences — Template for authors

Publisher: Frontiers Media
Categories Rank Trend in last 3 yrs
Astronomy and Astrophysics #23 of 88 down down by None rank
journal-quality-icon Journal quality:
Good
calendar-icon Last 4 years overview: 194 Published Papers | 1003 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 29/06/2020
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Related Journals

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Quality:  
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CiteRatio: 9.2
SJR: 2.067
SNIP: 0.962
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CiteRatio: 4.1
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open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.6
SJR: 0.682
SNIP: 1.274

Journal Performance & Insights

CiteRatio

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

A measure of average citations received per peer-reviewed paper published in the journal.

Measures weighted citations received by the journal. Citation weighting depends on the categories and prestige of the citing journal.

Measures actual citations received relative to citations expected for the journal's category.

5.2

108% from 2019

CiteRatio for Frontiers in Astronomy and Space Sciences from 2016 - 2020
Year Value
2020 5.2
2019 2.5
graph view Graph view
table view Table view

1.13

87% from 2019

SJR for Frontiers in Astronomy and Space Sciences from 2019 - 2020
Year Value
2020 1.13
2019 0.605
graph view Graph view
table view Table view

0.928

89% from 2019

SNIP for Frontiers in Astronomy and Space Sciences from 2019 - 2020
Year Value
2020 0.928
2019 0.492
graph view Graph view
table view Table view

insights Insights

  • CiteRatio of this journal has increased by 108% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

insights Insights

  • SJR of this journal has increased by 87% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 89% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Frontiers in Astronomy and Space Sciences

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Frontiers Media

Frontiers in Astronomy and Space Sciences

Frontiers in Astronomy and Space Sciences aims to provide rapid dissemination of peer-reviewed, cutting-edge research addressing any area of astronomy, astrophysics and space sciences. To accomplish its goals it embraces a combination of gold open access and an interactive rev...... Read More

Optics and Photonics

i
Last updated on
29 Jun 2020
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ISSN
2296-987X
i
Open Access
Yes
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
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Endnote Style
Download Available
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Bibliography Name
frontiersinSCNS_ENG_HUMS
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Citation Type
Numbered
[25]
i
Bibliography Example
Blonder GE, Tinkham M, Klapwijk TM. Transition from metallic to tunneling regimes in superconducting microconstrictions: Excess current, charge imbalance, and supercurrent conversion. Phys. Rev. B 25 (1982) 4515–4532.

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.3389/FSPAS.2018.00036
Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
Pablo F. de Salas1, S. Gariazzo1, Olga Mena1, C. A. Ternes1, Mariam Tórtola1

Abstract:

The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector The extraction of the neutrino mass ordering is a data-driven field e... The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector The extraction of the neutrino mass ordering is a data-driven field expected to evolve very rapidly in the next decade In this review, we both analyze the present status and describe the physics of subsequent prospects Firstly, the different current available tools to measure the neutrino mass ordering are described Namely, reactor, long-baseline (accelerator and atmospheric) neutrino beams, laboratory searches for beta and neutrinoless double beta decays and observations of the cosmic background radiation and the large scale structure of the universe are carefully reviewed Secondly, the results from an up-to-date comprehensive global fit are reported: the Bayesian analysis to the 2018 publicly available oscillation and cosmological data sets provides strong evidence for the normal neutrino mass ordering versus the inverted scenario, with a significance of 35 standard deviations This preference for the normal neutrino mass ordering is mostly due to neutrino oscillation measurements Finally, we shall also emphasize the future perspectives for unveiling the neutrino mass ordering In this regard, apart from describing the expectations from the aforementioned probes, we also focus on those arising from alternative and novel methods, as 21 cm cosmology, core-collapse supernova neutrinos and the direct detection of relic neutrinos read more read less

Topics:

Neutrino oscillation (70%)70% related to the paper, Neutrino (69%)69% related to the paper, Lepton (56%)56% related to the paper, Physics beyond the Standard Model (53%)53% related to the paper, Cosmic background radiation (51%)51% related to the paper
View PDF
206 Citations
open accessOpen access Journal Article DOI: 10.3389/FSPAS.2018.00047
An asymptotically safe guide to quantum gravity and matter
Astrid Eichhorn1

Abstract:

Asymptotic safety generalizes asymptotic freedom and could contribute to understanding physics beyond the Standard Model. It is a candidate scenario to provide an ultraviolet extension for the effective quantum field theory of gravity through an interacting fixed point of the Renormalization Group. Recently, asymptotic safety... Asymptotic safety generalizes asymptotic freedom and could contribute to understanding physics beyond the Standard Model. It is a candidate scenario to provide an ultraviolet extension for the effective quantum field theory of gravity through an interacting fixed point of the Renormalization Group. Recently, asymptotic safety has been established in specific gauge-Yukawa models in four dimensions in perturbation theory, providing a starting point for asymptotically safe model building. Moreover, an asymptotically safe fixed point might even be induced in the Standard Model under the impact of quantum fluctuations of gravity in the vicinity of the Planck scale. This review contains an overview of the key concepts of asymptotic safety, its application to matter and gravity models, exploring potential phenomenological implications and highlighting open questions. read more read less

Topics:

Asymptotic safety in quantum gravity (67%)67% related to the paper, Quantum gravity (65%)65% related to the paper, Asymptotic freedom (58%)58% related to the paper, Physics beyond the Standard Model (55%)55% related to the paper, Quantum field theory (55%)55% related to the paper
View PDF
196 Citations
open accessOpen access Journal Article DOI: 10.3389/FSPAS.2018.00044
Dark Energy in Light of Multi-Messenger Gravitational-Wave Astronomy
Jose María Ezquiaga1, Miguel Zumalacárregui2, Miguel Zumalacárregui3

Abstract:

Author(s): Ezquiaga, JM; Zumalacarregui, M | Abstract: Gravitational waves (GWs) provide a new tool to probe the nature of dark energy (DE) and the fundamental properties of gravity. We review the different ways in which GWs can be used to test gravity and models for late-time cosmic acceleration. Lagrangian-based gravitation... Author(s): Ezquiaga, JM; Zumalacarregui, M | Abstract: Gravitational waves (GWs) provide a new tool to probe the nature of dark energy (DE) and the fundamental properties of gravity. We review the different ways in which GWs can be used to test gravity and models for late-time cosmic acceleration. Lagrangian-based gravitational theories beyond general relativity (GR) are classified into those breaking fundamental assumptions, containing additional fields and massive graviton(s). In addition to Lagrangian based theories we present the effective theory of DE and the μ-Σ parametrization as general descriptions of cosmological gravity. Multi-messenger GW detections can be used to measure the cosmological expansion (standard sirens), providing an independent test of the DE equation of state and measuring the Hubble parameter. Several key tests of gravity involve the cosmological propagation of GWs, including anomalous GW speed, massive graviton excitations, Lorentz violating dispersion relation, modified GW luminosity distance and additional polarizations, which may also induce GW oscillations. We summarize present constraints and their impact on DE models, including those arising from the binary neutron star merger GW170817. Upgrades of LIGO-Virgo detectors to design sensitivity and the next generation facilities such as LISA or Einstein Telescope will significantly improve these constraints in the next two decades. read more read less

Topics:

General relativity (61%)61% related to the paper, Gravitational wave (59%)59% related to the paper, Dark energy (59%)59% related to the paper, Einstein Telescope (58%)58% related to the paper, Graviton (58%)58% related to the paper
View PDF
182 Citations
open accessOpen access Journal Article DOI: 10.3389/FSPAS.2019.00005
The role of magnetic field in molecular cloud formation and evolution
Patrick Hennebelle1, Patrick Hennebelle2, Shu-ichiro Inutsuka3

Abstract:

We review the role that magnetic field may have on the formation and evolution of molecular clouds. After a brief presentation and main assumptions leading to ideal MHD equations, their most important correction, namely the ion-neutral drift is described. The nature of the multi-phase interstellar medium (ISM) and the thermal... We review the role that magnetic field may have on the formation and evolution of molecular clouds. After a brief presentation and main assumptions leading to ideal MHD equations, their most important correction, namely the ion-neutral drift is described. The nature of the multi-phase interstellar medium (ISM) and the thermal processes that allows this gas to become denser are presented. Then we discuss our current knowledge of compressible magnetized turbulence, thought to play a fundamental role in the ISM. We also describe what is known regarding the correlation between the magnetic and the density fields. Then the influence that magnetic field may have on the interstellar filaments and the molecular clouds is discussed, notably the role it may have on the prestellar dense cores as well as regarding the formation of stellar clusters. Finally we briefly review its possible effects on the formation of molecular clouds themselves. We argue that given the magnetic intensities that have been measured, it is likely that magnetic field is i) responsible of reducing the star formation rate in dense molecular cloud gas by a factor of a few, ii) strongly shaping the interstellar gas by generating a lot of filaments and reducing the numbers of clumps, cores and stars, although its exact influence remains to be better understood. Moreover at small scales, magnetic braking is likely a dominant process that strongly modifies the outcome of the star formation process. Finally, we stress that inducing the formation of more massive stars, magnetic field could possibly enhance the impact of stellar feedback. read more read less

Topics:

Star formation (62%)62% related to the paper, Molecular cloud (61%)61% related to the paper, Interstellar medium (57%)57% related to the paper, Magnetohydrodynamics (51%)51% related to the paper
View PDF
143 Citations
open accessOpen access Journal Article DOI: 10.3389/FSPAS.2019.00023
Open questions in cosmic-ray research at ultrahigh energies

Abstract:

We review open questions and prospects for progress in ultrahigh-energy cosmic ray (UHECR) research, based on a series of discussions that took place during the “The High-Energy Universe: Gamma-Ray, Neutrino, and Cosmic-ray Astronomy” MIAPP workshop in 2018. Specifically, we overview open questions on the origin of the bulk o... We review open questions and prospects for progress in ultrahigh-energy cosmic ray (UHECR) research, based on a series of discussions that took place during the “The High-Energy Universe: Gamma-Ray, Neutrino, and Cosmic-ray Astronomy” MIAPP workshop in 2018. Specifically, we overview open questions on the origin of the bulk of UHECRs, the UHECR mass composition, the origin of the end of the cosmic-ray spectrum, the transition from Galactic to extragalactic cosmic rays, the effect of magnetic fields on the trajectories of UHECRs, anisotropy expectations for specific astrophysical scenarios, hadronic interactions, and prospects for discovering neutral particles as well as new physics at ultrahigh energies. We also briefly overview upcoming and proposed UHECR experiments and discuss their projected science reach. read more read less

Topics:

Cosmic ray (52%)52% related to the paper, Neutrino (51%)51% related to the paper
View PDF
136 Citations
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Frontiers in Astronomy and Space Sciences format uses frontiersinSCNS_ENG_HUMS citation style.

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Frequently asked questions

1. Can I write Frontiers in Astronomy and Space Sciences in LaTeX?

Absolutely not! Our tool has been designed to help you focus on writing. You can write your entire paper as per the Frontiers in Astronomy and Space Sciences guidelines and auto format it.

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Yes, the template is compliant with the Frontiers in Astronomy and Space Sciences guidelines. Our experts at SciSpace ensure that. If there are any changes to the journal's guidelines, we'll change our algorithm accordingly.

3. Can I cite my article in multiple styles in Frontiers in Astronomy and Space Sciences?

Of course! We support all the top citation styles, such as APA style, MLA style, Vancouver style, Harvard style, and Chicago style. For example, when you write your paper and hit autoformat, our system will automatically update your article as per the Frontiers in Astronomy and Space Sciences citation style.

4. Can I use the Frontiers in Astronomy and Space Sciences templates for free?

Sign up for our free trial, and you'll be able to use all our features for seven days. You'll see how helpful they are and how inexpensive they are compared to other options, Especially for Frontiers in Astronomy and Space Sciences.

5. Can I use a manuscript in Frontiers in Astronomy and Space Sciences that I have written in MS Word?

Yes. You can choose the right template, copy-paste the contents from the word document, and click on auto-format. Once you're done, you'll have a publish-ready paper Frontiers in Astronomy and Space Sciences that you can download at the end.

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It only takes a matter of seconds to edit your manuscript. Besides that, our intuitive editor saves you from writing and formatting it in Frontiers in Astronomy and Space Sciences.

7. Where can I find the template for the Frontiers in Astronomy and Space Sciences?

It is possible to find the Word template for any journal on Google. However, why use a template when you can write your entire manuscript on SciSpace , auto format it as per Frontiers in Astronomy and Space Sciences's guidelines and download the same in Word, PDF and LaTeX formats? Give us a try!.

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Of course! You can do this using our intuitive editor. It's very easy. If you need help, our support team is always ready to assist you.

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SciSpace's Frontiers in Astronomy and Space Sciences is currently available as an online tool. We're developing a desktop version, too. You can request (or upvote) any features that you think would be helpful for you and other researchers in the "feature request" section of your account once you've signed up with us.

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After writing your paper autoformatting in Frontiers in Astronomy and Space Sciences, you can download it in multiple formats, viz., PDF, Docx, and LaTeX.

12. Is Frontiers in Astronomy and Space Sciences's impact factor high enough that I should try publishing my article there?

To be honest, the answer is no. The impact factor is one of the many elements that determine the quality of a journal. Few of these factors include review board, rejection rates, frequency of inclusion in indexes, and Eigenfactor. You need to assess all these factors before you make your final call.

13. What is Sherpa RoMEO Archiving Policy for Frontiers in Astronomy and Space Sciences?

SHERPA/RoMEO Database

We extracted this data from Sherpa Romeo to help researchers understand the access level of this journal in accordance with the Sherpa Romeo Archiving Policy for Frontiers in Astronomy and Space Sciences. The table below indicates the level of access a journal has as per Sherpa Romeo's archiving policy.

RoMEO Colour Archiving policy
Green Can archive pre-print and post-print or publisher's version/PDF
Blue Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
Yellow Can archive pre-print (ie pre-refereeing)
White Archiving not formally supported
FYI:
  1. Pre-prints as being the version of the paper before peer review and
  2. Post-prints as being the version of the paper after peer-review, with revisions having been made.

14. What are the most common citation types In Frontiers in Astronomy and Space Sciences?

The 5 most common citation types in order of usage for Frontiers in Astronomy and Space Sciences are:.

S. No. Citation Style Type
1. Author Year
2. Numbered
3. Numbered (Superscripted)
4. Author Year (Cited Pages)
5. Footnote

15. How do I submit my article to the Frontiers in Astronomy and Space Sciences?

It is possible to find the Word template for any journal on Google. However, why use a template when you can write your entire manuscript on SciSpace , auto format it as per Frontiers in Astronomy and Space Sciences's guidelines and download the same in Word, PDF and LaTeX formats? Give us a try!.

16. Can I download Frontiers in Astronomy and Space Sciences in Endnote format?

Yes, SciSpace provides this functionality. After signing up, you would need to import your existing references from Word or Bib file to SciSpace. Then SciSpace would allow you to download your references in Frontiers in Astronomy and Space Sciences Endnote style according to Elsevier guidelines.

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