Example of Monthly Notices of the Royal Astronomical Society: Letters format
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Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format
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Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format Example of Monthly Notices of the Royal Astronomical Society: Letters format
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open access Open Access

Monthly Notices of the Royal Astronomical Society: Letters — Template for authors

Categories Rank Trend in last 3 yrs
Space and Planetary Science #13 of 97 down down by 3 ranks
Astronomy and Astrophysics #13 of 88 down down by 2 ranks
journal-quality-icon Journal quality:
High
calendar-icon Last 4 years overview: 852 Published Papers | 7833 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 22/07/2020
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Related Journals

open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.1
SJR: 1.099
SNIP: 1.093
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 6.8
SJR: 1.485
SNIP: 1.164
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.6
SJR: 0.682
SNIP: 1.274
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 7.7
SJR: 1.785
SNIP: 1.24

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.

9.2

12% from 2019

CiteRatio for Monthly Notices of the Royal Astronomical Society: Letters from 2016 - 2020
Year Value
2020 9.2
2019 10.5
2018 9.5
2017 8.7
2016 8.2
graph view Graph view
table view Table view

2.067

5% from 2019

SJR for Monthly Notices of the Royal Astronomical Society: Letters from 2016 - 2020
Year Value
2020 2.067
2019 1.964
2018 2.649
2017 2.372
2016 2.151
graph view Graph view
table view Table view

0.962

1% from 2019

SNIP for Monthly Notices of the Royal Astronomical Society: Letters from 2016 - 2020
Year Value
2020 0.962
2019 0.95
2018 1.077
2017 0.982
2016 1.07
graph view Graph view
table view Table view

insights Insights

  • CiteRatio of this journal has decreased by 12% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

insights Insights

  • SJR of this journal has increased by 5% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 1% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Monthly Notices of the Royal Astronomical Society: Letters

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Oxford University Press

Monthly Notices of the Royal Astronomical Society: Letters

MNRAS publishes the results of original research in astronomy and astrophysics, including work which is observational, theoretical or concerned with astronomical instrumentation. Assessment of whether papers fall within this scope is made by the members of the editorial board,...... Read More

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Last updated on
22 Jul 2020
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ISSN
1745-3925
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Acceptance Rate
Not provided
i
Frequency
Not provided
i
Open Access
No
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
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Bibliography Name
unsrt
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Citation Type
Numbered
[25]
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Bibliography Example
C. W. J. Beenakker. Specular andreev reflection in graphene. Phys. Rev. Lett., 97(6):067007, 2006.

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.1111/J.1745-3933.2011.01074.X
Too big to fail? The puzzling darkness of massive Milky Way subhaloes
Michael Boylan-Kolchin1, James S. Bullock1, Manoj Kaplinghat1

Abstract:

We show that dissipationless CDM simulations predict that the majority of themost massive subhalos of the Milky Way are too dense to host any of its brightsatellites (L V > 10 5 L ). These dark subhalos have circular velocities at infall ofV infall = 30 1070kms 1 and infall masses of [0:2 4] 10 M . Unless the Milky Way isa st... We show that dissipationless CDM simulations predict that the majority of themost massive subhalos of the Milky Way are too dense to host any of its brightsatellites (L V > 10 5 L ). These dark subhalos have circular velocities at infall ofV infall = 30 1070kms 1 and infall masses of [0:2 4] 10 M . Unless the Milky Way isa statistical anomaly, this implies that galaxy formation becomes e ectively stochasticat these masses. This is in marked contrast to the well-established monotonic relationbetween galaxy luminosity and halo circular velocity (or halo mass) for more massivehalos. We show that at least two (and typically four) of these massive dark subhalosare expected to produce a larger dark matter annihilation ux than Draco. It maybe possible to circumvent these conclusions if baryonic feedback in dwarf satellites ordi erent dark matter physics can reduce the central densities of massive subhalos byorder unity on a scale of 0.3 { 1 kpc.Key words: Galaxy: halo { galaxies: abundances { dark matter { cosmology: theory read more read less

Topics:

Dark matter halo (67%)67% related to the paper, Dwarf galaxy problem (64%)64% related to the paper, Baryonic dark matter (63%)63% related to the paper, Galaxy formation and evolution (61%)61% related to the paper, Self-interacting dark matter (61%)61% related to the paper
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1,280 Citations
open accessOpen access Journal Article DOI: 10.1111/J.1745-3933.2011.01147.X
Efficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole
Alexander Tchekhovskoy1, Ramesh Narayan2, Jonathan C. McKinney3

Abstract:

We describe global, 3D, time-dependent, non-radiative, general-relativistic, magnetohydrodynamic simulations of accreting black holes (BHs). The simulations are designed to transport a large amount of magnetic flux to the centre, more than the accreting gas can force into the BH. The excess magnetic flux remains outside the B... We describe global, 3D, time-dependent, non-radiative, general-relativistic, magnetohydrodynamic simulations of accreting black holes (BHs). The simulations are designed to transport a large amount of magnetic flux to the centre, more than the accreting gas can force into the BH. The excess magnetic flux remains outside the BH, impedes accretion, and leads to a magnetically arrested disc. We find powerful outflows. For a BH with spin parameter a = 0.5, the efficiency with which the accretion system generates outflowing energy in jets and winds is η ≈ 30 per cent. For a = 0.99, we find η ≈ 140 per cent, which means that more energy flows out of the BH than flows in. The only way this can happen is by extracting spin energy from the BH. Thus the a = 0.99 simulation represents an unambiguous demonstration, within an astrophysically plausible scenario, of the extraction of net energy from a spinning BH via the Penrose–Blandford–Znajek mechanism. We suggest that magnetically arrested accretion might explain observations of active galactic nuclei with apparent η ≈ few × 100 per cent. read more read less

Topics:

Active galactic nucleus (53%)53% related to the paper, Accretion (astrophysics) (52%)52% related to the paper, Black hole (50%)50% related to the paper
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858 Citations
open accessOpen access Journal Article DOI: 10.1111/J.1745-3933.2008.00537.X
Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
Alan R. Duffy1, Alan R. Duffy2, Joop Schaye1, Scott T. Kay2, Claudio Dalla Vecchia1

Abstract:

We use a combination of three large N-body simulations to investigate the dependence of dark matter halo concentrations on halo mass and redshift in the Wilkinson Microwave Anisotropy Probe year 5 (WMAP5) cosmology. The median relation between concentration and mass is adequately described by a power law for halo masses in th... We use a combination of three large N-body simulations to investigate the dependence of dark matter halo concentrations on halo mass and redshift in the Wilkinson Microwave Anisotropy Probe year 5 (WMAP5) cosmology. The median relation between concentration and mass is adequately described by a power law for halo masses in the range 1011–1015 h−1 M⊙ and redshifts z < 2, regardless of whether the halo density profiles are fitted using Navarro, Frenk & White or Einasto profiles. Compared with recent analyses of the Millennium Simulation, which uses a value of σ8 that is higher than allowed by WMAP5, z= 0 halo concentrations are reduced by factors ranging from 23 per cent at 1011 h−1 M⊙ to 16 per cent at 1014 h−1 M⊙. The predicted concentrations are much lower than inferred from X-ray observations of groups and clusters. read more read less

Topics:

Dark matter halo (66%)66% related to the paper, Cuspy halo problem (62%)62% related to the paper, Halo (60%)60% related to the paper, Dark matter (54%)54% related to the paper
View PDF
815 Citations
open accessOpen access Journal Article DOI: 10.1111/J.1745-3933.2007.00306.X
Information criteria for astrophysical model selection
Andrew R. Liddle1, Andrew R. Liddle2

Abstract:

Model selection is the problem of distinguishing competing models, perhaps featuring different numbers of parameters. The statistics literature contains two distinct sets of tools, those based on information theory such as the Akaike Information Criterion (AIC), and those on Bayesian inference such as the Bayesian evidence an... Model selection is the problem of distinguishing competing models, perhaps featuring different numbers of parameters. The statistics literature contains two distinct sets of tools, those based on information theory such as the Akaike Information Criterion (AIC), and those on Bayesian inference such as the Bayesian evidence and Bayesian Information Criterion (BIC). The Deviance Information Criterion combines ideas from both heritages; it is readily computed from Monte Carlo posterior samples and, unlike the AIC and BIC, allows for parameter degeneracy. I describe the properties of the information criteria, and as an example compute them from Wilkinson Microwave Anisotropy Probe 3-yr data for several cosmological models. I find that at present the information theory and Bayesian approaches give significantly different conclusions from that data. read more read less

Topics:

Bayesian information criterion (72%)72% related to the paper, Deviance information criterion (70%)70% related to the paper, Bayesian statistics (63%)63% related to the paper, Akaike information criterion (62%)62% related to the paper, Bayesian inference (58%)58% related to the paper
View PDF
725 Citations
open accessOpen access Journal Article DOI: 10.1093/MNRASL/SLV037
Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ 2
Michele Moresco1

Abstract:

One of the most compelling tasks of modern cosmology is to constrain the expansion history of the Universe, since this measurement can give insights on the nature of dark energy and help to estimate cosmological parameters. In this letter are presented two new measurements of the Hubble parameter H(z) obtained with the cosmic... One of the most compelling tasks of modern cosmology is to constrain the expansion history of the Universe, since this measurement can give insights on the nature of dark energy and help to estimate cosmological parameters. In this letter are presented two new measurements of the Hubble parameter H(z) obtained with the cosmic chronometer method up to z ∼ 2. Taking advantage of near-infrared spectroscopy of the few very massive and passive galaxies observed at z > 1.4 available in literature, the differential evolution of this population is estimated and calibrated with different stellar population synthesis models to constrain H(z), including in the final error budget all possible sources of systematic uncertainties (star formation history, stellar metallicity, model dependences). This analysis is able to extend significantly the redshift range coverage with respect to present-day constraints, crossing for the first time the limit at z ∼ 1.75. The new H(z) data are used to estimate the gain in accuracy on cosmological parameters with respect to previous measurements in two cosmological models, finding a small but detectable improvement (∼5 per cent) in particular on Ω_M and w_0. Finally, a simulation of a Euclid-like survey has been performed to forecast the expected improvement with future data. The provided constraints have been obtained just with the cosmic chronometers approach, without any additional data, and the results show the high potentiality of this method to constrain the expansion history of the Universe at these redshifts. read more read less

Topics:

Dark energy (58%)58% related to the paper, Hubble's law (58%)58% related to the paper, Redshift (56%)56% related to the paper, Cosmology (55%)55% related to the paper, Dark matter (54%)54% related to the paper
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646 Citations
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Frequently asked questions

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3. Can I cite my article in multiple styles in Monthly Notices of the Royal Astronomical Society: Letters?

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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 Monthly Notices of the Royal Astronomical Society: Letters?

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 Monthly Notices of the Royal Astronomical Society: Letters. 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 Monthly Notices of the Royal Astronomical Society: Letters?

The 5 most common citation types in order of usage for Monthly Notices of the Royal Astronomical Society: Letters are:.

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

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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 Monthly Notices of the Royal Astronomical Society: Letters Endnote style according to Elsevier guidelines.

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