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open access Open Access

Research in Astronomy and Astrophysics — Template for authors

Publisher: IOP Publishing
Categories Rank Trend in last 3 yrs
Astronomy and Astrophysics #48 of 88 down down by 12 ranks
Space and Planetary Science #60 of 97 down down by 12 ranks
journal-quality-icon Journal quality:
Medium
calendar-icon Last 4 years overview: 681 Published Papers | 1718 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 01/07/2020
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Related Journals

open access Open Access

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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
SJR: 1.099
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Quality:  
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Elsevier

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

Journal Performance & Insights

Impact Factor

CiteRatio

Determines the importance of a journal by taking a measure of frequency with which the average article in a journal has been cited in a particular year.

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

1.512

21% from 2018

Impact factor for Research in Astronomy and Astrophysics from 2016 - 2019
Year Value
2019 1.512
2018 1.254
2017 1.227
2016 1.371
graph view Graph view
table view Table view

2.5

19% from 2019

CiteRatio for Research in Astronomy and Astrophysics from 2016 - 2020
Year Value
2020 2.5
2019 2.1
2018 2.4
2017 2.5
2016 2.3
graph view Graph view
table view Table view

insights Insights

  • Impact factor of this journal has increased by 21% in last year.
  • This journal’s impact factor is in the top 10 percentile category.

insights Insights

  • CiteRatio of this journal has increased by 19% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

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.

0.516

8% from 2019

SJR for Research in Astronomy and Astrophysics from 2016 - 2020
Year Value
2020 0.516
2019 0.48
2018 0.668
2017 0.681
2016 0.629
graph view Graph view
table view Table view

0.617

25% from 2019

SNIP for Research in Astronomy and Astrophysics from 2016 - 2020
Year Value
2020 0.617
2019 0.495
2018 0.628
2017 0.491
2016 0.721
graph view Graph view
table view Table view

insights Insights

  • SJR of this journal has increased by 8% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 25% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Research in Astronomy and Astrophysics

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IOP Publishing

Research in Astronomy and Astrophysics

Research in Astronomy and Astrophysics is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics.... Read More

i
Last updated on
01 Jul 2020
i
ISSN
1674-4527
i
Impact Factor
High - 1.371
i
Acceptance Rate
Not Provided
i
Frequency
Not Provided
i
Open Access
Not Provided
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
i
Citation Type
Numbered
[25]
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Bibliography Example
Beenakker C W J 2006 Phys. Rev. Lett. 97 067007 URL 10.1103/PhysRevLett.97.067007

Top papers written in this journal

Journal Article DOI: 10.1088/1674-4527/12/9/003
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)

Abstract:

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, also called the Guo Shou Jing Telescope) is a special reflecting Schmidt telescope. LAMOST's special design allows both a large aperture (effective aperture of 3.6 m–4.9 m) and a wide field of view (FOV) (5°). It has an innovative active reflecting Schmidt... The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, also called the Guo Shou Jing Telescope) is a special reflecting Schmidt telescope. LAMOST's special design allows both a large aperture (effective aperture of 3.6 m–4.9 m) and a wide field of view (FOV) (5°). It has an innovative active reflecting Schmidt configuration which continuously changes the mirror's surface that adjusts during the observation process and combines thin deformable mirror active optics with segmented active optics. Its primary mirror (6.67 m × 6.05 m) and active Schmidt mirror (5.74m × 4.40m) are both segmented, and composed of 37 and 24 hexagonal sub-mirrors respectively. By using a parallel controllable fiber positioning technique, the focal surface of 1.75 m in diameter can accommodate 4000 optical fibers. Also, LAMOST has 16 spectrographs with 32 CCD cameras. LAMOST will be the telescope with the highest rate of spectral acquisition. As a national large scientific project, the LAMOST project was formally proposed in 1996, and approved by the Chinese government in 1997. The construction started in 2001, was completed in 2008 and passed the official acceptance in June 2009. The LAMOST pilot survey was started in October 2011 and the spectroscopic survey will launch in September 2012. Up to now, LAMOST has released more than 480000 spectra of objects. LAMOST will make an important contribution to the study of the large-scale structure of the Universe, structure and evolution of the Galaxy, and cross-identification of multi-waveband properties in celestial objects. read more read less

Topics:

LAMOST (71%)71% related to the paper, Primary mirror (59%)59% related to the paper, Schmidt camera (57%)57% related to the paper, Telescope (54%)54% related to the paper, Active optics (52%)52% related to the paper
View PDF
966 Citations
Journal Article DOI: 10.1088/1674-4527/12/7/002
LAMOST spectral survey — An overview
Gang Zhao1, Yong-Heng Zhao1, Yaoquan Chu2, Yaoquan Chu1, Yipeng Jing1, Licai Deng1

Abstract:

LAMOST (Large sky Area Multi-Object fiber Spectroscopic Telescope) is a Chinese national scientific research facility operated by National Astronomical Observatories, Chinese Academy of Sciences (NAOC). After two years of commissioning beginning in 2009, the telescope, instruments, software systems and operations are nearly r... LAMOST (Large sky Area Multi-Object fiber Spectroscopic Telescope) is a Chinese national scientific research facility operated by National Astronomical Observatories, Chinese Academy of Sciences (NAOC). After two years of commissioning beginning in 2009, the telescope, instruments, software systems and operations are nearly ready to begin the main science survey. Through a spectral survey of millions of objects in much of the northern sky, LAMOST will enable research in a number of contemporary cutting edge topics in astrophysics, such as discovery of the first generation stars in the Galaxy, pinning down the formation and evolution history of galaxies — especially the Milky Way and its central massive black hole, and looking for signatures of the distribution of dark matter and possible sub-structures in the Milky Way halo. To maximize the scientific potential of the facility, wide national participation and international collaboration have been emphasized. The survey has two major components: the LAMOST ExtraGAlactic Survey (LEGAS) and the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE). Until LAMOST reaches its full capability, the LEGUE portion of the survey will use the available observing time, starting in 2012. An overview of the LAMOST project and the survey that will be carried out in the next five to six years is presented in this paper. The science plan for the whole LEGUE survey, instrumental specifications, site conditions, and the descriptions of the current on-going pilot survey, including its footprints and target selection algorithm, will be presented as separate papers in this volume. read more read less

Topics:

LAMOST (62%)62% related to the paper
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749 Citations
open accessOpen access Journal Article DOI: 10.1088/1674-4527/14/10/002
Four new observational $H(z)$ data from luminous red galaxies in the Sloan Digital Sky Survey data release seven
Cong Zhang1, Han Zhang1, Shuo Yuan1, Siqi Liu1, Tong-Jie Zhang1, Yan-Chun Sun1

Abstract:

By adopting the differential age method, we select 17 832 luminous red galaxies from the Sloan Digital Sky Survey Data Release Seven covering redshift 0 < z < 0.4 to measure the Hubble parameter. Using the full spectrum fitt ing package UlySS, these spectra are reduced with single stellar population m odels and optimal age in... By adopting the differential age method, we select 17 832 luminous red galaxies from the Sloan Digital Sky Survey Data Release Seven covering redshift 0 < z < 0.4 to measure the Hubble parameter. Using the full spectrum fitt ing package UlySS, these spectra are reduced with single stellar population m odels and optimal age information from our selected sample is derived. With the decreasing age-redshift relation, four new observational H(z) data (OHD) points are obtained, which are H(z) = 69.0±19.6 km s 1 Mpc 1 at z = 0.07, H(z) = 68.6±26.2 km s 1 Mpc 1 at z = 0.12, H(z)=72.9±29.6 km s 1 Mpc 1 at z = 0.2 and H(z)=88.8±36.6 km s 1 Mpc 1 at z = 0.28, respectively. Combined with 21 other available OHD data points, the performance of the constraint on both flat and non -flatCDM models is presented. read more read less
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541 Citations
open accessOpen access Journal Article DOI: 10.1088/1674-4527/15/8/002
The first data release (DR1) of the LAMOST regular survey
A-Li Luo1, Yong-Heng Zhao1, Gang Zhao1, Licai Deng1, Xiaowei Liu2, Yipeng Jing1, Gang Wang1, Haotong Zhang1, Jianrong Shi1, Xiangqun Cui1, Yaoquan Chu3, Guoping Li1, Zhong-Rui Bai1, Yue Wu1, Yan Cai1, Shu-Yun Cao1, Zihuang Cao1, Jeffrey L. Carlin4, Jeffrey L. Carlin5, Hai-Yuan Chen1, Jian-Jun Chen1, Kunxin Chen1, Li Chen1, Xuelei Chen1, Xiao-Yan Chen1, Ying Chen1, Norbert Christlieb6, Jia-Ru Chu3, Chenzhou Cui1, Yi-Qiao Dong1, Bing Du1, Dongwei Fan1, Lei Feng1, Jian-Ning Fu7, Peng Gao1, Xuefei Gong1, Bozhong Gu1, Yan-Xin Guo1, Zhanwen Han1, Boliang He1, Jinliang Hou1, Yong-Hui Hou1, Wen Hou1, Hong-Zhuan Hu3, Ning-Sheng Hu1, Zhongwen Hu1, Zhi-Ying Huo1, Lei Jia1, Fang-Hua Jiang1, Xiang Jiang1, Zhibo Jiang1, Ge Jin3, Xiao Kong1, Xu Kong3, Ya-Juan Lei1, Aihua Li1, Changhua Li1, Guang-Wei Li1, Haining Li1, Jian Li1, Qi Li1, Shuang Li1, Sha-Sha Li1, Li Xinnan1, Yan Li1, Yin-Bi Li1, Ye-Ping Li1, Yuan Liang1, Chien-Cheng Lin1, Chao Liu1, Genrong Liu1, Guan-Qun Liu1, Zhi-Gang Liu3, Wen-Zhi Lu1, Yu Luo1, Yin-Dun Mao1, Heidi Jo Newberg4, Ji-Jun Ni1, Zhaoxiang Qi1, Yong-Jun Qi1, Shiyin Shen1, Huo-Ming Shi1, J. Song1, Yi-Han Song1, Ding-qiang Su1, Hongjun Su1, Zheng-Hong Tang1, Qing-Sheng Tao1, Yuan Tian1, Dan Wang1, D. Wang1, Fengfei Wang1, Guo-Min Wang1, Hai Wang1, Hongchi Wang1, Jian Wang3, Jia-Ning Wang1, Jianling Wang1, Jian-Ping Wang3, Junxian Wang3, Lei Wang1, Meng-Xin Wang1, Shou-Guan Wang1, Shu-Qing Wang1, Xia Wang1, Ya-nan Wang1, You Wang1, Yue-Fei Wang1, Y. Wang1, Peng Wei1, Ming-Zhi Wei1, Hong Wu1, Ke-Fei Wu1, Xue-Bing Wu2, Y. Wu1, Xiao-Zheng Xing3, Lingzhe Xu1, Xin-Qi Xu1, Yan Xu1, Tai-Sheng Yan1, Dehua Yang1, Haifeng Yang1, Hui-Qin Yang1, Ming Yang1, Zheng-Qiu Yao1, Yong Yu1, H.-L. Yuan1, Haibo Yuan2, Hailong Yuan1, Wei-Min Yuan1, Chao Zhai3, En-Peng Zhang1, Huawei Zhang2, Jian-Nan Zhang1, Li-Pin Zhang1, Wei Zhang1, Yong Zhang1, Yanxia Zhang1, Zheng-Chao Zhang1, Ming Zhao1, Fang Zhou1, Xu Zhou1, Jie Zhu1, Yongtian Zhu1, Si-Cheng Zou1, Fang Zuo1

Abstract:

The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in th... The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAMOST Pilot Data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAMOST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signal-to-noise ratio (SNR)>= 1 0. All data with SNR >= 2 are formally released as LAMOST DR1 under the LAMOST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters: late A, FGK-type stars with high quality spectra (1 061 918 entries), A-type stars (100 073 entries), and M-type stars (121 522 entries). This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided. read more read less

Topics:

LAMOST (58%)58% related to the paper
View PDF
513 Citations
open accessOpen access Journal Article DOI: 10.1088/1674-4527/10/6/001
Primordial black holes
Maxim Yu. Khlopov1

Abstract:

Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to restrict a ... Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to restrict a wide range of particle physics models, predicting an enhancement of the ultraviolet part of the spectrum of density perturbations, early dust-like stages, first order phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflationary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds. read more read less

Topics:

Primordial black hole (61%)61% related to the paper, Intermediate-mass black hole (56%)56% related to the paper, Binary black hole (55%)55% related to the paper, Stellar black hole (54%)54% related to the paper, Quasi-star (54%)54% related to the paper
View PDF
495 Citations
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Frequently asked questions

1. Can I write Research in Astronomy and Astrophysics in LaTeX?

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

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Yes, the template is compliant with the Research in Astronomy and Astrophysics 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 Research in Astronomy and Astrophysics?

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 Research in Astronomy and Astrophysics citation style.

4. Can I use the Research in Astronomy and Astrophysics 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 Research in Astronomy and Astrophysics.

5. Can I use a manuscript in Research in Astronomy and Astrophysics 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 Research in Astronomy and Astrophysics that you can download at the end.

6. How long does it usually take you to format my papers in Research in Astronomy and Astrophysics?

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

7. Where can I find the template for the Research in Astronomy and Astrophysics?

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 Research in Astronomy and Astrophysics'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 Research in Astronomy and Astrophysics 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.

10. I cannot find my template in your gallery. Can you create it for me like Research in Astronomy and Astrophysics?

Sure. You can request any template and we'll have it setup within a few days. You can find the request box in Journal Gallery on the right side bar under the heading, "Couldn't find the format you were looking for like Research in Astronomy and Astrophysics?”

11. What is the output that I would get after using Research in Astronomy and Astrophysics?

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

12. Is Research in Astronomy and Astrophysics'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 Research in Astronomy and Astrophysics?

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 Research in Astronomy and Astrophysics. 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 Research in Astronomy and Astrophysics?

The 5 most common citation types in order of usage for Research in Astronomy and Astrophysics 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 Research in Astronomy and Astrophysics?

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16. Can I download Research in Astronomy and Astrophysics 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 Research in Astronomy and Astrophysics Endnote style according to Elsevier guidelines.

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I spent hours with MS word for reformatting. It was frustrating - plain and simple. With SciSpace, I can draft my manuscripts and once it is finished I can just submit. In case, I have to submit to another journal it is really just a button click instead of an afternoon of reformatting.

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