Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
1436 | 2668 | 51.8 | 66% |
Hierarchy of classes |
The table includes all classes above and classes immediately below the current class. |
Cluster id | Level | Cluster label | #P |
---|---|---|---|
19 | 4 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 523489 |
19 | 3 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 118981 |
158 | 2 | GLOBULAR CLUSTERS GENERAL//ASTRONOMY & ASTROPHYSICS//STARS ABUNDANCES | 22875 |
1436 | 1 | STARS ABUNDANCES//NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES//STARS POPULATION II | 2668 |
Terms with highest relevance score |
rank | Term | termType | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|---|
1 | STARS ABUNDANCES | authKW | 1435293 | 29% | 16% | 784 |
2 | NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES | authKW | 1289484 | 16% | 26% | 433 |
3 | STARS POPULATION II | authKW | 950945 | 11% | 28% | 302 |
4 | NUCLEOSYNTHESIS | authKW | 496178 | 6% | 28% | 156 |
5 | GALAXY EVOLUTION | authKW | 466186 | 9% | 18% | 228 |
6 | GALAXY ABUNDANCES | authKW | 346257 | 6% | 19% | 161 |
7 | GALAXY HALO | authKW | 320132 | 8% | 13% | 220 |
8 | STARS CARBON | authKW | 282960 | 5% | 18% | 140 |
9 | JINA | address | 250882 | 2% | 39% | 56 |
10 | STARS AGB AND POST AGB | authKW | 248989 | 9% | 9% | 243 |
Web of Science journal categories |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | Astronomy & Astrophysics | 80812 | 71% | 0% | 1902 |
2 | Physics, Nuclear | 11959 | 20% | 0% | 545 |
3 | Physics, Particles & Fields | 486 | 5% | 0% | 143 |
4 | Nuclear Science & Technology | 283 | 4% | 0% | 101 |
5 | Physics, Multidisciplinary | 132 | 5% | 0% | 134 |
6 | Spectroscopy | 34 | 2% | 0% | 45 |
7 | Instruments & Instrumentation | 31 | 2% | 0% | 53 |
8 | Humanities, Multidisciplinary | -2 | 0% | 0% | 1 |
9 | Mineralogy | -3 | 0% | 0% | 1 |
10 | Multidisciplinary Sciences | -4 | 0% | 0% | 2 |
Address terms |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | JINA | 250882 | 2% | 39% | 56 |
2 | STELLAR PLANETARY ASTROPHYS | 139092 | 2% | 26% | 46 |
3 | DIPARTIMENTO FIS GEN | 129832 | 3% | 14% | 82 |
4 | JOINT NUCL ASTROPHYS | 120725 | 3% | 15% | 70 |
5 | STUDY COSM EVOLUT | 100198 | 1% | 52% | 17 |
6 | ASTRON ASTROPHYS | 76768 | 12% | 2% | 321 |
7 | GEPI | 73464 | 3% | 8% | 76 |
8 | GRAAL | 58211 | 1% | 18% | 28 |
9 | JINA EVOLUT ELEMENTS | 55238 | 0% | 37% | 13 |
10 | MCDONALD OBSERV | 53018 | 3% | 7% | 70 |
Journals |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | ASTRONOMY & ASTROPHYSICS | 62823 | 20% | 1% | 527 |
2 | ASTROPHYSICAL JOURNAL | 61764 | 24% | 1% | 652 |
3 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 21960 | 2% | 4% | 44 |
4 | NUCLEAR PHYSICS A | 19360 | 7% | 1% | 193 |
5 | PHYSICAL REVIEW C | 12767 | 7% | 1% | 188 |
6 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 5487 | 6% | 0% | 148 |
7 | ASTROPHYSICAL JOURNAL LETTERS | 5328 | 2% | 1% | 54 |
8 | ASTRONOMICAL JOURNAL | 4392 | 3% | 1% | 75 |
9 | ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 3928 | 1% | 2% | 14 |
10 | NUCLEAR SCIENCE AND ENGINEERING | 3642 | 1% | 1% | 33 |
Author Key Words |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
LCSH search | Wikipedia search |
---|---|---|---|---|---|---|---|
1 | STARS ABUNDANCES | 1435293 | 29% | 16% | 784 | Search STARS+ABUNDANCES | Search STARS+ABUNDANCES |
2 | NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES | 1289484 | 16% | 26% | 433 | Search NUCLEAR+REACTIONS+NUCLEOSYNTHESIS+ABUNDANCES | Search NUCLEAR+REACTIONS+NUCLEOSYNTHESIS+ABUNDANCES |
3 | STARS POPULATION II | 950945 | 11% | 28% | 302 | Search STARS+POPULATION+II | Search STARS+POPULATION+II |
4 | NUCLEOSYNTHESIS | 496178 | 6% | 28% | 156 | Search NUCLEOSYNTHESIS | Search NUCLEOSYNTHESIS |
5 | GALAXY EVOLUTION | 466186 | 9% | 18% | 228 | Search GALAXY+EVOLUTION | Search GALAXY+EVOLUTION |
6 | GALAXY ABUNDANCES | 346257 | 6% | 19% | 161 | Search GALAXY+ABUNDANCES | Search GALAXY+ABUNDANCES |
7 | GALAXY HALO | 320132 | 8% | 13% | 220 | Search GALAXY+HALO | Search GALAXY+HALO |
8 | STARS CARBON | 282960 | 5% | 18% | 140 | Search STARS+CARBON | Search STARS+CARBON |
9 | STARS AGB AND POST AGB | 248989 | 9% | 9% | 243 | Search STARS+AGB+AND+POST+AGB | Search STARS+AGB+AND+POST+AGB |
10 | NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES STARS ABUNDANCES | 227506 | 1% | 76% | 26 | Search NUCLEAR+REACTIONS+NUCLEOSYNTHESIS+ABUNDANCES+STARS+ABUNDANCES | Search NUCLEAR+REACTIONS+NUCLEOSYNTHESIS+ABUNDANCES+STARS+ABUNDANCES |
Core articles |
The table includes core articles in the class. The following variables is taken into account for the relevance score of an article in a cluster c: (1) Number of references referring to publications in the class. (2) Share of total number of active references referring to publications in the class. (3) Age of the article. New articles get higher score than old articles. (4) Citation rate, normalized to year. |
Rank | Reference | # ref. in cl. |
Shr. of ref. in cl. |
Citations |
---|---|---|---|---|
1 | AOKI, W , KAPPELER, F , GALLINO, R , BISTERZO, S , (2011) THE S PROCESS: NUCLEAR PHYSICS, STELLAR MODELS, AND OBSERVATIONS.REVIEWS OF MODERN PHYSICS. VOL. 83. ISSUE 1. P. 157 -193 | 242 | 76% | 170 |
2 | SNEDEN, C , COWAN, JJ , GALLINO, R , (2008) NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 46. ISSUE . P. 241 -288 | 154 | 78% | 316 |
3 | BISTERZO, S , GALLINO, R , STRANIERO, O , CRISTALLO, S , KAPPELER, F , (2011) THE S-PROCESS IN LOW-METALLICITY STARS - II. INTERPRETATION OF HIGH-RESOLUTION SPECTROSCOPIC OBSERVATIONS WITH ASYMPTOTIC GIANT BRANCH MODELS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 418. ISSUE 1. P. 284 -319 | 136 | 83% | 75 |
4 | KARAKAS, AI , LATTANZIO, JC , (2014) THE DAWES REVIEW 2: NUCLEOSYNTHESIS AND STELLAR YIELDS OF LOW- AND INTERMEDIATE-MASS SINGLE STARS.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. VOL. 31. ISSUE . P. - | 230 | 40% | 48 |
5 | KAPPELER, F , REIFARTH, R , LEDERER, C , (2014) NEUTRON REACTIONS IN ASTROPHYSICS.JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS. VOL. 41. ISSUE 5. P. - | 153 | 74% | 10 |
6 | PIGNATARI, M , HERWIG, F , HIRSCHI, R , BENNETT, M , ROCKEFELLER, G , FRYER, C , TIMMES, FX , RITTER, C , HEGER, A , JONES, S , ET AL (2016) NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z=0.02 AND Z=0.01.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. VOL. 225. ISSUE 2. P. - | 162 | 60% | 2 |
7 | BISTERZO, S , GALLINO, R , STRANIERO, O , CRISTALLO, S , KAPPELER, F , (2012) THE S-PROCESS IN LOW-METALLICITY STARS - III. INDIVIDUAL ANALYSIS OF CEMP-S AND CEMP-S/R WITH ASYMPTOTIC GIANT BRANCH MODELS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 422. ISSUE 1. P. 849-884 | 114 | 86% | 45 |
8 | HANSEN, TT , ANDERSEN, J , NORDSTROM, B , BEERS, TC , PLACCO, VM , YOON, J , BUCHHAVE, LA , (2016) THE ROLE OF BINARIES IN THE ENRICHMENT OF THE EARLY GALACTIC HALO II. CARBON-ENHANCED METAL-POOR STARS: CEMP-NO STARS.ASTRONOMY & ASTROPHYSICS. VOL. 586. ISSUE . P. - | 80 | 84% | 9 |
9 | YOON, J , BEERS, TC , PLACCO, VM , RASMUSSEN, KC , CAROLLO, D , HE, SY , HANSEN, TT , ROEDERER, IU , ZEANAH, J , (2016) OBSERVATIONAL CONSTRAINTS ON FIRST-STAR NUCLEOSYNTHESIS. I . EVIDENCE FOR MULTIPLE PROGENITORS OF CEMP-NO STARS.ASTROPHYSICAL JOURNAL. VOL. 833. ISSUE 1. P. - | 113 | 93% | 0 |
10 | FREBEL, A , (2010) STELLAR ARCHAEOLOGY: EXPLORING THE UNIVERSE WITH METAL-POOR STARS LUDWIG BIERMANN AWARD LECTURE 2009.ASTRONOMISCHE NACHRICHTEN. VOL. 331. ISSUE 5. P. 474-488 | 115 | 81% | 68 |
Classes with closest relation at Level 1 |