Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
20648 | 450 | 33.5 | 41% |
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 |
221 | 2 | ASTRONOMY & ASTROPHYSICS//STARS ACTIVITY//STARS OSCILLATIONS | 20606 |
20648 | 1 | STARS INDIVIDUAL ZETA AURIGAE//STARS CHROMOSPHERES//STARS INDIVIDUAL HR 6902 | 450 |
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 INDIVIDUAL ZETA AURIGAE | authKW | 339277 | 1% | 100% | 5 |
2 | STARS CHROMOSPHERES | authKW | 278591 | 11% | 9% | 48 |
3 | STARS INDIVIDUAL HR 6902 | authKW | 271422 | 1% | 100% | 4 |
4 | STARS INDIVIDUAL HR 2554 | authKW | 203566 | 1% | 100% | 3 |
5 | STARS INDIVIDUAL KQ PUP | authKW | 203566 | 1% | 100% | 3 |
6 | STARS INDIVIDUAL VV CEP | authKW | 203566 | 1% | 100% | 3 |
7 | STARS INDIVIDUAL ALPHA TAU | authKW | 180945 | 1% | 67% | 4 |
8 | STARS INDIVIDUAL ALPHA TAURI | authKW | 152673 | 1% | 75% | 3 |
9 | STARS INDIVIDUAL 22 VUL | authKW | 135711 | 0% | 100% | 2 |
10 | STARS INDIVIDUAL 32 CYG | authKW | 135711 | 0% | 100% | 2 |
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 | 24193 | 94% | 0% | 425 |
2 | Engineering, Aerospace | 9 | 1% | 0% | 4 |
3 | Physics, Multidisciplinary | 3 | 3% | 0% | 14 |
4 | Social Sciences, Interdisciplinary | 1 | 0% | 0% | 2 |
5 | History & Philosophy of Science | 0 | 0% | 0% | 1 |
6 | Meteorology & Atmospheric Sciences | 0 | 1% | 0% | 4 |
7 | Multidisciplinary Sciences | -0 | 0% | 0% | 1 |
8 | Geosciences, Multidisciplinary | -1 | 1% | 0% | 4 |
9 | Geochemistry & Geophysics | -1 | 0% | 0% | 2 |
10 | Mathematics, Interdisciplinary Applications | -1 | 0% | 0% | 1 |
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 | 98 BD ARAGO | 67855 | 0% | 100% | 1 |
2 | ASTRON GEOFIS SICA CIENCIAS ATMOSFER | 67855 | 0% | 100% | 1 |
3 | ASTRON OBSERV MADINGLEY RD | 67855 | 0% | 100% | 1 |
4 | ASTRON PROGRAMSCODE 681 CSC | 67855 | 0% | 100% | 1 |
5 | HELWAN OBSERV | 67855 | 0% | 100% | 1 |
6 | L3COM GOVT SCI INC | 67855 | 0% | 100% | 1 |
7 | PHYS TEORET PHYS | 67855 | 0% | 100% | 1 |
8 | STARLINK | 67855 | 0% | 100% | 1 |
9 | CODE 681 | 33927 | 0% | 50% | 1 |
10 | COMP SCI CORP ASTRON PROGRAM | 33927 | 0% | 50% | 1 |
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 | ASTROPHYSICAL JOURNAL | 20283 | 34% | 0% | 153 |
2 | ASTRONOMY & ASTROPHYSICS | 11110 | 20% | 0% | 91 |
3 | IAU SYMPOSIA | 3415 | 4% | 0% | 20 |
4 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 3285 | 4% | 0% | 16 |
5 | ASTROPHYSICS AND SPACE SCIENCE | 2806 | 5% | 0% | 23 |
6 | OBSERVATORY | 2323 | 1% | 1% | 5 |
7 | ASTRONOMICAL JOURNAL | 2273 | 5% | 0% | 22 |
8 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1956 | 8% | 0% | 36 |
9 | CHINESE ASTRONOMY AND ASTROPHYSICS | 1480 | 1% | 1% | 3 |
10 | LECTURE NOTES IN PHYSICS | 1018 | 1% | 0% | 5 |
Author Key Words |
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 | EATON, JA , (2008) A MODEL FOR THE CHROMOSPHERE/WIND OF 31 CYGNI AND ITS IMPLICATIONS FOR SINGLE STARS.ASTRONOMICAL JOURNAL. VOL. 136. ISSUE 5. P. 1964-1979 | 39 | 78% | 4 |
2 | EATON, JA , BELL, C , (1994) THE 1992/93 ECLIPSE OF 31-CYGNI.ASTRONOMICAL JOURNAL. VOL. 108. ISSUE 6. P. 2276-2298 | 34 | 83% | 9 |
3 | HARPER, GM , BROWN, A , BENNETT, PD , BAADE, R , WALDER, R , HUMMEL, CA , (2005) VLA OBSERVATIONS OF ZETA AURIGAE: CONFIRMATION OF THE SLOW ACCELERATION WIND DENSITY STRUCTURE.ASTRONOMICAL JOURNAL. VOL. 129. ISSUE 2. P. 1018 -1034 | 29 | 57% | 16 |
4 | O'GORMAN, E , HARPER, GM , BROWN, A , DRAKE, S , RICHARDS, AMS , (2013) MULTI-WAVELENGTH RADIO CONTINUUM EMISSION STUDIES OF DUST-FREE RED GIANTS.ASTRONOMICAL JOURNAL. VOL. 146. ISSUE 4. P. - | 26 | 46% | 2 |
5 | CARPENTER, KG , ROBINSON, RD , HARPER, GM , BENNETT, PD , BROWN, A , MULLAN, DJ , (1999) GHRS OBSERVATIONS OF COOL, LOW-GRAVITY STARS. V. THE OUTER ATMOSPHERE AND WIND OF THE NEARBY K SUPERGIANT LAMBDA VELORUM.ASTROPHYSICAL JOURNAL. VOL. 521. ISSUE 1. P. 382 -406 | 32 | 51% | 19 |
6 | KIRSCH, T , BAADE, R , REIMERS, D , (2001) THE WARM CIRCUMSTELLAR ENVELOPE AND WIND OF THE G9 IIB STAR HR 6902.ASTRONOMY & ASTROPHYSICS. VOL. 379. ISSUE 3. P. 925 -935 | 17 | 81% | 5 |
7 | CARPENTER, KG , (1992) ZETA-AURIGAE TYPE BINARIES.IAU SYMPOSIA. VOL. . ISSUE 151. P. 51 -59 | 20 | 95% | 0 |
8 | AYRES, TR , (2005) X-RAYS FROM HYBRID STARS.ASTROPHYSICAL JOURNAL. VOL. 618. ISSUE 1. P. 493-501 | 17 | 63% | 9 |
9 | HARPER, GM , GRIFFIN, REM , BENNETT, PD , O'RIAIN, N , (2016) ORBITALLY MODULATED PHOTOEXCITED SI I EMISSION IN THE ECLIPSING COMPOSITE-SPECTRUM BINARY ZETA AURIGAE.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 456. ISSUE 2. P. 1346 -1358 | 18 | 45% | 0 |
10 | AYRES, TR , BROWN, A , HARPER, GM , (2007) ALPHA TRA JUNIOR.ASTROPHYSICAL JOURNAL. VOL. 658. ISSUE 2. P. L107 -L110 | 16 | 62% | 2 |
Classes with closest relation at Level 1 |