Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
8992 | 1198 | 36.9 | 55% |
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 |
159 | 2 | WHITE DWARFS//NOVAE CATACLYSMIC VARIABLES//STARS AGB AND POST AGB | 22817 |
8992 | 1 | STARS AGB AND POST AGB//STARS INDIVIDUAL V4334 SGR//STARS INDIVIDUAL HD 56126 | 1198 |
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 AGB AND POST AGB | authKW | 597006 | 21% | 9% | 252 |
2 | STARS INDIVIDUAL V4334 SGR | authKW | 382305 | 1% | 100% | 15 |
3 | STARS INDIVIDUAL HD 56126 | authKW | 356818 | 1% | 100% | 14 |
4 | STARS INDIVIDUAL SAKURAIS OBJECT | authKW | 331331 | 1% | 100% | 13 |
5 | STARS INDIVIDUAL R CRB | authKW | 305844 | 1% | 100% | 12 |
6 | STARS INDIVIDUAL IRC10420 | authKW | 262149 | 1% | 86% | 12 |
7 | STARS INDIVIDUAL V652 HER | authKW | 254870 | 1% | 100% | 10 |
8 | STARS VARIABLES OTHER R CORONAE BOREALIS | authKW | 203896 | 1% | 100% | 8 |
9 | WJ MCDONALD OBSERV | address | 184231 | 2% | 34% | 21 |
10 | STARS INDIVIDUAL HD 179821 | authKW | 178409 | 1% | 100% | 7 |
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 | 69913 | 98% | 0% | 1178 |
2 | Engineering, Aerospace | -0 | 0% | 0% | 2 |
3 | Multidisciplinary Sciences | -2 | 0% | 0% | 1 |
4 | Spectroscopy | -2 | 0% | 0% | 4 |
5 | Automation & Control Systems | -3 | 0% | 0% | 1 |
6 | Meteorology & Atmospheric Sciences | -4 | 0% | 0% | 3 |
7 | Operations Research & Management Science | -4 | 0% | 0% | 1 |
8 | Physics, Nuclear | -5 | 0% | 0% | 3 |
9 | Geochemistry & Geophysics | -5 | 0% | 0% | 2 |
10 | Optics | -8 | 1% | 0% | 7 |
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 | WJ MCDONALD OBSERV | 184231 | 2% | 34% | 21 |
2 | STERRENKUNDE | 81256 | 4% | 6% | 53 |
3 | SPECIAL ASTROPHYS OBSERV | 60567 | 5% | 4% | 58 |
4 | WE OBSS | 58253 | 0% | 57% | 4 |
5 | CNRS LP 7801 | 50974 | 0% | 100% | 2 |
6 | STERRENKUNDE IVS | 33981 | 0% | 67% | 2 |
7 | 11 RUE UNIVERSITE | 25487 | 0% | 100% | 1 |
8 | ASTROF | 25487 | 0% | 100% | 1 |
9 | ASTRON CAS 519 | 25487 | 0% | 100% | 1 |
10 | ASTRON FM 20 | 25487 | 0% | 100% | 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 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 40123 | 8% | 2% | 91 |
2 | ASTRONOMY & ASTROPHYSICS | 39312 | 23% | 1% | 279 |
3 | ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 31105 | 4% | 2% | 53 |
4 | BALTIC ASTRONOMY | 22388 | 2% | 4% | 25 |
5 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 19957 | 16% | 0% | 186 |
6 | ASTROPHYSICAL BULLETIN | 18758 | 1% | 4% | 17 |
7 | ASTROPHYSICS AND SPACE SCIENCE | 12163 | 7% | 1% | 78 |
8 | ASTRONOMY REPORTS | 11416 | 3% | 2% | 30 |
9 | OBSERVATORY | 11324 | 2% | 2% | 18 |
10 | ASTROPHYSICAL JOURNAL | 10114 | 15% | 0% | 178 |
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 | KLOCHKOVA, VG , (2014) CIRCUMSTELLAR ENVELOPE MANIFESTATIONS IN THE OPTICAL SPECTRA OF EVOLVED STARS.ASTROPHYSICAL BULLETIN. VOL. 69. ISSUE 3. P. 279 -295 | 71 | 77% | 2 |
2 | GARCIA-HERNANDEZ, DA , RAO, NK , LAMBERT, DL , (2011) DUST AROUND R CORONAE BOREALIS STARS. I. SPITZER/INFRARED SPECTROGRAPH OBSERVATIONS.ASTROPHYSICAL JOURNAL. VOL. 739. ISSUE 1. P. - | 67 | 84% | 10 |
3 | CLAYTON, GC , (1996) THE R CORONAE BOREALIS STARS.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC. VOL. 108. ISSUE 721. P. 225-241 | 84 | 81% | 166 |
4 | GEZER, I , VAN WINCKEL, H , BOZKURT, Z , DE SMEDT, K , KAMATH, D , HILLEN, M , MANICK, R , (2015) THE WISE VIEW OF RV TAURI STARS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 453. ISSUE 1. P. 133 -146 | 56 | 70% | 2 |
5 | RAO, NK , LAMBERT, DL , (2015) MID-INFRARED VARIATIONS OF R CORONAE BOREALIS STARS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 447. ISSUE 4. P. 3664 -3677 | 38 | 93% | 1 |
6 | KLOCHKOVA, V , (2013) HIGH-LATITUDE SUPERGIANT V5112 SGR: ENRICHMENT OF THE ENVELOPE WITH HEAVY S-PROCESS METALS.ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS. VOL. 39. ISSUE 11. P. 765-775 | 40 | 82% | 1 |
7 | MONTIEL, EJ , CLAYTON, GC , MARCELLO, DC , LOCKMAN, FJ , (2015) WHAT IS THE SHELL AROUND R CORONAE BOREALIS?.ASTRONOMICAL JOURNAL. VOL. 150. ISSUE 1. P. - | 41 | 76% | 0 |
8 | HRIVNAK, BJ , LU, WX , NAULT, KA , (2015) VARIABILITY IN PROTO-PLANETARY NEBULAE. IV. LIGHT CURVE ANALYSIS OF FOUR OXYGEN-RICH, F SPECTRAL TYPE OBJECTS.ASTRONOMICAL JOURNAL. VOL. 149. ISSUE 6. P. - | 37 | 73% | 2 |
9 | KLOCHKOVA, VG , PANCHUK, VE , (2012) HIGH-LATITUDE SUPERGIANTS: ANOMALIES IN THE SPECTRUM OF LN HYA IN 2010.ASTRONOMY REPORTS. VOL. 56. ISSUE 2. P. 104-115 | 32 | 91% | 1 |
10 | KLOCHKOVA, VG , PANCHUK, VE , (2016) THE DETECTION OF HEAVY METALS IN THE CIRCUMSTELLAR ENVELOPES OF POST-AGB STARS.ASTRONOMY REPORTS. VOL. 60. ISSUE 3. P. 344 -355 | 35 | 71% | 0 |
Classes with closest relation at Level 1 |