Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
26004 | 265 | 35.0 | 58% |
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 |
26004 | 1 | STARS CARBON//ARMENIAN BRANCH//GALAXIES INDIVIDUAL NGC 147 NGC 185 NGC 205 | 265 |
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 CARBON | authKW | 754086 | 27% | 9% | 72 |
2 | ARMENIAN BRANCH | address | 309082 | 5% | 21% | 13 |
3 | GALAXIES INDIVIDUAL NGC 147 NGC 185 NGC 205 | authKW | 230455 | 1% | 100% | 2 |
4 | STARS SURVEY | authKW | 230455 | 1% | 100% | 2 |
5 | GALAXIES INDIVIDUAL NGC 185 | authKW | 205757 | 2% | 36% | 5 |
6 | CARBON STARS | authKW | 161307 | 3% | 20% | 7 |
7 | GALAXIES INDIVIDUAL NGC 205 | authKW | 151608 | 2% | 26% | 5 |
8 | GRP ASTROPHYS | address | 131441 | 3% | 13% | 9 |
9 | ARMENIA BRANCH | address | 115228 | 0% | 100% | 1 |
10 | ASTONOMICAL DATABASES MISCELLANEOUS | authKW | 115228 | 0% | 100% | 1 |
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 | 15275 | 98% | 0% | 259 |
2 | Multidisciplinary Sciences | 2 | 1% | 0% | 2 |
3 | Engineering, General | -0 | 0% | 0% | 1 |
4 | Computer Science, Interdisciplinary Applications | -0 | 0% | 0% | 1 |
5 | Spectroscopy | -0 | 0% | 0% | 1 |
6 | Physics, Multidisciplinary | -2 | 1% | 0% | 2 |
7 | Optics | -2 | 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 | ARMENIAN BRANCH | 309082 | 5% | 21% | 13 |
2 | GRP ASTROPHYS | 131441 | 3% | 13% | 9 |
3 | ARMENIA BRANCH | 115228 | 0% | 100% | 1 |
4 | V AMBARTSUMIAN BYURAKAN ASTROPHYS OBSERV | 115228 | 0% | 100% | 1 |
5 | OBSERV LAS CAMPANAS | 43205 | 1% | 13% | 3 |
6 | NEUENHEIMER FELD 561 | 38408 | 0% | 33% | 1 |
7 | CANADIAN GEMINI OFF | 11814 | 1% | 5% | 2 |
8 | GRP ASTRON | 11521 | 0% | 10% | 1 |
9 | LATMOS IPSL | 10861 | 2% | 2% | 5 |
10 | CEOU | 9214 | 1% | 4% | 2 |
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 | ASTRONOMICAL JOURNAL | 11053 | 14% | 0% | 37 |
2 | ASTRONOMY & ASTROPHYSICS | 10260 | 25% | 0% | 67 |
3 | ADVANCES IN SPACE RESEARCH-SERIES | 9065 | 6% | 0% | 17 |
4 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 7093 | 7% | 0% | 18 |
5 | ASTRONOMICHESKII ZHURNAL | 5444 | 4% | 0% | 10 |
6 | IAU SYMPOSIA | 5257 | 7% | 0% | 19 |
7 | ASTROPHYSICS | 4426 | 1% | 1% | 3 |
8 | BALTIC ASTRONOMY | 4047 | 2% | 1% | 5 |
9 | ASTROPHYSICAL JOURNAL | 2429 | 15% | 0% | 41 |
10 | OBSERVATORY | 1421 | 1% | 0% | 3 |
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 | GROENEWEGEN, MAT , (1999) CARBON STARS IN POPULATIONS OF DIFFERENT METALLICITY.ASYMPTOTIC GIANT BRANCH STARS. VOL. . ISSUE 191. P. 535 -544 | 24 | 75% | 0 |
2 | JUNG, MY , KO, J , KIM, JW , CHUN, SH , KIM, HI , SOHN, YJ , (2012) NEAR-INFRARED PROPERTIES OF ASYMPTOTIC GIANT BRANCH STARS IN NEARBY DWARF ELLIPTICAL GALAXY NGC 205.ASTRONOMY & ASTROPHYSICS. VOL. 543. ISSUE . P. - | 27 | 39% | 1 |
3 | SOHN, YJ , KANG, A , RHEE, J , SHIN, M , CHUN, MS , KIM, HI , (2006) NEAR-IR PHOTOMETRY OF ASYMPTOTIC GIANT BRANCH STARS IN THE DWARF ELLIPTICAL GALAXY NGC 147.ASTRONOMY & ASTROPHYSICS. VOL. 445. ISSUE 1. P. 69-77 | 25 | 47% | 19 |
4 | BATTINELLI, P , DEMERS, S , (2005) THE CALIBRATION OF THE METALLICITY VERSUS C/M RELATION.ASTRONOMY & ASTROPHYSICS. VOL. 434. ISSUE 2. P. 657-663 | 27 | 42% | 43 |
5 | AZZOPARDI, M , (1999) CARBON STARS IN NEARBY LOCAL GROUP GALAXIES.ASTROPHYSICS AND SPACE SCIENCE. VOL. 265. ISSUE 1-4. P. 291-299 | 22 | 61% | 8 |
6 | CHUN, SH , JUNG, M , KANG, M , KIM, JW , SOHN, YJ , (2015) NEAR-INFRARED PHOTOMETRIC PROPERTIES OF ASYMPTOTIC GIANT BRANCH STARS IN THE DWARF IRREGULAR GALAXY IC 1613.ASTRONOMY & ASTROPHYSICS. VOL. 578. ISSUE . P. - | 22 | 38% | 1 |
7 | MAURON, N , GIGOYAN, KS , BERLIOZ-ARTHAUD, P , KLOTZ, A , (2014) COOL CARBON STARS IN THE HALO AND IN DWARF GALAXIES: H ALPHA, COLOURS, AND VARIABILITY.ASTRONOMY & ASTROPHYSICS. VOL. 562. ISSUE . P. - | 21 | 39% | 5 |
8 | BATTINELLI, P , DEMERS, S , MANNUCCI, F , (2007) THE ASSESSMENT OF THE NEAR INFRARED IDENTIFICATION OF CARBON STARS - I. THE LOCAL GROUP GALAXIES WLM, IC 10 AND NGC 6822.ASTRONOMY & ASTROPHYSICS. VOL. 474. ISSUE 1. P. 35 -+ | 20 | 49% | 14 |
9 | SI, JM , LI, YB , LUO, AL , TU, LP , SHI, ZX , ZHANG, JN , WEI, P , ZHAO, G , WU, YH , WU, FC , ET AL (2015) IDENTIFYING CARBON STARS FROM THE LAMOST PILOT SURVEY WITH THE EFFICIENT MANIFOLD RANKING ALGORITHM.RESEARCH IN ASTRONOMY AND ASTROPHYSICS. VOL. 15. ISSUE 10. P. 1671 -1694 | 17 | 46% | 2 |
10 | GIGOYAN, KS , SARKISSIAN, A , RUSSEIL, D , MAURON, N , KOSTANDYAN, G , VARTANIAN, R , ABRAHAMYAN, HV , PARONYAN, GM , (2015) INVESTIGATION OF FAINT GALACTIC CARBON STARS FROM THE FIRST BYURAKAN SPECTRAL SKY SURVEY. II. EARLY-TYPE CARBON STARS.ASTROPHYSICS. VOL. 58. ISSUE 3. P. 369 -379 | 17 | 47% | 0 |
Classes with closest relation at Level 1 |