Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
25117 | 290 | 45.9 | 73% |
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 |
8 | 3 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 146114 |
0 | 2 | GALAXIES EVOLUTION//ASTRONOMY & ASTROPHYSICS//MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 61580 |
25117 | 1 | RADIASTRON ASTROFIS//DUST EXTINCTION//GALAXIES SPIRAL | 290 |
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 | RADIASTRON ASTROFIS | address | 329040 | 2% | 63% | 5 |
2 | DUST EXTINCTION | authKW | 322332 | 38% | 3% | 110 |
3 | GALAXIES SPIRAL | authKW | 300804 | 32% | 3% | 92 |
4 | STERRENKUNDIG OBSERV | address | 227330 | 11% | 7% | 31 |
5 | RADIATIVE TRANSFER | authKW | 208884 | 36% | 2% | 105 |
6 | GALAXIES ISM | authKW | 144294 | 29% | 2% | 84 |
7 | GALAXIES INDIVIDUAL NGC 891 | authKW | 142132 | 3% | 15% | 9 |
8 | 21 CM LINE | authKW | 105294 | 0% | 100% | 1 |
9 | 3D CONTINUUM RADIATIVE TRANSFER | authKW | 105294 | 0% | 100% | 1 |
10 | ASTRON HISPANO | address | 105294 | 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 | 16071 | 96% | 0% | 278 |
2 | Spectroscopy | 12 | 2% | 0% | 7 |
3 | Optics | 1 | 2% | 0% | 7 |
4 | Computer Science, Interdisciplinary Applications | 0 | 1% | 0% | 3 |
5 | Engineering, Aerospace | 0 | 0% | 0% | 1 |
6 | Multidisciplinary Sciences | 0 | 0% | 0% | 1 |
7 | Computer Science, Artificial Intelligence | -0 | 0% | 0% | 1 |
8 | Physics, Mathematical | -1 | 0% | 0% | 1 |
9 | Meteorology & Atmospheric Sciences | -1 | 0% | 0% | 1 |
10 | Geosciences, Multidisciplinary | -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 | RADIASTRON ASTROFIS | 329040 | 2% | 63% | 5 |
2 | STERRENKUNDIG OBSERV | 227330 | 11% | 7% | 31 |
3 | ASTRON HISPANO | 105294 | 0% | 100% | 1 |
4 | ASTRON SPACE EDUC | 105294 | 0% | 100% | 1 |
5 | IPAC EXTRAGALACT DATABASE NED | 105294 | 0% | 100% | 1 |
6 | IPAC EXTRAGLACT DATABASE | 105294 | 0% | 100% | 1 |
7 | RADIASTRONOM ASTROPHYS | 105294 | 0% | 100% | 1 |
8 | STEM REO | 105294 | 0% | 100% | 1 |
9 | URA1757 | 105294 | 0% | 100% | 1 |
10 | K TEYN ASTRON POB 800 | 52646 | 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 | ASTRONOMY & ASTROPHYSICS | 11439 | 26% | 0% | 74 |
2 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 10441 | 23% | 0% | 66 |
3 | BALTIC ASTRONOMY | 9475 | 3% | 1% | 8 |
4 | ASTRONOMICAL JOURNAL | 5361 | 9% | 0% | 27 |
5 | ASTROPHYSICAL JOURNAL | 3049 | 17% | 0% | 48 |
6 | ASTRONOMY AND COMPUTING | 2628 | 1% | 1% | 2 |
7 | ASTROPHYSICS AND SPACE SCIENCE | 990 | 4% | 0% | 11 |
8 | JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 741 | 2% | 0% | 7 |
9 | ACTA ASTRONOMICA | 655 | 1% | 0% | 2 |
10 | BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA | 570 | 0% | 1% | 1 |
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 | DUST EXTINCTION | 322332 | 38% | 3% | 110 | Search DUST+EXTINCTION | Search DUST+EXTINCTION |
2 | GALAXIES SPIRAL | 300804 | 32% | 3% | 92 | Search GALAXIES+SPIRAL | Search GALAXIES+SPIRAL |
3 | RADIATIVE TRANSFER | 208884 | 36% | 2% | 105 | Search RADIATIVE+TRANSFER | Search RADIATIVE+TRANSFER |
4 | GALAXIES ISM | 144294 | 29% | 2% | 84 | Search GALAXIES+ISM | Search GALAXIES+ISM |
5 | GALAXIES INDIVIDUAL NGC 891 | 142132 | 3% | 15% | 9 | Search GALAXIES+INDIVIDUAL+NGC+891 | Search GALAXIES+INDIVIDUAL+NGC+891 |
6 | 21 CM LINE | 105294 | 0% | 100% | 1 | Search 21+CM+LINE | Search 21+CM+LINE |
7 | 3D CONTINUUM RADIATIVE TRANSFER | 105294 | 0% | 100% | 1 | Search 3D+CONTINUUM+RADIATIVE+TRANSFER | Search 3D+CONTINUUM+RADIATIVE+TRANSFER |
8 | DUST EXTINCTIONE | 105294 | 0% | 100% | 1 | Search DUST+EXTINCTIONE | Search DUST+EXTINCTIONE |
9 | GALACTIC STRUCTURE B75 DEGREES FIELDS | 105294 | 0% | 100% | 1 | Search GALACTIC+STRUCTURE+B75+DEGREES+FIELDS | Search GALACTIC+STRUCTURE+B75+DEGREES+FIELDS |
10 | GALAXIES DUST EXTINCTION | 105294 | 0% | 100% | 1 | Search GALAXIES+DUST+EXTINCTION | Search GALAXIES+DUST+EXTINCTION |
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 | LEE, D , BAES, M , SEON, KI , CAMPS, P , VERSTOCKEN, S , HAN, W , (2016) RADIATIVE TRANSFER IN DISC GALAXIES - V. THE ACCURACY OF THE KB APPROXIMATION.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 463. ISSUE 3. P. 2912 -2921 | 50 | 74% | 0 |
2 | SAFTLY, W , BAES, M , DE GEYTER, G , CAMPS, P , RENAUD, F , GUEDES, J , DE LOOZE, I , (2015) LARGE AND SMALL-SCALE STRUCTURES AND THE DUST ENERGY BALANCE PROBLEM IN SPIRAL GALAXIES.ASTRONOMY & ASTROPHYSICS. VOL. 576. ISSUE . P. - | 40 | 49% | 5 |
3 | BAES, M , CAMPS, P , FRITZ, J , DE LOOZE, I , HUGHES, TM , VIAENE, S , GENTILE, G , DE GEYTER, G , (2014) THE DISTRIBUTION OF INTERSTELLAR DUST IN CALIFA EDGE-ON GALAXIES VIA OLIGOCHROMATIC RADIATIVE TRANSFER FITTING.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 441. ISSUE 1. P. 869 -885 | 50 | 35% | 17 |
4 | BAES, M , VERSTAPPEN, J , DE LOOZE, I , FRITZ, J , SAFTLY, W , PEREZ, EV , STALEVSKI, M , VALCKE, S , (2011) EFFICIENT THREE-DIMENSIONAL NLTE DUST RADIATIVE TRANSFER WITH SKIRT.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. VOL. 196. ISSUE 2. P. - | 40 | 45% | 44 |
5 | POPESCU, CC , TUFFS, RJ , DOPITA, MA , FISCHERA, J , KYLAFIS, ND , MADORE, BF , (2011) MODELLING THE SPECTRAL ENERGY DISTRIBUTION OF GALAXIES V. THE DUST AND PAH EMISSION SEDS OF DISK GALAXIES.ASTRONOMY & ASTROPHYSICS. VOL. 527. ISSUE . P. - | 48 | 32% | 70 |
6 | HOLWERDA, BW , KEEL, WC , (2013) THE OCCULTING GALAXY PAIR UGC 3995 DUST PROPERTIES FROM HST AND CALIFA DATA.ASTRONOMY & ASTROPHYSICS. VOL. 556. ISSUE . P. - | 32 | 55% | 7 |
7 | HOLWERDA, BW , BALDRY, IK , ALPASLAN, M , BAUER, A , BLAND-HAWTHORN, J , BROUGH, S , BROWN, MJI , CLUVER, ME , CONSELICE, C , DRIVER, SP , ET AL (2015) GALAXY AND MASS ASSEMBLY (GAMA) BLENDED SPECTRA CATALOGUE: STRONG GALAXY-GALAXY LENS AND OCCULTING GALAXY PAIR CANDIDATES.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 449. ISSUE 4. P. 4277 -4287 | 33 | 52% | 1 |
8 | BIANCHI, S , (2008) DUST EXTINCTION AND EMISSION IN A CLUMPY GALACTIC DISK AN APPLICATION OF THE RADIATIVE TRANSFER CODE TRADING.ASTRONOMY & ASTROPHYSICS. VOL. 490. ISSUE 1. P. 461 -475 | 35 | 51% | 58 |
9 | STEINACKER, J , BAES, M , GORDON, KD , (2013) THREE-DIMENSIONAL DUST RADIATIVE TRANSFER.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 51. VOL. 51. ISSUE . P. 63 -104 | 48 | 29% | 26 |
10 | HOLWERDA, BW , MEYER, M , REGAN, M , CALZETTI, D , GORDON, KD , SMITH, JD , DALE, D , ENGELBRACHT, CW , JARRETT, T , THORNLEY, M , ET AL (2007) GAPS IN THE CLOUD COVER? COMPARING EXTINCTION MEASURES IN SPIRAL DISKS.ASTRONOMICAL JOURNAL. VOL. 134. ISSUE 4. P. 1655-1661 | 36 | 51% | 3 |
Classes with closest relation at Level 1 |