Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
170 | 4039 | 34.9 | 62% |
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 |
170 | 1 | NOVAE CATACLYSMIC VARIABLES//STARS DWARF NOVAE//CATACLYSMIC VARIABLES | 4039 |
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 | NOVAE CATACLYSMIC VARIABLES | authKW | 5468098 | 31% | 57% | 1272 |
2 | STARS DWARF NOVAE | authKW | 2552846 | 10% | 87% | 389 |
3 | CATACLYSMIC VARIABLES | authKW | 1152532 | 6% | 63% | 242 |
4 | STARS NOVAE CATACLYSMIC VARIABLES | authKW | 1082402 | 5% | 65% | 221 |
5 | BINARIES CLOSE | authKW | 877527 | 18% | 16% | 725 |
6 | STARS CATACLYSMIC VARIABLES | authKW | 586042 | 2% | 92% | 84 |
7 | ACCRETION ACCRETION DISKS | authKW | 458732 | 16% | 10% | 628 |
8 | ACCRETION ACCRETION DISCS | authKW | 428405 | 9% | 15% | 373 |
9 | WHITE DWARFS | authKW | 358155 | 9% | 13% | 358 |
10 | NOVAE | authKW | 242756 | 2% | 37% | 88 |
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 | 237572 | 99% | 1% | 3987 |
2 | Engineering, Aerospace | -0 | 0% | 0% | 8 |
3 | Multidisciplinary Sciences | -5 | 0% | 0% | 4 |
4 | Literature | -6 | 0% | 0% | 1 |
5 | Meteorology & Atmospheric Sciences | -6 | 0% | 0% | 17 |
6 | Language & Linguistics | -6 | 0% | 0% | 1 |
7 | Acoustics | -12 | 0% | 0% | 1 |
8 | Physics, Fluids & Plasmas | -18 | 0% | 0% | 3 |
9 | Mathematics, Interdisciplinary Applications | -18 | 0% | 0% | 1 |
10 | Spectroscopy | -20 | 0% | 0% | 5 |
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 | ASTRON | 90022 | 21% | 1% | 867 |
2 | VARIABLE STAR SECT | 82295 | 0% | 78% | 14 |
3 | BACKYARD ASTROPHYS | 76511 | 0% | 56% | 18 |
4 | BIOSPHERE GEOSPHERE SYST | 70346 | 0% | 85% | 11 |
5 | HIDA OBSERV | 53769 | 1% | 17% | 41 |
6 | POLARIS OBSERV | 53746 | 0% | 89% | 8 |
7 | N COPERNICUS ASTRON | 50414 | 1% | 18% | 37 |
8 | VARIABLE STAR SECT BAA VSS | 46292 | 0% | 88% | 7 |
9 | BACKYARD ASTROPHYS FLANDERS | 45349 | 0% | 100% | 6 |
10 | MULLARD SPACE SCI | 42518 | 3% | 5% | 119 |
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 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 191864 | 26% | 2% | 1055 |
2 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 97820 | 6% | 5% | 261 |
3 | ACTA ASTRONOMICA | 73682 | 2% | 12% | 79 |
4 | ASTROPHYSICAL JOURNAL | 70930 | 21% | 1% | 861 |
5 | ASTRONOMY & ASTROPHYSICS | 62111 | 16% | 1% | 646 |
6 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 51467 | 4% | 4% | 161 |
7 | ASTRONOMY REPORTS | 18392 | 2% | 4% | 70 |
8 | ASTRONOMICAL JOURNAL | 17883 | 5% | 1% | 185 |
9 | ASTROPHYSICS AND SPACE SCIENCE | 15438 | 4% | 1% | 162 |
10 | NEW ASTRONOMY | 12767 | 1% | 3% | 50 |
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 | NOVAE CATACLYSMIC VARIABLES | 5468098 | 31% | 57% | 1272 | Search NOVAE+CATACLYSMIC+VARIABLES | Search NOVAE+CATACLYSMIC+VARIABLES |
2 | STARS DWARF NOVAE | 2552846 | 10% | 87% | 389 | Search STARS+DWARF+NOVAE | Search STARS+DWARF+NOVAE |
3 | CATACLYSMIC VARIABLES | 1152532 | 6% | 63% | 242 | Search CATACLYSMIC+VARIABLES | Search CATACLYSMIC+VARIABLES |
4 | STARS NOVAE CATACLYSMIC VARIABLES | 1082402 | 5% | 65% | 221 | Search STARS+NOVAE+CATACLYSMIC+VARIABLES | Search STARS+NOVAE+CATACLYSMIC+VARIABLES |
5 | BINARIES CLOSE | 877527 | 18% | 16% | 725 | Search BINARIES+CLOSE | Search BINARIES+CLOSE |
6 | STARS CATACLYSMIC VARIABLES | 586042 | 2% | 92% | 84 | Search STARS+CATACLYSMIC+VARIABLES | Search STARS+CATACLYSMIC+VARIABLES |
7 | ACCRETION ACCRETION DISKS | 458732 | 16% | 10% | 628 | Search ACCRETION+ACCRETION+DISKS | Search ACCRETION+ACCRETION+DISKS |
8 | ACCRETION ACCRETION DISCS | 428405 | 9% | 15% | 373 | Search ACCRETION+ACCRETION+DISCS | Search ACCRETION+ACCRETION+DISCS |
9 | WHITE DWARFS | 358155 | 9% | 13% | 358 | Search WHITE+DWARFS | Search WHITE+DWARFS |
10 | NOVAE | 242756 | 2% | 37% | 88 | Search NOVAE | Search NOVAE |
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 | DE MARTINO, D , GANSICKE, BT , FERRARIO, L , (2015) MAGNETIC WHITE DWARFS.SPACE SCIENCE REVIEWS. VOL. 191. ISSUE 1-4. P. 111 -169 | 270 | 62% | 22 |
2 | KATO, T , (2015) WZ SGE-TYPE DWARF NOVAE.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 67. ISSUE 6. P. - | 189 | 95% | 2 |
3 | KOPPELMAN, MD , BILLINGS, G , OGMEN, Y , HEATHCOTE, B , GOMEZ, TL , VOLOSHINA, I , RETTER, A , MULARCZYK, K , ZLOCZEWSKI, K , OLECH, A , ET AL (2009) SURVEY OF PERIOD VARIATIONS OF SUPERHUMPS IN SU UMA-TYPE DWARF NOVAE.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 61. ISSUE . P. S395 -S616 | 172 | 95% | 32 |
4 | KATO, T , UEMURA, M , ISHIOKA, R , NOGAMI, D , KUNJAYA, C , BABA, H , YAMAOKA, H , (2004) VARIABLE STAR NETWORK: WORLD CENTER FOR TRANSIENT OBJECT ASTRONOMY AND VARIABLE STARS.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 56. ISSUE 1. P. S1 -S54 | 308 | 60% | 42 |
5 | GANSICKE, BT , DILLON, M , SOUTHWORTH, J , THORSTENSEN, JR , RODRIGUEZ-GIL, P , AUNGWEROJWIT, A , MARSH, TR , SZKODY, P , BARROS, SCC , CASARES, J , ET AL (2009) SDSS UNVEILS A POPULATION OF INTRINSICALLY FAINT CATACLYSMIC VARIABLES AT THE MINIMUM ORBITAL PERIOD.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 397. ISSUE 4. P. 2170 -2188 | 156 | 87% | 80 |
6 | AK, T , BILIR, S , AK, S , COSKUNOGLU, KB , EKER, Z , (2010) THE AGE OF CATACLYSMIC VARIABLES: A KINEMATICAL STUDY.NEW ASTRONOMY. VOL. 15. ISSUE 6. P. 491 -508 | 166 | 91% | 4 |
7 | LADOUS, C , (1990) A CATALOG OF LOW-RESOLUTION IUE SPECTRA OF DWARF NOVAE AND NOVA-LIKE STARS.SPACE SCIENCE REVIEWS. VOL. 52. ISSUE 3-4. P. 203-706 | 304 | 98% | 13 |
8 | KATO, T , HAMBSCH, FJ , MAEHARA, H , MASI, G , NOCENTINI, F , DUBOVSKY, PA , KUDZEJ, I , IMAMURA, K , OGI, M , TANABE, K , ET AL (2014) SURVEY OF PERIOD VARIATIONS OF SUPERHUMPS IN SU UMA-TYPE DWARF NOVAE. V. THE FIFTH YEAR (2012-2013).PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 66. ISSUE 2. P. - | 132 | 95% | 10 |
9 | KATO, T , HAMBSCH, FJ , DUBOVSKY, PA , KUDZEJ, I , MONARD, B , MILLER, I , ITOH, H , KIYOTA, S , MASUMOTO, K , FUKUSHIMA, D , ET AL (2015) SURVEY OF PERIOD VARIATIONS OF SUPERHUMPS IN SU UMA-TYPE DWARF NOVAE. VII. THE SEVENTH YEAR (2014-2015).PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 67. ISSUE 6. P. - | 131 | 95% | 4 |
10 | KATO, T , DUBOVSKY, PA , KUDZEJ, I , HAMBSCH, FJ , MILLER, I , OHSHIMA, T , NAKATA, C , KAWABATA, M , NISHINO, H , MASUMOTO, K , ET AL (2014) SURVEY OF PERIOD VARIATIONS OF SUPERHUMPS IN SU UMA-TYPE DWARF NOVAE. VI. THE SIXTH YEAR (2013-2014).PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 66. ISSUE 5. P. - | 129 | 93% | 5 |
Classes with closest relation at Level 1 |