Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
9534 | 1147 | 47.5 | 79% |
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 |
215 | 2 | X RAYS BINARIES//BLACK HOLE PHYSICS//ACCRETION ACCRETION DISKS | 20680 |
9534 | 1 | X RAYS BINARIES//X RAYS GALAXIES//BLACK HOLE PHYSICS | 1147 |
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 | X RAYS BINARIES | authKW | 1877795 | 47% | 13% | 537 |
2 | X RAYS GALAXIES | authKW | 1004703 | 38% | 9% | 438 |
3 | BLACK HOLE PHYSICS | authKW | 423817 | 25% | 5% | 291 |
4 | X RAYS INDIVIDUAL HLX 1 | authKW | 266203 | 1% | 100% | 10 |
5 | X RAYS INDIVIDUAL NGC 5408 X 1 | authKW | 239583 | 1% | 100% | 9 |
6 | GALAXIES INDIVIDUAL NGC 1313 | authKW | 221823 | 1% | 56% | 15 |
7 | GALAXIES INDIVIDUAL NGC 5408 | authKW | 215623 | 1% | 90% | 9 |
8 | GALAXIES INDIVIDUAL ESO 243 49 | authKW | 186342 | 1% | 100% | 7 |
9 | X RAYS INDIVIDUAL ESO 243 49 HLX 1 | authKW | 186342 | 1% | 100% | 7 |
10 | GALAXIES INDIVIDUAL M31 | authKW | 180664 | 6% | 10% | 67 |
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 | 65873 | 98% | 0% | 1119 |
2 | Engineering, Aerospace | 27 | 1% | 0% | 11 |
3 | Meteorology & Atmospheric Sciences | 8 | 1% | 0% | 17 |
4 | Geosciences, Multidisciplinary | 0 | 1% | 0% | 17 |
5 | Physics, Multidisciplinary | -0 | 2% | 0% | 20 |
6 | Physics, Particles & Fields | -1 | 1% | 0% | 9 |
7 | Mathematics, Applied | -15 | 0% | 0% | 1 |
8 | Mathematics | -18 | 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 | XRAY OBSERV ASTRON GRP | 113573 | 1% | 53% | 8 |
2 | THEORET ASTROPHYS GRP | 90873 | 2% | 14% | 25 |
3 | XRAY OBSERVAT ASTRON GRP | 61360 | 1% | 16% | 14 |
4 | AIMCEA IRFU S | 53241 | 0% | 100% | 2 |
5 | ASTROPHYS INTERACT MULTIECHELLES UMR 7158 | 53241 | 0% | 100% | 2 |
6 | SPACE SCI SOLAR ENERGY PLICAT UZAYM | 53241 | 0% | 100% | 2 |
7 | ASTROPHYS OFF | 35484 | 1% | 22% | 6 |
8 | ASTRON | 30565 | 23% | 0% | 269 |
9 | CURTIN RADIO ASTRON | 29634 | 1% | 16% | 7 |
10 | CEA SACLAY FEDERAT C | 26620 | 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 | ASTROPHYSICAL JOURNAL | 68668 | 39% | 1% | 449 |
2 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 33997 | 21% | 1% | 237 |
3 | ASTRONOMISCHE NACHRICHTEN | 10175 | 3% | 1% | 36 |
4 | ASTRONOMY & ASTROPHYSICS | 7720 | 11% | 0% | 122 |
5 | ASTROPHYSICAL JOURNAL LETTERS | 7565 | 4% | 1% | 42 |
6 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 6699 | 3% | 1% | 31 |
7 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 4430 | 2% | 1% | 28 |
8 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 3119 | 1% | 1% | 10 |
9 | ASTRONOMICAL JOURNAL | 2103 | 3% | 0% | 34 |
10 | IAU SYMPOSIA | 1596 | 2% | 0% | 22 |
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 | FENG, H , SORIA, R , (2011) ULTRALUMINOUS X-RAY SOURCES IN THE CHANDRA AND XMM-NEWTON ERA.NEW ASTRONOMY REVIEWS. VOL. 55. ISSUE 5-6. P. 166 -183 | 167 | 67% | 135 |
2 | FABBIANO, G , (2006) POPULATIONS OF X-RAY SOURCES IN GALAXIES.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 44. ISSUE . P. 323-366 | 163 | 72% | 164 |
3 | GLADSTONE, JC , COPPERWHEAT, C , HEINKE, CO , ROBERTS, TP , CARTWRIGHT, TF , LEVAN, AJ , GOAD, MR , (2013) OPTICAL COUNTERPARTS OF THE NEAREST ULTRALUMINOUS X-RAY SOURCES.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. VOL. 206. ISSUE 2. P. - | 99 | 88% | 16 |
4 | ZAMPIERI, L , ROBERTS, TP , (2009) LOW-METALLICITY NATAL ENVIRONMENTS AND BLACK HOLE MASSES IN ULTRALUMINOUS X-RAY SOURCES.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 400. ISSUE 2. P. 677 -686 | 94 | 72% | 63 |
5 | BERGHEA, CT , DUDIK, RP , TINCHER, J , WINTER, LM , (2013) THE LOCAL ENVIRONMENT OF ULTRALUMINOUS X-RAY SOURCES VIEWED BY XMM-NEWTON'S OPTICAL MONITOR.ASTROPHYSICAL JOURNAL. VOL. 776. ISSUE 2. P. - | 83 | 73% | 6 |
6 | BERGHEA, CT , WEAVER, KA , COLBERT, EJM , ROBERTS, TP , (2008) PARADIGM THAT ULTRALUMINOUS X-RAY SOURCES AS A CLASS REPRESENT ACCRETING INTERMEDIATE-MASS BLACK HOLES.ASTROPHYSICAL JOURNAL. VOL. 687. ISSUE 1. P. 471-487 | 84 | 77% | 36 |
7 | FENG, H , TAO, L , KAARET, P , GRISE, F , (2016) NATURE OF THE SOFT ULX IN NGC 247: SUPER-EDDINGTON OUTFLOW AND TRANSITION BETWEEN THE SUPERSOFT AND SOFT ULTRALUMINOUS REGIMES.ASTROPHYSICAL JOURNAL. VOL. 831. ISSUE 2. P. - | 67 | 84% | 0 |
8 | LUANGTIP, W , ROBERTS, TP , DONE, C , (2016) THE X-RAY SPECTRAL EVOLUTION OF THE ULTRALUMINOUS X-RAY SOURCE HOLMBERG IX X-1.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 460. ISSUE 4. P. 4417 -4432 | 59 | 87% | 1 |
9 | LIU, QZ , MIRABEL, IF , (2005) A CATALOGUE OF ULTRALUMINOUS X-RAY SOURCES IN EXTERNAL GALAXIES.ASTRONOMY & ASTROPHYSICS. VOL. 429. ISSUE 3. P. 1125-1129 | 99 | 65% | 54 |
10 | SORIA, R , KONG, A , (2016) REVISITING THE ULTRALUMINOUS SUPERSOFT SOURCE IN M 101: AN OPTICALLY THICK OUTFLOW MODEL.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 456. ISSUE 2. P. 1837 -1858 | 63 | 62% | 5 |
Classes with closest relation at Level 1 |