Class information for:
Level 1: STARS NEUTRON//STARS MAGNETARS//STARS INDIVIDUAL SGR 190014

Basic class information
ID Publications Average number
of references		 Avg. shr. active
ref. in WoS
2641 2111 37.5 69%


Bar chart of Publication_year

Last years might be incomplete

Classes in level above (level 2)


ID, lev.
above		 Publications Label for level above
1352 7816 STARS NEUTRON//DENSE MATTER//STARS MAGNETARS

Terms with highest relevance score


Rank Term Type of term Relevance score
(tfidf)		 Class's shr.
of term's tot.
occurrences		 Shr. of publ.
in class containing
term		 Num. of publ.
in class
1 STARS NEUTRON Author keyword 196 18% 48% 1010
2 STARS MAGNETARS Author keyword 88 59% 5% 98
3 STARS INDIVIDUAL SGR 190014 Author keyword 52 100% 1% 18
4 STARS INDIVIDUAL SGR 1806 20 Author keyword 35 89% 1% 16
5 PULSARS INDIVIDUAL 4U 014261 Author keyword 30 100% 1% 12
6 PULSARS INDIVIDUAL 1E 2259586 Author keyword 26 100% 1% 11
7 DENSE MATTER Author keyword 24 17% 6% 133
8 PULSARS INDIVIDUAL 1E 10481 5937 Author keyword 23 100% 0% 10
9 PULSARS INDIVIDUAL SGR 05014516 Author keyword 21 90% 0% 9
10 STARS MAGNETIC FIELDS Author keyword 20 10% 9% 182

Web of Science journal categories

Author Key Words


Rank Web of Science journal category Relevance score
(tfidf)		 Class's shr.
of term's tot.
occurrences		 Shr. of publ.
in class containing
term		 Num. of publ.
in class		 LCSH search Wikipedia search
1 STARS NEUTRON 196 18% 48% 1010 Search STARS++NEUTRON Search STARS++NEUTRON
2 STARS MAGNETARS 88 59% 5% 98 Search STARS+MAGNETARS Search STARS+MAGNETARS
3 STARS INDIVIDUAL SGR 190014 52 100% 1% 18 Search STARS++INDIVIDUAL+SGR+190014 Search STARS++INDIVIDUAL+SGR+190014
4 STARS INDIVIDUAL SGR 1806 20 35 89% 1% 16 Search STARS++INDIVIDUAL+SGR+1806+20 Search STARS++INDIVIDUAL+SGR+1806+20
5 PULSARS INDIVIDUAL 4U 014261 30 100% 1% 12 Search PULSARS++INDIVIDUAL+4U+014261 Search PULSARS++INDIVIDUAL+4U+014261
6 PULSARS INDIVIDUAL 1E 2259586 26 100% 1% 11 Search PULSARS++INDIVIDUAL+1E+2259586 Search PULSARS++INDIVIDUAL+1E+2259586
7 DENSE MATTER 24 17% 6% 133 Search DENSE+MATTER Search DENSE+MATTER
8 PULSARS INDIVIDUAL 1E 10481 5937 23 100% 0% 10 Search PULSARS++INDIVIDUAL+1E+10481+5937 Search PULSARS++INDIVIDUAL+1E+10481+5937
9 PULSARS INDIVIDUAL SGR 05014516 21 90% 0% 9 Search PULSARS+INDIVIDUAL+SGR+05014516 Search PULSARS+INDIVIDUAL+SGR+05014516
10 STARS MAGNETIC FIELDS 20 10% 9% 182 Search STARS++MAGNETIC+FIELDS Search STARS++MAGNETIC+FIELDS

Key Words Plus


Rank Web of Science journal category Relevance score
(tfidf)		 Class's shr.
of term's tot.
occurrences		 Shr. of publ.
in class containing
term		 Num. of
publ. in
class
1 SOFT GAMMA REPEATERS 365 71% 14% 299
2 MAGNETIZED NEUTRON STARS 184 57% 10% 219
3 SGR 190014 179 72% 7% 139
4 XTE J1810 197 138 89% 3% 63
5 X RAY PULSAR 134 51% 9% 187
6 4U 014261 131 86% 3% 67
7 RX J07204 3125 127 84% 3% 69
8 1E 2259586 121 82% 3% 70
9 RESONANT CYCLOTRON SCATTERING 99 83% 3% 55
10 SOFT GAMMA REPEATER 87 86% 2% 44

Journals

Reviews


Title Publ. year Cit. Active references % act. ref.
to same field
The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars 2008 331 239 90%
Neutron star cooling 2004 362 85 52%
THE SOFT GAMMA-REPEATERS AS VERY STRONGLY MAGNETIZED NEUTRON-STARS .1. RADIATIVE MECHANISM FOR OUTBURSTS 1995 801 68 35%
Minimal cooling of neutron stars: A new paradigm 2004 206 106 55%
Physics of strongly magnetized neutron stars 2006 286 283 40%
Discovery of luminous pulsed hard X-ray emission from anomalous X-ray pulsars 1RXS J1708-4009, 4U 0142+61, and 1E 2259-586 by Integral and RXTE 2006 115 96 77%
Neutrino emission from neutron stars 2001 209 139 53%
Optical, ultraviolet, and infrared observations of isolated neutron stars 2011 19 97 69%
The cooling of compact stars 2006 141 101 46%
LOW-MAGNETIC-FIELD MAGNETARS 2013 5 68 93%

Address terms


Rank Address term Relevance score
(tfidf)		 Class's shr.
of term's tot.
occurrences		 Shr. of publ.
in class containing
term		 Num. of
publ. in
class
1 SPACE SCI OFF 4 17% 0.9% 20
2 SEZ MILANO G OCCHIALINI 4 26% 0.6% 12
3 XINJIANG ASTRON OBSERV 4 16% 0.9% 20
4 ASTRON OBSERV ROME 3 100% 0.1% 3
5 STRUCT EVOLUT CELESTIAL OBJECT 3 60% 0.1% 3
6 DSM IRFU SERV ASTROPHYS 2 27% 0.4% 8
7 DIPARTMENTO FIS ENRICO FERMI 2 67% 0.1% 2
8 ICRABR 2 67% 0.1% 2
9 CHANGCHUN OBSERV 2 29% 0.2% 5
10 NSSTC 2 10% 0.7% 15

Related classes at same level (level 1)


Rank Relatedness score Related classes
1 0.0000218282 DENSE MATTER//FLUIDS ALL SCALES//DIPARTIMENTO FIS G MARCONI
2 0.0000147333 PULSARS GENERAL//ISM INDIVIDUAL CRAB NEBULA//ISM INDIVIDUAL OBJECTS CRAB NEBULA
3 0.0000128498 DENSE MATTER//QUARK STARS//STRANGE QUARK MATTER
4 0.0000117457 OPTICAL COUNTERPARTS//GRB OPTICAL COUNTERPARTS//OPTICAL TRANSIENTS
5 0.0000102416 NEUTRON STAR MAGNETIC FIELDS//DOUBLE ELECTRON SYSTEM//STRONG MAGNETIC FIELD
6 0.0000094689 TORSION ALFVEN VIBRATIONS//HIGH ENERGY ASTROPHYS ISOTOPE STUDIES//LCTA
7 0.0000091465 PULSARS GENERAL//PULSARS INDIVIDUAL PSR J10230038//PULSARS INDIVIDUAL PSR B1620 26
8 0.0000078862 SYMMETRY ENERGY//NUCLEAR MATTER//BRUECKNER HARTREE FOCK APPROACH
9 0.0000062280 COMPENSATION EQUATION//ANOMALOUS THREE BOSON INTERACTION//EFFECTIVE FOUR FERMION INTERACTION
10 0.0000061884 X RAYS BINARIES//PULSARS INDIVIDUAL HERCULES X 1//STARS INDIVIDUAL HERCULES X 1