diff --git "a/KAILAS_UAT_Labeler_Demo.ipynb" "b/KAILAS_UAT_Labeler_Demo.ipynb" new file mode 100644--- /dev/null +++ "b/KAILAS_UAT_Labeler_Demo.ipynb" @@ -0,0 +1,2468 @@ +{ + "cells": [ + { + "cell_type": "markdown", + "id": "807c463e-cd0f-4ffb-b974-b19a33a674bb", + "metadata": { + "tags": [] + }, + "source": [ + "# Demo of the KAILAS UAT labeler capabilities\n", + "This notebooks shows how to use KAILAS to automatically tag text with Unified Astronomy Thesaurus concepts" + ] + }, + { + "cell_type": "markdown", + "id": "1fbf6cb4-1110-4883-9ffd-d39d81e4301a", + "metadata": {}, + "source": [ + "## Preliminaries\n", + "1. load UAT concepts\n", + "2. load a dataset" + ] + }, + { + "cell_type": "code", + "execution_count": 1, + "id": "9bc5eaae-4e37-425f-9a0e-b6a7e8eca3e0", + "metadata": {}, + "outputs": [], + "source": [ + "# We need to build version of the UAT that is more suited to our needs\n", + "# Download the original here: https://github.com/astrothesaurus/UAT/blob/master/UAT.json\n", + "# and replace the path to it below\n", + "# build the UAT labels dict\n", + "import json\n", + "with open('./UAT_list.json', 'r') as f:\n", + " uat_list = json.load(f)\n", + "\n", + "# build the dict that matches UAT ID (numbers) to common names\n", + "uat_names = {}\n", + "for entry in uat_list:\n", + " uat_id = entry['uri'].split('/')[-1]\n", + " uat_names[uat_id] = entry['name'].lower().strip()\n", + "\n", + "# sort by key\n", + "uat_names = dict(sorted(uat_names.items()))" + ] + }, + { + "cell_type": "code", + "execution_count": 2, + "id": "72e8f308-9e17-49a4-b520-a8ec05df3152", + "metadata": { + "scrolled": true + }, + "outputs": [ + { + "data": { + "text/plain": [ + "{'0': 'dc stars',\n", + " '10': 'absolute magnitude',\n", + " '100': 'astrophysical explosive burning',\n", + " '1000': 'main sequence stars',\n", + " '1001': 'major axis',\n", + " '1002': 'makemake',\n", + " '1003': 'maksutov telescopes',\n", + " '1004': 'manganese stars',\n", + " '1005': 'mantle',\n", + " '1006': 'markarian galaxies',\n", + " '1007': 'mars',\n", + " '1008': 'mars trojans',\n", + " '1009': 'martian satellites',\n", + " '101': 'astrophysical fluid dynamics',\n", + " '1010': 'mascon',\n", + " '1011': 'mass-to-light ratio',\n", + " '1012': 'mass ratio',\n", + " '1013': 'mass spectrometers',\n", + " '1014': 'matter density',\n", + " '1015': 'maunder minimum',\n", + " '1016': 'maximal kerr black holes',\n", + " '1017': 'me stars',\n", + " '1018': 'me variable stars',\n", + " '1019': 'mean anomaly',\n", + " '102': 'astrophysical magnetism',\n", + " '1020': 'mean matter density',\n", + " '1021': 'medium band photometry',\n", + " '1022': 'megalithic astronomy',\n", + " '1023': 'megamasers',\n", + " '1024': 'mercury (planet)',\n", + " '1025': 'mercury-manganese stars',\n", + " '1026': 'meridian',\n", + " '1027': 'meridian circles',\n", + " '1028': 'mesogranulation',\n", + " '1029': 'mesopause',\n", + " '103': 'astrophysical masers',\n", + " '1030': 'mesosphere',\n", + " '1031': 'metallicity',\n", + " '1032': 'metal line absorbers',\n", + " '1033': 'meteor radiants',\n", + " '1034': 'meteor showers',\n", + " '1035': 'meteor streams',\n", + " '1036': 'meteor trails',\n", + " '1037': 'meteorite composition',\n", + " '1038': 'meteorites',\n", + " '1039': 'meteoroid dust clouds',\n", + " '104': 'astrophysical processes',\n", + " '1040': 'meteoroids',\n", + " '1041': 'meteors',\n", + " '1042': 'methane',\n", + " '1043': 'astronomical methods',\n", + " '1044': 'michelson interferometers',\n", + " '1045': 'michelson interferometry',\n", + " '1046': 'microgravity',\n", + " '1047': 'micrometeorites',\n", + " '1048': 'micrometeoroids',\n", + " '1049': 'milky way dark matter halo',\n", + " '105': 'astrophysicists',\n", + " '1050': 'milky way disk',\n", + " '1051': 'milky way dynamics',\n", + " '1052': 'milky way evolution',\n", + " '1053': 'milky way formation',\n", + " '1054': 'milky way galaxy',\n", + " '1055': 'milky way galaxy fountains',\n", + " '1056': 'milky way galaxy physics',\n", + " '1057': 'milky way magnetic fields',\n", + " '1058': 'milky way mass',\n", + " '1059': 'milky way rotation',\n", + " '106': 'astrosphere interstellar medium interactions',\n", + " '1060': 'milky way stellar halo',\n", + " '1061': 'millimeter astronomy',\n", + " '1062': 'millisecond pulsars',\n", + " '1063': 'mini neptunes',\n", + " '1064': 'minor axis',\n", + " '1065': 'minor planets',\n", + " '1066': 'mira variable stars',\n", + " '1067': 'mira variable stars',\n", + " '1068': 'missing mass',\n", + " '1069': 'modified newtonian dynamics',\n", + " '107': 'astrospheres',\n", + " '1070': 'moldavites',\n", + " '1071': 'radical-radical recombination',\n", + " '1072': 'molecular clouds',\n", + " '1073': 'molecular gas',\n", + " '1074': 'solar mottles',\n", + " '1075': 'moving cluster parallax',\n", + " '1076': 'moving clusters',\n", + " '1077': 'multi-color photometry',\n", + " '1078': 'multi-periodic pulsation',\n", + " '1079': 'multi-periodic variable stars',\n", + " '108': 'asymptotic giant branch',\n", + " '1080': 'multiple mirror telescopes',\n", + " '1081': 'multiple stars',\n", + " '1082': 'n-body problem',\n", + " '1083': 'n-body simulations',\n", + " '1084': 'n galaxies',\n", + " '1085': 'n stars',\n", + " '1086': 'nadir',\n", + " '1087': 'naked singularities',\n", + " '1088': 'narrow band photometry',\n", + " '1089': 'natural satellites (solar system)',\n", + " '109': 'ataxites',\n", + " '1090': 'nautical almanacs',\n", + " '1091': 'navarro-frenk-white profile',\n", + " '1092': 'near-earth objects',\n", + " '1093': 'near infrared astronomy',\n", + " '1094': 'near ultraviolet astronomy',\n", + " '1095': 'nebulae',\n", + " '1096': 'neptune',\n", + " '1097': 'neptune trojans',\n", + " '1098': 'neptunian satellites',\n", + " '1099': 'neutral hydrogen clouds',\n", + " '11': 'abundance ratios',\n", + " '110': 'aten group',\n", + " '1100': 'neutrino astronomy',\n", + " '1101': 'neutrino decoupling',\n", + " '1102': 'neutrino masses',\n", + " '1103': 'neutrino oscillation',\n", + " '1104': 'neutrino oscillations',\n", + " '1105': 'neutrino telescopes',\n", + " '1106': 'neutron interferometry',\n", + " '1107': 'neutron star cores',\n", + " '1108': 'neutron stars',\n", + " '1109': 'newtonian cosmology',\n", + " '111': 'atira group',\n", + " '1110': 'newtonian gravitation',\n", + " '1111': 'newtonian telescopes',\n", + " '1112': 'night sky brightness',\n", + " '1113': 'night vision',\n", + " '1114': 'nitrous oxide',\n", + " '1115': 'noctilucent clouds',\n", + " '1116': 'non-gaussianity',\n", + " '1117': 'non-radial pulsations',\n", + " '1118': 'non-standard theories of gravity',\n", + " '1119': 'non-thermal radiation sources',\n", + " '112': 'atmospheric circulation',\n", + " '1120': 'nonclassical interferometry',\n", + " '1121': 'nonrotating black holes',\n", + " '1122': 'nonstandard evolution',\n", + " '1123': 'north celestial pole',\n", + " '1124': 'north ecliptic pole',\n", + " '1125': 'north galactic pole',\n", + " '1126': 'nova-like variable stars',\n", + " '1127': 'novae',\n", + " '1128': 'nuclear abundances',\n", + " '1129': 'nuclear astrophysics',\n", + " '113': 'atmospheric effects',\n", + " '1130': 'nucleated dwarf galaxies',\n", + " '1131': 'nucleosynthesis',\n", + " '1132': 'o subgiant stars',\n", + " '1133': 'o associations',\n", + " '1134': 'o clusters',\n", + " '1135': 'o dwarf stars',\n", + " '1136': 'o giant stars',\n", + " '1137': 'o stars',\n", + " '1138': 'o subdwarf stars',\n", + " '1139': 'o supergiant stars',\n", + " '114': 'atmospheric extinction',\n", + " '1140': 'ob associations',\n", + " '1141': 'ob stars',\n", + " '1142': 'ob supergiant stars',\n", + " '1143': 'oblateness',\n", + " '1144': 'oblique rotators',\n", + " '1145': 'observational astronomy',\n", + " '1146': 'observational cosmology',\n", + " '1147': 'observatories',\n", + " '1148': 'occultation',\n", + " '1149': 'occulting disks',\n", + " '115': 'atmospheric refraction',\n", + " '1150': 'ocean-atmosphere interactions',\n", + " '1151': 'ocean planets',\n", + " '1152': 'ocean tides',\n", + " '1153': 'oe stars',\n", + " '1154': 'oef stars',\n", + " '1155': 'of stars',\n", + " '1156': 'oh/ir stars',\n", + " '1157': 'oort cloud',\n", + " '1158': 'oort cloud objects',\n", + " '1159': 'oort constants',\n", + " '116': 'atmospheric science',\n", + " '1160': 'open star clusters',\n", + " '1161': 'open universe',\n", + " '1162': 'opik theory',\n", + " '1163': 'opposition',\n", + " '1164': 'optical bursts',\n", + " '1165': 'optical double stars',\n", + " '1166': 'optical flares',\n", + " '1167': 'optical identification',\n", + " '1168': 'optical interferometry',\n", + " '1169': 'optical observation',\n", + " '117': 'atmospheric scintillation',\n", + " '1170': 'optical observatories',\n", + " '1171': 'optical phase shifting interferometry',\n", + " '1172': 'optical position',\n", + " '1173': 'optical pulsars',\n", + " '1174': 'optical telescopes',\n", + " '1175': 'orbit determination',\n", + " '1176': 'orbital anomalies',\n", + " '1177': 'orbital elements',\n", + " '1178': 'orbital evolution',\n", + " '1179': 'orbital motion',\n", + " '118': 'atmospheric tides',\n", + " '1180': 'orbital nodes',\n", + " '1181': 'orbital resonances',\n", + " '1182': 'orbital theory',\n", + " '1183': 'orbiters',\n", + " '1184': 'orbits',\n", + " '1185': 'orcus',\n", + " '1186': 'origin of the universe',\n", + " '1187': 'orreries',\n", + " '1188': 'oscillating universe',\n", + " '1189': 'osculating orbit',\n", + " '119': 'atomic interferometry',\n", + " '1190': 'osculatory elements',\n", + " '1191': 'solar system gas giant planets',\n", + " '1192': 'overabundances',\n", + " '1193': 'oxygen burning',\n", + " '1194': 'ozone layer',\n", + " '1195': 'p-process',\n", + " '1196': 'parabolic orbit',\n", + " '1197': 'parallax',\n", + " '1198': 'parallel field',\n", + " '1199': 'parsec',\n", + " '12': 'accelerating universe',\n", + " '120': 'australites',\n", + " '1200': 'partial eclipses',\n", + " '1201': 'chemically peculiar giant stars',\n", + " '1202': 'peculiar variable stars',\n", + " '1203': 'penrose limit',\n", + " '1204': 'penrose process',\n", + " '1205': 'penumbra',\n", + " '1206': 'penumbral filaments',\n", + " '1207': 'periapsis',\n", + " '1208': 'periastron',\n", + " '1209': 'perigee',\n", + " '121': 'automated telescopes',\n", + " '1210': 'perihelion',\n", + " '1211': 'period determination',\n", + " '1212': 'periodic orbit',\n", + " '1213': 'periodic variable stars',\n", + " '1214': 'perseus cluster',\n", + " '1215': 'perturbation methods',\n", + " '1216': 'pg 1159 stars',\n", + " '1217': 'phase angle',\n", + " '1218': 'phase defect',\n", + " '1219': 'phase effect',\n", + " '122': 'automatic patrol telescopes',\n", + " '1220': 'phase error',\n", + " '1221': 'phase switching',\n", + " '1222': 'philosophy of astronomy',\n", + " '1223': 'photodissociation regions',\n", + " '1224': 'photoelectric magnitude',\n", + " '1225': 'photoelectric photometry',\n", + " '1226': 'photogrammetry',\n", + " '1227': 'photographic astrometry',\n", + " '1228': 'photographic magnitude',\n", + " '1229': 'photographic photometry',\n", + " '123': 'autumnal equinox',\n", + " '1230': 'photoheliographs',\n", + " '1231': 'photometric parallax',\n", + " '1232': 'photometric standard stars',\n", + " '1233': 'photometric systems',\n", + " '1234': 'photometry',\n", + " '1235': 'photon decoupling',\n", + " '1236': 'photon sphere',\n", + " '1237': 'stellar photospheres',\n", + " '1238': 'photovisual magnitude',\n", + " '1239': 'pickup ions',\n", + " '124': 'azimuth',\n", + " '1240': 'plages',\n", + " '1241': 'planet formation',\n", + " '1242': 'planet hosting stars',\n", + " '1243': 'planetary alignment',\n", + " '1244': 'planetary atmospheres',\n", + " '1245': 'planetary boundary layers',\n", + " '1246': 'planetary bow shocks',\n", + " '1247': 'planetary cores',\n", + " '1248': 'planetary interior',\n", + " '1249': 'planetary nebulae',\n", + " '125': 'b subgiant stars',\n", + " '1250': 'planetary nebulae nuclei',\n", + " '1251': 'planetary polar regions',\n", + " '1252': 'planetary probes',\n", + " '1253': 'planetary ring divisions',\n", + " '1254': 'planetary rings',\n", + " '1255': 'planetary science',\n", + " '1256': 'planetary structure',\n", + " '1257': 'planetary system formation',\n", + " '1258': 'planetary theory',\n", + " '1259': 'planetesimals',\n", + " '126': 'b dwarf stars',\n", + " '1260': 'solar system planets',\n", + " '1261': 'plasma astrophysics',\n", + " '1262': 'plasma clouds',\n", + " '1263': 'plasma jets',\n", + " '1264': 'plasmapause',\n", + " '1265': 'plate tectonics',\n", + " '1266': 'plutinos',\n", + " '1267': 'pluto',\n", + " '1268': 'plutoids',\n", + " '1269': 'pogson scale',\n", + " '127': 'b giant stars',\n", + " '1270': 'x-ray point sources',\n", + " '1271': 'pointing accuracy',\n", + " '1272': 'pointing error',\n", + " '1273': 'polar caps',\n", + " '1274': 'polar jets',\n", + " '1275': 'polar orbit',\n", + " '1276': 'polar tides',\n", + " '1277': 'polarimeters',\n", + " '1278': 'polarimetry',\n", + " '1279': 'polarimetry [exoplanets]',\n", + " '128': 'b stars',\n", + " '1280': 'polycyclic aromatic hydrocarbons',\n", + " '1281': 'polytropes',\n", + " '1282': 'population i stars',\n", + " '1283': 'population ii cepheid variable stars',\n", + " '1284': 'population ii stars',\n", + " '1285': 'population iii stars',\n", + " '1286': 'position angle',\n", + " '1287': 'post-asymptotic giant branch',\n", + " '1288': 'pp waves',\n", + " '1289': 'pre-main sequence',\n", + " '129': 'b subdwarf stars',\n", + " '1290': 'pre-main sequence stars',\n", + " '1291': 'pre-solar nebulae',\n", + " '1292': 'primordial black holes',\n", + " '1293': 'primordial galaxies',\n", + " '1294': 'primordial magnetic fields',\n", + " '1295': 'proper motions',\n", + " '1296': 'proplyds',\n", + " '1297': 'protoclusters',\n", + " '1298': 'protogalaxies',\n", + " '1299': 'proton-proton reaction',\n", + " '13': 'accreting binary stars',\n", + " '130': 'b supergiant stars',\n", + " '1300': 'protoplanetary disks',\n", + " '1301': 'protoplanetary nebulae',\n", + " '1302': 'protostars',\n", + " '1303': 'ptolemy stones',\n", + " '1304': 'pulsar planets',\n", + " '1305': 'pulsar timing method',\n", + " '1306': 'pulsars',\n", + " '1307': 'pulsating variable stars',\n", + " '1308': 'pulsation frequency method',\n", + " '1309': 'pulsation modes',\n", + " '131': 'baade-wesselink method',\n", + " '1310': 'purkinje effect',\n", + " '1311': 'pv telescopii variable stars',\n", + " '1312': 'quadrants',\n", + " '1313': 'quantum cosmology',\n", + " '1314': 'quantum gravity',\n", + " '1315': 'quaoar',\n", + " '1316': 'quasar-galaxy pairs',\n", + " '1317': 'quasar absorption line spectroscopy',\n", + " '1318': 'quasar microlensing',\n", + " '1319': 'quasars',\n", + " '132': 'bailey type stars',\n", + " '1320': 'quasinormal modes',\n", + " '1321': 'quiescent solar prominence',\n", + " '1322': 'quiet sun',\n", + " '1323': 'quintessence',\n", + " '1324': 'r-process',\n", + " '1325': 'r associations',\n", + " '1326': 'r coronae borealis stars',\n", + " '1327': 'r coronae borealis variable stars',\n", + " '1328': 'r stars',\n", + " '1329': 'radar astronomy',\n", + " '133': \"baily's beads\",\n", + " '1330': 'radar telescopes',\n", + " '1331': 'radial pulsations',\n", + " '1332': 'radial velocity',\n", + " '1333': 'radial velocity methods [exoplanets]',\n", + " '1334': 'radiative braking',\n", + " '1335': 'radiative transfer',\n", + " '1336': 'radiative transfer equation',\n", + " '1337': 'radio astrometry',\n", + " '1338': 'radio astronomy',\n", + " '1339': 'radio bursts',\n", + " '134': 'baker-nunn cameras',\n", + " '1340': 'radio continuum emission',\n", + " '1341': 'radio cores',\n", + " '1342': 'solar radio flares',\n", + " '1343': 'radio galaxies',\n", + " '1344': 'radio hot spots',\n", + " '1345': 'radio interferometers',\n", + " '1346': 'radio interferometry',\n", + " '1347': 'radio jets',\n", + " '1348': 'radio lobes',\n", + " '1349': 'radio loud quasars',\n", + " '135': 'barium stars',\n", + " '1350': 'radio observatories',\n", + " '1351': 'radio occultation',\n", + " '1352': 'radio plumes',\n", + " '1353': 'radio pulsars',\n", + " '1354': 'radio quiet quasars',\n", + " '1355': 'radio receivers',\n", + " '1356': 'radio source catalogs',\n", + " '1357': 'radio source counts',\n", + " '1358': 'radio sources',\n", + " '1359': 'radio spectroscopy',\n", + " '136': 'barred spiral galaxies',\n", + " '1360': 'radio telescopes',\n", + " '1361': 'radioheliographs',\n", + " '1362': 'rapid bursts',\n", + " '1363': 'rapid stellar oscillations',\n", + " '1364': 'rc aurigae stars',\n", + " '1365': 'recombination (cosmology)',\n", + " '1366': 'recurrent novae',\n", + " '1367': 'red dwarf flare stars',\n", + " '1368': 'red giant branch',\n", + " '1369': 'red giant bump',\n", + " '137': 'baryogenesis',\n", + " '1370': 'red giant clump',\n", + " '1371': 'red giant tip',\n", + " '1372': 'red giant stars',\n", + " '1373': 'red sequence galaxies',\n", + " '1374': 'red straggler stars',\n", + " '1375': 'red supergiant stars',\n", + " '1376': 'reddened stars',\n", + " '1377': 'reddening law',\n", + " '1378': 'redshift surveys',\n", + " '1379': 'redshifted',\n", + " '138': 'baryon acoustic oscillations',\n", + " '1380': 'reflecting telescopes',\n", + " '1381': 'reflection nebulae',\n", + " '1382': 'refracting telescopes',\n", + " '1383': 'reionization',\n", + " '1384': 'reissner-nordström black holes',\n", + " '1385': 'relativistic aberration',\n", + " '1386': 'relativistic binary stars',\n", + " '1387': 'relativistic cosmology',\n", + " '1388': 'relativistic disks',\n", + " '1389': 'relativistic fluid dynamics',\n", + " '139': 'baryon density',\n", + " '1390': 'relativistic jets',\n", + " '1391': 'relativistic mechanics',\n", + " '1392': 'relativistic stars',\n", + " '1393': 'relativity',\n", + " '1394': 'relaxation time',\n", + " '1395': 'remote telescope astrophotography',\n", + " '1396': 'resonant kuiper belt objects',\n", + " '1397': 'rgb photometry',\n", + " '1398': 'rgu photometry',\n", + " '1399': 'right ascension',\n", + " '14': 'accretion',\n", + " '140': 'baryonic dark matter',\n", + " '1400': 'ring galaxies',\n", + " '1401': 'ring nebulae',\n", + " '1402': 'ring singularities',\n", + " '1403': 'ritchey-chrétien telescopes',\n", + " '1404': 'roche limit',\n", + " '1405': 'roche lobe',\n", + " '1406': 'rotating black holes',\n", + " '1407': 'rotating shells',\n", + " '1408': 'rotation powered pulsars',\n", + " '1409': 'rovers',\n", + " '141': 'bautz-morgan type',\n", + " '1410': 'rr lyrae variable stars',\n", + " '1411': 'rr telescopii stars',\n", + " '1412': 'rra stars',\n", + " '1413': 'rrab variable stars',\n", + " '1414': 'rrb stars',\n", + " '1415': 'rrc variable stars',\n", + " '1416': 'rs canum venaticorum variable stars',\n", + " '1417': 'runaway stars',\n", + " '1418': 'rv tauri variable stars',\n", + " '1419': 's-process',\n", + " '142': 'be stars',\n", + " '1420': 's doradus stars',\n", + " '1421': 's stars',\n", + " '1422': 's vulpeculae stars',\n", + " '1423': 'sagittarius dwarf spheroidal galaxy',\n", + " '1424': 'saros cycle',\n", + " '1425': 'natural satellite formation',\n", + " '1426': 'saturn',\n", + " '1427': 'saturnian satellites',\n", + " '1428': 'scalar-tensor-vector gravity',\n", + " '1429': 'scale height',\n", + " '143': 'be type stars',\n", + " '1430': 'scattered disk objects',\n", + " '1431': 'schmidt-cassegrain telescopes',\n", + " '1432': 'schmidt cameras',\n", + " '1433': 'schwarzschild black holes',\n", + " '1434': 'schwarzschild metric',\n", + " '1435': 'schwarzschild radius',\n", + " '1436': 'sculptor dwarf elliptical galaxy',\n", + " '1437': 'seasonal phenomena',\n", + " '1438': 'secondary cosmic rays',\n", + " '1439': 'secular parallax',\n", + " '144': 'bediasites',\n", + " '1440': 'sedna',\n", + " '1441': 'selenology',\n", + " '1442': 'semi-barium stars',\n", + " '1443': 'semi-detached binary stars',\n", + " '1444': 'semi-regular variable stars',\n", + " '1445': 'semimajor axis',\n", + " '1446': 'semiminor axis',\n", + " '1447': 'seyfert galaxies',\n", + " '1448': \"seyfert's sextet\",\n", + " '1449': 'shadow bands',\n", + " '145': 'bekenstein-hawking entropy',\n", + " '1450': 'shell burning',\n", + " '1451': 'shepherd satellites',\n", + " '1452': 'short period comets',\n", + " '1453': 'short period variable stars',\n", + " '1454': 'siderostats',\n", + " '1455': 'sigma8',\n", + " '1456': 'silicate grains',\n", + " '1457': 'silicon burning',\n", + " '1458': 'silicon monoxide masers',\n", + " '1459': 'silicon stars',\n", + " '146': 'beryllium abundance',\n", + " '1460': 'single-dish antennas',\n", + " '1461': 'single x-ray stars',\n", + " '1462': 'sky brightness',\n", + " '1463': 'sky noise',\n", + " '1464': 'sky surveys',\n", + " '1465': 'sloan photometry',\n", + " '1466': 'slow irregular variable stars',\n", + " '1467': 'slow novae',\n", + " '1468': 'small magellanic cloud',\n", + " '1469': 'small solar system bodies',\n", + " '147': 'bessel photometry',\n", + " '1470': 'sociology of astronomy',\n", + " '1471': 'soft gamma-ray repeaters',\n", + " '1472': 'solar-planetary interactions',\n", + " '1473': 'solar-terrestrial interactions',\n", + " '1474': 'solar abundances',\n", + " '1475': 'solar activity',\n", + " '1476': 'solar physics',\n", + " '1477': 'solar atmosphere',\n", + " '1478': 'solar atmospheric motions',\n", + " '1479': 'solar chromosphere',\n", + " '148': 'beta cephei variable stars',\n", + " '1480': 'solar composition',\n", + " '1481': 'solar constant',\n", + " '1482': 'solar core',\n", + " '1483': 'solar corona',\n", + " '1484': 'solar coronal holes',\n", + " '1485': 'solar coronal loops',\n", + " '1486': 'solar coronal streamers',\n", + " '1487': 'solar cycle',\n", + " '1488': 'solar radius',\n", + " '1489': 'solar eclipses',\n", + " '149': 'beta lyrae stars',\n", + " '1490': 'solar electromagnetic emission',\n", + " '1491': 'solar energetic particles',\n", + " '1492': 'solar evolution',\n", + " '1493': 'solar extreme ultraviolet emission',\n", + " '1494': 'solar faculae',\n", + " '1495': 'solar filaments',\n", + " '1496': 'solar flares',\n", + " '1497': 'solar gamma-ray emission',\n", + " '1498': 'solar granulation',\n", + " '1499': 'solar instruments',\n", + " '15': 'achondrites',\n", + " '150': 'bianchi cosmology',\n", + " '1500': 'solar interior',\n", + " '1501': 'solar spectral irradiance',\n", + " '1502': 'solar macrospicules',\n", + " '1503': 'solar magnetic fields',\n", + " '1504': 'solar magnetic reconnection',\n", + " '1505': 'solar magnetism',\n", + " '1506': 'solar mass',\n", + " '1507': 'solar motion',\n", + " '1508': 'solar nebulae',\n", + " '1509': 'solar neighborhood',\n", + " '151': 'big bang nucleosynthesis',\n", + " '1510': 'solar neutrino problem',\n", + " '1511': 'solar neutrinos',\n", + " '1512': 'solar neutrons',\n", + " '1513': 'solar observatories',\n", + " '1514': 'solar optical telescopes',\n", + " '1515': 'solar oscillations',\n", + " '1516': 'solar parallax',\n", + " '1517': 'solar particle emission',\n", + " '1518': 'solar photosphere',\n", + " '1519': 'solar prominences',\n", + " '152': 'big bang theory',\n", + " '1520': 'solar properties',\n", + " '1521': 'solar radiation',\n", + " '1522': 'solar radio emission',\n", + " '1523': 'solar radio telescopes',\n", + " '1524': 'solar rotation',\n", + " '1525': 'solar spicules',\n", + " '1526': 'solar storm',\n", + " '1527': 'solar surface',\n", + " '1528': 'solar system',\n", + " '1529': 'solar system astronomy',\n", + " '153': 'binary pulsars',\n", + " '1530': 'solar system formation',\n", + " '1531': 'solar telescopes',\n", + " '1532': 'solar transition region',\n", + " '1533': 'solar ultraviolet emission',\n", + " '1534': 'solar wind',\n", + " '1535': 'solar wind termination',\n", + " '1536': 'solar x-ray emission',\n", + " '1537': 'solstice',\n", + " '1538': 'south celestial pole',\n", + " '1539': 'south ecliptic pole',\n", + " '154': 'binary stars',\n", + " '1540': 'south galactic pole',\n", + " '1541': 'space astrometry',\n", + " '1542': 'space debris',\n", + " '1543': 'space observatories',\n", + " '1544': 'space plasmas',\n", + " '1545': 'space probes',\n", + " '1546': 'space research',\n", + " '1547': 'space telescopes',\n", + " '1548': 'space vehicle instruments',\n", + " '1549': 'space vehicles',\n", + " '155': 'bipolar nebulae',\n", + " '1550': 'spacetime metric',\n", + " '1551': 'special relativity',\n", + " '1552': 'speckle interferometry',\n", + " '1553': 'spectral index',\n", + " '1554': 'spectrometers',\n", + " '1555': 'spectrophotometric standards',\n", + " '1556': 'spectrophotometry',\n", + " '1557': 'spectroscopic binary stars',\n", + " '1558': 'spectroscopy',\n", + " '1559': 'spiral arms',\n", + " '156': 'bipolar sunspot groups',\n", + " '1560': 'spiral galaxies',\n", + " '1561': 'spiral pitch angle',\n", + " '1562': 'spokes',\n", + " '1563': 'standard candles',\n", + " '1564': 'standard stars',\n", + " '1565': 'star forming regions',\n", + " '1566': 'star atlases',\n", + " '1567': 'star clusters',\n", + " '1568': 'star counts',\n", + " '1569': 'star formation',\n", + " '157': 'bl herculis variable stars',\n", + " '1570': 'starburst galaxies',\n", + " '1571': 'starlight polarization',\n", + " '1572': 'starspots',\n", + " '1573': 'statistical parallax',\n", + " '1574': 'steady-state theory',\n", + " '1575': \"stephan's quintet\",\n", + " '1576': 'stellar-interstellar interactions',\n", + " '1577': 'stellar abundances',\n", + " '1578': 'stellar accretion',\n", + " '1579': 'stellar accretion disks',\n", + " '158': 'bl lacertae objects',\n", + " '1580': 'stellar activity',\n", + " '1581': 'stellar ages',\n", + " '1582': 'stellar associations',\n", + " '1583': 'stellar astronomy',\n", + " '1584': 'stellar atmospheres',\n", + " '1585': 'stellar atmospheric opacity',\n", + " '1586': 'stellar bow shocks',\n", + " '1587': 'stellar bridges',\n", + " '1588': 'stellar chemical composition',\n", + " '1589': 'stellar classification',\n", + " '159': 'black hole physics',\n", + " '1590': 'stellar colors',\n", + " '1591': 'stellar composition',\n", + " '1592': 'stellar cores',\n", + " '1593': 'stellar diffusion',\n", + " '1594': 'galaxy stellar disks',\n", + " '1595': 'stellar distance',\n", + " '1596': 'stellar dynamics',\n", + " '1597': 'stellar effective temperatures',\n", + " '1598': 'stellar elemental abundances',\n", + " '1599': 'stellar evolution',\n", + " '16': 'active galactic nuclei',\n", + " '160': 'black hole spin-flip',\n", + " '1600': 'stellar evolutionary tracks',\n", + " '1601': 'stellar faculae',\n", + " '1602': 'stellar feedback',\n", + " '1603': 'stellar flares',\n", + " '1604': 'stellar gas distribution',\n", + " '1605': 'stellar inner cores',\n", + " '1606': 'stellar interiors',\n", + " '1607': 'stellar jets',\n", + " '1608': 'stellar kinematics',\n", + " '1609': 'stellar luminosities',\n", + " '161': 'black hole thermodynamics',\n", + " '1610': 'stellar magnetic fields',\n", + " '1611': 'stellar mass black holes',\n", + " '1612': 'stellar mass functions',\n", + " '1613': 'stellar mass loss',\n", + " '1614': 'stellar masses',\n", + " '1615': 'stellar motion',\n", + " '1616': 'stellar nucleosynthesis',\n", + " '1617': 'stellar oscillations',\n", + " '1618': 'stellar parallax',\n", + " '1619': 'stellar phenomena',\n", + " '162': 'black holes',\n", + " '1620': 'stellar photometry',\n", + " '1621': 'stellar physics',\n", + " '1622': 'stellar populations',\n", + " '1623': 'stellar processes',\n", + " '1624': 'stellar properties',\n", + " '1625': 'stellar pulsations',\n", + " '1626': 'stellar radii',\n", + " '1627': 'stellar remnants',\n", + " '1628': 'stellar rings',\n", + " '1629': 'stellar rotation',\n", + " '163': 'blank fields',\n", + " '1630': 'stellar spectral lines',\n", + " '1631': 'stellar structures',\n", + " '1632': 'stellar surfaces',\n", + " '1633': 'stellar tracking devices',\n", + " '1634': 'stellar types',\n", + " '1635': 'stellar wind bubbles',\n", + " '1636': 'stellar winds',\n", + " '1637': 'stellar x-ray flares',\n", + " '1638': 'stone circles',\n", + " '1639': 'stratopause',\n", + " '164': 'blazars',\n", + " '1640': 'stratosphere',\n", + " '1641': 'strömgren photometry',\n", + " '1642': 'strömgren spheres',\n", + " '1643': 'strong gravitational lensing',\n", + " '1644': 'strontium stars',\n", + " '1645': 'su ursae majoris stars',\n", + " '1646': 'subgiant stars',\n", + " '1647': 'submillimeter astronomy',\n", + " '1648': 'substellar companion stars',\n", + " '1649': 'summer solstice',\n", + " '165': 'blue compact dwarf galaxies',\n", + " '1650': 'sunspot cycle',\n", + " '1651': 'sunspot groups',\n", + " '1652': 'sunspot number',\n", + " '1653': 'sunspots',\n", + " '1654': 'sunyaev-zeldovich effect',\n", + " '1655': 'super earths',\n", + " '1656': 'superbubbles',\n", + " '1657': 'superclusters',\n", + " '1658': 'supergalactic coordinate system',\n", + " '1659': 'supergalactic latitude',\n", + " '166': 'blue cloud galaxies',\n", + " '1660': 'supergalactic longitude',\n", + " '1661': 'supergiant stars',\n", + " '1662': 'supergranulation',\n", + " '1663': 'supermassive black holes',\n", + " '1664': 'supernova dynamics',\n", + " '1665': 'supernova evolution',\n", + " '1666': 'supernova neutrinos',\n", + " '1667': 'supernova remnants',\n", + " '1668': 'supernovae',\n", + " '1669': 'surface gravity',\n", + " '167': 'blue loop',\n", + " '1670': 'surface photometry',\n", + " '1671': 'surveys',\n", + " '1672': 'sx arietis variable stars',\n", + " '1673': 'sx phoenicis variable stars',\n", + " '1674': 'symbiotic binary stars',\n", + " '1675': 'symbiotic novae',\n", + " '1676': 'synodic period',\n", + " '1677': 'syzygy',\n", + " '1678': 't associations',\n", + " '1679': 't dwarfs',\n", + " '168': 'blue straggler stars',\n", + " '1680': 't subdwarfs',\n", + " '1681': 't tauri stars',\n", + " '1682': 'tailed radio galaxies',\n", + " '1683': 'technetium stars',\n", + " '1684': 'astronomical techniques',\n", + " '1685': 'teharonhiawako',\n", + " '1686': 'tektites',\n", + " '1687': 'telescope focal plane photography',\n", + " '1688': 'telescope mounts',\n", + " '1689': 'telescopes',\n", + " '169': 'blueshifted',\n", + " '1690': 'termination shock',\n", + " '1691': 'tertiary stars',\n", + " '1692': 'the moon',\n", + " '1693': 'the sun',\n", + " '1694': 'thermosphere',\n", + " '1695': 'three-body problem',\n", + " '1696': 'tidal disruption',\n", + " '1697': 'tidal distortion',\n", + " '1698': 'tidal friction',\n", + " '1699': 'tidal interaction',\n", + " '17': 'active galaxies',\n", + " '170': \"bode's law\",\n", + " '1700': 'tidal radius',\n", + " '1701': 'tidal tails',\n", + " '1702': 'tides',\n", + " '1703': 'timing variation methods',\n", + " '1704': 'total eclipses',\n", + " '1705': 'trans-neptunian objects',\n", + " '1706': 'trans-planckian physics',\n", + " '1707': 'transit duration variation method',\n", + " '1708': 'transit instruments',\n", + " '1709': 'transit photometry',\n", + " '171': 'bok globules',\n", + " '1710': 'transit timing variation method',\n", + " '1711': 'transits',\n", + " '1712': 'triangulum galaxy',\n", + " '1713': 'trigonometric parallax',\n", + " '1714': 'trinary stars',\n", + " '1715': 'trojan asteroids',\n", + " '1716': 'trojan planets',\n", + " '1717': 'tropopause',\n", + " '1718': 'troposphere',\n", + " '1719': 'true anomaly',\n", + " '172': 'bolides',\n", + " '1720': 'true position',\n", + " '1721': 'turnoff point',\n", + " '1722': 'twilight',\n", + " '1723': 'two-body problem',\n", + " '1724': 'two-color diagrams',\n", + " '1725': 'two-dimensional gravity',\n", + " '1726': 'two-spectrum binary stars',\n", + " '1727': 'twotinos',\n", + " '1728': 'type ia supernovae',\n", + " '1729': 'type ib supernovae',\n", + " '173': 'bolometric correction',\n", + " '1730': 'type ic supernovae',\n", + " '1731': 'type ii supernovae',\n", + " '1732': 'u geminorum stars',\n", + " '1733': 'ultra-high-energy cosmic radiation',\n", + " '1734': 'ultracompact dwarf galaxies',\n", + " '1735': 'ultraluminous infrared galaxies',\n", + " '1736': 'ultraviolet astronomy',\n", + " '1737': 'ultraviolet color',\n", + " '1738': 'ultraviolet extinction',\n", + " '1739': 'ultraviolet observatories',\n", + " '174': 'bondi accretion',\n", + " '1740': 'ultraviolet photometry',\n", + " '1741': 'ultraviolet sources',\n", + " '1742': 'ultraviolet surveys',\n", + " '1743': 'ultraviolet telescopes',\n", + " '1744': 'umbra',\n", + " '1745': 'unbarred spiral galaxies',\n", + " '1746': 'uncharged black holes',\n", + " '1747': 'underabundances',\n", + " '1748': 'upper atmosphere',\n", + " '1749': 'upsilon sagittarii stars',\n", + " '175': 'borasisi',\n", + " '1750': 'uranian satellites',\n", + " '1751': 'uranus',\n", + " '1752': 'urca process',\n", + " '1753': 'ursa minor dwarf spheroidal galaxy',\n", + " '1754': 'uu herculis stars',\n", + " '1755': 'uv ceti stars',\n", + " '1756': 'uv persei stars',\n", + " '1757': 'ux ursae majoris stars',\n", + " '1758': 'van allen radiation belts',\n", + " '1759': 'variable radiation sources',\n", + " '176': 'boron abundance',\n", + " '1760': 'variable star period change',\n", + " '1761': 'variable stars',\n", + " '1762': 'varuna',\n", + " '1763': 'venus',\n", + " '1764': 'vernal equinox',\n", + " '1765': 'vertical circle',\n", + " '1766': 'very large array',\n", + " '1767': 'very large telescope',\n", + " '1768': 'very long baseline interferometers',\n", + " '1769': 'very long baseline interferometry',\n", + " '177': 'bouwers telescope',\n", + " '1770': 'very small grains',\n", + " '1771': 'vilnius photometry',\n", + " '1772': 'virgo cluster',\n", + " '1773': 'virgo supercluster',\n", + " '1774': 'virtual observatories',\n", + " '1775': 'visibility function',\n", + " '1776': 'optical astronomy',\n", + " '1777': 'visual binary stars',\n", + " '1778': 'visual observation',\n", + " '1779': 'voids',\n", + " '178': 'bp stars',\n", + " '1780': 'volcanoes',\n", + " '1781': 'von zeipel theorem',\n", + " '1782': 'vy sculpturis stars',\n", + " '1783': 'w ursae majoris variable stars',\n", + " '1784': 'w virginis variable stars',\n", + " '1785': 'walraven photometry',\n", + " '1786': 'warm-hot intergalactic medium',\n", + " '1787': 'warm dark matter',\n", + " '1788': 'warm ionized medium',\n", + " '1789': 'warm neutral medium',\n", + " '179': 'brane cosmology',\n", + " '1790': 'water masers',\n", + " '1791': 'water vapor',\n", + " '1792': 'waveband photometry',\n", + " '1793': 'wc stars',\n", + " '1794': 'wcn stars',\n", + " '1795': 'weak-line t tauri stars',\n", + " '1796': 'weak g band stars',\n", + " '1797': 'weak gravitational lensing',\n", + " '1798': 'white dwarf evolution',\n", + " '1799': 'white dwarf stars',\n", + " '18': 'active sun',\n", + " '180': 'bright nebulae',\n", + " '1800': 'wide-field telescopes',\n", + " '1801': 'wide binary stars',\n", + " '1802': 'wilson-bappu effect',\n", + " '1803': 'wilson effect',\n", + " '1804': 'winter solstice',\n", + " '1805': 'wn stars',\n", + " '1806': 'wolf-rayet stars',\n", + " '1807': 'wolf diagram',\n", + " '1808': 'wormholes',\n", + " '1809': 'wz sagittae stars',\n", + " '181': 'brightest cluster galaxies',\n", + " '1810': 'x-ray astronomy',\n", + " '1811': 'x-ray binary stars',\n", + " '1812': 'x-ray bright point',\n", + " '1813': 'x-ray bursters',\n", + " '1814': 'x-ray bursts',\n", + " '1815': 'x-ray detectors',\n", + " '1816': 'solar x-ray flares',\n", + " '1817': 'x-ray identification',\n", + " '1818': 'x-ray novae',\n", + " '1819': 'x-ray observatories',\n", + " '182': 'brightness temperature',\n", + " '1820': 'x-ray photometry',\n", + " '1821': 'x-ray quasars',\n", + " '1822': 'x-ray sources',\n", + " '1823': 'x-ray stars',\n", + " '1824': 'x-ray surveys',\n", + " '1825': 'x-ray telescopes',\n", + " '1826': 'xenobiology',\n", + " '1827': 'y dwarfs',\n", + " '1828': 'yellow hypergiant stars',\n", + " '1829': 'yellow straggler stars',\n", + " '183': 'broad-absorption line quasar',\n", + " '1830': 'yerkes classification',\n", + " '1831': 'yoke mounts',\n", + " '1832': 'young disk cepheid variable stars',\n", + " '1833': 'young star clusters',\n", + " '1834': 'young stellar objects',\n", + " '1835': 'z andromedae stars',\n", + " '1836': 'z camelopardalis stars',\n", + " '1837': 'zeeman-doppler imaging',\n", + " '1838': 'zenith',\n", + " '1839': 'zenith hourly rate',\n", + " '184': 'broad band photometry',\n", + " '1840': 'zenith telescopes',\n", + " '1841': 'zenith tubes',\n", + " '1842': 'zero-age horizontal branch stars',\n", + " '1843': 'zero-age main sequence stars',\n", + " '1844': 'zirconium stars',\n", + " '1845': 'zodiacal cloud',\n", + " '1846': 'zone of totality',\n", + " '1847': 'zz ceti stars',\n", + " '1848': 'dz stars',\n", + " '1849': 'dq stars',\n", + " '185': 'brown dwarfs',\n", + " '1850': 'shell stars',\n", + " '1851': 'transient sources',\n", + " '1852': 'x-ray transient sources',\n", + " '1853': 'gamma-ray transient sources',\n", + " '1854': 'ultraviolet transient sources',\n", + " '1855': 'astronomy software',\n", + " '1856': 'astronomy web services',\n", + " '1857': 'astronomical simulations',\n", + " '1858': 'astronomy data analysis',\n", + " '1859': 'astronomy data modeling',\n", + " '186': 'burkert profile',\n", + " '1860': 'astronomy data acquisition',\n", + " '1861': 'astronomy data reduction',\n", + " '1862': 'software licensing',\n", + " '1863': 'public domain software',\n", + " '1864': 'publicly available software',\n", + " '1865': 'software available on request',\n", + " '1866': 'open source software',\n", + " '1867': 'private software',\n", + " '1868': 'history of astronomy',\n", + " '1869': 'software documentation',\n", + " '187': 'burst astrophysics',\n", + " '1870': 'educational software',\n", + " '1871': 'software tutorials',\n", + " '1872': 'fast solar wind',\n", + " '1873': 'slow solar wind',\n", + " '1874': 'solar meridional circulation',\n", + " '1875': 'solar granules',\n", + " '1876': 'rrd variable stars',\n", + " '1877': 'magellanic irregular galaxies',\n", + " '1878': 'gamma-ray bursters',\n", + " '1879': 'circumgalactic medium',\n", + " '188': 'bv photometry',\n", + " '1880': 'galaxy dark matter halos',\n", + " '1881': 'stellar coronal mass ejections',\n", + " '1882': 'astrostatistics',\n", + " '1883': 'algorithms',\n", + " '1884': 'astrostatistics distributions',\n", + " '1885': 'astrostatistics strategies',\n", + " '1886': 'astrostatistics techniques',\n", + " '1887': 'astrostatistics tools',\n", + " '1888': 'expectation-maximization algorithm',\n", + " '1889': 'markov chain monte carlo',\n", + " '189': 'bw stars',\n", + " '1890': 'affine invariant',\n", + " '1891': 'gibbs sampler',\n", + " '1892': 'importance sampling',\n", + " '1893': 'metropolis-hastings',\n", + " '1894': 'nested sampling',\n", + " '1895': 'gamma distribution',\n", + " '1896': 'normal distribution',\n", + " '1897': 'pareto distribution',\n", + " '1898': 'poisson distribution',\n", + " '1899': 'sampling distribution',\n", + " ...}" + ] + }, + "execution_count": 2, + "metadata": {}, + "output_type": "execute_result" + } + ], + "source": [ + "uat_names" + ] + }, + { + "cell_type": "code", + "execution_count": 3, + "id": "688bdebb-f711-49c7-8c1b-f9ede9529ce8", + "metadata": {}, + "outputs": [ + { + "name": "stderr", + "output_type": "stream", + "text": [ + "Using custom data configuration fgrezes--SciX_UAT_keywords-789597c18f53575e\n", + "Reusing dataset parquet (/proj.adsnlp/jupyter-lab/one/ads/.cache/huggingface/datasets/adsabs___parquet/fgrezes--SciX_UAT_keywords-789597c18f53575e/0.0.0/7328ef7ee03eaf3f86ae40594d46a1cec86161704e02dd19f232d81eee72ade8)\n" + ] + }, + { + "data": { + "application/json": { + "ascii": false, + "bar_format": null, + "colour": null, + "elapsed": 0.00523829460144043, + "initial": 0, + "n": 0, + "ncols": null, + "nrows": null, + "postfix": null, + "prefix": "", + "rate": null, + "total": 2, + "unit": "it", + "unit_divisor": 1000, + "unit_scale": false + }, + "application/vnd.jupyter.widget-view+json": { + "model_id": "dce86036a5284c87beb55eb33a8e6f97", + "version_major": 2, + "version_minor": 0 + }, + "text/plain": [ + " 0%| | 0/2 [00:00J (q ~ 0.02), making HD 136164 Ab the youngest substellar companion with a dynamical mass estimate. The new mass and newly constrained orbital eccentricity (e = 0.44 ± 0.03) and separation (22.5 ± 1 au) could indicate that the companion formed via the low-mass tail of the initial mass function. Our atmospheric fit to a SPHINX M-dwarf model grid suggests a subsolar C/O ratio of 0.45 and 3 × solar metallicity, which could indicate formation in a circumstellar disk via disk fragmentation. Either way, the revised mass estimate likely excludes bottom-up formation via core accretion in a circumstellar disk. HD 136164 Ab joins a select group of young substellar objects with dynamical mass estimates; epoch astrometry from future Gaia data releases will constrain the dynamical mass of this crucial object further.\n", + "\n", + "AUTHOR ASSIGNED: ['brown dwarfs', 'substellar companion stars', 'orbit determination', 'orbits']\n", + "MODEL ASSIGNED: [('radial velocity', '0.8792'), ('exoplanets', '0.8334'), ('exoplanet detection methods', '0.5305'), ('exoplanet dynamics', '0.3328'), ('extrasolar gaseous giant planets', '0.2636')]\n", + "\n", + "NEXT SCORES [('direct imaging', '0.0761'), ('transit photometry', '0.0569'), ('exoplanet atmospheres', '0.0440'), ('exoplanet evolution', '0.0425'), ('exoplanet structure', '0.0157'), ('brown dwarfs', '0.0146'), ('exoplanet systems', '0.0138'), ('solar-terrestrial interactions', '0.0083'), ('atmospheric composition', '0.0079'), ('natural satellites (extrasolar)', '0.0056'), ('interferometers', '0.0056'), ('gaussian processes regression', '0.0049'), ('exoplanet atmospheric variability', '0.0043'), ('exoplanet atmospheric composition', '0.0028'), ('astrometry', '0.0023'), ('interplanetary magnetic fields', '0.0019'), ('solar analogs', '0.0016')]\n", + "\n", + "\n" + ] + } + ], + "source": [ + "# MAIN DEMO \n", + "# pick some samples from our dataset\n", + "# this is a list of strings\n", + "\n", + "num_pred = 3\n", + "start = 510\n", + "\n", + "temp_dataset = uat_dataset['val'][start:start+num_pred]\n", + "sentences = [str(t)+' '+str(a) for t,a in zip(temp_dataset['title'],\n", + " temp_dataset['abstract'])\n", + " if t\n", + " ]\n", + "\n", + "# make predictions\n", + "all_sentence_scores = pipe(sentences)\n", + "\n", + "# we need to change the output of the model to strings to make it compatible with the next version.\n", + "# it's best to think of the outputs as labels anyways, not as integers\n", + "all_sentence_scores = [[{'label':str(s['label']), 'score':s['score']} for s in sample_scores] for sample_scores in all_sentence_scores]\n", + "\n", + "# format for readability, and show top k scores\n", + "threshold = 0.15\n", + "top_sentence_scores = [[ {'label':uat_names[l['label']], 'score':l['score']} \n", + " for l in top_k_scores(s, k=1000) if l['score']>=threshold] \n", + " for s in all_sentence_scores]\n", + "\n", + "next_sentence_scores = [[ {'label':uat_names[l['label']], 'score':l['score']} \n", + " for l in top_k_scores(s, k=1000) if l['score']<=threshold and l['score']>=0.01*threshold] \n", + " for s in all_sentence_scores]\n", + "\n", + "for i in range(min(10,num_pred)):\n", + " print('BIBCODE:', temp_dataset['bibcode'][i])\n", + " print('\\tTITLE:', temp_dataset['title'][i])\n", + " print('\\tABSTRACT:', temp_dataset['abstract'][i])\n", + " print()\n", + " print('AUTHOR ASSIGNED:', temp_dataset['verified_uat_labels'][i])\n", + "\n", + " if len(top_sentence_scores[i])>0:\n", + " print('MODEL ASSIGNED:', [(x['label'], '{:.4f}'.format(x['score'])) for x in top_sentence_scores[i]] )\n", + " print()\n", + " print('NEXT SCORES', [(x['label'], '{:.4f}'.format(x['score'])) for x in next_sentence_scores[i]] )\n", + " \n", + " print() \n", + " print()\n" + ] + }, + { + "cell_type": "code", + "execution_count": 8, + "id": "9d90c6a5-7a0a-4762-ae5d-33523bd6bc9a", + "metadata": { + "tags": [] + }, + "outputs": [], + "source": [ + "# Note: truncation is in effect and long sentences will only take into account the first 512 tokens\n", + "sentences = [' '.join(['1' for i in range(j) ]) for j in range(505,515)]\n", + "sentence_scores = pipe(sentences)" + ] + }, + { + "cell_type": "code", + "execution_count": 9, + "id": "e4b80a73-577a-464c-add2-2356c3adff18", + "metadata": { + "tags": [] + }, + "outputs": [ + { + "data": { + "text/plain": [ + "[(505, [{'label': 2189, 'score': 0.8530406355857849}]),\n", + " (506, [{'label': 2189, 'score': 0.8583861589431763}]),\n", + " (507, [{'label': 2189, 'score': 0.8545922040939331}]),\n", + " (508, [{'label': 2189, 'score': 0.8484249114990234}]),\n", + " (509, [{'label': 2189, 'score': 0.8524807095527649}]),\n", + " (510, [{'label': 2189, 'score': 0.8559486269950867}]),\n", + " (511, [{'label': 2189, 'score': 0.8559486865997314}]),\n", + " (512, [{'label': 2189, 'score': 0.8559486269950867}]),\n", + " (513, [{'label': 2189, 'score': 0.8559486269950867}]),\n", + " (514, [{'label': 2189, 'score': 0.8559486865997314}])]" + ] + }, + "execution_count": 9, + "metadata": {}, + "output_type": "execute_result" + } + ], + "source": [ + "[(len(sent.split()), top_k_scores(scores, k=1)) for sent, scores in zip(sentences,sentence_scores)]" + ] + }, + { + "cell_type": "code", + "execution_count": 10, + "id": "0cd3c521-b25e-4768-b3f8-14f28d9c9c48", + "metadata": { + "tags": [] + }, + "outputs": [], + "source": [ + "# Demo with manually input astro sentences\n", + "sentences = ['This work discusses a junction-less nanowire tunnel field effect transistor (JLN-TFET) that combines the advantages of a junction-less field effect transistor (JLFET) and a tunnel field effect transistor (TFET). With a hetero-structure device made of silicon (Si) and germanium (Ge), an amalgamation of gate engineering and channel engineering is investigated. To eliminate junctions in the structure, a uniformly high dosage of doping (1019cm-3) has been employed throughout. In contrast to the source work function, which is set at 5.93 eV, the gate work function is set at 4.5 eV. When compared to junction less nanowire tunnel FET (JLTFET), the modified gate-all-around hetero junction less nanowire tunnel field effect transistor (GAA-H-JLNTFET) performs better. The proposed structure GAA-H-JLNTFET exhibits the ON current (ION) 6.5 × 10−5µA/m, the off current (IOFF) measures 2.97 × 10−20µA/m, the subthreshold slope (SS) is 12mV/Dec, and ION/IOFFis≈1015which makes them immune to short channel effect and suitable for low power application in Nano regime. Further, in this work, the proposed structure is utilized to implement the dielectric modulated low-power biosensor. The drain current is taken as the sensitivity parameter. Five different biomolecules sensitivity are measured and found better than the previous published results. For the simulation and analysis, the Silvaco Atlas 2D simulator with non-local band-to-band tunneling is used. ',\n", + " 'We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0). These include the complete sample of all suitable SNe Ia discovered in the last four decades at redshift z ≤ 0.01, collected and calibrated from ≥1000 HST orbits, more than doubling the sample whose size limits the precision of the direct determination of H 0. The Cepheids are calibrated geometrically from Gaia EDR3 parallaxes, masers in NGC 4258 (here tripling that sample of Cepheids), and detached eclipsing binaries in the Large Magellanic Cloud. All Cepheids in these anchors and SN Ia hosts were measured with the same instrument (WFC3) and filters (F555W, F814W, F160W) to negate zero-point errors. We present multiple verifications of Cepheid photometry and six tests of background determinations that show Cepheid measurements are accurate in the presence of crowded backgrounds. The SNe Ia in these hosts calibrate the magnitude-redshift relation from the revised Pantheon+ compilation, accounting here for covariance between all SN data and with host properties and SN surveys matched throughout to negate systematics. We decrease the uncertainty in the local determination of H 0 to 1 km s-1 Mpc-1 including systematics. We present results for a comprehensive set of nearly 70 analysis variants to explore the sensitivity of H 0 to selections of anchors, SN surveys, redshift ranges, the treatment of Cepheid dust, metallicity, form of the period-luminosity relation, SN color, peculiar-velocity corrections, sample bifurcations, and simultaneous measurement of the expansion history. Our baseline result from the Cepheid-SN Ia sample is H 0 = 73.04 ± 1.04 km s-1 Mpc-1, which includes systematic uncertainties and lies near the median of all analysis variants. We demonstrate consistency with measures from HST of the TRGB between SN Ia hosts and NGC 4258, and include them simultaneously to yield 72.53 ± 0.99 km s-1 Mpc-1. The inclusion of high-redshift SNe Ia yields H 0 = 73.30 ± 1.04 km s-1 Mpc-1 and q 0 = -0.51 ± 0.024. We find a 5σ difference with the prediction of H 0 from Planck cosmic microwave background observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date. The source of this now long-standing discrepancy between direct and cosmological routes to determining H 0 remains unknown.',\n", + " 'We use archival COBE/DIRBE data to construct a map of polycyclic aromatic hydrocarbon (PAH) emission in the λ-Orionis region. The presence of the 3.3 μm PAH feature within the DIRBE 3.5 μm band and the corresponding lack of significant PAH spectral features in the adjacent DIRBE bands (1.25, 2.2, and 4.9 μm) enable estimation of the PAH contribution to the 3.5 μm data. Having the shortest wavelength of known PAH features, the 3.3 μm feature probes the smallest PAHs, which are also the leading candidates for carriers of anomalous microwave emission (AME). We use this map to investigate the association between the AME and the emission from PAH molecules. We find that the spatial correlation in λ-Orionis is higher between AME and far-infrared dust emission (as represented by the DIRBE 240 μm map) than it is between our PAH map and AME. This finding, in agreement with previous studies using PAH features at longer wavelengths, is in tension with the hypothesis that AME is due to spinning PAHs. However, the expected correlation between mid-infrared and microwave emission could potentially be degraded by different sensitivities of each emission mechanism to local environmental conditions even if PAHs are the carriers of both.',\n", + " 'THis is a noew sentence with typoes and not really about astro anyways',\n", + " ]\n", + "\n", + "\n", + "all_sentence_scores = pipe(sentences)\n", + "# again convert to strings, to future-proof\n", + "all_sentence_scores = [[{'label':str(s['label']), 'score':s['score']} for s in sample_scores] for sample_scores in all_sentence_scores]\n", + "\n", + "top_sentence_scores = [[ {'label':uat_names[l['label']], 'score':l['score']} \n", + " for l in top_k_scores(s, k=3)] \n", + " for s in all_sentence_scores]" + ] + }, + { + "cell_type": "code", + "execution_count": 11, + "id": "c7aea0c3-ae49-464a-bca9-ae46cbeb1cbc", + "metadata": { + "tags": [] + }, + "outputs": [ + { + "data": { + "text/plain": [ + "[[{'label': 'astronomical instrumentation', 'score': 0.9473740458488464},\n", + " {'label': 'astronomy data modeling', 'score': 0.49145984649658203},\n", + " {'label': 'space vehicle instruments', 'score': 0.39475584030151367}],\n", + " [{'label': 'hubble constant', 'score': 0.993058443069458},\n", + " {'label': 'cosmology', 'score': 0.006782000884413719},\n", + " {'label': 'planetary nebulae', 'score': 0.001997443614527583}],\n", + " [{'label': 'interstellar dust', 'score': 0.9986469149589539},\n", + " {'label': 'polycyclic aromatic hydrocarbons', 'score': 0.99810791015625},\n", + " {'label': 'interstellar medium', 'score': 0.9940189123153687}],\n", + " [{'label': 'time series analysis', 'score': 0.2862895429134369},\n", + " {'label': 'astronomy data analysis', 'score': 0.08515171706676483},\n", + " {'label': 'optical telescopes', 'score': 0.04666740819811821}]]" + ] + }, + "execution_count": 11, + "metadata": {}, + "output_type": "execute_result" + } + ], + "source": [ + "top_sentence_scores" + ] + }, + { + "cell_type": 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"execution_count": 12, + "metadata": {}, + "output_type": "execute_result" + } + ], + "source": [ + "# the score for every label is available\n", + "all_sentence_scores[0]" + ] + } + ], + "metadata": { + "kernelspec": { + "display_name": "Python 3.8", + "language": "python", + "name": "python3.8" + }, + "language_info": { + "codemirror_mode": { + "name": "ipython", + "version": 3 + }, + "file_extension": ".py", + "mimetype": "text/x-python", + "name": "python", + "nbconvert_exporter": "python", + "pygments_lexer": "ipython3", + "version": "3.8.18" + } + }, + "nbformat": 4, + "nbformat_minor": 5 +}