2024RAA....24f5012S


Query : 2024RAA....24f5012S

2024RAA....24f5012S - Research in Astron. and astroph., 24, part no 6, 5012 (2024/June-0)

Astronomical Knowledge Entity Extraction in Astrophysics Journal Articles via Large Language Models.

SHAO W., ZHANG R., JI P., FAN D., HU Y., YAN X., CUI C., TAO Y., MI L. and CHEN L.

Abstract (from CDS):

Astronomical knowledge entities, such as celestial object identifiers, are crucial for literature retrieval and knowledge graph construction, and other research and applications in the field of astronomy. Traditional methods of extracting knowledge entities from texts face numerous challenging obstacles that are difficult to overcome. Consequently, there is a pressing need for improved methods to efficiently extract them. This study explores the potential of pre-trained Large Language Models (LLMs) to perform astronomical knowledge entity extraction (KEE) task from astrophysical journal articles using prompts. We propose a prompting strategy called Prompt-KEE, which includes five prompt elements, and design eight combination prompts based on them. We select four representative LLMs (Llama-2-70B, GPT-3.5, GPT-4, and Claude 2) and attempt to extract the most typical astronomical knowledge entities, celestial object identifiers and telescope names, from astronomical journal articles using these eight combination prompts. To accommodate their token limitations, we construct two data sets: the full texts and paragraph collections of 30 articles. Leveraging the eight prompts, we test on full texts with GPT-4 and Claude 2, on paragraph collections with all LLMs. The experimental results demonstrate that pre-trained LLMs show significant potential in performing KEE tasks, but their performance varies on the two data sets. Furthermore, we analyze some important factors that influence the performance of LLMs in entity extraction and provide insights for future KEE tasks in astrophysical articles using LLMs. Finally, compared to other methods of KEE, LLMs exhibit strong competitiveness in multiple aspects.

Abstract Copyright: © 2024. National Astronomical Observatories

Journal keyword(s): astronomical databases: miscellaneous - virtual observatory tools - methods: data analysis

Simbad objects: 32

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Number of rows : 32
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 2MASS J00372064+4016376 sg* 00 37 20.6400062208 +40 16 37.706986056   16.085 15.854     ~ 5 0
2 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
3 LAMOST J004936.61+375022.7 Opt 00 49 36.6180000 +37 50 22.761600           ~ 1 0
4 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
5 FRB 20201124A rB 05 07 57.600 +26 11 24.00           ~ 307 0
6 NGC 1866 GlC 05 13 38.920 -65 27 52.75           ~ 437 0
7 V* UV Aur C* 05 21 48.9129714624 +32 30 40.177664388   12.46 10.41 9.15   C8,1Je 223 0
8 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
9 SMP LMC 88 PN 05 42 33.193 -70 29 24.08 17.119 17.335 16.825 16.260 16.226 ~ 35 0
10 TYC 1951-656-1 Pe* 09 16 08.8168539480 +23 07 34.851924948   11.44 10.40     C-H 5 0
11 Ton 580 Bla 11 31 09.4824534600 +31 14 05.506804464   16.22 16.05 15.8   ~ 156 1
12 V* BI Cru Sy* 12 23 25.9932684936 -62 38 15.988288740 12.06 12.18 11.00 10.71   M0/1e 144 0
13 V* RT Cru Sy* 12 34 53.7361211904 -64 33 56.099018448   12.20 11.35 12.09   M4/5e 107 0
14 1SWASP J133417.80+394314.4 EB* 13 34 17.7929911512 +39 43 14.248689888     14.86     K2V 12 0
15 PB 1309 Sy1 14 04 38.7980689872 +43 27 07.452879120   16.12 15.76     ~ 134 0
16 WRAY 16-148 Sy* 14 14 09.4115687736 -63 25 46.319333808   14.293 13.168 13.393   Me 141 1
17 TYC 2562-783-1 Pe* 15 10 03.3016410720 +30 54 07.357976928   13.50 11.38     C-H 15 0
18 WRAY 16-180 Sy* 15 24 49.7859801424 -51 49 52.587850026     15.501   13.128 M3.5-7e 70 1
19 V* AS Ser EB* 15 38 49.0208409480 +02 15 30.211375932   12.17 11.39 11.382 11.119 F2 32 0
20 WRAY 16-193 Sy* 15 54 44.4419004792 -55 29 34.028008224     17.762   12.783 M6.5 45 2
21 WRAY 16-208 Sy* 16 14 01.1094201648 -56 59 28.043753388     16.00     M8/9e 93 1
22 EM* AS 221 Sy* 17 12 12.8624441616 -32 37 46.747096500     16.0     M4 44 1
23 WRAY 15-1655 Sy* 17 15 19.8214542048 -31 33 53.392793688   17.1 14.39 13.87   M7e 31 0
24 2MASS J17232128-3031358 LP* 17 23 21.2811364368 -30 31 35.947664040           ~ 5 0
25 PN K 5-8 Sy* 17 39 17.1500502264 -35 46 59.308763160           M1.5 20 0
26 IRAS 17415-3441 Sy? 17 44 53.1227902440 -34 42 39.720593376           ~ 4 0
27 EM* AS 245 Sy* 17 51 00.9152897544 -22 19 35.061285684   11 17.810   14.000 M6 48 1
28 PN H 2-34 Sy* 17 58 28.0351570704 -28 33 42.018717960     17.676 15.62 13.215 ~ 26 1
29 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
30 PN K 3-9 Sy* 18 40 24.1837249512 -08 43 46.321900536         12.47 M3 39 1
31 V* RR Tel Sy* 20 04 18.5404499712 -55 43 33.153979080 9.93 11.33 10.81 11.689   M5e 550 0
32 V* ZZ Psc WD* 23 28 47.6365087803 +05 14 54.235051503   13.217   13.106   DA4.1 536 0

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