238:(GRBs) and other bright gamma-ray transients with energies ranging from 50 keV to 2 MeV. GTM is made up of two identical modules on opposite sides of the FS-8B. Each module has four sensor units facing different directions, covering half of the sky. The two modules will then cover the entire sky, including the direction obscured by the Earth. The sensor units consist of a
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make it possible to use these correlations to constrain cosmological parameters. As a result, more GRB monitors, such as GTM, can provide greater sky coverage and location capability, allowing for the discovery of more GRB afterglows, host galaxies, and redshifts, all of which are highly desirable.
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GRBs are the universe's most energetic explosions. However, there is significant overlap in the duration comparison of SGRBs and LGRBs, complicating a clear distinction between the two types of GRBs. Actually, many other classification methods, such as hardness ratio, time and lag, encounter
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Chang, Hsiang-Kuang; Lin, Chi-Hsun; Tsao, Che-Chih; Chu, Che-Yen; Yang, Shun-Chia; Huang, Chien-You; Wang, Chao-Hsi; Su, Tze-Hsiang; Chung, Yun-Hsin; Chang, Yung-Wei; Gong, Zi-Jun; Hsiang, Jr-Yue; Lai, Keng-Li; Lin, Tsu-Hsuan; Lu, Chia-Yu (2022-01-15).
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overlapping issues. To advance our understanding of GRB classification based on their true progenitor mechanisms, more GRB monitors, such as GTM, can increase the number of GRB databases, which is very useful.
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with 16 pixel channels. GTM is expected to detect approximately 50 GRBs per year. It is expected to launch in 2026.
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The repository that stores the code for
Science Data Center (SDC) of Gamma-ray Transients Monitor is on GitHub.
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354:"The Gamma-ray Transients Monitor (GTM) on board Formosat-8B and its GRB detection efficiency"
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Using the above relationships, GRBs can be viewed as a type of
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array (50 mm x 50 mm x 8 mm) that is readout by
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The first astronomical CubeSat funded by Taiwan Space Agency
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GTM master and slave modules after assembly process.
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219:of Taiwan. It is a secondary payload on board
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393:Huang, Chien-You Jason (2023-10-18),
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240:Gadolinium Aluminum Gallium Garnet
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63:https://crab0.astr.nthu.edu.tw/#
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459:Space telescopes orbiting Earth
314:"Gamma-ray Transients Monitor"
257:It is a collaboration between
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288:for measuring distances that
259:National Tsing Hua University
234:The goal of GTM is to track
217:space astronomical telescope
209:Gamma-ray Transients Monitor
163:Gamma-ray Transients Monitor
22:Gamma-ray Transients Monitor
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438:: CS1 maint: url-status (
358:Advances in Space Research
336:: CS1 maint: url-status (
416:"Gamma-Ray Bursts (GRBs)"
371:10.1016/j.asr.2021.10.044
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292:cannot probe. The large
225:remote-sensing satellite
223:-8B (FS-8B), which is a
290:supernovae of type Ia
77:Spacecraft properties
474:Satellites of Taiwan
464:Gamma-ray telescopes
46:Gamma-ray astronomy
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171:GAGG Semiconductor
124:Orbital parameters
396:PbU-Jason/GTM_SDC
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364:(2): 1249–1255.
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423:. Retrieved
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321:. Retrieved
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248:scintillator
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100:Payload mass
92:Manufacturer
43:Mission type
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420:GTM Science
184:Wavelengths
138:Inclination
87:Formosat-8B
453:Categories
425:2024-07-23
402:2024-07-27
323:2024-07-23
301:References
242:(GAGG) (a
380:0273-1177
294:redshifts
202:GTM logo
469:CubeSats
434:cite web
332:cite web
221:Formosat
129:Altitude
51:Operator
276:Science
179:all-sky
142:97 deg.
111:2 Watts
59:Website
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132:561 km
103:1.9 kg
108:Power
440:link
376:ISSN
338:link
267:TASA
265:and
252:SiPM
229:TASA
168:Type
160:Name
155:Main
95:TASA
54:TASA
366:doi
318:GTM
213:GTM
83:Bus
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
