GRBNanoSats - User contributions [en]

Monitoring HE sky with small satellites - Presentations

2022-09-10T16:28:26Z

HKChang: /* Presentations from Brno 2022 Workshop */

== Presentations from Brno 2022 Workshop ==

Table under construction

{| class="wikitable sortable"
|-
! Title !! Author || Time
|-
| [[Media:BISSALDI_Brno_GRBs_220906.pdf|Gamma Ray Burst Science]] || Elisabetta Bissaldi || Sep 6 09:00
|-
| Magnetars and Terrestrial Gamma-ray Flashes || Oli Roberts || Sep 6 09:30
|-
| Distributed architectures in high-energy astrophysics || Michele Lavagna || Sep 6 10:00
|-
| HERMES || Fabrizio Fiore || Sep 6 11:00
|-
| BurstCube || Jeremy Perkins || Sep 6 11:15
|-
| [[:Media:GRID_Current_Status_and_Scientific_Results.pdf|GRID]] || Xutao Zheng || Sep 6 11:30
|-
| [[:Media:Ripa_GRBAlpha_and_VZLUSAT-2.pdf|GRBAlpha and VZLUSAT-2]] || Jakub Ripa || Sep 6 11:45
|-
| GALI || Roi Rahin || Sep 6 12:00
|-
| [[:Media:RDunwoody_EIRSAT1_GRBNanoSats_Sept2022.pdf|EIRSAT-1]] || Rachel Dunwoody || Sep 6 12:15
|-
| [https://nasa-gcn.github.io/gcn-presentation/ New GCN] || Leo Singer || Sep 6 13:50
|-
| [[:Media:EBurns_v2_Joint_Localization_between_gamma-rays_and_New_IPN.pdf|Joint Localization between gamma-rays & GW, new IPN]] || Eric Burns || Sep 6 14:10
|-
| [[:Media:BCTools-GRBSmallSatsBrno-Israel.pdf|Pipelines and response functions]] || Israel Martinez || Sep 6 14:30
|-
| GBM data analysis tools || Adam Goldstein || Sep 6 14:50
|-
| [[:Media:Tohuvavohu_How_to_Find_Them.pdf|Follow-up coordination]] || Aaron Tohuvavohu || Sep 6 15:10
|-
| GRB followup with robotic telescopes || Martin Jelinek || Sep 6 15:30
|-
| Satellite formations for astronomical observations || Klaus Schilling || Sep 6 16:10
|-
| Overview of inter-satellite communication (challenges and opportunities) || Robert Mearns || Sep 6 16:30
|-
| The SatNOGS network || András Pál || Sep 6 16:50
|-
| A new equatorial ground station for HERMES and small HEA missions || Fabrizio Fiore || Sep 6 17:10
|-
| GlowBug || Matthew Kerr || Sep 7 09:00
|-
| MoonBeam || Michelle Hui || Sep 7 09:15
|-
| [[:Media:GTM-20220907Brno.pdf|GTM]] || Hsiang-Kuang Chang || Sep 7 09:30
|-
| Starburst || Dan Kocevski || Sep 7 09:45
|-
| BlackCAT || Abe Falcone || Sep 7 10:00
|-
| QUVIK || Norbert Werner || Sep 7 10:15
|-
| [[:Media:Grb_cubesat_Takahashi.pdf|In-orbit degradation of the Hamamatsu MPPCs]] || Hiromitsu Takahashi || Sep 7 11:00
|-
| Low-Earth background and SiPM detectors || Lee Mitchell || Sep 7 11:20
|-
| Authorisations and other paper-work challenges || David Murphy || Sep 7 11:40
|-
| [[:Media:20220907_Educational_experience_with_the_GRID_mission_Monitoring_the_high-energy_sky_with_small_satellites.pdf|Educational experience with the GRID mission]] || Ming Zeng || Sep 7 12:00
|-
| Educational experience with the EIRSAT-1 mission || Lorraine Hanlon || Sep 7 12:20
|-
| LUVS || Aaron Tohuvavohu || Sep 7 14:00
|-
| [[:Media:GECAM_Shaolin.pdf|GECAM]] || Shaolin Xiong || Sep 7 14:15
|-
| [[:Media:Merlin_Kole_Polar.pdf|Polar-2]] || Merlin Reynaard Kole || Sep 7 14:30
|-
| Light-1 || Lolowa Alkindi || Sep 7 14:45
|-
| CAMELOT prototype design || Laszlo Meszaros || Sep 7 15:00
|-
| [[:Media:Lucchetta_MeVCube_Brno22.pdf|MeVCube]] || Giulio Lucchetta || Sep 7 15:15
|-
| Fermi GBM GRB localization algorithm || Michael Briggs || Sep 7 15:45
|-
| [[:Media:Nazgul_2022_Burges.pdf|A statistical approach to GRB triangulation]] || Michael Burges || Sep 7 16:00
|-
| Sky localization of long gamma ray bursts from an orbiting satellite || Sharon Mitrani || Sep 7 16:15
|-
| SpIRIT/SkyHopper || Robert Mearns || Sep 8 09:00
|-
| ALBATROS || Luciano Burdieri || Sep 8 09:15
|-
| [[:Media:3UTransat_GODET_v3.pdf|3UTransat]] || Olivier Godet || Sep 8 09:30
|-
| [[:Media:PETREL_GRB_SmallSat_YYatsu.pdf|PETREL (Wide field UV Transient survey)]] || Yoichi Yatsu || Sep 8 09:45
|-
| [[:Media:Brno_gifts.pdf|GIFTS]] || Sheila McBreen || Sep 8 10:00
|-
| [[:Media:Bhalerao_Daksha.pdf|Daksha]] || Varun Bhalerao || Sep 8 10:15
|-
| [[:Media:Svom_Brno_Schanne-presented.pdf|SVOM]] || Stéphane Schanne || Sep 8 11:00
|-
| [[:Media:Solar_flare_smallsats_inglis.pdf|Solar flare science with smallsats: possibilities and challenges]] || Andrew Inglis || Sep 8 11:15
|-
| Introducing CATCH: the Chasing All Transients Constellation Hunters || Lian Tao || Sep 8 11:30
|-
| The GALI-ISS Mission || Julia Salh || Sep 8 11:45
|-
| [[:Media:Presentation_COMPOL_Laurent.pdf|COMPOL: a gamma-ray polarimeter in a 3U nanosat]] || Philippe Laurent || Sep 8 12:00
|-
| [[:Media:Uliyanov_Brno_comcube.pdf|The COMCUBE project for GRB polarimetry]] || Alexey Uliyanov || Sep 8 12:15
|}

File:GTM-20220907Brno.pdf

2022-09-10T16:10:49Z

HKChang:

GTM slides in Brno2022

File:GTM10grbnano.pdf

2022-04-08T02:30:33Z

HKChang:

GTM presentation on Feb 3, 2022

GTM

2022-01-17T23:55:25Z

HKChang: /* Gamma-ray Transients Monitor */

The Gamma-ray Transients Monitor (GTM) is a secondary payload on board Formosat-8B (FS-8B), a Taiwanese remote-sensing satellite scheduled to launch in 2025. The goal of GTM is to monitor Gamma Ray Bursts (GRBs) and other bright gamma-ray transients in the energy range from 50 keV to 2 MeV. GTM consists of two identical modules located on two opposite sides of FS-8B. Each module has four sensor units facing different directions to cover half of the sky. The two modules will then cover the whole sky, including the direction occulted by the Earth. Each sensor unit is composed of a GAGG scintillator array (50 mm x 50 mm x 8 mm) to be readout by SiPM with 16 pixel-channels. GTM is expected to detect about 40 GRBs per year.

Gamma-ray Transients Monitor (GTM)

2022-01-17T13:08:40Z

HKChang:

Gamma-ray Transients Monitor (GTM)

2022-01-17T13:07:35Z

HKChang: Created page with "The Gamma-ray Transients Monitor (GTM) is a secondary payload on board Formosat-8B (FS-8B), a Taiwanese remote-sensing satellite scheduled to launch in 2025. The goal of GTM i..."

The Gamma-ray Transients Monitor (GTM) is a secondary payload on board Formosat-8B (FS-8B), a Taiwanese remote-sensing satellite scheduled to launch in 2025. The goal of GTM is to monitor Gamma Ray Bursts (GRBs) and other bright gamma-ray transients in the energy range from 50 keV to 2 MeV. GTM consists of two identical modules located on two opposite sides of FS-8B. Each module has four sensor units facing different directions to cover half of the sky. The two modules will then cover the whole sky, including the direction occulted by the Earth. Each sensor unit is composed of a GAGG scintillator array (50 mm �x 50 mm �x 8 mm) to be readout by SiPM with 16 pixel-channels. GTM is expected to detect about 40 GRBs per year.