Submission declined on 13 May 2024 by
Cambalachero (
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Submission declined on 26 January 2024 by
Ldm1954 (
talk). This draft's references do not show that the subject
qualifies for a Wikipedia article. In summary, the draft needs to Declined by
Ldm1954 5 months ago.
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Hsiang-Kuang Chang (born 1964) is a Taiwanese high energy astrophysicist. [1] [2] [3]. He is currently a senior professor at the Institute of Astronomy, National Tsing Hua University [4]. He is the principal investigator of GTM project. It is the first astronomical telescope of Taiwan [5] [6].
Prof. Hsiang-Kuang Chang | |
---|---|
張祥光 | |
![]() | |
Born | 1964 Taipei, Taiwan |
Other names | Prof. HK |
Education | National Tsing Hua University, BS
National Taipei University, MS Bonn University, DNS |
Years active | 1997-present |
Known for | GTM, the first space astronomical telescope of Taiwan [7] |
Website | http://www.phys.nthu.edu.tw/~hkchang/ |
Hsiang-Kuang Chang was born in Taipei, Taiwan in 1964. He holds a Bachelor of Science in Physics from the Department of Physics, National Tsing Hua University (NTHU), Hsinchu which he completed in 1987. After that, he completed a Master of Science in Physics, Institute of Physics, National Taiwan University (NTU), Taipei, in 1991. He then moved to Bonn University in Germany to do his PhD under Wolfgang Kundt, which he completed in 1994 [8]. He worked as a Postdoctoral Research Associate at Los Alamos National Lab, USA between 1994 and 1996 after which he moved back to National Tsing Hua University [1].
Hsiang-Kuang Chang became an assistant professor in NTHU in 1997 [9]. He held the chairing position in Department of Physics, National Tsing Hua University between 2008 and 2011. He was also the president of the National Committee of Republic of China (ROC) for Committee on Space Research (COSPAR), 2022-2023 [10]. He is currently the Vice President for General Affairs at NTHU, a position which he had held before in 2014 - 2015 academic year [1] [11]. One of his most notable work include the Nature paper titled "Ambient acoustic imaging in helioseismology" [12] [13].
He has also studied trans-neptunian objects, by seeing the occultation of X-rays from Scorpius X-1 by them [14]. He was also the Taiwan lead of The Nuclear Compton Telescope (NCT) project [15] [16], which a balloon-borne telescope designed to study astrophysical sources of gamma-ray emission with high spectral resolution, moderate angular resolution, and novel sensitivity to gamma-ray polarization [17] [18]. It was a collaborative effort between UC Berkley, NTHU and NCT among many others [19] [20]. Later, NASA took up the mission as a SMEX mission. Renamed as The Compton Spectrometer and Imager (COSI) [21] [22] [23], it is a 0.2–5 MeV Compton telescope capable of imaging, spectroscopy, and polarimetry of astrophysical sources [24]. He was also a part of UltraFast [25] project [1]. It was a multi-fiber fast photometer planned to mount on UT2 ( Kueyen) of ESO's Very Large Telescope (VLT) at Cerro Paranal, Chile.
He has various academic interests ranging from Pulsars (PSR), Anomalous X-ray Pulsars (AXP) and Soft Gamma Repeaters (SGR) - magnetar, X-ray binaries (XRB), Gamma Ray Bursts (GRB), Supernova Remnants (SNR) and Cosmic Rays (CR), Galactic 511 keV emission, Active Galactic Nuclei (AGN), Search for white dwarf p-mode oscillation, Trans-Neptunian Objects (TNO), etc [1] [26] [27] [28].
Hsiang-Kuang Chang is the PI of the Gamma-ray Transients Monitor (GTM). It is a secondary payload on board board Formosat-8B [29] [30]. It is the first space astronomical telescope of Taiwan [5] [31]. 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 [29]. It will be launched by TASA in 2027.
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cite web}}
: CS1 maint: numeric names: authors list (
link)
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Submission declined on 13 May 2024 by
Cambalachero (
talk). This draft's references do not show that the subject
qualifies for a Wikipedia article. In summary, the draft needs to
Where to get help
How to improve a draft
You can also browse Wikipedia:Featured articles and Wikipedia:Good articles to find examples of Wikipedia's best writing on topics similar to your proposed article. Improving your odds of a speedy review To improve your odds of a faster review, tag your draft with relevant WikiProject tags using the button below. This will let reviewers know a new draft has been submitted in their area of interest. For instance, if you wrote about a female astronomer, you would want to add the Biography, Astronomy, and Women scientists tags. Editor resources
| ![]() |
Submission declined on 26 January 2024 by
Ldm1954 (
talk). This draft's references do not show that the subject
qualifies for a Wikipedia article. In summary, the draft needs to Declined by
Ldm1954 5 months ago.
| ![]() |
Hsiang-Kuang Chang (born 1964) is a Taiwanese high energy astrophysicist. [1] [2] [3]. He is currently a senior professor at the Institute of Astronomy, National Tsing Hua University [4]. He is the principal investigator of GTM project. It is the first astronomical telescope of Taiwan [5] [6].
Prof. Hsiang-Kuang Chang | |
---|---|
張祥光 | |
![]() | |
Born | 1964 Taipei, Taiwan |
Other names | Prof. HK |
Education | National Tsing Hua University, BS
National Taipei University, MS Bonn University, DNS |
Years active | 1997-present |
Known for | GTM, the first space astronomical telescope of Taiwan [7] |
Website | http://www.phys.nthu.edu.tw/~hkchang/ |
Hsiang-Kuang Chang was born in Taipei, Taiwan in 1964. He holds a Bachelor of Science in Physics from the Department of Physics, National Tsing Hua University (NTHU), Hsinchu which he completed in 1987. After that, he completed a Master of Science in Physics, Institute of Physics, National Taiwan University (NTU), Taipei, in 1991. He then moved to Bonn University in Germany to do his PhD under Wolfgang Kundt, which he completed in 1994 [8]. He worked as a Postdoctoral Research Associate at Los Alamos National Lab, USA between 1994 and 1996 after which he moved back to National Tsing Hua University [1].
Hsiang-Kuang Chang became an assistant professor in NTHU in 1997 [9]. He held the chairing position in Department of Physics, National Tsing Hua University between 2008 and 2011. He was also the president of the National Committee of Republic of China (ROC) for Committee on Space Research (COSPAR), 2022-2023 [10]. He is currently the Vice President for General Affairs at NTHU, a position which he had held before in 2014 - 2015 academic year [1] [11]. One of his most notable work include the Nature paper titled "Ambient acoustic imaging in helioseismology" [12] [13].
He has also studied trans-neptunian objects, by seeing the occultation of X-rays from Scorpius X-1 by them [14]. He was also the Taiwan lead of The Nuclear Compton Telescope (NCT) project [15] [16], which a balloon-borne telescope designed to study astrophysical sources of gamma-ray emission with high spectral resolution, moderate angular resolution, and novel sensitivity to gamma-ray polarization [17] [18]. It was a collaborative effort between UC Berkley, NTHU and NCT among many others [19] [20]. Later, NASA took up the mission as a SMEX mission. Renamed as The Compton Spectrometer and Imager (COSI) [21] [22] [23], it is a 0.2–5 MeV Compton telescope capable of imaging, spectroscopy, and polarimetry of astrophysical sources [24]. He was also a part of UltraFast [25] project [1]. It was a multi-fiber fast photometer planned to mount on UT2 ( Kueyen) of ESO's Very Large Telescope (VLT) at Cerro Paranal, Chile.
He has various academic interests ranging from Pulsars (PSR), Anomalous X-ray Pulsars (AXP) and Soft Gamma Repeaters (SGR) - magnetar, X-ray binaries (XRB), Gamma Ray Bursts (GRB), Supernova Remnants (SNR) and Cosmic Rays (CR), Galactic 511 keV emission, Active Galactic Nuclei (AGN), Search for white dwarf p-mode oscillation, Trans-Neptunian Objects (TNO), etc [1] [26] [27] [28].
Hsiang-Kuang Chang is the PI of the Gamma-ray Transients Monitor (GTM). It is a secondary payload on board board Formosat-8B [29] [30]. It is the first space astronomical telescope of Taiwan [5] [31]. 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 [29]. It will be launched by TASA in 2027.
{{
cite web}}
: CS1 maint: numeric names: authors list (
link)
{{
cite web}}
: |last=
has generic name (
help); External link in |last=
(
help)
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