Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Hakim L Malasan"'
Autor:
Hakim L. Malasan, Rosa M. Ros, Chatief Kunjaya, Endang Soegiartini, null Aprilia, Riska W. Romadhonia
Publikováno v:
Proceedings of the International Astronomical Union. 15:30-33
Youths and kids in Indonesia since almost two decades ago have been showing significant increase of interest in space sciences, especially astronomy. One of the main factors is due to the annual event of National Science Olympiad which includes Astro
Autor:
A. T. P. Jatmiko, Mochamad Irfan, Dhimaz Gilang Ramadhan, Geavani Eva Ramadhania, Hakim L. Malasan, E. I. Akbar, Aprilia Aprilia, Ade Nur Istiqomah
Publikováno v:
Journal of Mathematical and Fundamental Sciences, Vol 51, Iss 3, Pp 243-251 (2019)
Hα line variations of 8 B-emission (Be) stars are presented. Stars that are listed in the Bright Star Catalogue were observed in 2009 at the Bosscha Observatory, Lembang, Indonesia. It was found that 4 stars showed phase changing from Be double-peak
Publikováno v:
Journal of Physics: Conference Series. 2214:012004
Vision is a continuous two-dimensional (2-D) image that can be perceived by human visual system. Mathematically, image is a 2-D function that expresses the intensity of light. This research introduces the fundamental ideas of computer vision. We used
Autor:
Boonrucksar Soonthornthum, Hakim L. Malasan, Chan Oeurn Chey, Hasan Abu Kassim, Khin Swe Myint, Cynthia Celebre, Pham Ngoc Diep, Abel Yang
Publikováno v:
EPJ Web of Conferences, Vol 240, p 00001 (2020)
Autor:
T Yamamuro, Hideyo Kawakita, Akira Arai, Evaria Puspitaningrum, Irham T Andika, Robiatul Muztaba, Imanul Jihad, Hakim L Malasan
Publikováno v:
Indonesian Journal of Physics. 27:1-8
In 2015, the Institute Teknologi Bandung (ITB) signed a Memorandum of Understanding with Sangyou Kyoto University (KSU). One realization of collaboration between ITB and KSU is observational program of Novae using a compact spectrograph NEO-R1000 (No
Publikováno v:
IOP Conference Series: Earth and Environmental Science. 537:012008
Spectroscopic observations of standard stars (spectrophotometric) have been carried out at Bosscha Observatory ITB (latitude= 6°49′28″ S, longitude= 107°36′56″ E, altitude=1310 m) using the Celestron C-11 reflector (D=11 inches, F/10.0), eq
Publikováno v:
Journal of Physics: Conference Series. 1523:012001
Wolf-Rayet (WR) stars exhibit broad emission lines in their spectra. Based on the featured lines, they are classified into three types: nitrogen-rich WN, carbon-rich WC, and oxygen-rich WO. Broad emission lines indicate high expansion velocity and al
Autor:
Azlizan Adhyaqsa, Hakim L. Malasan, Dimas A. Prabowo, Aprilia, L. Puspitarini, M. Rafif Rabbani
Publikováno v:
Journal of Physics: Conference Series. 1523:012018
We report an optical spectroscopic observational program of emission-line objects at Bosscha Observatory. The observations were conducted on 18 nights between May to July 2019. We employ the spectrograph NEO-R1000 (R∼1000) equipped with SBIG ST-8 X
Publikováno v:
Publications of The Korean Astronomical Society. 30:251-254
Low resolution spectra of Nova Delphini 2013 (V339 Del) in the optical range have been obtained at Bosscha Observatory, Indonesia during its maximum light (V = 4.3). Spectra were observed from August 16 to 27, 2013. The GAO-ITB RTS 20.3 cm telescope,
Autor:
A. Yamani, Hakim L. Malasan
Publikováno v:
Publications of The Korean Astronomical Society. 30:715-718
Astronomy is a popular topic for the public in term of astronomical phenomenon such as occultations, solar and lunar eclipses or meteor showers. In term of education, astronomy also is popular as one of the world Science Olympiads. Social media, as t