Tae-Geun Ji
YOU?
Author Swipe
View article: Telescope control software and proto-model siderostat for the SDSS-V Local Volume Mapper
Telescope control software and proto-model siderostat for the SDSS-V Local Volume Mapper Open
The fifth Sloan Digital Sky Survey (SDSS-V) Local Volume Mapper (LVM) is a wide-field integral field unit (IFU) survey that uses an array of four 160 mm fixed telescopes with siderostats to minimize the number of moving parts. Individual t…
View article: Maunakea Spectroscopic Explorer exposure time calculator for end-to-end simulator: to optimizing spectrograph design and observing simulation
Maunakea Spectroscopic Explorer exposure time calculator for end-to-end simulator: to optimizing spectrograph design and observing simulation Open
The Maunakea Spectroscopic Explorer (MSE) project will provide multi-object\nspectroscopy in the optical and near-infrared bands using an 11.25-m aperture\ntelescope, repurposing the original Canada-France-Hawaii Telescope (CFHT) site.\nMS…
View article: Intensive Monitoring Survey of Nearby Galaxies (IMSNG)
Intensive Monitoring Survey of Nearby Galaxies (IMSNG) Open
Intensive Monitoring Survey of Nearby Galaxies (IMSNG) is a high cadence observation program monitoring nearby galaxies with high probabilities of hosting supernovae (SNe). IMSNG aims to constrain the SN explosion mechanism by inferring si…
View article: Intensive Monitoring Survey of Nearby Galaxies (IMSNG)
Intensive Monitoring Survey of Nearby Galaxies (IMSNG) Open
Intensive Monitoring Survey of Nearby Galaxies (IMSNG) is a high cadence observation program monitoring nearby galaxies with high probabilities of hosting supernovae (SNe). IMSNG aims to constrain the SN explosion mechanism by inferring si…
View article: The Infrared Medium-deep Survey. VI. Discovery of Faint Quasars at z ∼ 5 with a Medium-band-based Approach
The Infrared Medium-deep Survey. VI. Discovery of Faint Quasars at z ∼ 5 with a Medium-band-based Approach Open
The faint quasars with M 1450 > −24 mag are known to hold the key to the determination of the ultraviolet emissivity for the cosmic reionization. But only a few have been identified so far because of the limitations on the survey data. Her…
View article: The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17
The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17 Open
The low dust temperatures (<14 K) of Planck Galactic cold clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. “TOP-SCOPE” is a joint survey program targeting ∼2000 PGCCs in J = 1–0…