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中央研究院天文及天文物理研究所
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Extragalactic Astronomy

Thumbnails showing the Chandra X-ray brightness distribution in the 0.5 - 7.0 keV band for 28 systems selected from the HIFLUGS sample. The color bar indicates the X-ray surface brightness in units of photon counts s^-1 arcsec^-2 cm^-2. The black and cyan crosses in each panel show the positions of the X-ray brightness peak and the BCG, respectively. The white horizontal bar in each panel corresponds to a spatial scale of 60''.
Systematic Perturbations of the Thermodynamic Properties in Cool Cores of HIFLUGCS Galaxy Clusters
A dusty star-forming galaxy (DSFG) was discovered in the halo of a quasar pair system UM287, which also hosts an enormous Lyman-alpha nebula (ELAN). With observational evidence here is a proposed scenario of this system where over the past ∼100 Myr the DSFG has moved from south to north by ∼100 kpc in projected distance with a projected velocity of ∼1000 km/s; in the meantime, the DSFG experiences ram-pressure stripping and the stripped gas has been slowly entrained via shocks and gas mixing by the massive (∼10^12–10^13 Msun) hot halo of UM 287 with a virial radius of ∼150 kpc. The Slug-DSFG has also been experiencing strangulation, where the hot halo stops further accretion of cold gas so the gas reservoir has slowly drained out, therefore decreasing both the gas fraction and gas-to-dust ratios.
A dusty star-forming galaxy experiencing ram-pressure stripping in one of the most massive galaxy systems at cosmic noon
Overview of the ALMA spectra plotted in their rest-frame frequencies from a complete sample of bright dusty star-forming galaxies, or the submillimeter galaxies (SMGs), that were undergoing very active phases of star formation. The locations of strong molecular and atomic lines are marked. Redshift distribution of this bright SMG sample is determined robustly via these line detection, and it is found that brighter SMGs are located at higher redshifts, suggesting that the most active phases of stellar mass buildup across the cosmic time occurred earlier than what has been predicted by theoretical models.
The distance distributions of bright dusty star-forming galaxies
Top: X-ray surface brightness of the galaxy cluster MACS J1311.0-0310 taken by the Chandra X-ray Observatory (left) and its X-ray residual image after removing the mean profile (right). Bottom: X-ray surface brightness of a simulated galaxy cluster produced by our hydrodynamic simulation (left) and its X-ray residual image (right).
Gas Density Perturbations in the Cool Cores of CLASH Galaxy Clusters
Left: X-ray surface brightness of the galaxy cluster Abell 907 taken by the Chandra X-ray Observatory. Right: Residual image of X-ray surface brightness after subtracting its global profile from the original image.
Line-of-Sight Gas Sloshing in the Cool Core of Abell 907
Top Left: X-ray surface brightness of the galaxy cluster RX J1347.5-1145 taken by the Chandra X-ray Observatory. The white contours show the surface mass density map of this galaxy cluster measured by the strong-lensing analysis using Hubble Space Telescope (HST). Top Right: Same as top left but for the image of the Sunyaev-Zel'dovich effect observed by ALMA. Bottom Left: Same as top left but for the X-ray residual image after removing the global profile of this galaxy cluster from top left. Bottom Right: Same as top right, but for the residual image of the Sunyaev-Zel'dovich effect.
A Cool Core Disturbed: Observational Evidence for the Coexistence of Subsonic Sloshing Gas and Stripped Shock-heated Gas around the Core of RX J1347.5-1145
STUDIES is a multi-year JCMT Large Program, to obtain extremely deep submillimeter images of the distant universe. The goal is to understand the origin of the far-infrared cosmic background radiation and the history of the cosmic star formation. Buy detecting a large sample of faint distant dusty galaxies that give rise to the far-infrared background, we can study when and where most of the stars in the universe form, and how these affect the evolution of galaxies. The figure shows the STUDIES 450 micron image of the center of the COSMOS survey field, using the data collected during the first year of STUDIES observations. It detects nearly 100 faint galaxies (small circles) at high significance levels, and is the deepest 450 micron image by far.
STUDIES (SCUBA-2 Ultra Deep Imaging EAO Survey)
Left: Bulk velocity (v_bulk) map of the intracluster medium in the core of the X-ray brightest galaxy cluster, the Perseus cluster, with respect to the redshift z = 0.017284 (heliocentric correction applied) in units of km/s. Right: Line-of-sight velocity dispersion (σ_v) of the intracluster medium in units of km/s. The Chandra X-ray contours are overlaid.
Atmospheric gas dynamics in the Perseus cluster observed with Hitomi
Top: Median sSFR of SF galaxies as a function of redshift in the field (dotted), groups (dashed), and clusters (solid). Bottom: The logarithmic ratio of sSFR for group to field galaxies (dashed), and for cluster to field galaxies (solid). At fixed masses, the decrease level is very similar for cluster galaxies or group galaxies in different redshift ranges, and the reduction offset is seen <0.4 dex for clusters and <0.2 dex for groups. That is, the decrease of sSFRs for the group to field galaxies and for the cluster to field ones is independent of redshift, implying an universal slow quenching mechanism acting in the dense environments since z ~ 1.1.
First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. I. The role of group or cluster environment in star formation quenching from z = 0.2 to 1.1
Top: Median sSFR of SF galaxies as a function of redshift in the field (dotted), groups (dashed), and clusters (solid). Bottom: The logarithmic ratio of sSFR for group to field galaxies (dashed), and for cluster to field galaxies (solid). At fixed masses, the decrease level is very similar for cluster galaxies or group galaxies in different redshift ranges, and the reduction offset is seen <0.4 dex for clusters and <0.2 dex for groups. That is, the decrease of sSFRs for the group to field galaxies and for the cluster to field ones is independent of redshift, implying an universal slow quenching mechanism acting in the dense environments since z ~ 1.1.
First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. I. The role of group or cluster environment in star formation quenching from z = 0.2 to 1.1
Top: The quiescent fraction from the radial (solid lines) and density (dashed lines) contribution. Three stellar mass ranges are plotted: 10.1<log10(Ms/Me)<10.5 (green), 10.5<log10(Ms/Me)<10.9 (blue), and log10(Ms/Me)>10.9 (gold). Bottom: The excess of the quiescent fraction (Δ) from the radial (solid lines) and density (dashed lines) contribution relative to the fraction from the field. For less massive galaxies, the Δ in groups or clusters has a radial gradient, implying that the location of the less massive galaxies in their parent halo has an additional effect on their star formation quenching.
The Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments
Top: The quiescent fraction from the radial (solid lines) and density (dashed lines) contribution. Three stellar mass ranges are plotted: 10.1<log10(Ms/Me)<10.5 (green), 10.5<log10(Ms/Me)<10.9 (blue), and log10(Ms/Me)>10.9 (gold). Bottom: The excess of the quiescent fraction (Δ) from the radial (solid lines) and density (dashed lines) contribution relative to the fraction from the field. For less massive galaxies, the Δ in groups or clusters has a radial gradient, implying that the location of the less massive galaxies in their parent halo has an additional effect on their star formation quenching.
The Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments
Top: The quiescent fraction from the radial (solid lines) and density (dashed lines) contribution. Three stellar mass ranges are plotted: 10.1<log10(Ms/Me)<10.5 (green), 10.5<log10(Ms/Me)<10.9 (blue), and log10(Ms/Me)>10.9 (gold). Bottom: The excess of the quiescent fraction (Δ) from the radial (solid lines) and density (dashed lines) contribution relative to the fraction from the field. For less massive galaxies, the Δ in groups or clusters has a radial gradient, implying that the location of the less massive galaxies in their parent halo has an additional effect on their star formation quenching.
The Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments
We simulated the evolution of a spiral galaxy with N-body/SPH (Aoyama, Hou, Hirashita, et al. 2017). We implemented the evolution of dust in the simulation. This figure shows the face-on view of the surface densities of small grains (left-hand column) and large grains (right-hand column) at t = 1 and 5 Gyr (top to bottom). We observe that at 1 Gyr, the stellar dust production is still important, which predicts much more large grains than small grains. At 5 Gyr, interstellar processing of dust (especially, dust disruption by shattering and dust growth by accretion) makes the enhancement of small grains. The results are consistent with the observed radial distribution of dust grains.
Dust evolution simulation in a spiral galaxy
Hubble Space Telescope image of the most distant strong lensing galaxy known at z = 1.62.
Discovery of a Strong Lens Galaxy Embedded in a Cluster at z = 1.62
The first ALMA-Taiwan result published with Cycle 0 data. Gamma-ray burst host galaxies are observed at 345 GHz with ALMA (left panels) and compared to Hubble Space Telescope images (right). In the ALMA panels, black boxes indicate the optical positions of the host galaxies. Only one host galaxies was detected (lower panel) and a strong upper limit was set to the second one, indicating that host galaxies are luminous infrared galaxies with star formation rates of a few tens of solar mass per year. (Wang et al. 2012, ApJL, 761, 32)
The first ALMA-Taiwan result published with Cycle 0 data
The green triangles represent predictions of the stellar mass growth of BCGs by a highly successful galaxy formation model (Guo et al. 2011), which are found to agree fairly well with our Spitzer and WISE infrared observations for a large sample of BCGs (blue points and the pink star), down to z~0.5 or so. Below that redshift, there is some hint of different behavior between the model and data, in the sense that the model BCGs continue to grow, while the observed ones slow down their growth considerably. (Lin et al. 2013, ApJ, 771, 61)
Predictions of the stellar mass growth of BCGs
a picture of a galaxy cluster observed by the WISE and Spitzer Space Telescopes. The bright galaxy at the center is the BCG.
BCG
NGC 4418 is nearby luminous infrared galaxy whose nucleus is deeply shrouded in dust.
Gauging the Hidden Hot Nucleus of NGC 4418 with submillimeter Interferometry
This sequence of images, taken over a 13-year span by NASA's Hubble Space Telescope, reveals changes in a black-hole-powered jet of hot gas in the giant elliptical galaxy M87. The observations show that the river of plasma, traveling at nearly the speed of light, may follow the spiral structure of the black hole's magnetic field, which astronomers think is coiled like a helix. The magnetic field is believed to arise from a spinning accretion disk of material around a black hole. Although the magnetic field cannot be seen, its presence is inferred by the confinement of the jet along a narrow cone emanating from the black hole. The visible portion of the jet extends 5,000 light-years. M87 resides at the center of the neighboring Virgo cluster of roughly 2,000 galaxies, located 50 million light-years away (Meyer et al. 2013, ApJ: http://adsabs.harvard.edu/abs/2013ApJ...774L..21M).
Hubble Takes Movies of Space Slinky in M87

Research of extragalaxy is one of the most dynamic areas of contemporary astronomy. Members of ASIAA extragalactic group have been working on all these various and wide ranging studies, from clusters of galaxies to active galactic nuclei, from nearby galaxies to high-z galaxies. Particular interests are the formation and evolution of galaxies, the interaction of galaxies, the interstellar medium in galaxies, the activities of AGNs and starbursts, and so on. The ASIAA extragalactic group studies using a combination of multi-wavelength observations (radio, IR, optical and X-ray), advanced analysis techniques, and theoretical works including magnetohydrodynamical modelling.

Research Members (28)

Wang, Wei-Hao 王為豪 cv Deputy Director; Research Fellow
Research Interest: Multiwavelength observational studies of galaxy formation and evolution at high redshift
Hirashita, Hiroyuki 平下博之 cv Research Fellow
Research Interest: Theory of galaxy evolution and metal enrichment
Koch, Patrick 高培邁 cv Research Fellow
Research Interest: Theory: CMB, SZ effect, clusters of galaxies, magnetic fields, plasma physics Observation: Radio interferometry with AMiBA and SMA.
Lin, Li-Hwai 林俐暉 cv Research Fellow
Research Interest: Galaxy Evolution; Interacting Galaxies; Galaxy Clusters; Optical/Infrared Astronomy
Lin, Yen-Ting 林彥廷 cv Research Fellow
Research Interest: galaxy formation and evolution; clusters of galaxies
Matsushita, Satoki 松下聰樹 cv Research Fellow
Research Interest: Starbursts, AGNs.
Okumura, Teppei 奧村哲平 cv Research Fellow
Research Interest: Observational cosmology, Large-scale structure of the Universe, Analysis of large data set and simulations, Galaxy redshift surveys, Gravitational lensing, Dark matter and Dark energy, Modified gravity theory
Umetsu, Keiichi 梅津敬一 cv Research Fellow
Research Interest: Observational Cosmology, Structure Formation in the Universe, Dark Matter, Clusters of Galaxies, Gravitational Lensing
Asada, Keiichi 浅田圭一 cv Associate Research Fellow (Tenured)
Research Interest: Active Galactic Nuclei;Black Hole, Jet, Accretion Flow, VLBI Polarimetry, Site testing, VLBI commissioning
Sakamoto, Kazushi 坂本和 cv Associate Research Fellow (Tenured)
Research Interest: Structure, Dynamics, and Evolution of Galaxies
Chen, Chian-Chou 陳建州 cv Assistant Research Fellow
Research Interest: Observational cosmology; Galaxy formation and evolution; Dusty galaxy; OIR/FIR/Submm astrophysics
Oyama, Yoichi 大山陽一 cv Senior Research Scientist
Research Interest: Optical/Infrared Spectroscopic Studies of Star-forming Galaxies, (U)LIRGs, and high-z AGNs (quasars)
Chou, Chueh-Yi 周瞿毅 cv Assistant Research Engineer
Research Interest: I am interested in studying space density evolution and kinematic properties of galaxy mergers from 0 < z < 1 in order to further understand the evolution trends of different types of mergers and the details of galactic color transformations. It is very interesting to study star formation histories of resolved stellar populations in nearby galaxy mergers. This is very important in knowing the mechanism of triggering star formations and constraining merging timescales.
Ho, Paul 賀曾樸 cv Corresponding Research Fellow
Research Interest: Radio Astronomy
Lim, Jeremy 林仁良 cv Adjunct Research Fellow; University of Hong Kong
Research Interest: Host Galaxies of AGNs and QSOs (Interstellar Medium), Radio Galaxies (Interstellar Medium).
Chang, Tzu-Ching 張慈錦 cv Visiting Scholar (JPL, Caltech)
Research Interest: 21-cm Cosmology; Cosmic Reionization; Gravitational Lensing; Large-scale Structure
Inoue, Makoto 井上允 cv Distinguished Visiting Scholar
Research Interest: Physics and evolution of Active Galactic Nuclei (AGN): super massive black hole (SMBH) and relativistic jet, from observational point of view. Using Very Long Baseline Interferometry (VLBI) technique, I am challenging to image the Event Horizon of SMBH.
Nakamura, Masanori 中村雅德 cv Visiting Scholar (NIT, Hachinohe College)
Research Interest: Black holes, Accretion disks, Jets
Suyu, Sherry 蘇游瑄 cv Visiting Scholar(Max Planck Institute for Astrophysics)
Research Interest: Observational cosmology, Galaxy formation and evolution, Dark matter halos of galaxies, Gravitational lensing, Bayesian data analysis methods
Yen, Chien-Chang 嚴健彰 cv Visiting Scholar (Dept. Math, FJCU)
Research Interest: Numerical Simulation
Hsieh, Bau-Ching 謝寶慶 cv SuMire Project Research Manager
Research Interest: Evolution of galaxies and clusters, interactive galaxies, extremely red objects (ERO).
Lin, Kai-Yang 林凱揚 cv Research Support Staff
Research Interest: Galaxy cluster
Huang, Chih-Wei Locutus 黃智威 cv GLT/VLBI Support Scientist
Research Interest: Cosmic Microwave Background, Galaxy Clusters, Observational Cosmology
Jian, Hung-Yu 簡鴻裕 cv Support Scientist
Research Interest: Large-Scale Structures, Galaxy evolution, Galaxy group and cluster finding
Yan, Chi-Hung 顏吉鴻 cv OIR/EPO Support Engineer
Research Interest: OIR Image Pipeline, Radio Astronomy
Chiang, I-Da 江宜達 cv Postdoc Fellow
Research Interest: Interstellar dust, molecular gas, radio data reduction, ISM in the nearby galaxies, multiwavelength observation of ISM
Romero-Canizales, Cristina 羅夢柔 cv Postdoc Fellow
Research Interest: Observations of Luminous infrared galaxies and transients (supernovae, tidal disruption events)
Bower, Geoffrey 包傑夫 cv RCUH Research Fellow / ASIAA Research Scientist
Research Interest: Transient radio sources, black holes, radio cosmology, VLBI, radio instrumentation and techniques.

Journal Papers (699)

  1. Chen K-J; Tang C-Y; Whalen DJ; Ho M-Y; Tsai S-H; Ou P-S; Ono M, "How Population III Supernovae Determined the Properties of the First Galaxies" , ApJ: 964(1), id.91 (12pp), Mar, 2024 [SCI] ( ADS | Fulltext )
  2. Hsu Q-N; Cowie LL; Chen C-C; Barger AJ, "A Full Resolution of the 450 μm Extragalactic Background Light" , ApJ: 964(2), L32 (7pp), Apr, 2024 [SCI] ( ADS | Fulltext )
  3. Tang C-Y; Chen K-J, "Clumpy Structures within the Turbulent Primordial Cloud" , MNRAS: 529(4), 4248-4261, Mar, 2024 [SCI] ( ADS | Fulltext )
  4. Chiang ID; Hirashita H; Chastenet J; Koch EW; Leroy AK; Rosolowsky E; Sandstrom KM; Sardone A; Sun J; Williams TG, "Kpc-scale properties of dust temperature in terms of dust mass and star formation activity" , MNRAS: 520, 5506-5520, April, 2023 [SCI] ( ADS | Fulltext )
  5. Lin C-H; Chen K-J; Hwang C-Y, "Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies" , ApJ: 952(2), id.121 (13 pp), Aug, 2023 [SCI] ( ADS | Fulltext )
  6. Chuang Y-T; Okumura T; Shirasaki M, "Distinguishing between ΛCDM and f(R) gravity models using halo ellipticity correlations in simulations" , MNRAS: 515(3), 4464-4470, Sep, 2022 [SCI] ( ADS | Fulltext )
  7. Hirashita H; Chiang ID, "Analytic models of dust temperature in high-redshift galaxies" , MNRAS: 516(2), 1612-1623, Oct, 2022 [SCI] ( ADS | Fulltext )
  8. Hirashita H; Lan T-W, "Shattering as a source of small grains in the circum-galactic medium" , MNRAS: 505(2), 1794–1805, Aug, 2021 [SCI] ( ADS | Fulltext )
  9. Huang Y-H; Hirashita H; Hsu Y-H; Lin Y-T; Nelson D; Cooper AP, "Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations" , MNRAS: 501(1), 1336-1351, Feb, 2021 [SCI] ( ADS | Fulltext )
  10. Lin Y-H; Hirashita H; Camps P; Baes M, "Geometry effects on dust attenuation curves with different grain sources at high redshift" , MNRAS: 507(2), 2755-2765, Oct, 2021 [SCI] ( ADS | Fulltext )
  11. Lo W-P; Asada K; Matsushita S; Nakamura M; Pu H-Y; Tseng C; Akiyama K; Algaba JC; Bower GC; Rao R; Koay JY; Koch PM; Koyama S; Ho PTP; Inoue M, "Constraints on the Mass Accretion Rate onto the Supermassive Black Hole of Cygnus A Using the Submillimeter Array" , ApJ: 911(1), id.35 (11pp), Apr, 2021 [SCI] ( ADS | Fulltext )
  12. Okumura T; Hayashi M; Chiu I-N; Lin Y-T; Osato K; Hsieh B-C; Lin S-C, "Angular clustering and host halo properties of [OII] emitters at z>1 in the Subaru HSC survey" , PASJ: 73(4), 1186-1207, Aug, 2021 [SCI] ( ADS | Fulltext )
  13. Ueda S; Umetsu K; Ng F; Ichinohe Y; Kitayama T; Molnar SM, "Systematic Perturbations of the Thermodynamic Properties in Cool Cores of HIFLUGCS Galaxy Clusters" , ApJ: 922(1), id.81 (17pp), Nov, 2021 [SCI] ( ADS | Fulltext )
  14. Agrawal A; Okumura T; Futamase T, "Standard candles and sirens rescue H0" , ApJ: 904(2), id.169 (6pp), Dec, 2020 [SCI] ( ADS | Fulltext )
  15. Aoyama S; Hirashita H; Nagamine K, "Galaxy simulation with the evolution of grain size distribution" , MNRAS: 491(3), 3844-3859, Jan, 2020 [SCI] ( ADS | Fulltext )
  16. Hirashita H; Deng W; Murga MS, "Spectral energy distributions of dust and PAHs based on the evolution of grain size distribution in galaxies" , MNRAS: 499(2), 3046-3060, Oct, 2020 [SCI] ( ADS | Fulltext )
  17. Hirashita H; Hoang T, "Effects of rotational disruption on the evolution of grain size distribution in galaxies" , MNRAS: 494(1), 1058-1070, Apr, 2020 [SCI] ( ADS | Fulltext )
  18. Hirashita H; Lin C-Y, "Dust abundance and grain size in galaxy halos" , Planet Space Sci: 183, id.104504 (11pp.), Apr, 2020 [SCI] ( ADS | Fulltext )
  19. Hirashita H; Murga MS, "Self-consistent modelling of aromatic dust species and extinction curves in galaxy evolution" , MNRAS: 492(3), 3779-3793, Mar, 2020 [SCI] ( ADS | Fulltext )
  20. Jian H-Y; Lin L; Koyama Y; ...Umetsu K; Hsieh B-C; Higuchi Y; ...; Chang YY, "Redshift Evolution of Green Valley Galaxies in Different Environments from the Hyper Suprime-Cam Survey" , ApJ: 894(2), id.125 (18pp.), May, 2020 [SCI] ( ADS | Fulltext )
  21. Kuo CY; Hsiang JY; Chung HH;...; Chang YY; ...; Matsushita S; et al., "A More Efficient Search for H2O Megamaser Galaxies: The Power of X-Ray and Mid-infrared Photometry" , ApJ: 892(1), id.18 (22 pp.), Mar, 2020 [SCI] ( ADS | Fulltext )
  22. Lim C-F; Chen C-C; Smail I; Wang W-H; Tee W-L; Lin Y-T; ...; Toba Y; Chang Y-Y; ...; Simpson JM, "SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). IV. Spatial Clustering and Halo Masses of Submillimeter Galaxies" , ApJ: 895(2), id.104 (18pp.), Jun, 2020 [SCI] ( ADS | Fulltext )
  23. Lim C-F; Wang W-H; ...; Chen C-C; Chang Y-Y; Simpson JM; Toba Y; ...; Hsu L-T; Lin M-Y; Lin W-C; et al., "SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies" , ApJ: 889(2), id.80 (33pp.), Feb, 2020 [SCI] ( ADS | Fulltext )
  24. Lin L; Ellison SL; Pan H-A; et al., "ALMaQUEST. IV. The ALMA-MaNGA QUEnching and STar Formation (ALMaQUEST) Survey" , ApJ: 903(2), id.145 (19pp.), Nov, 2020 [SCI] ( ADS | Fulltext )
  25. Okumura T; Taruya A, "Anisotropies of galaxy ellipticity correlations in real and redshift space: Angular dependence in linear tidal alignment model" , MNRAS: 493(1), L124-128 (5 pp.), Mar, 2020 [SCI] ( ADS | Fulltext )
  26. Okumura T; Taruya A; Nishimichi T, "Testing tidal alignment models for anisotropic correlations of halo ellipticities with N-body simulations" , MNRAS: 494(1), 694-702 (9pp.), May, 2020 [SCI] ( ADS | Fulltext )
  27. Pan H-A; Lin L; Hsieh B-C; et al., "SDSS-IV MaNGA: The Nature of an Off-galaxy H α Blob -- A Multi-wavelength View of Offset Cooling in a Merging Galaxy Group" , ApJ: 903(1), id.16 (17pp.), Nov, 2020 [SCI] ( ADS | Fulltext )
  28. Simpson JM; Smail I; Dudzevičiūtė U; ...; Hsieh BC; Wang WH; ...; Chen C-C; et al., "An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2-COSMOS field" , MNRAS: 495(3), 3409-3430, May, 2020 [SCI] ( ADS | Fulltext )
  29. Toba Y; Goto T; Oi N; ...; Hsieh BC; ...; Ohyama Y; et al., "Search for Optically Dark Infrared Galaxies without Counterparts of Subaru Hyper Suprime-Cam in the AKARI North Ecliptic Pole Wide Survey Field" , ApJ: 899(1), id.35 (17pp.), Aug, 2020 [SCI] ( ADS | Fulltext )
  30. Toba Y; Wang W-H; Nagao T; ...; Lim C-F; Chang Y-Y; et al., "SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy: WISE 1013+6112" , ApJ: 889(2), id.76 (9 pp.), Feb, 2020 [SCI] ( ADS | Fulltext )
  31. Toba Y; Yamada S; Ueda Y; ...; Wang W-H; et al., "NuSTAR Discovery of a Compton-thick, Dust-obscured Galaxy: WISE J0825+3002" , ApJ: 888(1), id. 8 (8 pp.), Jan, 2020 [SCI] ( ADS | Fulltext )
  32. Ueda S; Ichinohe Y; Molnar SM; Umetsu K; et al., "Gas Density Perturbations in the Cool Cores of CLASH Galaxy Clusters" , ApJ: 892(2), id.100 (20pp.), Apr, 2020 [SCI] ( ADS | Fulltext )
  33. Agrawal A; Okumura T; Futamase T, "Constraining neutrino mass and dark energy with peculiar velocities and lensing dispersions of Type Ia supernovae" , Phys Rev D: 100(6), id. 063534 (8 pp.), Sep, 2019 [SCI] ( ADS | Fulltext )
  34. Aoyama S; Hirashita H; Lim C-F; Chang YY; Wang W-H; et al., "Comparison of cosmological simulations and deep submillimetre galaxy surveys" , MNRAS: 484(2), 1852-1864, Apr, 2019 [SCI] ( ADS | Fulltext )
  35. Bower GC; Dexter J; Asada K; ..., Ho P; Inoue M; ...; Matsushita S; ...; Nakamura M; ...; Rao R; et al., "ALMA Observations of the Terahertz Spectrum of Sagittarius A*" , ApJL: 881(1), id. L2 (7 pp.), Aug, 2019 [SCI] ( ADS | Fulltext )
  36. Hirashita H; Aoyama S, "Remodelling the evolution of grain size distribution in galaxies" , MNRAS: 482(2), 2555-2572, Jan, 2019 [SCI] ( ADS | Fulltext )
  37. Hirashita H; Inoue AK, "Radiation-pressure-driven dust transport to galaxy haloes at z ∼ 10" , MNRAS: 487(1), 961-974, July, 2019 [SCI] ( ADS | Fulltext )
  38. Hou K-C; Aoyama S; Hirashita H; et al., "Dust scaling relations in a cosmological simulation" , MNRAS: 485(2), 1727-1744, May, 2019 [SCI] ( ADS | Fulltext )
  39. Hsu L-T; Lin L; Dickinson M; ...; Hsieh BC; Wang WH; ...; Yan CH; ...; Wang SY, "Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North Field" , ApJ: 871(2), 233 (14 pp.), Feb, 2019 [SCI] ( ADS | Fulltext )
  40. Koay JY; Jauncey Dl; Hovatta T; et al., "The presence of interstellar scintillation in the 15 GHz interday variability of 1158 OVRO-monitored blazars" , MNRAS: 489(4), 5365-5380, Nov, 2019 [SCI] ( ADS | Fulltext )
  41. Lin L; Hsieh B-C; Pan H-A; et al., "SDSS-IV MaNGA: Inside-out versus Outside-in Quenching of Galaxies in Different Local Environments" , ApJ: 872(1), 50 (14 pp.), Feb, 2019 [SCI] ( ADS | Fulltext )
  42. Lin L; Pan H-A; ...; Hsieh B-C; et al., "The ALMaQUEST Survey: The Molecular Gas Main Sequence and the Origin of the Star-forming Main Sequence" , ApJL: 884(2), id.L33 (5pp.), Oct, 2019 [SCI] ( ADS | Fulltext )
  43. Liu H-M; Hirashita H, "Expected dust grain-size distributions in galaxies detected by ALMA at z > 7" , MNRAS: 490(1), 540-549, Nov, 2019 [SCI] ( ADS | Fulltext )
  44. Ohyama Y; Sakamoto K; Aalto S; Gallagher JS III, "Dusty Superwind from a Galaxy with a Compact Obscured Nucleus: Optical Spectroscopic Study of NGC 4418" , ApJ: 871(2), id. 191 (26 pp.), Feb, 2019 [SCI] ( ADS | Fulltext )
  45. Okumura T; Taruya A; Nishimichi T, "Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features" , Phys Rev D: 100(10), id. 103507 (22 pp.), Nov, 2019 [SCI] ( ADS | Fulltext )
  46. Pan H-A; Lin L; Hsieh B-C; ...; Hsu CH; Keenan R; et al., "SDSS-IV MaNGA: Spatial Evolution of Star Formation Triggered by Galaxy Interactions" , ApJ: 881(2), id. 119 (14 pp.), Aug, 2019 [SCI] ( ADS | Fulltext )
  47. Rau S-J; Hirashita H;Murga M, "Modelling the evolution of PAH abundance in galaxies" , MNRAS: 489(4), 5218-5224, Nov, 2019 [SCI] ( ADS | Fulltext )
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  49. Toba Y; Ueda Y; Matsuoka K; …; Wang WH; Chang YY, "Does the mid-infrared-hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?" , MNRAS: 484(1), 196-203, Mar, 2019 [SCI] ( ADS | Fulltext )
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