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Exploring the star formation histories of galaxies in different environments from MaNGA spectra.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 60, doi. 10.1017/S1743921319004770
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First [NII] 122 μ m line detection in a starburst pair at z = 4.7.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 283, doi. 10.1017/S1743921319004782
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Modeling the panchromatic emission of galaxies with CIGALE.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 129, doi. 10.1017/S1743921319004769
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Panchromatic study of the first galaxies in cosmological simulations.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 240, doi. 10.1017/S1743921319004757
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A historical overview of galaxy surveys.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 1, doi. 10.1017/S1743921319004800
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IAU volume 15 issue 341 Cover and Back matter.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. b1, doi. 10.1017/S1743921319009311
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- Article
IAU volume 15 issue 341 Cover and Front matter.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. f1, doi. 10.1017/S174392131900930X
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- Article
A new galaxy Spectral Energy Distribution model with the evolution of dust consistent with chemical evolution.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 152, doi. 10.1017/S1743921319004794
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Going beyond galaxy ages with dense basis star formation history reconstruction.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 134, doi. 10.1017/S1743921319004733
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Propeties of H alpha emitters at z ∼ 2.3: Derivation of H alpha luminosity from multi-band photometry.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 316, doi. 10.1017/S1743921319002783
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Modelling the emission of passive galaxy candidates at z∼3.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 44, doi. 10.1017/S1743921319003065
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Census of and Lyα, [Oiii]5007, Hα, and [Ciii]158 μm line emission wiht ∼1000 galaxies at z = 4.9 – 7.0 revealed with Subaru/HSC, Spitzer, and ALMA.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 206, doi. 10.1017/S1743921319002618
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Panchromatic SED fitting codes and modelling techniques.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 26, doi. 10.1017/S1743921319003016
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HELP project - a dreamed-of multiwavelength dataset for SED fitting: The influence of used models for the main physical properties of galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 39, doi. 10.1017/S174392131900471X
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Modeling galaxy evolution at high-redshift in highly overdense and normal regions.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 299, doi. 10.1017/S1743921319004721
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Tips learned from panchromatic modeling of AGNs.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 167, doi. 10.1017/S1743921319002771
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Dust evolution in galaxies at z > 7.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 312, doi. 10.1017/S1743921319003107
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Pushing the technical frontier: From overwhelmingly large data sets to machine learning.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 88, doi. 10.1017/S1743921319003077
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Properties of LBGs with [OIII] detection at z > 3: The importance of including nebular emission data in SED fitting.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 201, doi. 10.1017/S174392131900276X
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Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 143, doi. 10.1017/S1743921319002746
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Radiative properties of the first galaxies: Rapid transition from blue to red.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 261, doi. 10.1017/S1743921319003004
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Spectral study of scattered light by interstellar dust grains.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 302, doi. 10.1017/S1743921319002990
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Direct collapse to SMBH seeds in cosmological halos with radiation transfer.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 289, doi. 10.1017/S1743921319002941
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Mid-infrared PAH emission from star-forming galaxies selected at 250 μ m.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 281, doi. 10.1017/S1743921319002928
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Probing the luminous and dark matter profiles in the inner regions of a group-scale lens at z = 0.6.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 318, doi. 10.1017/S1743921319002916
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The average FIR SED of proto-clusters at z = 4.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 17, doi. 10.1017/S1743921319002904
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The diagnostic power of radio spectra from star-forming galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 177, doi. 10.1017/S1743921319002898
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The onset of star formation 250 million years after the Big Bang.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 221, doi. 10.1017/S1743921319002886
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Challenges in modelling the rest-frame ultraviolet/optical spectra of galaxies at the high-redshift frontier.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 187, doi. 10.1017/S1743921319002862
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Mentari: A pipeline to model the galaxy SED using semi analytic models.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 119, doi. 10.1017/S1743921319002813
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Systematic errors in dust mass fits: The role of dust opacity.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 196, doi. 10.1017/S1743921319002801
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Subaru/HSC identifications of protocluster candidates at z ∼ 6–7: Implications for cosmic reionization.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 231, doi. 10.1017/S1743921319002795
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Stellar population synthesis of galaxies with chemical evolution model.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 147, doi. 10.1017/S1743921319002758
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Panchromatic Analysis for Nature of HIgh- z galaxies Tool (PANHIT).
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 285, doi. 10.1017/S1743921319002606
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The environment of large equivalent width Lyα emitters at z ∼ 3.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 277, doi. 10.1017/S1743921319002631
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Magneto-Hydrodynamic simulations on galaxy modeling.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 320, doi. 10.1017/S174392131900231X
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Pop III Supernova Feedback on the Formation of the First Galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 253, doi. 10.1017/S1743921319002564
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Evolution histories of massive galaxies at z ∼2 over the past 3 Gyr.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 50, doi. 10.1017/S1743921319002734
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Spatially resolved dust-to-gas mass ratios in nearby galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 78, doi. 10.1017/S1743921319002710
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Which attenuation curves for star-forming galaxies?
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 70, doi. 10.1017/S1743921319002692
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Spatially resolved stellar mass buildup and quenching in massive disk galaxies over the last 10 Gyr revealed with spatially resolved SED fitting.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 55, doi. 10.1017/S1743921319002680
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The spectral energy distributions of active galactic nuclei.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 21, doi. 10.1017/S1743921319002667
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High-resolution radiation transfer modelling of barred galaxies.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 65, doi. 10.1017/S1743921319002643
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Automatic classification of sources in large astronomical catalogs.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 109, doi. 10.1017/S1743921319002576
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Evolutionary Population Synthesis model with binary stars – Yunnan-II model.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 35, doi. 10.1017/S174392131900262X
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First galaxy SED: Contribution from pre-main-sequence stars.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 287, doi. 10.1017/S174392131900259X
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ALMA detection of the [OIII] 88 μ m line in a highly-magnified Lyman break galaxy at z = 6.1.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 309, doi. 10.1017/S174392131900245X
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Detections of far-infrared [OIII] and dust emission in a galaxy at z = 8.312: Early metal enrichment in the heart of the reionization era.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 211, doi. 10.1017/S1743921319002436
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The distribution and physical properties of high-redshift [Oiii] emitters in a cosmological hydrodynamics simulation.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 249, doi. 10.1017/S1743921319002424
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Optical properties of infrared-bright dust-obscured galaxies viewed with Subaru Hyper Suprime-Cam.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 292, doi. 10.1017/S1743921319002400
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