The ALPINE−ALMA [C ii ] Survey: on the nature of an extremely obscured serendipitous galaxy |
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The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]–SFR relation over the last 13 Gyr |
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The ALPINE–ALMA [CII] survey: Luminosity function of serendipitous [CII] line emitters at z ∼ 5 |
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The ALPINE-ALMA [CII] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements |
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The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe |
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The ALPINE-ALMA [CII] survey: Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6 |
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The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z ∼ 5 |
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Appendix A : The atomic physics of oxygen |
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The broad OVI absorber at z=3.02 toward CTQ 325 |
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[C II] and ^12^CO(1-0) emission maps in HLSJ091828.6+514223: a strongly lensed interacting system at z = 5.24 |
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[C II] AND12CO |
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Chapter 1 : How to Derive Oxygen Abundances |
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Chapter 2 : A Panorama of Oxygen in the Universe |
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Chapter 3 : Oxygen Production and Destruction |
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Chapter 4 : The Evolution of Oxygen in Galaxies |
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Chemical abundances in DLAs and the distant universe |
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Clumpy galaxies seen in H {alpha}: inflated observed clump properties due to limited spatial resolution and sensitivity |
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CO map and steep Kennicutt-Schmidt relation in the extended UV disk of M 63 |
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CODEX: measuring the acceleration of the universe and beyond |
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A complete census ofHerschel-detected infrared sources within theHSTFrontier Fields |
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Constraining the star formation histories of gamma-ray burst host galaxies from their observed abundance patterns |
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Cosmic dynamics in the era of Extremely Large Telescopes |
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The cosmic microwave background radiation temperature at z_abs_ = 3.025 toward QSO 0347-3819 |
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DeepHerschelview of obscured star formation in the Bullet cluster |
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Detection of Wolf-Rayet stars in host galaxies of gamma-ray bursts (GRBs): are GRBs produced by runaway massive stars ejected from high stellar density regions? |
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DISCOVERY OF “WARM DUST” GALAXIES IN CLUSTERS ATz∼ 0.3: EVIDENCE FOR STRIPPING OF COOL DUST IN THE DENSE ENVIRONMENT? |
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Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7 |
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Erratum: “A mature dusty star-forming galaxy hosting GRB 080607 at z = 3.036” (2010, ApJ, 723, L218) |
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ESPRESSO: A High Resolution Spectrograph for the Combined Coudé Focus of the VLT |
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An extendedHerscheldrop-out source in the center of AS1063: a normal dusty galaxy atz= 6.1 or SZ substructures? |
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Far-infrared constraints on the contamination by dust-obscured galaxies of high-zdropout searches |
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The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster |
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Foreword |
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From ESPRESSO to CODEX |
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Gravitationally lensed galaxies at 2 < z < 3.5: direct abundance measurements of Ly {alpha} emitters |
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The Herschel Lensing Survey (HLS): Overview |
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High-redshift starbursting dwarf galaxies revealed by {gamma}-ray burst afterglows |
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Improving the identification of high-zHerschelsources with position priors and optical/NIR and FIR/mm photometric redshifts |
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Infrared Galaxies in the Field of the Massive Cluster Abell S1063: Discovery of a Luminous Kiloparsec-sized H ii Region in a Gravitationally Lensed Infrared-luminous Galaxy at z = 0.6 |
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The kinematic signature of damped Lyman alpha systems: using theD-index to screen for high column density H i absorbers★ |
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KMOS LENsing Survey (KLENS): Morpho-kinematic analysis of star-forming galaxies at z ~ 2 |
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The low-mass end of the fundamental relation for gravitationally lensed star-forming galaxies at 1 < z < 6 |
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Massive, Absorption-selected Galaxies at Intermediate Redshifts |
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Metal abundances and kinematics of quasar absorbers. II. Absorption systems toward Q0347-3819 and APM BR J0307-4945 |
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The metal-strong damped Ly{alpha} systems |
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Millimeter astronomy |
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Molecular emission from a galaxy associated with a z ~ 2.2 damped Ly{alpha} absorber |
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Molecular gas content in typical L* galaxies at z ∼ 1.5 − 3 |
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Molecular gas in high-velocity clouds: revisited scenario |
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Molecular gas properties of a lensed star-forming galaxy at z ~ 3.6: a case study |
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The multi-phase cold fountain in M82 revealed by a wide, sensitive map of the molecular interstellar medium |
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Multiply lensed star forming clumps in the A521-sys1 galaxy at redshift 1 |
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A new comprehensive set of elemental abundances in DLAs. III. Star formation histories |
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New constraints on dust emission and UV attenuation ofz= 6.5–7.5 galaxies from millimeter observations |
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New emerging results on molecular gas, stars, and dust at z ~ 2, as revealed by low star formation rate and low stellar mass star-forming galaxies |
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On the Incidence of Strong MgiiAbsorbers along Gamma-Ray Burst Sight Lines |
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On the stellar masses of giant clumps in distant star-forming galaxies |
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Physics of a clumpy lensed galaxy at z=1.6 |
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Probing the Interstellar Medium and Stellar Environments of Long-Duration GRBs |
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Propriétés Résolues des Galaxies Fortement Lentillées |
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Reconciling the metallicity distributions of gamma-ray burst, damped Ly{alpha}, and Lyman break galaxies at z~3 |
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Resolved properties of high redshift lensed galaxies. |
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Resolving The ISM Surrounding GRBs with Afterglow Spectroscopy |
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Rest-frame UV to optical X-shooter spectrum of the gravitationally lensed galaxy 'the 8 o'clock arc': Dissection of its physical properties |
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A search of CO emission lines in blazars: the low molecular gas content of BL Lac objects compared to quasars |
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SHARDS: A GLOBAL VIEW OF THE STAR FORMATION ACTIVITY ATz∼ 0.84 andz∼ 1.23 |
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Signatures of cool gas fueling a star-forming galaxy at redshift 2.3. |
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Spectral classification of emission-line galaxies |
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Star formation histories, extinction, and dust properties of strongly lensedz~ 1.5–3 star-forming galaxies from theHerschelLensing Survey |
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Strong magnetic fields in normal galaxies at high redshift. |
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Temporal Variation in the Abundance of Excited Fe[FORMULA][F][SUP]+[/SUP][/F][/FORMULA] Near a Gamma-Ray Burst Afterglow |
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Towards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at <i>z</i> ∼ 1 |
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UVES observations of a damped Lyαsystem at $\mathsf{{\vec z}_{abs} = 4.466}$ towards the quasar APM BR J0307-4945 |
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XQ-100: A legacy survey of one hundred 3.5 ≲z≲ 4.5 quasars observed with VLT/X-shooter |
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মুখবন্ধ |
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