Objectives of the Millimetron Space Observatory science program and technical capabilities of its realization
ID Novikov, SF Likhachev, YA Shchekinov… - Physics …, 2021 - iopscience.iop.org
We present the scientific program of the Spectr-M project aimed at the creation and
operation of the Millimetron Space Observatory (MSO) planned for launch in the late 2020s …
operation of the Millimetron Space Observatory (MSO) planned for launch in the late 2020s …
An extreme protocluster of luminous dusty starbursts in the early universe
I Oteo, RJ Ivison, L Dunne… - The Astrophysical …, 2018 - iopscience.iop.org
We report the identification of an extreme protocluster of galaxies in the early universe
whose core (nicknamed Distant Red Core, DRC, because of its very red color in Herschel …
whose core (nicknamed Distant Red Core, DRC, because of its very red color in Herschel …
Discovery of an enormous Lyα Nebula in a massive galaxy overdensity at z= 2.3
Abstract Enormous Lyα nebulae (ELANe), unique tracers of galaxy density peaks, are
predicted to lie at the nodes and intersections of cosmic filamentary structures. Previous …
predicted to lie at the nodes and intersections of cosmic filamentary structures. Previous …
ALMA deep field in SSA22: Survey design and source catalog of a 20 arcmin2 survey at 1.1 mm
To search for dust-obscured star-formation activity in the early Universe, it is essential to
obtain a deep and wide submillimeter/millimeter map. The advent of the Atacama Large …
obtain a deep and wide submillimeter/millimeter map. The advent of the Atacama Large …
A theory for the variation of dust attenuation laws in galaxies
D Narayanan, C Conroy, R Davé… - The Astrophysical …, 2018 - iopscience.iop.org
In this paper, we provide a physical model for the origin of variations in the shapes and
bump strengths of dust attenuation laws in galaxies by combining a large suite of …
bump strengths of dust attenuation laws in galaxies by combining a large suite of …
Inspiraling halo accretion mapped in Ly α emission around a z ∼ 3 quasar
F Arrigoni Battaia, JX Prochaska… - Monthly Notices of …, 2018 - academic.oup.com
In an effort to search for Ly α emission from circum-and intergalactic gas on scales of
hundreds of kpc around z∼ 3 quasars, and thus characterize the physical properties of the …
hundreds of kpc around z∼ 3 quasars, and thus characterize the physical properties of the …
The IRX–β dust attenuation relation in cosmological galaxy formation simulations
D Narayanan, R Davé, BD Johnson… - Monthly Notices of …, 2018 - academic.oup.com
We utilize a series of galaxy formation simulations to investigate the relationship between
the ultraviolet (UV) slope, β, and the infrared excess (IRX) in the spectral energy distributions …
the ultraviolet (UV) slope, β, and the infrared excess (IRX) in the spectral energy distributions …
[C ii] 158 μm emission as an indicator of galaxy star formation rate
Observations of local star-forming galaxies (SFGs) show a tight correlation between their
singly ionized carbon line luminosity () and star formation rate (SFR), suggesting that may be …
singly ionized carbon line luminosity () and star formation rate (SFR), suggesting that may be …
Radiative Transfer in Lyα Nebulae. I. Modeling a Continuous or Clumpy Spherical Halo with a Central Source
To understand the mechanism behind high-z Lyα nebulae, we simulate the scattering of Lyα
in a H i halo about a central Lyα source. For the first time, we consider both smooth and …
in a H i halo about a central Lyα source. For the first time, we consider both smooth and …
ODIN: Where Do Lyα Blobs Live? Contextualizing Blob Environments within Large-scale Structure
V Ramakrishnan, B Moon, SH Im… - The Astrophysical …, 2023 - iopscience.iop.org
While many Lyα blobs (LABs) are found in and around several well-known protoclusters at
high redshift, how they trace the underlying large-scale structure is still poorly understood. In …
high redshift, how they trace the underlying large-scale structure is still poorly understood. In …