THE GAS MASS OF STAR-FORMING GALAXIES AT z ≈ 1.3

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Star Forming Galaxies at z > 5

We present recent progress in searching for galaxies at redshift from z ≃ 5 to z ≃ 10. Wide-field and senstive surveys with 8m class telescopes have been providing more than several hundreds of star forming galaxies at z ≃ 5 – 7 that are probed in the optical window. These galaxies are used to study the early cosmic star formation activity as well as the early structure formation in the univers...

متن کامل

A survey of the cold molecular gas in gravitationally lensed star - forming galaxies at z > 2

Using the Australia Telescope Compact Array (ATCA), we conducted a survey of CO J = 1− 0 and J = 2− 1 line emission towards strongly lensed high-redshift dusty star forming galaxies (DSFGs) previously discovered with the South Pole Telescope (SPT). Our sample comprises 17 sources that had CO-based spectroscopic redshifts obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) and ...

متن کامل

Dust and gas in star forming galaxies at z ~ 3 - extending galaxy uniformity

We present millimetre dust emission measurements of two Lyman Break Galaxies at z ∼ 3 and construct for the first time fully sampled infrared spectral energy distributions (SEDs), from mid-IR to the Rayleigh-Jeans tail, of individually detected, unlensed, UV-selected, main sequence (MS) galaxies at z = 3. The SED modelling of the two sources confirms previous findings, based on stacked ensemble...

متن کامل

Molecular Gas in Submillimetre-Faint, Star-Forming Ultraluminous Galaxies at z>1

We present interferometric CO observations of twelve z∼2 submillimetre-faint, starforming radio galaxies (SFRGs) which are thought to be ultraluminous infrared galaxies (ULIRGs) possibly dominated by warmer dust (Tdust > ∼ 40 K) than submillimetre galaxies (SMGs) of similar luminosities. Four other CO-observed SFRGs are included from the literature, and all observations are taken at the Plateau...

متن کامل

Dust and gas in star forming galaxies at z ~ 3 - extending

We present millimetre dust emission measurements of two Lyman Break Galaxies at z ∼ 3 and construct for the first time fully sampled infrared spectral energy distributions (SEDs), from mid-IR to the Rayleigh-Jeans tail, of individually detected, unlensed, UV-selected, main sequence (MS) galaxies at z = 3. The SED modelling of the two sources confirms previous findings, based on stacked ensemble...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2016

ISSN: 2041-8213

DOI: 10.3847/2041-8205/818/2/l28