CO excitation of normal star-forming galaxies out to z= 1.5 as regulated by the properties of their interstellar medium
We investigate the CO excitation of normal (near-IR selected BzK) star-forming (SF) disk
galaxies at z= 1.5 using IRAM Plateau de Bure observations of the CO [2–1], CO [3–2], and …
galaxies at z= 1.5 using IRAM Plateau de Bure observations of the CO [2–1], CO [3–2], and …
The Herschel Comprehensive (U) LIRG emission survey (HERCULES): CO ladders, fine structure lines, and neutral gas cooling
MJF Rosenberg, PP Van Der Werf, S Aalto… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT (Ultra) luminous infrared galaxies ((U) LIRGs) are objects characterized by their
extreme infrared (8–1000 μm) luminosities (L LIRG> 10 11 L☉ and L ULIRG> 10 12 L☉) …
extreme infrared (8–1000 μm) luminosities (L LIRG> 10 11 L☉ and L ULIRG> 10 12 L☉) …
L'CO/LFIR Relations with CO Rotational Ladders of Galaxies Across the Herschel SPIRE Archive
We present a catalog of all CO (J= 4-3 through J= 13-12)),[CI],[NII] lines available from
extragalactic spectra from the Herschel SPIRE Fourier Transform Spectrometer (FTS) …
extragalactic spectra from the Herschel SPIRE Fourier Transform Spectrometer (FTS) …
Prospects for detecting C II emission during the Epoch of reionization
We produce simulations of the atomic C ii line emission in large sky fields in order to
determine the current and future prospects for mapping this line during the high-redshift …
determine the current and future prospects for mapping this line during the high-redshift …
The origins of [C II] emission in local star-forming galaxies
KV Croxall, JD Smith, E Pellegrini… - The Astrophysical …, 2017 - iopscience.iop.org
The [C ii] 158 μm fine-structure line is the brightest emission line observed in local star-
forming galaxies. As a major coolant of the gas-phase interstellar medium,[C ii] balances the …
forming galaxies. As a major coolant of the gas-phase interstellar medium,[C ii] balances the …
CO emission in distant galaxies on and above the main sequence
We present the detection of multiple carbon monoxide CO line transitions with ALMA in a
few tens of infrared-selected galaxies on and above the main sequence at z= 1.1− 1.7. We …
few tens of infrared-selected galaxies on and above the main sequence at z= 1.1− 1.7. We …
Co excitation, molecular gas density, and interstellar radiation field in local and high-redshift galaxies
We study the carbon monoxide (CO) excitation, mean molecular gas density, and interstellar
radiation field (ISRF) intensity in a comprehensive sample of 76 galaxies from local to high …
radiation field (ISRF) intensity in a comprehensive sample of 76 galaxies from local to high …
Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas
The most intensively star-forming galaxies are extremely luminous at far-infrared (FIR)
wavelengths, highly obscured at optical and ultraviolet wavelengths, and lie at≥ 1–3. We …
wavelengths, highly obscured at optical and ultraviolet wavelengths, and lie at≥ 1–3. We …
THE IONIZED GAS IN NEARBY GALAXIES AS TRACED BY THE 122 AND 205 μm TRANSITIONS
R Herrera-Camus, A Bolatto, JD Smith… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT The [N ii] 122 and 205 μm transitions are powerful tracers of the ionized gas in
the interstellar medium. By combining data from 21 galaxies selected from the Herschel …
the interstellar medium. By combining data from 21 galaxies selected from the Herschel …
A far-infrared spectroscopic survey of intermediate redshift (ultra) luminous infrared galaxies
GE Magdis, D Rigopoulou, R Hopwood… - The Astrophysical …, 2014 - iopscience.iop.org
We present Herschel far-IR photometry and spectroscopy as well as ground-based CO
observations of an intermediate redshift (0.21⩽ z⩽ 0.88) sample of Herschel-selected (ultra) …
observations of an intermediate redshift (0.21⩽ z⩽ 0.88) sample of Herschel-selected (ultra) …