The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types

Abstract

We analyze the applicability of far-infrared fine-structure lines [CII] 158 micron, [OI] 63 micron and [OIII] 88 micron to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and compare with a broad sample of galaxies of various types and metallicities in the literature. We study the trends and scatter in the relation between the SFR (as traced by GALEX FUV and MIPS 24 micron) and far-infrared line emission, on spatially resolved and global galaxy scales, in dwarf galaxies. We assemble far-infrared line measurements from the literature and infer whether the far-infrared lines can probe the SFR (as traced by the total-infrared luminosity) in a variety of galaxy populations. In metal-poor dwarfs, the [OI] and [OIII] lines show the strongest correlation with the SFR with an uncertainty on the SFR estimates better than a factor of 2, while the link between [CII] emission and the SFR is more dispersed (uncertainty factor of 2.6). The increased scatter in the SFR-L([CII]) relation towards low metal abundances, warm dust temperatures, large filling factors of diffuse, highly ionized gas suggests that other cooling lines start to dominate depending on the density and ionization state of the gas. For the literature sample, we evaluate the correlations for a number of different galaxy populations. The [CII] and [OI] lines are considered to be reliable SFR tracers in starburst galaxies, recovering the star formation activity within an uncertainty of factor 2. [Abridged]

35 pages, 13 figures, accepted for publication in A&A on May 7th 2014

References in corpus (29)

• Theory of Star Formation
• UV Star Formation Rates in the Local Universe
• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range
• A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
• An H-alpha Imaging Survey of Galaxies in the Local 11 Mpc Volume
• Metallicity Effects on Dust Properties in Starbursting Galaxies
• High resolution mid-infrared spectroscopy of ultraluminous infrared galaxies
• The Behavior of the Aromatic Features in M101 HII Regions: Evidence for Dust Processing
• A Compendium of Far-Infrared Line and Continuum Emission for 227 Galaxies Observed by the Infrared Space Observatory
• The origin of dwarf ellipticals in the Virgo cluster
• Stellar Evolutionary Effects on the Abundances of PAH and SN-Condensed Dust in Galaxies
• Near-Infrared and Star-forming properties of Local Luminous Infrared Galaxies
• [CII] 158$\mu$m Emission and Metallicity in PDRs
• Converting H$\alpha$ Luminosities into Star Formation Rates
• Ultraviolet Through Far-Infrared Spatially Resolved Analysis of the Recent Star Formation in M81 (NGC3031)
• Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
• Imaging the Molecular Gas in a z=3.9 Quasar Host Galaxy at 0.3" Resolution: A Central, Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255
• A Detection of [CII] line emission in the z=4.7 QSO BR1202-0725
• Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS
• Extragalactic Constraints on the Initial Mass Function
• First Detection of the [OIII] 88 micron Line at High Redshifts: Characterizing the Starburst and Narrow Line Regions in Extreme Luminosity Systems
• A Herschel Survey of the [N II] 205 micron Line in Local Luminous Infrared Galaxies --- The [N II] 205 micron Emission as a Star Formation Rate Indicator
• Hot Dust and PAH Emission at Low Metallicity: A Spitzer Survey of Local Group and Other Nearby Dwarf Galaxies
• The Nature of Infrared Emission in the Local Group Dwarf Galaxy NGC 6822 As Revealed by Spitzer
• Modeling the effects of dust evolution on the SEDs of galaxies of different morphological type
• Heating of blue compact dwarf galaxies: gas distribution and photoionization by stars in I Zw 18
• The 2nd Generation z(Redshift) and Early Universe Spectrometer Part I: First-light observation of a highly lensed local-ULIRG analog at high-z
• Star Formation Rates in Resolved Galaxies: Calibrations with Near and Far Infrared Data for NGC5055 and NGC6946

Cited by in corpus (315)

• A Luminous Quasar at Redshift 7.642
• Pōniuā'ena: A Luminous $z=7.5$ Quasar Hosting a 1.5 Billion Solar Mass Black Hole
• An ALMA [CII] survey of 27 quasars at z>5.94
• A Herschel/PACS Far Infrared Line Emission Survey of Local Luminous Infrared Galaxies
• The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
• "Big Three Dragons": a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 $\mu$m, [CII] 158 $\mu$m, and Dust Continuum with ALMA
• The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
• The Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy
• The assembly of "normal" galaxies at z=7 probed by ALMA
• Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch
• Detection of the Far-infrared [O III] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era
• Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6
• Rotation in [CII]-emitting gas in two galaxies at a redshift of 6.8
• Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe
• RELICS: Reionization Lensing Cluster Survey
• Very extended cold gas, star formation and outflows in the halo of a bright QSO at z>6
• High-redshift star formation in the ALMA era
• The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
• Bright [CII] and dust emission in three z>6.6 quasar host galaxies observed by ALMA
• The [CII] 158 micron line emission in high-redshift galaxies
• [CII] 158 $\mu$m Emission as a Star Formation Tracer
• On the [CII]-SFR relation in high redshift galaxies
• Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?
• Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
• Photodissociation and X-Ray Dominated Regions
• The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
• The nature of the [CII] emission in dusty star-forming galaxies from the SPT survey
• Tracing the reionization epoch with ALMA: [CII] emission in z~7 galaxies
• The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements
• ALMA uncovers the [CII] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
• Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies
• Kiloparsec-scale gaseous clumps and star formation at $z=5-7$
• Extended ionised and clumpy gas in a normal galaxy at z=7.1 revealed by ALMA
• Star formation rate and dynamical mass of 10^8 solar mass black hole host galaxies at redshift 6
• First Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7
• Deep into the structure of the first galaxies: SERRA views
• A Cold, Massive, Rotating Disk Galaxy 1.5 Billion Years after the Big Bang
• Normal, Dust-Obscured Galaxies in the Epoch of Reionization
• Zooming on the internal structure of $z\simeq 6$ galaxies
• The impact of chemistry on the structure of high-z galaxies
• ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z=4.8
• The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7
• A Herschel [CII] Galactic plane survey III: [CII] as a tracer of star formation
• Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
• [CII] emission in z ~ 6 strongly lensed, star-forming galaxies
• SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC
• The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5
• Copious Amounts of Dust and Gas in a z=7.5 Quasar Host Galaxy
• The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
• The compact, ~1 kpc host galaxy of a quasar at z=7.1
• Widespread QSO-driven outflows in the early Universe
• Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
• The Origins of [CII] Emission in Local Star-forming Galaxies
• The Spatially Resolved [CII] Cooling Line Deficit in Galaxies
• Missing [CII] emission from early galaxies
• Kinematics of $z\ge 6$ galaxies from [CII] line emission
• The Herschel Dwarf Galaxy Survey: II. Physical conditions, origin of [CII] emission, and porosity of the multiphase low-metallicity ISM
• The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
• A physical model for [CII] line emission from galaxies
• Stochastic star formation in early galaxies: JWST implications
• SHINING, A Survey of Far Infrared Lines in Nearby Galaxies. II: Line-Deficit Models, AGN impact, [CII]-SFR Scaling Relations, and Mass-Metallicity Relation in (U)LIRGS
• The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
• The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at $z\approx 7$
• ALMA reveals metals yet no dust within multiple components in CR7
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] line and dust emission in 6<z<8 galaxies
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• Detecting and Characterizing Young Quasars I: Systemic Redshifts and Proximity Zones Measurements
• ALMA Characterises the Dust Temperature of z ~ 5.5 Star-Forming Galaxies
• A survey of high-$z$ galaxies: SERRA simulations
• Probing the interstellar medium and star formation of the Most Luminous Quasar at z=6.3
• A wide dispersion in star formation rate and dynamical mass of 10^8 solar mass black hole host galaxies at redshift 6
• A merger in the dusty, $z=7.5$ galaxy A1689-zD1?
• Probing Cosmic Dawn with Emission Lines: Predicting Infrared and Nebular Line Emission for ALMA and JWST
• ALMA [CII] detection of a redshift 7 lensed galaxy behind RXJ1347.1-1145
• The ALMA REBELS Survey: Specific Star-Formation Rates in the Reionization Era
• Resolved UV and [CII] structures of luminous galaxies within the epoch of reionisation
• The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies
• Line-Intensity Mapping: Theory Review
• Intensity mapping of [CII] from early galaxies
• 400 pc Imaging of a Massive Quasar Host Galaxy at a Redshift of 6.6
• Dual constraints with ALMA: new [O III] 88 $\mu$m and dust-continuum observations reveal the ISM conditions of luminous LBGs at $z\sim 7$
• A kiloparsec view of a typical star-forming galaxy when the Universe was ~1 Gyr old. Part I. Outflow, halo, and interstellar medium properties
• An ALMA multi-line survey of the interstellar medium of the redshift 7.5 quasar host galaxy J1342+0928
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-Luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation
• On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements
• A Far-Infrared Spectroscopic Survey of Intermediate Redshift (Ultra) Luminous Infrared Galaxies
• Far-infrared metallicity diagnostics: Application to local ultraluminous infrared galaxies
• Accurate dust temperature determination in a $z=7.13$ galaxy
• SHINING, A Survey of Far Infrared Lines in Nearby Galaxies. I: Survey Description, Observational Trends, and Line Diagnostics
• CO line emission from galaxies in the Epoch of Reionization
• The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 μm Transitions
• ALMA Reveals Weak [NII] Emission in "Typical" Galaxies and Intense Starbursts at z=5-6
• ALMA detection of extended [CII] emission in Himiko at z=6.6
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• The spatially resolved Kennicutt-Schmidt relation in the HI dominated regions of spiral and dwarf irregular galaxies
• The Absence of [CII] 158$\mu$m Emission in Spectroscopically-Confirmed Galaxies at $z>8$
• Resolved [CII] Emission from z>6 Quasar Host -- Companion Galaxy Pairs
• Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high-$z$ galaxies
• Star Formation Rates from [CII] 158 um and Mid Infrared Emission Lines for Starbursts and AGN
• [CII] 158 micron Emission from the Host Galaxies of Damped Lyman Alpha Systems
• Bright [CII] 158$\mu$m emission in a quasar host galaxy at $z=6.54$
• Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionised gas
• Deep ALMA redshift search of a z~12 GLASS-JWST galaxy candidate
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• No evidence for enhanced [OIII] 88um emission in a z~6 quasar compared to its companion starbursting galaxy
• Constraining the evolution of CII intensity through the end stages of reionization
• The [NII] 205 micron Emission in Local Luminous Infrared Galaxies
• The Nature of High ${[\mathrm{OIII}]}_{88\mu \mathrm{m}}$/${[\mathrm{CII}]}_{158\mu \mathrm{m}}$ Galaxies in the Epoch of Reionization: Low Carbon Abundance and a Top-Heavy IMF?
• ALMA Lensing Cluster Survey: Bright [CII] 158 $\mu$m Lines from a Multiply Imaged Sub-$L^{\star }$ Galaxy at $z=6.0719$
• ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
• Predicting FIR lines from simulated galaxies
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• Far-Infrared Properties of the Bright, Gravitationally Lensed Quasar J0439+1634 at z=6.5
• The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?
• Physical constraints on the extended interstellar medium of the z=6.42 quasar J1148+5251: [CII] 158um, [NII] 205um and [OI] 146um observations
• The Pan-STARRS1 z>5.6 quasar survey II: Discovery of 55 Quasars at 5.6<z<6.5
• A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
• Tracing Molecular Gas in z $\simeq$ 6 Galaxies with [C$\mathrm{II}$]
• Spectroscopically resolved far-IR observations of the massive star-forming region G5.89--0.39
• The ALMA REBELS Survey: Efficient Ly$\alpha$ Transmission of UV-Bright z$\simeq$7 Galaxies from Large Velocity Offsets and Broad Line Widths
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• First Results from the $Herschel$ and ALMA Spectroscopic Surveys of the SMC: The Relationship Between [CII]-bright Gas and CO-bright Gas at Low Metallicity
• The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation
• [CII] 158 Micron Emission from z~4 HI Absorption-Selected Galaxies
• Neutral gas heating by X-rays in primitive galaxies: Infrared observations of IZw18 with Herschel
• Probing the Nature of High Redshift Weak Emission Line Quasars: A Young Quasar with a Starburst Host Galaxy
• High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
• A new look at the infrared properties of z $\sim$ 5 galaxies
• [C II] emission from galactic nuclei in the presence of X-rays
• The CO-dark molecular gas mass in 30 Doradus
• The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
• RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
• The ALPINE-ALMA [CII] Survey: A Triple Merger at z~4.56
• Multitracer cosmological line intensity mapping mock lightcone simulation
• MIRI/JWST observations reveal an extremely obscured starburst in the z=6.9 system SPT0311-58
• The Local [CII] 158 um Emission Line Luminosity Function
• The [CII]--SFR correlation in dwarf galaxies across cosmic time
• GRB 980425 host: [CII], [OI] and CO lines reveal recent enhancement of star formation due to atomic gas inflow
• Synthetic [CII] emission maps of a simulated molecular cloud in formation
• Lyα emission from galaxies in the Epoch of Reionization
• Detections of [OIII] 88 $\mu$m in Two Quasars in the Reionization Epoch
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Identifying candidate z~4.5 [CII] emitters
• Structure and kinematics of a massive galaxy at z ~ 7
• Neutrino Properties with Ground-Based Millimeter-Wavelength Line Intensity Mapping
• Forecasting [C II] line-intensity mapping measurements between the end of reionization and the epoch of galaxy assembly
• Mapping metals at high redshift with far-infrared lines
• Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Studying high-z galaxies with [CII] intensity mapping
• The effect of non-equilibrium metal cooling on the interstellar medium
• Using [CII] 158 micron Emission From Isolated ISM Phases as a Star-Formation Rate Indicator
• Herschel Spectroscopic Observations of LITTLE THINGS Dwarf Galaxies
• An analytic model for OIII fine structure emission from high redshift galaxies
• No [CII] or dust detection in two Little Red Dots at z${}_{\mathrm{spec}}$ > 7
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• A multi-wavelength exploration of the [CII]/IR ratio in H-ATLAS/GAMA galaxies out to z=0.2
• The Survey of Lines in M31 (SLIM): Investigating the Origins of [CII] Emission
• Two Modes of LyC Escape From Bursty Star Formation: Implications for [C II] Deficits and the Sources of Reionization
• KROSS: Mapping the Ha emission across the star-formation sequence at z~1
• Star formation law in the EoR from [CII] and CIII] lines
• Galaxy Formation Through Filamentary Accretion at z=6.1
• A comprehensive view of the interstellar medium in a quasar host galaxy at z~6.4
• Intensity Mapping in the Presence of Foregrounds and Correlated Continuum Emission
• ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
• Spatially-resolved H$\alpha$ and ionizing photon production efficiency in the lensed galaxy MACS1149-JD1 at a redshift of 9.11
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies
• SOFIA/FIFI-LS Full-disk [CII] Mapping and CO-dark Molecular Gas across the Nearby Spiral Galaxy NGC 6946
• Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
• A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO 420-G13 probes an elusive radio jet
• Characterizing the Multi-Phase Origin of [CII] Emission in M101 and NGC 6946 with Velocity Resolved Spectroscopy
• ALMA detection of [CII] 158 micron emission from a strongly lensed z=2 star-forming galaxy
• High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
• Signature of the first galaxies in JWST deep field observations
• The ALMA-CRISTAL Survey: Spatial extent of [CII] line emission in star-forming galaxies at $z=4-6$
• Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
• Spectral Energy Distributions of Companion Galaxies to z$\sim$6 Quasars
• Blind millimeter line emitter search using ALMA data toward gravitational lensing clusters
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• Inferring physical properties of galaxies from their emission line spectra
• LIMFAST. II. Line Intensity Mapping as a Probe of High-Redshift Galaxy Formation
• High-redshift quasars and their host galaxies II: multiphase gas and stellar kinematics
• The black hole and host galaxy growth in an isolated $z\sim 6$ QSO observed with ALMA
• Bridging Optical and Far-Infrared Emission-Line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 $\mu \mathrm{m}$/SFR at $z>6$
• ALMA Observation of a $z\gtrsim 10$ Galaxy Candidate Discovered with JWST
• GAME: GAlaxy Machine learning for Emission lines
• The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at $6\le z\le 8$
• GA-NIFS and EIGER: A merging quasar host at z=7 with an overmassive black hole
• The spectral energy distribution of the hyperluminous, hot dust-obscured galaxy W2246$-$0526
• The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
• Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations
• Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies
• First detection of the [OI] 63-um emission from a redshift 6 dusty galaxy
• Feeding the spider with carbon -- [CII] emission from the circum galactic medium and active galactic nucleus
• Accurate dust temperature and star formation rate in the most luminous $z>6$ quasar in the HYPerluminous quasars at the Epoch of ReionizatION (HYPERION) sample
• Early galaxy growth: mergers or gravitational instability?
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• The high-ionization IR fine-structure lines as bolometric indicators of the AGN power: study of the complete 12 micron AGN sample
• FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
• Interpreting ALMA non-detections of JWST super-early galaxies
• Atomic and molecular gas as traced by [C II] emission
• Regulating Star Formation in Nearby Dusty Galaxies: Low Photoelectric Efficiencies in the Most Compact Systems
• ALMA [CII] 158um imaging of an HI-Selected Major Merger at z~4
• The observed cosmic star formation rate density has an evolution which resembles a Γ(a, bt) distribution and can be described successfully by only 2 parameters
• The ALMA Patchy Deep Survey: A blind search for [CII] emitters at z~4.5
• Stellar cluster formation in a Milky Way-sized galaxy at z>4 -- I. The proto-globular cluster population and the imposter amongst us
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• ISM conditions in z~0.2 Lyman-Break Analogs
• The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines
• The Lyman Alpha Reference Sample XI: Efficient Turbulence Driven Lyα Escape and the Analysis of IR, CO and [C II]158 μm
• ColdSIM predictions of [C II] emission in primordial galaxies
• The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z=5.66
• The Survey of Lines in M31 (SLIM): The Drivers of the [CII]/TIR Variation
• [CII] map of the molecular ring and arms of the spiral galaxy NGC 7331
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
• The archival discovery of a strong Lyman-$\alpha$ and [CII] emitter at z = 7.677
• The ALMA-ALPINE [CII] survey: sub-kpc morphology of 3 main-sequence galaxy systems at z~4.5 revealed by ALMA
• Updated measurements of [O III] 88 $\mu$m, [C II] 158 $\mu$m, and Dust Continuum Emission from a z=7.2 Galaxy
• Molecular gas and dust properties in $z>7$ quasar hosts
• Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
• Synergizing 21 cm and sub-millimetre surveys during reionization: new empirical insights
• The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• The prospects for observing [OIII] 52 micron emission from galaxies during the Epoch of Reionization
• CONCERTO: Extracting the power spectrum of the [C II ] emission line
• Calibration of mid- to far-infrared spectral lines in galaxies
• Far-Infrared and [CII] observations of a z=7 blazar
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Tomography of the environment of the COSMOS/AzTEC-3 submillimeter galaxy at z=5.3 revealed by Lyalpha and MUSE observations
• Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z${}_{[CII]}$ = 6.827 using NOEMA
• Carbon envelopes around merging galaxies at z ~ 4.5
• Origin of the Galaxy Mass-Metallicity-Star-Formation Relation
• The Case for Thermalization as a Contributor to the [CII] Deficit
• Compact [C II] emitters around a C IV absorption complex at redshift 5.7
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• Spritz is sparkling: simulated CO and [CII] luminosities
• The Unusual AGN Host NGC 1266: Evidence for Shocks in a Molecular Gas Rich S0 Galaxy with a Low Luminosity Nucleus
• Infrared fine-structure lines at high redshift
• Neon and [CII] 158 micron Emission Line Profiles in Dusty Starbursts and Active Galactic Nuclei
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• SOFIA-upGREAT imaging spectroscopy of the [C II] 158um fine structure line of the Sgr B region in the Galactic center
• Detection of the [O I] 63 $\mu$m emission line from the $z=6.04$ quasar J2054-0005
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
• A Molecular Gas Ring Hidden in the Sombrero Galaxy
• $\text{Herschel}$ Photometric Observations of $\mathrm{L}\mathrm{ITTLE}$ $\mathrm{T}\mathrm{HINGS}$ Dwarf Galaxies
• The host galaxies of radio-loud quasars at z>5 with ALMA
• Another X-ray UFO without a momentum-boosted molecular outflow. ALMA CO(1-0) observations of the galaxy pair IRAS 05054+1718
• A puzzling non-detection of [O III] and [C II] from a $z\approx 7.7$ galaxy observed with ALMA
• Observations of [OI]63micron line emission in main-sequence galaxies at z~1.5
• The spatially-resolved correlation between [NII] 205 μm line emission and the 24 μm continuum in nearby galaxies
• ALMA Imaging of the CO(7-6) Line Emission in the Submillimeter Galaxy LESS 073 at redshift 4.755${}^{\star }$
• C II radiative cooling of the Galactic diffuse interstellar medium: Insight about the star formation in Damped Lyman-alpha systems
• Limited impact of jet induced feedback in the multi-phase nuclear interstellar medium of 4C12.50
• Simulated [CII] in high-z galaxies
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited
• Environmental effects in Herschel observations of the ionized carbon content of star forming dwarf galaxies in the Virgo cluster
• Detections of [C II] 158 $\mu$m and [O III] 88 $\mu$m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• ALPINE: A Large Survey to Understand Teenage Galaxies
• Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy
• A Herschel mapping of [C ii], [O i] and [O iii] lines from the circumnuclear region of M31
• Galaxies into the Dark Ages
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Probing the Epoch of Reionization using synergies of line intensity mapping
• The [NII] 205 $\mu$m line emission from high-z SMGs and QSOs
• Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII]
• The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of $z\sim 5$ galaxies
• Disentangling emission from star-forming regions in the Magellanic Clouds: Linking [OIII]88 micron and 24 micron
• CONCERTO at APEX -- On-sky performance in continuum
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• A [CII]-158-micron Survey of DLA galaxies at z~4: Observations of Dense and Metal-Enriched Neutral Gas within the Circumgalactic Medium of Star-Forming Galaxies
• Spatially resolved H$\alpha$ emission in B14-65666: compact starbursts, ionizing efficiency and gas kinematics in an advanced merger at the Epoch of Reionization
• A tentative $\sim$1000 km s${}^{-1}$ offset between the [CII] 158 $\mu$m and Ly$\alpha$ line emission in a star-forming galaxy at $z=7.2$
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• Amaryllis: a digital twin of the earliest galaxies in the Universe
• The origin and evolution of the [CII] deficit in HII regions and star-forming molecular clouds
• The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim 5$
• Full disc [CII] mapping of nearby star-forming galaxies: SOFIA FIFI/LS observations of NGC 3627, NGC 4321, and NGC 6946
• Physical conditions in the gas phases of the giant HII region LMC-N11: II. Origin of [CII] and fraction of CO-dark gas
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• High$-z$ [OI] emission lines: ColdSIM simulations and ALMA observations
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• Tight correlation of star formation with [Ci] and CO lines across cosmic time
• Gas-Poor Hosts and Gas-Rich Companions of $z\approx$3.5 Radio Active Galactic Nuclei: ALMA Insights into Jet Triggering and Feedback
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~0 ECO volume-limited star-forming galaxy sample
• Measuring the ISM Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C II]
• Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
• An Atlas of Star-Forming Galaxy Equivalent Widths
• The Close AGN Reference Survey (CARS): SOFIA detects spatially-resolved [CII] emission in the luminous AGN HE0433-1028
• LMC+: Large-scale mapping of [CII] and [OIII] in the LMC molecular ridge, I. Dataset and line ratio analyses
• Comparison of Cross-Correlation Methods for Line Intensity Mapping
• Unveiling the evolution of the CO excitation ladder through cross-correlation of CONCERTO-like experiments and galaxy redshift surveys
• Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk
• The Galaxy Evolution Probe
• The Impact of Powerful Jets on the Far-infrared Emission of an Extreme Radio Quasar at z~6
• The ALMA View of High-Redshift Galaxy Formation
• Uncovering the absorbed atomic Universe with the [OI]63um line
• Bright beacons? ALMA non-detection of a supposedly bright [OI] 63-um line in a redshift-6 dusty galaxy
• Evaluating star formation rates at z = 5