kiyer/astro_corpus_entities · Datasets at Hugging Face

name stringlengths 1 11.3k	aliases listlengths 0 3.27k	kind stringclasses 9 values	role stringclasses 4 values	salience stringclasses 3 values	claims listlengths 0 21	bibcode stringlengths 19 19
212Po	[ "polonium-212" ]	object	subject	high	[ { "is_quantitative": false, "text": "The alpha-decay width of 212Po is calculated using a quartetting wave function approach and agrees fairly well with the measured value." }, { "is_quantitative": false, "text": "The alpha-cluster preformation probability and alpha-decay width of 212Po are micr...	2016MNRAS.461.4335A
quartetting wave function approach	[ "quartetting" ]	method	subject	high	[ { "is_quantitative": false, "text": "The quartetting wave function approach is improved by implementing four-nucleon correlations to describe alpha preformation in 212Po." } ]	2016MNRAS.461.4335A
208Pb	[ "lead-208" ]	object	used	medium	[ { "is_quantitative": false, "text": "The measured density distribution of the 208Pb core is used to calculate the alpha-decay width of 212Po." } ]	2016MNRAS.461.4335A
Ponos	[ "Ponos zoom-in numerical simulations" ]	simulation	subject	high	[ { "is_quantitative": true, "text": "The Ponos simulations model dark matter substructures in massive elliptical galaxy halos with virial masses of 1.2 !x 10^{13} M_sun and 6.5 !x 10^{12} M_sun down to z = 0." }, { "is_quantitative": true, "text": "The simulations resolve halos with up to 921,651...	2016A&A...594A..93C
dark matter substructures	[ "subhalos" ]	concept	subject	high	[ { "is_quantitative": true, "text": "Subhalos with M_sub < 10^9 M_sun contribute between one-fifth and one-third of the total projected mass fraction in massive elliptical halos." }, { "is_quantitative": false, "text": "Baryonic contraction increases the number of massive subhalos in the inner re...	2016A&A...594A..93C
baryonic contraction	[]	concept	subject	medium	[ { "is_quantitative": false, "text": "Baryonic contraction produces a super-isothermal total density profile and increases the number of massive subhalos in the inner regions of the main host." } ]	2016A&A...594A..93C
gravitational lenses	[]	concept	compared	low	[ { "is_quantitative": false, "text": "The host density profiles and projected subhalo mass fractions from the Ponos simulations are broadly consistent with observations of gravitational lenses." } ]	2016A&A...594A..93C
Auger Engineering Radio Array	[ "AERA" ]	facility	subject	high	[ { "is_quantitative": true, "text": "AERA consists of more than 150 autonomous radio stations with different spacings, covering an area of about 17 km^2." }, { "is_quantitative": true, "text": "AERA detects radio emission from extensive air showers with energies beyond 10^17 eV in the 30 - 80 MHz...	2017JCoPh.330..566S
Pierre Auger Cosmic-Ray Observatory	[ "Auger Observatory" ]	facility	used	medium	[]	2017JCoPh.330..566S
Auger surface detector	[]	facility	used	medium	[ { "is_quantitative": false, "text": "The Auger surface detector is used to cross-calibrate AERA's radio radiation energy measurements to establish cosmic-ray energy scales." } ]	2017JCoPh.330..566S
radiation energy	[]	concept	subject	high	[ { "is_quantitative": false, "text": "The radiation energy emitted by air showers in the form of radio emission is measured and calibrated against the cosmic-ray energy scale." } ]	2017JCoPh.330..566S
lattice field theory methods	[ "lattice methods" ]	method	subject	high	[ { "is_quantitative": false, "text": "Lattice field theory methods are increasingly applied to calculate ground-state and thermal properties of strongly interacting non-relativistic few- and many-body systems." } ]	2013Icar..223..460S
hybrid Monte Carlo	[]	method	subject	medium	[ { "is_quantitative": false, "text": "Hybrid Monte Carlo techniques have recently crossed over from quantum chromodynamics to condensed matter, atomic, and low-energy nuclear physics." } ]	2013Icar..223..460S
improved effective actions	[]	method	subject	medium	[ { "is_quantitative": false, "text": "Improved effective actions have recently been applied to non-relativistic strongly interacting many-body systems." } ]	2013Icar..223..460S
fermions in the limit of unitarity	[]	concept	subject	medium	[ { "is_quantitative": false, "text": "Lattice methods are used to determine the ground- and excited-state properties of fermions in the limit of unitarity." } ]	2013Icar..223..460S
intragroup medium	[ "intragroup" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The intragroup medium has lower entropy levels and different radial profiles compared to the intracluster medium due to weakly supersonic gas inflow and less effective conversion of kinetic to thermal energy." } ]	2016ApJ...830..141L
intracluster medium	[ "intracluster" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The intracluster medium experiences highly supersonic gas inflow across the system boundary, leading to strong accretion shocks and substantial conversion of bulk kinetic into thermal energy." } ]	2016ApJ...830..141L
ESO 3060170	[]	object	subject	medium	[ { "is_quantitative": false, "text": "X-ray observations of the galaxy group ESO 3060170 out to its virial radius show entropy profiles that match theoretical expectations of starved inflow in low-redshift or poor environments." } ]	2016ApJ...830..141L
RXJ1159+5531	[]	object	subject	medium	[ { "is_quantitative": false, "text": "X-ray observations of the galaxy group RXJ1159+5531 out to its virial radius show entropy profiles that match theoretical expectations of starved inflow in low-redshift or poor environments." } ]	2016ApJ...830..141L
iron nanoparticles	[ "metallic iron nanoparticles", "iron clusters", "ultrasmall iron clusters" ]	concept	subject	high	[ { "is_quantitative": true, "text": "Iron nanoparticles are stable against sublimation in the interstellar radiation field down to a radius of ≃4.5 Å, and potentially smaller." }, { "is_quantitative": false, "text": "Iron nanoparticles can acquire negative charges, particularly in interstellar en...	2017AdSpR..59..736B
photoelectric heating	[ "photoelectric heating rate" ]	concept	subject	medium	[ { "is_quantitative": true, "text": "The photoelectric heating rate from dust may be increased by up to tens of percent if ≳10% of interstellar iron is in the form of ultrasmall iron clusters." } ]	2017AdSpR..59..736B
interstellar dust	[ "dust" ]	concept	mentioned	low	[]	2017AdSpR..59..736B
QSOs	[ "QSO" ]	concept	subject	high	[ { "is_quantitative": true, "text": "The host galaxies of nine QSOs at 0.1 < z < 0.2 have black hole masses of 3x10^7 M_sun to 3x10^9 M_sun and far-infrared luminosities of ~ several times 10^11 L_sun." }, { "is_quantitative": true, "text": "The observed L_[OI]63um/L_FIR and L_[CII]/L_FIR ratios ...	2016A&A...595A..83E
Herschel Space Observatory	[ "Herschel" ]	facility	used	high	[]	2016A&A...595A..83E
[O I] 63 um	[ "[O I] 63 μm" ]	concept	subject	high	[ { "is_quantitative": true, "text": "The [O I] 63 um emission is detected in 6 out of 8 observed QSO sources." } ]	2016A&A...595A..83E
[C II] 158 um	[ "[C II] 158 μm", "[C II]" ]	concept	subject	high	[ { "is_quantitative": true, "text": "The [C II] 158 um emission is detected in 8 out of 9 observed QSO sources." } ]	2016A&A...595A..83E
W0752+19	[]	object	subject	high	[ { "is_quantitative": true, "text": "Shows an additional broad velocity component (~720 km s^-1) and exceptionally strong [O I] 63 um emission with L_[OI]63um/L_FIR of 10^-2." }, { "is_quantitative": true, "text": "The gas with broad velocity width in W0752+19 has n_H >= 10^4.3 cm^-3 and G_0 > 10...	2016A&A...595A..83E
Sloan Digital Sky Survey	[ "SDSS" ]	survey	used	medium	[]	2016A&A...595A..83E
ULIRGs	[ "local ULIRGs", "local (U)LIRGs" ]	concept	compared	medium	[]	2016A&A...595A..83E
ammonia	[ "14NH3", "15NH3", "ammonia isotopomers" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The hyperfine structure of the rotation-inversion (v2 = 0+, 0-, 1+, 1-) states of 14NH3 and 15NH3 is rationalized in terms of effective hyperfine-structure functions." }, { "is_quantitative": false, "text": "The deperturbed band centers of ammonia can serve a...	2016AJ....152...83L
effective hyperfine-structure functions	[ "hfs functions" ]	method	subject	high	[ { "is_quantitative": false, "text": "The hfs functions are determined by fitting to available experimental data using Hougen's effective hyperfine-structure Hamiltonian within the framework of the non-rigid inverter theory." }, { "is_quantitative": false, "text": "The fitted hfs functions involv...	2016AJ....152...83L
Hougen's effective hyperfine-structure Hamiltonian	[]	method	used	medium	[]	2016AJ....152...83L
non-rigid inverter theory	[]	method	used	medium	[]	2016AJ....152...83L
proton-to-electron mass ratio	[]	concept	mentioned	low	[]	2016AJ....152...83L
atmospheric depth of the shower maximum	[ "X_max", "X<sub>max</sub>" ]	concept	subject	high	[ { "is_quantitative": false, "text": "X_max is strongly correlated with the mass of the primary cosmic ray because it depends on the interaction cross section of the primary with atmospheric constituents." }, { "is_quantitative": true, "text": "X_max can be reconstructed using radio signal amplit...	2017JCAP...01..027C
Auger Engineering Radio Array	[ "AERA" ]	facility	used	high	[ { "is_quantitative": true, "text": "AERA measures the electric field emitted by secondary particles of extensive air showers in the 30-80 MHz band." } ]	2017JCAP...01..027C
cosmic-ray mass composition	[]	concept	subject	medium	[ { "is_quantitative": true, "text": "The statistical determination of the cosmic-ray mass composition is possible through the study of a large number of cosmic rays above 10^17 eV using radio detectors with a duty cycle close to 100%." } ]	2017JCAP...01..027C
scalar-tensor theories of gravity	[ "ST theories", "ST" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The parameter space of scalar-tensor theories of gravity can be constrained by the stability properties of highly compact, massive neutron stars." }, { "is_quantitative": false, "text": "Observations of the most massive neutron stars support a bound on the ST...	2016PhRvD..94d4062O
neutron stars	[ "compact stars", "stars" ]	concept	subject	high	[ { "is_quantitative": false, "text": "Highly compact neutron stars in scalar-tensor gravity can become unstable, with the instability driving the stars to collapse in some cases." } ]	2016PhRvD..94d4062O
general relativity	[]	concept	compared	low	[]	2016PhRvD..94d4062O
magnetic flux ropes	[ "MFR", "MFRs" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The closed quasi-separatrix layer (QSL) structure surrounding the MFR becomes smaller as a consequence of flare occurrence." }, { "is_quantitative": false, "text": "The twist number of the MFR varies more sensitively than other parameters with the occurrence ...	2016ApJ...827L..27P
active region 12017	[ "AR 12017" ]	object	subject	high	[ { "is_quantitative": true, "text": "AR 12017 triggered 12 flares from 2014 March 28-29 due to intermittent eruptions of a filament." }, { "is_quantitative": false, "text": "Flares in AR 12017 during 2014 March 28-29 were mainly triggered by kink instability." } ]	2016ApJ...827L..27P
Helioseismic and Magnetic Imager	[ "HMI" ]	facility	used	medium	[]	2016ApJ...827L..27P
Solar Dynamics Observatory	[ "SDO" ]	facility	used	low	[]	2016ApJ...827L..27P
nonlinear force-free field model	[ "NLFFF" ]	method	used	medium	[]	2016ApJ...827L..27P
kink instability	[]	concept	subject	medium	[ { "is_quantitative": false, "text": "Kink instability is found to be the main trigger for the 12 flares observed in AR 12017 from 2014 March 28-29." } ]	2016ApJ...827L..27P
PHENIX experiment	[ "PHENIX" ]	facility	used	high	[ { "is_quantitative": true, "text": "The PHENIX experiment measured the cumulants (C_n, n=1,...,4) of net-charge distributions within pseudorapidity \|η\| < 0.35 in Au+Au collisions at center-of-mass energies of 7.7 to 200 GeV." } ]	2016MNRAS.461.4505J
net-charge multiplicity distributions	[ "net-charge distributions" ]	concept	subject	high	[ { "is_quantitative": false, "text": "The ratios of cumulants (C_1/C_2, C_3/C_1) of the net-charge distributions are well described by expectations from negative binomial distributions." }, { "is_quantitative": true, "text": "No nonmonotonic behavior is observed in the ratios of the cumulants of ...	2016MNRAS.461.4505J
Relativistic Heavy Ion Collider	[ "RHIC" ]	facility	used	medium	[]	2016MNRAS.461.4505J
lattice quantum-chromodynamics	[ "lattice QCD" ]	method	compared	medium	[ { "is_quantitative": false, "text": "The measured values of C_1/C_2 and C_3/C_1 can be directly compared to lattice quantum-chromodynamics calculations to extract the chemical freeze-out temperature and baryon chemical potential." } ]	2016MNRAS.461.4505J
thermal-statistical analysis model	[]	method	compared	medium	[ { "is_quantitative": false, "text": "The extracted baryon chemical potentials from the net-charge cumulants are in excellent agreement with a thermal-statistical analysis model." } ]	2016MNRAS.461.4505J
1H 0323+342	[]	object	subject	high	[ { "is_quantitative": true, "text": "The Hbeta emission line in 1H 0323+342 has a delayed response of 14.8_{-2.7}^{+3.9} days with respect to the SDSS g' light curve in the rest frame." }, { "is_quantitative": true, "text": "The optical Fe II variations in 1H 0323+342 show a reverberation delay o...	2016ARep...60..563S
Lijiang 2.4 m Telescope	[]	facility	used	medium	[ { "is_quantitative": false, "text": "Used to monitor 1H 0323+342 for more than two months." } ]	2016ARep...60..563S
SDSS g'	[]	survey	used	low	[]	2016ARep...60..563S
Magorrian relation	[]	concept	compared	low	[ { "is_quantitative": true, "text": "Predicts a black hole mass for 1H 0323+342 that is one order of magnitude larger than the reverberation mapping mass." } ]	2016ARep...60..563S
compressed sensing	[]	method	subject	high	[ { "is_quantitative": false, "text": "Compressed sensing techniques are modified to be compatible with the Gaussian process framework for fast, simultaneous multi-planet radial velocity searches." }, { "is_quantitative": false, "text": "The compressed sensing method produces a periodogram-like ou...	2017MNRAS.465..997C
Gaussian process	[]	method	used	high	[ { "is_quantitative": false, "text": "Gaussian processes are integrated with compressed sensing techniques to model radial velocity data." } ]	2017MNRAS.465..997C
Lomb-Scargle periodogram	[]	method	compared	medium	[ { "is_quantitative": false, "text": "The proposed compressed sensing tool has a similar aspect to the Lomb-Scargle periodogram but exhibits fewer peaks due to aliasing." } ]	2017MNRAS.465..997C
HD 69830	[]	object	subject	medium	[ { "is_quantitative": false, "text": "Analysis of HD 69830 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." } ]	2017MNRAS.465..997C
HD 10180	[]	object	subject	medium	[ { "is_quantitative": false, "text": "Analysis of HD 10180 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." } ]	2017MNRAS.465..997C
55 Cnc	[]	object	subject	high	[ { "is_quantitative": false, "text": "Analysis of 55 Cnc radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." }, { "is_quantitative": false, "text": "55 Cnc e and f could have been respectively detected and suspected in early measuremen...	2017MNRAS.465..997C
GJ 876	[]	object	subject	high	[ { "is_quantitative": false, "text": "Analysis of GJ 876 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." }, { "is_quantitative": false, "text": "Frequencies due to dynamical interactions in GJ 876 can be resolved using the compress...	2017MNRAS.465..997C
Lick Observatory	[]	facility	used	low	[]	2017MNRAS.465..997C
Hobby-Eberly Telescope	[]	facility	used	low	[]	2017MNRAS.465..997C
Epsilon Eridani	[]	object	subject	high	[ { "is_quantitative": false, "text": "Simultaneous ground-based radial velocity and space-based photometric measurements were obtained to explore methods of distinguishing stellar photospheric velocities from Keplerian motion." } ]	2016ApJ...830...84K
Dalmatian	[]	software	subject	medium	[ { "is_quantitative": false, "text": "Dalmatian is an MCMC spot modeling code that fits photometric and RV measurements simultaneously." } ]	2016ApJ...830...84K
FF' method	[]	method	subject	medium	[ { "is_quantitative": false, "text": "The FF' method uses photometric measurements to predict the stellar activity signal in simultaneous RV measurements." } ]	2016ApJ...830...84K
HH' method	[]	method	subject	high	[ { "is_quantitative": false, "text": "The HH' method is a new technique that uses H-alpha measurements as input into the FF' model to predict stellar activity signals." } ]	2016ApJ...830...84K
Microvariability and Oscillations of STars telescope	[ "MOST" ]	facility	used	medium	[ { "is_quantitative": false, "text": "MOST photometry of Epsilon Eridani is strongly correlated with simultaneous ground-based H-alpha measurements." } ]	2016ApJ...830...84K
COSMOS J100054.83+023126.2	[]	object	subject	high	[ { "is_quantitative": true, "text": "COSMOS J100054.83+023126.2 is detected in H I 21 cm emission at z = 0.376, representing the highest redshift H I emission detection to date." }, { "is_quantitative": true, "text": "The total H I mass of the galaxy is (2.9 \u0000 1.0) \u0000 10^10 M_sun." }, ...	2016A&A...594A..74C
COSMOS H I Large Extragalactic Survey	[ "CHILES" ]	survey	used	high	[ { "is_quantitative": true, "text": "CHILES is designed to simultaneously observe H I from z = 0 to z ~ 0.5." }, { "is_quantitative": true, "text": "The first 178 hr of CHILES data were used to detect H I emission in a galaxy at z = 0.376." } ]	2016A&A...594A..74C
Karl G. Jansky Very Large Array	[ "VLA" ]	facility	used	medium	[]	2016A&A...594A..74C
Large Millimeter Telescope	[ "LMT" ]	facility	used	medium	[]	2016A&A...594A..74C
TorPeDO	[ "dual torsion pendulum sensor" ]	facility	subject	high	[ { "is_quantitative": false, "text": "TorPeDO is a dual torsion pendulum sensor designed to measure local gravitational forces to high precision and explore low-frequency gravitational-force noise." }, { "is_quantitative": true, "text": "The sensor features two torsion pendulums with a common sus...	2016JKAS...49..137H
Newtonian Noise	[]	concept	mentioned	medium	[]	2016JKAS...49..137H
gravitational wave detectors	[]	facility	mentioned	low	[]	2016JKAS...49..137H
sunward-propagating Alfvénic fluctuations	[ "SAFs" ]	concept	subject	high	[ { "is_quantitative": true, "text": "The percentage of SAFs increases gradually with heliocentric distance, from about 2.7% at 1.0 au to about 8.7% at 5.5 au." }, { "is_quantitative": false, "text": "SAFs can occur in the anti-sunward magnetic sector with a strong positive correlation between mag...	2016ApJ...831..133H
anti-sunward-propagating Alfvénic fluctuations	[ "AFs" ]	concept	mentioned	low	[]	2016ApJ...831..133H
Voyager 2	[]	facility	used	high	[ { "is_quantitative": false, "text": "Voyager 2 measurements inside 6 au were used to identify and statistically analyze sunward-propagating Alfvénic fluctuations." } ]	2016ApJ...831..133H
Wind	[]	facility	used	high	[ { "is_quantitative": false, "text": "Wind spacecraft measurements were used to analyze sunward-propagating Alfvénic fluctuations at 1 au." } ]	2016ApJ...831..133H
FRB 150418	[]	object	subject	high	[ { "is_quantitative": false, "text": "The reported radio counterpart of FRB 150418 is consistent with scintillating radio emission from a compact active galactic nucleus, which would invalidate its association with the FRB." } ]	2016ApJ...828...98R
interstellar scintillation	[ "refractive scintillation" ]	concept	subject	high	[ { "is_quantitative": false, "text": "Refractive scintillation in the ionized interstellar medium of the Milky Way can explain the observed 5.5 and 7.5 GHz variability of the putative FRB 150418 counterpart." } ]	2016ApJ...828...98R
active galactic nucleus	[ "AGN" ]	concept	subject	medium	[ { "is_quantitative": true, "text": "The putative counterpart of FRB 150418 is consistent with a radio-loud AGN having a brightness temperature T_b >= 10^9 K." } ]	2016ApJ...828...98R
VISTA Variables in Via Lactea	[ "VVV" ]	survey	used	high	[ { "is_quantitative": false, "text": "The VVV survey database is used to measure proper motions in the densest regions of the Milky Way bulge and southern plane." } ]	2017MNRAS.468.1123S
Two Micron All Sky Survey	[ "2MASS" ]	survey	used	medium	[ { "is_quantitative": false, "text": "The large time baseline between 2MASS and VVV observations is utilized to obtain 2MASS-VVV proper motions." } ]	2017MNRAS.468.1123S
VVV high proper motion stars catalogue	[]	dataset	subject	high	[ { "is_quantitative": true, "text": "The catalogue includes 3003 moving stellar sources with Ks <= 13.5 in the VVV survey area." }, { "is_quantitative": false, "text": "The catalogue is in very good agreement with proper motion data supplied in IR catalogues outside the densest zone of the Milky ...	2017MNRAS.468.1123S
M-dwarfs	[]	concept	subject	medium	[ { "is_quantitative": false, "text": "The majority of the proper motion objects in the VVV high proper motion catalogue are nearby M-dwarfs." } ]	2017MNRAS.468.1123S
common proper motion binary candidates	[]	concept	subject	medium	[ { "is_quantitative": true, "text": "57 common proper motion binary candidates are identified, including two new systems within 30 pc of the Sun." } ]	2017MNRAS.468.1123S
GALactic Archeology with Hermes	[ "GALAH" ]	survey	subject	high	[ { "is_quantitative": true, "text": "The GALAH survey targets 1 million stars brighter than magnitude V = 14 at a resolution of 28 000 with a goal to measure the abundances of 29 elements." }, { "is_quantitative": true, "text": "GALAH data quality exhibits fibre cross-talk levels of ≲0.5 per cent...	2017MNRAS.465.4026B
HERMES	[]	facility	used	medium	[ { "is_quantitative": true, "text": "HERMES is a fibre-fed, multi-object spectrograph mounted on the 3.9-m Anglo-Australian Telescope." } ]	2017MNRAS.465.4026B
Anglo-Australian Telescope	[ "AAT" ]	facility	used	low	[]	2017MNRAS.465.4026B
IRAF	[]	software	used	medium	[ { "is_quantitative": false, "text": "The GALAH reduction pipeline is built using existing IRAF routines to ensure simple maintenance and reliability." } ]	2017MNRAS.465.4026B
GALAH reduction pipeline	[]	software	subject	high	[ { "is_quantitative": false, "text": "The pipeline is optimized for speed, accuracy, and consistency to produce fully calibrated spectra for subsequent stellar atmospheric parameter estimation." } ]	2017MNRAS.465.4026B
Higgs boson	[ "H" ]	concept	subject	high	[ { "is_quantitative": true, "text": "For a Higgs boson with a mass of 125 GeV, the upper bound on the branching fraction of H to invisible particles is set to 0.28 at 95% confidence level, assuming the Standard Model production cross section." } ]	2016A&A...593A.130H
ATLAS detector	[ "ATLAS" ]	facility	used	high	[ { "is_quantitative": true, "text": "Recorded 20.3 fb^{-1} of proton-proton collision data at a centre-of-mass energy of 8 TeV at the LHC." } ]	2016A&A...593A.130H
Higgs-portal dark matter	[]	concept	subject	medium	[ { "is_quantitative": false, "text": "The branching fraction limit of H to invisible particles is converted into upper bounds on the dark-matter-nucleon scattering cross section as a function of the dark-matter particle mass." } ]	2016A&A...593A.130H
LHC	[]	facility	used	low	[]	2016A&A...593A.130H
star-forming galaxies	[ "SFGs" ]	concept	subject	high	[ { "is_quantitative": true, "text": "Massive star-forming galaxies at z = 2.2-2.5 commonly exhibit extremely compact dust emission with R_1/2,870 μm < 1.5 kpc, which is more than a factor of 2 smaller than their rest-optical sizes." }, { "is_quantitative": true, "text": "These galaxies have high ...	2017AcA....67...51R
Atacama Large Millimeter/submillimeter Array	[ "ALMA" ]	facility	used	medium	[]	2017AcA....67...51R
quiescent galaxies	[]	concept	compared	medium	[ { "is_quantitative": false, "text": "The rest-frame far-infrared sizes of massive star-forming galaxies at z = 2.2-2.5 are comparable with the optical sizes of massive quiescent galaxies at similar redshifts." } ]	2017AcA....67...51R

212Po

[ "polonium-212" ]

object

subject

high

[ { "is_quantitative": false, "text": "The alpha-decay width of 212Po is calculated using a quartetting wave function approach and agrees fairly well with the measured value." }, { "is_quantitative": false, "text": "The alpha-cluster preformation probability and alpha-decay width of 212Po are micr...

2016MNRAS.461.4335A

quartetting wave function approach

[ "quartetting" ]

method

subject

high

[ { "is_quantitative": false, "text": "The quartetting wave function approach is improved by implementing four-nucleon correlations to describe alpha preformation in 212Po." } ]

2016MNRAS.461.4335A

208Pb

[ "lead-208" ]

object

used

medium

[ { "is_quantitative": false, "text": "The measured density distribution of the 208Pb core is used to calculate the alpha-decay width of 212Po." } ]

2016MNRAS.461.4335A

Ponos

[ "Ponos zoom-in numerical simulations" ]

simulation

subject

high

[ { "is_quantitative": true, "text": "The Ponos simulations model dark matter substructures in massive elliptical galaxy halos with virial masses of 1.2 !x 10^{13} M_sun and 6.5 !x 10^{12} M_sun down to z = 0." }, { "is_quantitative": true, "text": "The simulations resolve halos with up to 921,651...

2016A&A...594A..93C

dark matter substructures

[ "subhalos" ]

concept

subject

high

[ { "is_quantitative": true, "text": "Subhalos with M_sub < 10^9 M_sun contribute between one-fifth and one-third of the total projected mass fraction in massive elliptical halos." }, { "is_quantitative": false, "text": "Baryonic contraction increases the number of massive subhalos in the inner re...

2016A&A...594A..93C

baryonic contraction

[]

concept

subject

medium

[ { "is_quantitative": false, "text": "Baryonic contraction produces a super-isothermal total density profile and increases the number of massive subhalos in the inner regions of the main host." } ]

2016A&A...594A..93C

gravitational lenses

[]

concept

compared

low

[ { "is_quantitative": false, "text": "The host density profiles and projected subhalo mass fractions from the Ponos simulations are broadly consistent with observations of gravitational lenses." } ]

2016A&A...594A..93C

Auger Engineering Radio Array

[ "AERA" ]

facility

subject

high

[ { "is_quantitative": true, "text": "AERA consists of more than 150 autonomous radio stations with different spacings, covering an area of about 17 km^2." }, { "is_quantitative": true, "text": "AERA detects radio emission from extensive air showers with energies beyond 10^17 eV in the 30 - 80 MHz...

2017JCoPh.330..566S

Pierre Auger Cosmic-Ray Observatory

[ "Auger Observatory" ]

facility

used

medium

[]

2017JCoPh.330..566S

Auger surface detector

[]

facility

used

medium

[ { "is_quantitative": false, "text": "The Auger surface detector is used to cross-calibrate AERA's radio radiation energy measurements to establish cosmic-ray energy scales." } ]

2017JCoPh.330..566S

radiation energy

[]

concept

subject

high

[ { "is_quantitative": false, "text": "The radiation energy emitted by air showers in the form of radio emission is measured and calibrated against the cosmic-ray energy scale." } ]

2017JCoPh.330..566S

lattice field theory methods

[ "lattice methods" ]

method

subject

high

[ { "is_quantitative": false, "text": "Lattice field theory methods are increasingly applied to calculate ground-state and thermal properties of strongly interacting non-relativistic few- and many-body systems." } ]

2013Icar..223..460S

hybrid Monte Carlo

[]

method

subject

medium

[ { "is_quantitative": false, "text": "Hybrid Monte Carlo techniques have recently crossed over from quantum chromodynamics to condensed matter, atomic, and low-energy nuclear physics." } ]

2013Icar..223..460S

improved effective actions

[]

method

subject

medium

[ { "is_quantitative": false, "text": "Improved effective actions have recently been applied to non-relativistic strongly interacting many-body systems." } ]

2013Icar..223..460S

fermions in the limit of unitarity

[]

concept

subject

medium

[ { "is_quantitative": false, "text": "Lattice methods are used to determine the ground- and excited-state properties of fermions in the limit of unitarity." } ]

2013Icar..223..460S

intragroup medium

[ "intragroup" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The intragroup medium has lower entropy levels and different radial profiles compared to the intracluster medium due to weakly supersonic gas inflow and less effective conversion of kinetic to thermal energy." } ]

2016ApJ...830..141L

intracluster medium

[ "intracluster" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The intracluster medium experiences highly supersonic gas inflow across the system boundary, leading to strong accretion shocks and substantial conversion of bulk kinetic into thermal energy." } ]

2016ApJ...830..141L

ESO 3060170

[]

object

subject

medium

[ { "is_quantitative": false, "text": "X-ray observations of the galaxy group ESO 3060170 out to its virial radius show entropy profiles that match theoretical expectations of starved inflow in low-redshift or poor environments." } ]

2016ApJ...830..141L

RXJ1159+5531

[]

object

subject

medium

[ { "is_quantitative": false, "text": "X-ray observations of the galaxy group RXJ1159+5531 out to its virial radius show entropy profiles that match theoretical expectations of starved inflow in low-redshift or poor environments." } ]

2016ApJ...830..141L

iron nanoparticles

[ "metallic iron nanoparticles", "iron clusters", "ultrasmall iron clusters" ]

concept

subject

high

[ { "is_quantitative": true, "text": "Iron nanoparticles are stable against sublimation in the interstellar radiation field down to a radius of ≃4.5 Å, and potentially smaller." }, { "is_quantitative": false, "text": "Iron nanoparticles can acquire negative charges, particularly in interstellar en...

2017AdSpR..59..736B

photoelectric heating

[ "photoelectric heating rate" ]

concept

subject

medium

[ { "is_quantitative": true, "text": "The photoelectric heating rate from dust may be increased by up to tens of percent if ≳10% of interstellar iron is in the form of ultrasmall iron clusters." } ]

2017AdSpR..59..736B

interstellar dust

[ "dust" ]

concept

mentioned

low

[]

2017AdSpR..59..736B

QSOs

[ "QSO" ]

concept

subject

high

[ { "is_quantitative": true, "text": "The host galaxies of nine QSOs at 0.1 < z < 0.2 have black hole masses of 3x10^7 M_sun to 3x10^9 M_sun and far-infrared luminosities of ~ several times 10^11 L_sun." }, { "is_quantitative": true, "text": "The observed L_[OI]63um/L_FIR and L_[CII]/L_FIR ratios ...

2016A&A...595A..83E

Herschel Space Observatory

[ "Herschel" ]

facility

used

high

[]

2016A&A...595A..83E

[O I] 63 um

[ "[O I] 63 μm" ]

concept

subject

high

[ { "is_quantitative": true, "text": "The [O I] 63 um emission is detected in 6 out of 8 observed QSO sources." } ]

2016A&A...595A..83E

[C II] 158 um

[ "[C II] 158 μm", "[C II]" ]

concept

subject

high

[ { "is_quantitative": true, "text": "The [C II] 158 um emission is detected in 8 out of 9 observed QSO sources." } ]

2016A&A...595A..83E

W0752+19

[]

object

subject

high

[ { "is_quantitative": true, "text": "Shows an additional broad velocity component (~720 km s^-1) and exceptionally strong [O I] 63 um emission with L_[OI]63um/L_FIR of 10^-2." }, { "is_quantitative": true, "text": "The gas with broad velocity width in W0752+19 has n_H >= 10^4.3 cm^-3 and G_0 > 10...

2016A&A...595A..83E

Sloan Digital Sky Survey

[ "SDSS" ]

survey

used

medium

[]

2016A&A...595A..83E

ULIRGs

[ "local ULIRGs", "local (U)LIRGs" ]

concept

compared

medium

[]

2016A&A...595A..83E

ammonia

[ "14NH3", "15NH3", "ammonia isotopomers" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The hyperfine structure of the rotation-inversion (v2 = 0+, 0-, 1+, 1-) states of 14NH3 and 15NH3 is rationalized in terms of effective hyperfine-structure functions." }, { "is_quantitative": false, "text": "The deperturbed band centers of ammonia can serve a...

2016AJ....152...83L

effective hyperfine-structure functions

[ "hfs functions" ]

method

subject

high

[ { "is_quantitative": false, "text": "The hfs functions are determined by fitting to available experimental data using Hougen's effective hyperfine-structure Hamiltonian within the framework of the non-rigid inverter theory." }, { "is_quantitative": false, "text": "The fitted hfs functions involv...

2016AJ....152...83L

Hougen's effective hyperfine-structure Hamiltonian

[]

method

used

medium

[]

2016AJ....152...83L

non-rigid inverter theory

[]

method

used

medium

[]

2016AJ....152...83L

proton-to-electron mass ratio

[]

concept

mentioned

low

[]

2016AJ....152...83L

atmospheric depth of the shower maximum

[ "X_max", "X<sub>max</sub>" ]

concept

subject

high

[ { "is_quantitative": false, "text": "X_max is strongly correlated with the mass of the primary cosmic ray because it depends on the interaction cross section of the primary with atmospheric constituents." }, { "is_quantitative": true, "text": "X_max can be reconstructed using radio signal amplit...

2017JCAP...01..027C

Auger Engineering Radio Array

[ "AERA" ]

facility

used

high

[ { "is_quantitative": true, "text": "AERA measures the electric field emitted by secondary particles of extensive air showers in the 30-80 MHz band." } ]

2017JCAP...01..027C

cosmic-ray mass composition

[]

concept

subject

medium

[ { "is_quantitative": true, "text": "The statistical determination of the cosmic-ray mass composition is possible through the study of a large number of cosmic rays above 10^17 eV using radio detectors with a duty cycle close to 100%." } ]

2017JCAP...01..027C

scalar-tensor theories of gravity

[ "ST theories", "ST" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The parameter space of scalar-tensor theories of gravity can be constrained by the stability properties of highly compact, massive neutron stars." }, { "is_quantitative": false, "text": "Observations of the most massive neutron stars support a bound on the ST...

2016PhRvD..94d4062O

neutron stars

[ "compact stars", "stars" ]

concept

subject

high

[ { "is_quantitative": false, "text": "Highly compact neutron stars in scalar-tensor gravity can become unstable, with the instability driving the stars to collapse in some cases." } ]

2016PhRvD..94d4062O

general relativity

[]

concept

compared

low

[]

2016PhRvD..94d4062O

magnetic flux ropes

[ "MFR", "MFRs" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The closed quasi-separatrix layer (QSL) structure surrounding the MFR becomes smaller as a consequence of flare occurrence." }, { "is_quantitative": false, "text": "The twist number of the MFR varies more sensitively than other parameters with the occurrence ...

2016ApJ...827L..27P

active region 12017

[ "AR 12017" ]

object

subject

high

[ { "is_quantitative": true, "text": "AR 12017 triggered 12 flares from 2014 March 28-29 due to intermittent eruptions of a filament." }, { "is_quantitative": false, "text": "Flares in AR 12017 during 2014 March 28-29 were mainly triggered by kink instability." } ]

2016ApJ...827L..27P

Helioseismic and Magnetic Imager

[ "HMI" ]

facility

used

medium

[]

2016ApJ...827L..27P

Solar Dynamics Observatory

[ "SDO" ]

facility

used

low

[]

2016ApJ...827L..27P

nonlinear force-free field model

[ "NLFFF" ]

method

used

medium

[]

2016ApJ...827L..27P

kink instability

[]

concept

subject

medium

[ { "is_quantitative": false, "text": "Kink instability is found to be the main trigger for the 12 flares observed in AR 12017 from 2014 March 28-29." } ]

2016ApJ...827L..27P

PHENIX experiment

[ "PHENIX" ]

facility

used

high

[ { "is_quantitative": true, "text": "The PHENIX experiment measured the cumulants (C_n, n=1,...,4) of net-charge distributions within pseudorapidity |η| < 0.35 in Au+Au collisions at center-of-mass energies of 7.7 to 200 GeV." } ]

2016MNRAS.461.4505J

net-charge multiplicity distributions

[ "net-charge distributions" ]

concept

subject

high

[ { "is_quantitative": false, "text": "The ratios of cumulants (C_1/C_2, C_3/C_1) of the net-charge distributions are well described by expectations from negative binomial distributions." }, { "is_quantitative": true, "text": "No nonmonotonic behavior is observed in the ratios of the cumulants of ...

2016MNRAS.461.4505J

Relativistic Heavy Ion Collider

[ "RHIC" ]

facility

used

medium

[]

2016MNRAS.461.4505J

lattice quantum-chromodynamics

[ "lattice QCD" ]

method

compared

medium

[ { "is_quantitative": false, "text": "The measured values of C_1/C_2 and C_3/C_1 can be directly compared to lattice quantum-chromodynamics calculations to extract the chemical freeze-out temperature and baryon chemical potential." } ]

2016MNRAS.461.4505J

thermal-statistical analysis model

[]

method

compared

medium

[ { "is_quantitative": false, "text": "The extracted baryon chemical potentials from the net-charge cumulants are in excellent agreement with a thermal-statistical analysis model." } ]

2016MNRAS.461.4505J

1H 0323+342

[]

object

subject

high

[ { "is_quantitative": true, "text": "The Hbeta emission line in 1H 0323+342 has a delayed response of 14.8_{-2.7}^{+3.9} days with respect to the SDSS g' light curve in the rest frame." }, { "is_quantitative": true, "text": "The optical Fe II variations in 1H 0323+342 show a reverberation delay o...

2016ARep...60..563S

Lijiang 2.4 m Telescope

[]

facility

used

medium

[ { "is_quantitative": false, "text": "Used to monitor 1H 0323+342 for more than two months." } ]

2016ARep...60..563S

SDSS g'

[]

survey

used

low

[]

2016ARep...60..563S

Magorrian relation

[]

concept

compared

low

[ { "is_quantitative": true, "text": "Predicts a black hole mass for 1H 0323+342 that is one order of magnitude larger than the reverberation mapping mass." } ]

2016ARep...60..563S

compressed sensing

[]

method

subject

high

[ { "is_quantitative": false, "text": "Compressed sensing techniques are modified to be compatible with the Gaussian process framework for fast, simultaneous multi-planet radial velocity searches." }, { "is_quantitative": false, "text": "The compressed sensing method produces a periodogram-like ou...

2017MNRAS.465..997C

Gaussian process

[]

method

used

high

[ { "is_quantitative": false, "text": "Gaussian processes are integrated with compressed sensing techniques to model radial velocity data." } ]

2017MNRAS.465..997C

Lomb-Scargle periodogram

[]

method

compared

medium

[ { "is_quantitative": false, "text": "The proposed compressed sensing tool has a similar aspect to the Lomb-Scargle periodogram but exhibits fewer peaks due to aliasing." } ]

2017MNRAS.465..997C

HD 69830

[]

object

subject

medium

[ { "is_quantitative": false, "text": "Analysis of HD 69830 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." } ]

2017MNRAS.465..997C

HD 10180

[]

object

subject

medium

[ { "is_quantitative": false, "text": "Analysis of HD 10180 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." } ]

2017MNRAS.465..997C

55 Cnc

[]

object

subject

high

[ { "is_quantitative": false, "text": "Analysis of 55 Cnc radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." }, { "is_quantitative": false, "text": "55 Cnc e and f could have been respectively detected and suspected in early measuremen...

2017MNRAS.465..997C

GJ 876

[]

object

subject

high

[ { "is_quantitative": false, "text": "Analysis of GJ 876 radial velocity data using the compressed sensing method yields results fully compatible with previous analyses." }, { "is_quantitative": false, "text": "Frequencies due to dynamical interactions in GJ 876 can be resolved using the compress...

2017MNRAS.465..997C

Lick Observatory

[]

facility

used

low

[]

2017MNRAS.465..997C

Hobby-Eberly Telescope

[]

facility

used

low

[]

2017MNRAS.465..997C

Epsilon Eridani

[]

object

subject

high

[ { "is_quantitative": false, "text": "Simultaneous ground-based radial velocity and space-based photometric measurements were obtained to explore methods of distinguishing stellar photospheric velocities from Keplerian motion." } ]

2016ApJ...830...84K

Dalmatian

[]

software

subject

medium

[ { "is_quantitative": false, "text": "Dalmatian is an MCMC spot modeling code that fits photometric and RV measurements simultaneously." } ]

2016ApJ...830...84K

FF' method

[]

method

subject

medium

[ { "is_quantitative": false, "text": "The FF' method uses photometric measurements to predict the stellar activity signal in simultaneous RV measurements." } ]

2016ApJ...830...84K

HH' method

[]

method

subject

high

[ { "is_quantitative": false, "text": "The HH' method is a new technique that uses H-alpha measurements as input into the FF' model to predict stellar activity signals." } ]

2016ApJ...830...84K

Microvariability and Oscillations of STars telescope

[ "MOST" ]

facility

used

medium

[ { "is_quantitative": false, "text": "MOST photometry of Epsilon Eridani is strongly correlated with simultaneous ground-based H-alpha measurements." } ]

2016ApJ...830...84K

COSMOS J100054.83+023126.2

[]

object

subject

high

[ { "is_quantitative": true, "text": "COSMOS J100054.83+023126.2 is detected in H I 21 cm emission at z = 0.376, representing the highest redshift H I emission detection to date." }, { "is_quantitative": true, "text": "The total H I mass of the galaxy is (2.9 \u0000 1.0) \u0000 10^10 M_sun." }, ...

2016A&A...594A..74C

COSMOS H I Large Extragalactic Survey

[ "CHILES" ]

survey

used

high

[ { "is_quantitative": true, "text": "CHILES is designed to simultaneously observe H I from z = 0 to z ~ 0.5." }, { "is_quantitative": true, "text": "The first 178 hr of CHILES data were used to detect H I emission in a galaxy at z = 0.376." } ]

2016A&A...594A..74C

Karl G. Jansky Very Large Array

[ "VLA" ]

facility

used

medium

[]

2016A&A...594A..74C

Large Millimeter Telescope

[ "LMT" ]

facility

used

medium

[]

2016A&A...594A..74C

TorPeDO

[ "dual torsion pendulum sensor" ]

facility

subject

high

[ { "is_quantitative": false, "text": "TorPeDO is a dual torsion pendulum sensor designed to measure local gravitational forces to high precision and explore low-frequency gravitational-force noise." }, { "is_quantitative": true, "text": "The sensor features two torsion pendulums with a common sus...

2016JKAS...49..137H

Newtonian Noise

[]

concept

mentioned

medium

[]

2016JKAS...49..137H

gravitational wave detectors

[]

facility

mentioned

low

[]

2016JKAS...49..137H

sunward-propagating Alfvénic fluctuations

[ "SAFs" ]

concept

subject

high

[ { "is_quantitative": true, "text": "The percentage of SAFs increases gradually with heliocentric distance, from about 2.7% at 1.0 au to about 8.7% at 5.5 au." }, { "is_quantitative": false, "text": "SAFs can occur in the anti-sunward magnetic sector with a strong positive correlation between mag...

2016ApJ...831..133H

anti-sunward-propagating Alfvénic fluctuations

[ "AFs" ]

concept

mentioned

low

[]

2016ApJ...831..133H

Voyager 2

[]

facility

used

high

[ { "is_quantitative": false, "text": "Voyager 2 measurements inside 6 au were used to identify and statistically analyze sunward-propagating Alfvénic fluctuations." } ]

2016ApJ...831..133H

Wind

[]

facility

used

high

[ { "is_quantitative": false, "text": "Wind spacecraft measurements were used to analyze sunward-propagating Alfvénic fluctuations at 1 au." } ]

2016ApJ...831..133H

FRB 150418

[]

object

subject

high

[ { "is_quantitative": false, "text": "The reported radio counterpart of FRB 150418 is consistent with scintillating radio emission from a compact active galactic nucleus, which would invalidate its association with the FRB." } ]

2016ApJ...828...98R

interstellar scintillation

[ "refractive scintillation" ]

concept

subject

high

[ { "is_quantitative": false, "text": "Refractive scintillation in the ionized interstellar medium of the Milky Way can explain the observed 5.5 and 7.5 GHz variability of the putative FRB 150418 counterpart." } ]

2016ApJ...828...98R

active galactic nucleus

[ "AGN" ]

concept

subject

medium

[ { "is_quantitative": true, "text": "The putative counterpart of FRB 150418 is consistent with a radio-loud AGN having a brightness temperature T_b >= 10^9 K." } ]

2016ApJ...828...98R

VISTA Variables in Via Lactea

[ "VVV" ]

survey

used

high

[ { "is_quantitative": false, "text": "The VVV survey database is used to measure proper motions in the densest regions of the Milky Way bulge and southern plane." } ]

2017MNRAS.468.1123S

Two Micron All Sky Survey

[ "2MASS" ]

survey

used

medium

[ { "is_quantitative": false, "text": "The large time baseline between 2MASS and VVV observations is utilized to obtain 2MASS-VVV proper motions." } ]

2017MNRAS.468.1123S

VVV high proper motion stars catalogue

[]

dataset

subject

high

[ { "is_quantitative": true, "text": "The catalogue includes 3003 moving stellar sources with Ks <= 13.5 in the VVV survey area." }, { "is_quantitative": false, "text": "The catalogue is in very good agreement with proper motion data supplied in IR catalogues outside the densest zone of the Milky ...

2017MNRAS.468.1123S

M-dwarfs

[]

concept

subject

medium

[ { "is_quantitative": false, "text": "The majority of the proper motion objects in the VVV high proper motion catalogue are nearby M-dwarfs." } ]

2017MNRAS.468.1123S

common proper motion binary candidates

[]

concept

subject

medium

[ { "is_quantitative": true, "text": "57 common proper motion binary candidates are identified, including two new systems within 30 pc of the Sun." } ]

2017MNRAS.468.1123S

GALactic Archeology with Hermes

[ "GALAH" ]

survey

subject

high

[ { "is_quantitative": true, "text": "The GALAH survey targets 1 million stars brighter than magnitude V = 14 at a resolution of 28 000 with a goal to measure the abundances of 29 elements." }, { "is_quantitative": true, "text": "GALAH data quality exhibits fibre cross-talk levels of ≲0.5 per cent...

2017MNRAS.465.4026B

HERMES

[]

facility

used

medium

[ { "is_quantitative": true, "text": "HERMES is a fibre-fed, multi-object spectrograph mounted on the 3.9-m Anglo-Australian Telescope." } ]

2017MNRAS.465.4026B

Anglo-Australian Telescope

[ "AAT" ]

facility

used

low

[]

2017MNRAS.465.4026B

IRAF

[]

software

used

medium

[ { "is_quantitative": false, "text": "The GALAH reduction pipeline is built using existing IRAF routines to ensure simple maintenance and reliability." } ]

2017MNRAS.465.4026B

GALAH reduction pipeline

[]

software

subject

high

[ { "is_quantitative": false, "text": "The pipeline is optimized for speed, accuracy, and consistency to produce fully calibrated spectra for subsequent stellar atmospheric parameter estimation." } ]

2017MNRAS.465.4026B

Higgs boson

[ "H" ]

concept

subject

high

[ { "is_quantitative": true, "text": "For a Higgs boson with a mass of 125 GeV, the upper bound on the branching fraction of H to invisible particles is set to 0.28 at 95% confidence level, assuming the Standard Model production cross section." } ]

2016A&A...593A.130H

ATLAS detector

[ "ATLAS" ]

facility

used

high

[ { "is_quantitative": true, "text": "Recorded 20.3 fb^{-1} of proton-proton collision data at a centre-of-mass energy of 8 TeV at the LHC." } ]

2016A&A...593A.130H

Higgs-portal dark matter

[]

concept

subject

medium

[ { "is_quantitative": false, "text": "The branching fraction limit of H to invisible particles is converted into upper bounds on the dark-matter-nucleon scattering cross section as a function of the dark-matter particle mass." } ]

2016A&A...593A.130H

LHC

[]

facility

used

low

[]

2016A&A...593A.130H

star-forming galaxies

[ "SFGs" ]

concept

subject

high

[ { "is_quantitative": true, "text": "Massive star-forming galaxies at z = 2.2-2.5 commonly exhibit extremely compact dust emission with R_1/2,870 μm < 1.5 kpc, which is more than a factor of 2 smaller than their rest-optical sizes." }, { "is_quantitative": true, "text": "These galaxies have high ...

2017AcA....67...51R

Atacama Large Millimeter/submillimeter Array

[ "ALMA" ]

facility

used

medium

[]

2017AcA....67...51R

quiescent galaxies

[]

concept

compared

medium

[ { "is_quantitative": false, "text": "The rest-frame far-infrared sizes of massive star-forming galaxies at z = 2.2-2.5 are comparable with the optical sizes of massive quiescent galaxies at similar redshifts." } ]

2017AcA....67...51R