Search Publications

New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies
DOI: 10.1093/mnras/stu2029 Bibcode: 2014MNRAS.445.4287T

Slemer, Alessandra; Girardi, Léo; Marigo, Paola +4 more

We extend the PARSEC library of stellar evolutionary tracks by computing new models of massive stars, from 14 to 350 M. The input physics is the same used in the PARSEC V1.1 version, but for the mass-loss rate from considering the most recent updates in the literature. We focus on low metallicity, Z = 0.001 and Z = 0.004, for which the…

2014 Monthly Notices of the Royal Astronomical Society
eHST 416
The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
DOI: 10.1093/mnras/stu1622 Bibcode: 2014MNRAS.444.2960D

Dickinson, M.; Ferguson, H. C.; Giavalisco, M. +16 more

We measure new estimates for the galaxy stellar mass function and star formation rates for samples of galaxies at z ∼ 4, 5, 6 and 7 using data in the CANDELS GOODS South field. The deep near-infrared observations allow us to construct the stellar mass function at z ≥ 6 directly for the first time. We estimate stellar masses for our sample by fitti…

2014 Monthly Notices of the Royal Astronomical Society
eHST 273
Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies
DOI: 10.1093/mnras/stu1395 Bibcode: 2014MNRAS.444..268R

Richard, Johan; Kneib, Jean-Paul; Egami, Eiichi +9 more

Extending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the distant Universe via gravitational lensing by massive galaxy clusters. Here, we present models of the mass distribution in the six HFF cluster lenses, derived from a joi…

2014 Monthly Notices of the Royal Astronomical Society
eHST 206
Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7
DOI: 10.1093/mnras/stu1618 Bibcode: 2014MNRAS.445.3200S

Charlot, Stéphane; Richard, Johan; Siana, Brian +8 more

We present deep spectroscopy of 17 very low mass (M ≃ 2.0 × 106-1.4 × 109 M) and low luminosity (MUV ≃ -13.7 to -19.9) gravitationally lensed galaxies in the redshift range z ≃ 1.5-3.0. Deep rest-frame ultraviolet spectra reveal large equivalent width emission from numerous emission lines (N…

2014 Monthly Notices of the Royal Astronomical Society
eHST 204
Inference of the cold dark matter substructure mass function at z = 0.2 using strong gravitational lenses
DOI: 10.1093/mnras/stu943 Bibcode: 2014MNRAS.442.2017V

Vegetti, S.; Treu, T.; Auger, M. W. +2 more

We present the results of a search for galaxy substructures in a sample of 11 gravitational lens galaxies from the Sloan Lens ACS Survey by Bolton et al. We find no significant detection of mass clumps, except for a luminous satellite in the system SDSS J0956+5110. We use these non-detections, in combination with a previous detection in the system…

2014 Monthly Notices of the Royal Astronomical Society
eHST 188
The bright end of the galaxy luminosity function at z≃7: before the onset of mass quenching?
DOI: 10.1093/mnras/stu449 Bibcode: 2014MNRAS.440.2810B

Taniguchi, Y.; Bowler, R. A. A.; McLure, R. J. +9 more

We present the results of a new search for bright star-forming galaxies at redshift z ≃ 7 within the UltraVISTA second data release (DR2) and UKIDSS (UKIRT Infrared Deep Sky Survey) UDS (Ultra Deep Survey) DR10 data, which together provide 1.65 deg2 of near-infrared imaging with overlapping optical and Spitzer data. Using a full photome…

2014 Monthly Notices of the Royal Astronomical Society
eHST 188
MUSE sneaks a peek at extreme ram-pressure stripping events - I. A kinematic study of the archetypal galaxy ESO137-001
DOI: 10.1093/mnras/stu2092 Bibcode: 2014MNRAS.445.4335F

Fumagalli, Michele; Fossati, Matteo; Sun, Ming +4 more

We present Multi Unit Spectroscopic Explorer (MUSE) observations of ESO137-001, a spiral galaxy infalling towards the centre of the massive Norma cluster at z ∼ 0.0162. During the high-velocity encounter of ESO137-001 with the intracluster medium, a dramatic ram-pressure stripping event gives rise to an extended gaseous tail, traced by our MUSE ob…

2014 Monthly Notices of the Royal Astronomical Society
eHST 180
The ATLAS3D Project - XXVIII. Dynamically driven star formation suppression in early-type galaxies
DOI: 10.1093/mnras/stu570 Bibcode: 2014MNRAS.444.3427D

Krajnović, Davor; Emsellem, Eric; Sarzi, Marc +22 more

We present measurements of the star formation rate (SFR) in the early-type galaxies (ETGs) of the ATLAS3D sample, based on Wide-field Infrared Survey Explorer (WISE) 22 µm and Galaxy Evolution Explorer far-ultraviolet emission. We combine these with gas masses estimated from 12CO and H I data in order to investigate the…

2014 Monthly Notices of the Royal Astronomical Society
eHST 174
The AIMSS Project - I. Bridging the star cluster-galaxy divide†‡§¶
DOI: 10.1093/mnras/stu1186 Bibcode: 2014MNRAS.443.1151N

Penny, Samantha J.; Forbes, Duncan A.; Romanowsky, Aaron J. +16 more

We describe the structural and kinematic properties of the first compact stellar systems discovered by the Archive of Intermediate Mass Stellar Systems project. These spectroscopically confirmed objects have sizes (∼6 < Re [pc] < 500) and masses (∼2 × 106 < M*/M < 6 × 109) spannin…

2014 Monthly Notices of the Royal Astronomical Society
eHST 160
Nuclear star clusters in 228 spiral galaxies in the HST/WFPC2 archive: catalogue and comparison to other stellar systems
DOI: 10.1093/mnras/stu797 Bibcode: 2014MNRAS.441.3570G

Böker, Torsten; Georgiev, Iskren Y.

We present a catalogue of photometric and structural properties of 228 nuclear star clusters (NSCs) in nearby late-type disc galaxies. These new measurements are derived from a homogeneous analysis of all suitable Wide Field Planetary Camera 2 (WFPC2) images in the Hubble Space Telescope (HST) archive. The luminosity and size of each NSC are deriv…

2014 Monthly Notices of the Royal Astronomical Society
eHST 153