Search Publications

Far-UV HST Spectroscopy of an Unusual Hydrogen-poor Superluminous Supernova: SN2017egm
DOI: 10.3847/1538-4357/aabad5 Bibcode: 2018ApJ...858...91Y

Brown, P. J.; Quimby, R.; Lunnan, R. +4 more

SN2017egm is the closest (z = 0.03) H-poor superluminous supernova (SLSN-I) detected to date, and a rare example of an SLSN-I in a massive, metal-rich galaxy. We present the HST UV and optical spectra covering 1000-5500 Å, taken at +3 day relative to the peak. Our data reveal two absorption systems at redshifts matching the host galaxy NGC 3191 (z…

2018 The Astrophysical Journal
eHST 33
Progenitor Mass Distribution for Core-collapse Supernova Remnants in M31 and M33
DOI: 10.3847/1538-4357/aac6e1 Bibcode: 2018ApJ...861...92D

Dolphin, Andrew E.; Williams, Benjamin F.; Dalcanton, Julianne J. +3 more

Using the star formation histories (SFHs) near 94 supernova remnants (SNRs), we infer the progenitor mass distribution for core-collapse supernovae. We use Bayesian inference and model each SFH with multiple bursts of star formation (SF), one of which is assumed to be associated with the SNR. Assuming single-star evolution, the minimum mass of CCS…

2018 The Astrophysical Journal
eHST 33
The infrared-radio correlation of spheroid- and disc-dominated star-forming galaxies to z ∼ 1.5 in the COSMOS field
DOI: 10.1093/mnras/stx3234 Bibcode: 2018MNRAS.475..827M

Zamorani, Giovanni; Schinnerer, Eva; Murphy, Eric J. +14 more

Using infrared data from the Herschel Space Observatory and Karl G. Jansky Very Large Array 3 GHz observations in the COSMOS field, we investigate the redshift evolution of the infrared-radio correlation (IRRC) for star-forming galaxies (SFGs) we classify as either spheroid- or disc-dominated based on their morphology. The sample predominantly con…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 33
Host galaxies of SNe Ic-BL with and without long gamma-ray bursts
DOI: 10.1051/0004-6361/201833209 Bibcode: 2018A&A...617A.105J

Salvaterra, R.; Kaper, L.; Renzo, M. +5 more

Broad-line Ic supernovae (SNe Ic-BL) are a very rare class of core-collapse supernovae exhibiting high ejecta velocities and high kinetic energies. They are the only type of SNe that accompany long gamma-ray burst (GRB) explosions. Systematic differences found in the spectra of SNe Ic-BL with and without GRBs (GRB-SNe and SNe Ic-BL, respectively) …

2018 Astronomy and Astrophysics
eHST 33
Direct Imaging of the HD 35841 Debris Disk: A Polarized Dust Ring from Gemini Planet Imager and an Outer Halo from HST/STIS
DOI: 10.3847/1538-3881/aacbc9 Bibcode: 2018AJ....156...47E

Duchêne, Gaspard; Esposito, Thomas M.; Oppenheimer, Rebecca +55 more

We present new high resolution imaging of a light-scattering dust ring and halo around the young star HD 35841. Using spectroscopic and polarimetric data from the Gemini Planet Imager in H-band (1.6 µm), we detect the highly inclined (i = 85°) ring of debris down to a projected separation of ∼12 au (∼0.″12) for the first time. Optical imagin…

2018 The Astronomical Journal
Gaia eHST 33
Discovery of a Transiting Adolescent Sub-Neptune Exoplanet with K2
DOI: 10.3847/1538-3881/aaeed7 Bibcode: 2018AJ....156..302D

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +19 more

The role of stellar age in the measured properties and occurrence rates of exoplanets is not well understood. This is in part due to a paucity of known young planets and the uncertainties in age-dating for most exoplanet host stars. Exoplanets with well-constrained ages, particularly those which are young, are useful as benchmarks for studies aimi…

2018 The Astronomical Journal
Gaia 33
Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 ≲ z ≲ 1: inside-out stellar mass buildup and quenching
DOI: 10.1093/mnras/sty1771 Bibcode: 2018MNRAS.479.5083A

Abdurro'uf; Akiyama, Masayuki

We investigate a relation between surface densities of star formation rate (SFR) and stellar mass (M*) at a ∼1 kpc scale namely spatially resolved star formation main sequence (SFMS) in massive (log (M*/M) > 10.5) face-on disc galaxies at 0.01 < z < 0.02 and 0.8 < z < 1.8 and examine evolution of th…

2018 Monthly Notices of the Royal Astronomical Society
eHST 33
The envelope of the power spectra of over a thousand δ Scuti stars. The T̅eff - νmax scaling relation
DOI: 10.1051/0004-6361/201731803 Bibcode: 2018A&A...614A..46B

García, R. A.; Roca Cortés, T.; Barceló Forteza, S.

CoRoT and Kepler high-precision photometric data allowed the detection and characterization of the oscillation parameters in stars other than the Sun. Moreover, thanks to the scaling relations, it is possible to estimate masses and radii for thousands of solar-type oscillating stars. Recently, a Δν - ρ relation has been found for δ Scuti stars. No…

2018 Astronomy and Astrophysics
CoRoT 33
Upper Limits on the Presence of Central Massive Black Holes in Two Ultra-compact Dwarf Galaxies in Centaurus A
DOI: 10.3847/1538-4357/aabae5 Bibcode: 2018ApJ...858...20V

Romanowsky, Aaron J.; Neumayer, Nadine; Strader, Jay +10 more

The recent discovery of massive black holes (BHs) in the centers of high-mass ultra-compact dwarf galaxies (UCDs) suggests that at least some are the stripped nuclear star clusters of dwarf galaxies. We present the first study that investigates whether such massive BHs, and therefore stripped nuclei, also exist in low-mass (M < 107 M…

2018 The Astrophysical Journal
eHST 33
The Rest-frame Optical Sizes of Massive Galaxies with Suppressed Star Formation at z ∼ 4
DOI: 10.3847/1538-4357/aae3e8 Bibcode: 2018ApJ...867....1K

Toft, Sune; Kubo, Mariko; Tanaka, Masayuki +3 more

We present the rest-frame optical sizes of massive quiescent galaxies (QGs) at z ∼ 4 measured at the K‧-band with the Infrared Camera and Spectrograph and adaptive optics (AO) facility, AO188, on the Subaru telescope. Based on a deep multiwavelength catalog in the Subaru XMM-Newton Deep Survey Field, covering a wide wavelength range from the u-ban…

2018 The Astrophysical Journal
eHST 33