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
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
Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts z ∼ 2.3-4.1
DOI: 10.3847/1538-4357/aaa3dc Bibcode: 2018ApJ...853..191S

Koekemoer, Anton M.; Inoue, Akio K.; Jiang, Linhua +9 more

We present observations of escaping Lyman Continuum (LyC) radiation from 34 massive star-forming galaxies (SFGs) and 12 weak AGN with reliably measured spectroscopic redshifts at z≃ 2.3{--}4.1. We analyzed Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) mosaics of the Early Release Science (ERS) field in three UVIS filters to sample the re…

2018 The Astrophysical Journal
eHST 32
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ∼ 4.5 [C II] Emitters
DOI: 10.3847/1538-4357/aac6ba Bibcode: 2018ApJ...861..100C

Thomson, A. P.; Scott, D.; Smail, Ian +18 more

We report the results of a search for serendipitous [C II] 157.74 µm emitters at z ≃ 4.4-4.7 using the Atacama Large Millimeter/submillimeter Array (ALMA). The search exploits the AS2UDS continuum survey, which covers ∼50 arcmin2 of the sky toward 695 luminous (S 870 ≳ 1 mJy) submillimeter galaxies (SMGs), selected from…

2018 The Astrophysical Journal
Herschel 32
A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu II and Zn II Lines
DOI: 10.3847/1538-4357/aab71f Bibcode: 2018ApJ...857....2R

Roederer, Ian U.; Barklem, Paul S.

We present new abundances derived from Cu I, Cu II, Zn I, and Zn II lines in six warm (5766 ≤ {T}eff} ≤ 6427 K), metal-poor (-2.50 ≤ [Fe/H] ≤ -0.95) dwarf and subgiant (3.64 ≤ log g ≤ 4.44) stars. These abundances are derived from archival high-resolution ultraviolet spectra from the Space Telescope Imaging Spectrograph on board the Hub…

2018 The Astrophysical Journal
Gaia eHST 32
A Non-thermal Pulsed X-Ray Emission of AR Scorpii
DOI: 10.3847/1538-4357/aaa23d Bibcode: 2018ApJ...853..106T

Cheng, K. S.; Takata, J.; Kong, A. K. H. +5 more

We report the analysis result of UV/X-ray emission from AR Scorpii, which is an intermediate polar (IP) composed of a magnetic white dwarf and an M-type star, with the XMM-Newton data. The X-ray/UV emission clearly shows a large variation over the orbit, and their intensity maximum (or minimum) is located at the superior conjunction (or inferior c…

2018 The Astrophysical Journal
XMM-Newton 32
The MASSIVE Survey. IX. Photometric Analysis of 35 High-mass Early-type Galaxies with HST WFC3/IR
DOI: 10.3847/1538-4357/aab1f3 Bibcode: 2018ApJ...856...11G

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +3 more

We present near-infrared observations of 35 of the most massive early-type galaxies in the local universe. The observations were made using the infrared channel of the Hubble Space Telescope Wide Field Camera 3 (WFC3) in the F110W (1.1 µm) filter. We measured surface brightness profiles and elliptical isophotal fit parameters from the nuclea…

2018 The Astrophysical Journal
eHST 32
Galaxy Mergers up to Z < 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3-15 kpc
DOI: 10.3847/1538-4357/aae847 Bibcode: 2018ApJ...868...46S

Brammer, Gabriel; Marchesini, Danilo; Tadaki, Ken-ichi +7 more

We present a study of the influence of galaxy mergers on star formation at 0.3 < z < 2.5. Major mergers are selected from the CANDELS/3D-HST catalog using a peak-finding algorithm. Mergers have projected galaxy nucleus separation of their members between 3 and 15 kpc. We compare the star formation activity in merging and nonmerging galaxies …

2018 The Astrophysical Journal
eHST 32