Search Publications

Constraints on Non-flat Cosmologies with Massive Neutrinos after Planck 2015
DOI: 10.3847/0004-637X/829/2/61 Bibcode: 2016ApJ...829...61C

Ratra, Bharat; Chen, Yun; Biesiada, Marek +2 more

We investigate two dark energy cosmological models (I.e., the ΛCDM and ϕCDM models) with massive neutrinos assuming two different neutrino mass hierarchies in both the spatially flat and non-flat scenarios, where in the ϕCDM model the scalar field possesses an inverse power-law potential, V(ϕ) ∝ ϕ (α > 0). Cosmic microwave backgr…

2016 The Astrophysical Journal
Planck 74
Space Telescope and Optical Reverberation Mapping Project. IV. Anomalous Behavior of the Broad Ultraviolet Emission Lines in NGC 5548
DOI: 10.3847/0004-637X/824/1/11 Bibcode: 2016ApJ...824...11G

Im, M.; Geier, S.; Brandt, W. N. +98 more

During an intensive Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) UV monitoring campaign of the Seyfert 1 galaxy NGC 5548 performed from 2014 February to July, the normally highly correlated far UV continuum and broad emission line variations decorrelated for ∼60-70 days, starting ∼75 days after the first HST/COS observation. Foll…

2016 The Astrophysical Journal
IUE eHST 74
Low-metallicity Absorbers Account for Half of the Dense Circumgalactic Gas at z ≲ 1
DOI: 10.3847/0004-637X/831/1/95 Bibcode: 2016ApJ...831...95W

Prochaska, J. Xavier; Lehner, Nicolas; Howk, J. Christopher +2 more

We present an analysis of the metallicity distribution of the dense circumgalactic medium (CGM) of galaxies at 0.1 ≲ z ≲ 1.1 as probed by partial Lyman limit systems (pLLSs, 16.1 < log {N}{{H}{{I}}} < 17.2) and LLSs (17.2 ≤ log {N}{{H}{{I}}} < 17.7 in our sample). The new H I-selected sample, drawn from our Hubble Sp…

2016 The Astrophysical Journal
eHST 73
The BOSS Emission-line Lens Survey. III. Strong Lensing of Lyα Emitters by Individual Galaxies
DOI: 10.3847/0004-637X/824/2/86 Bibcode: 2016ApJ...824...86S

Brownstein, Joel R.; Marques-Chaves, Rui; Oguri, Masamune +8 more

We introduce the Baryon Oscillation Spectroscopic Survey (BOSS) Emission-Line Lens Survey GALaxy-Lyα EmitteR sYstems (BELLS GALLERY) Survey, which is a Hubble Space Telescope program to image a sample of galaxy-scale strong gravitational lens candidate systems with high-redshift Lyα emitters (LAEs) as the background sources. The goal of the BELLS …

2016 The Astrophysical Journal
eHST 73
First Observational Support for Overlapping Reionized Bubbles Generated by a Galaxy Overdensity
DOI: 10.3847/2041-8205/818/1/L3 Bibcode: 2016ApJ...818L...3C

Maiolino, R.; Dickinson, M.; Giavalisco, M. +21 more

We present an analysis of deep Hubble Space Telescope (HST) multi-band imaging of the BDF field specifically designed to identify faint companions around two of the few Lyα emitting galaxies spectroscopically confirmed at z ∼ 7. Although separated by only 4.4 proper Mpc these galaxies cannot generate H II regions large enough to explain the visibi…

2016 The Astrophysical Journal
eHST 73
Timing Observations of PSR J1023+0038 During a Low-mass X-Ray Binary State
DOI: 10.3847/0004-637X/830/2/122 Bibcode: 2016ApJ...830..122J

Deller, Adam T.; Bogdanov, Slavko; Hessels, Jason W. T. +5 more

Transitional millisecond pulsars (tMSPs) switch, on roughly multi-year timescales, between rotation-powered radio millisecond pulsar (RMSP) and accretion-powered low-mass X-ray binary (LMXB) states. The tMSPs have raised several questions related to the nature of accretion flow in their LMXB state and the mechanism that causes the state switch. Th…

2016 The Astrophysical Journal
XMM-Newton 73
Marginalizing Instrument Systematics in HST WFC3 Transit Light Curves
DOI: 10.3847/0004-637X/819/1/10 Bibcode: 2016ApJ...819...10W

Wakeford, H. R.; Sing, D. K.; Deming, D. +2 more

Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) infrared observations at 1.1-1.7 µm probe primarily the H2O absorption band at 1.4 µm, and have provided low-resolution transmission spectra for a wide range of exoplanets. We present the application of marginalization based on Gibson to analyze exoplanet transit light …

2016 The Astrophysical Journal
eHST 73
Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5 < z < 3
DOI: 10.3847/2041-8205/820/1/L1 Bibcode: 2016ApJ...820L...1K

Bell, Eric F.; Ferguson, Henry C.; Grogin, Norman A. +16 more

We present estimates of intrinsic scatter in the star formation rate (SFR)-stellar mass (M*) correlation in the redshift range 0.5< z< 3.0 and in the mass range {10}7< {M}*< {10}11M. We utilize photometry in the Hubble Ultradeep Field (HUDF12) and Ultraviolet Ultra Deep Field (UVU…

2016 The Astrophysical Journal
eHST 72
The Properties of the Circumgalactic Medium in Red and Blue Galaxies: Results from the COS-GASS+COS-Halos Surveys
DOI: 10.3847/1538-4357/833/2/259 Bibcode: 2016ApJ...833..259B

Heckman, Timothy; Saintonge, Amelie; Davé, Romeel +7 more

We use the combined data from the COS-GASS and COS-Halos surveys to characterize the Circum-Galactic Medium (CGM) surrounding typical low-redshift galaxies in the mass range {M}* ∼ {10}9.5-11.5 {M}, and over a range of impact parameters extending to just beyond the halo virial radius (R vir). We find t…

2016 The Astrophysical Journal
eHST 72
Proplyds Around a B1 Star: 42 Orionis in NGC 1977
DOI: 10.3847/2041-8205/826/1/L15 Bibcode: 2016ApJ...826L..15K

Fang, Min; Facchini, Stefano; Clarke, Cathie J. +1 more

We present the discovery of seven new proplyds (I.e., sources surrounded by cometary Hα emission characteristic of offset ionization fronts (IFs)) in NGC 1977, located about 30‧ north of the Orion Nebula Cluster (ONC) at a distance of ∼400 pc. Each of these proplyds is situated at projected distances 0.04-0.27 pc from the B1V star 42 Orionis (c Or…

2016 The Astrophysical Journal
eHST 71