Search Publications

Old but Still Warm: Far-UV Detection of PSR B0950+08
DOI: 10.3847/1538-4357/aa947c Bibcode: 2017ApJ...850...79P

Pavlov, G. G.; Guillot, S.; Kargaltsev, O. +3 more

We report on a Hubble Space Telescope detection of the nearby, old pulsar B0950+08 (d≃ 262 pc, spin-down age 17.5 Myr) in two far-ultraviolet (FUV) bands. We measured the mean flux densities {\bar{f}}ν =109+/- 6 nJy and 83 ± 14 nJy in the F125LP and F140LP filters (pivot wavelengths 1438 and 1528 Å). Using the FUV data together with pre…

2017 The Astrophysical Journal
eHST 36
The nearby Type Ibn supernova 2015G: signatures of asymmetry and progenitor constraints
DOI: 10.1093/mnras/stx1885 Bibcode: 2017MNRAS.471.4381S

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Wood-Vasey, W. Michael +24 more

We present the results of an extensive observational campaign on the nearby Type Ibn SN 2015G, including data from radio through ultraviolet wavelengths. SN 2015G was asymmetric, showing late-time nebular lines redshifted by ∼1000 km s-1. It shared many features with the prototypical SN Ibn 2006jc, including extremely strong He I emissi…

2017 Monthly Notices of the Royal Astronomical Society
eHST 36
A Catalog of Stellar Unified Properties (CATSUP) for 951 FGK-Stars within 30 pc
DOI: 10.3847/1538-4357/aa8b0f Bibcode: 2017ApJ...848...34H

Smith, Graeme H.; Shkolnik, Evgenya L.; Somers, Garrett +6 more

Almost every star in our Galaxy is likely to harbor a terrestrial planet, but accurate measurements of an exoplanet’s mass and radius demand accurate knowledge of the properties of its host star. The imminent TESS and CHEOPS missions are slated to discover thousands of new exoplanets. Along with WFIRST, which will directly image nearby planets, th…

2017 The Astrophysical Journal
Gaia XMM-Newton 36
Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems
DOI: 10.1093/mnras/stx154 Bibcode: 2017MNRAS.467.1714T

Smalley, Barry; Hellier, Coel; Triaud, Amaury H. M. J. +16 more

We report the detection of two new systems containing transiting planets. Both were identified by WASP as worthy transiting planet candidates. Radial velocity observations quickly verified that the photometric signals were indeed produced by two transiting hot Jupiters. Our observations also show the presence of additional Doppler signals. In addi…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 36
MC2: Subaru and Hubble Space Telescope Weak-lensing Analysis of the Double Radio Relic Galaxy Cluster PLCK G287.0+32.9
DOI: 10.3847/1538-4357/aa998c Bibcode: 2017ApJ...851...46F

Koekemoer, Anton M.; Seitz, Stella; Gruen, Daniel +6 more

The second most significant detection of the Planck Sunyaev-Zel’dovich survey, PLCK G287.0+32.9 (z = 0.385), boasts two similarly bright radio relics and a radio halo. One radio relic is located ∼ 400 {kpc} NW of the X-ray peak and the other ∼ 2.8 Mpc to the SE. This large difference suggests that a complex merging scenario is required. A key miss…

2017 The Astrophysical Journal
Planck eHST 36
Detection of a Hydrogen Corona in HST Lyα Images of Europa in Transit of Jupiter
DOI: 10.3847/1538-3881/153/2/67 Bibcode: 2017AJ....153...67R

Roth, Lorenz; Strobel, Darrell F.; Becker, Tracy M. +4 more

We report far-ultraviolet observations of Europa in transit of Jupiter obtained with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope on six occasions between 2014 December and 2015 March. Absorption of Jupiter’s bright hydrogen Lyα dayglow is detected in a region several moon radii above the limb in all observations. The obs…

2017 The Astronomical Journal
eHST 36
Thermally anomalous features in the subsurface of Enceladus's south polar terrain
DOI: 10.1038/s41550-017-0063 Bibcode: 2017NatAs...1E..63L

Sotin, C.; Lorenz, R. D.; West, R. D. +15 more

Saturn's moon Enceladus is an active world. In 2005, the Cassini spacecraft witnessed for the first time water-rich jets venting from four anomalously warm fractures (called sulci) near its south pole1,2. Since then, several observations have provided evidence that the source of the material ejected from Enceladus is a large underground…

2017 Nature Astronomy
Cassini 36
Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110+6459. II. What is Missed at the Normal Resolution of the Hubble Space Telescope?
DOI: 10.3847/1538-4357/aa775e Bibcode: 2017ApJ...843...79R

Rigby, J. R.; Sharon, K.; Gladders, M. D. +6 more

For lensed galaxy SGAS J111020.0+645950.8 at redshift z = 2.481, which is magnified by a factor of 28 ± 8, we analyze the morphology of star formation, as traced by rest-frame ultraviolet emission, in both the highly magnified source plane and simulations of how this galaxy would appear without lensing magnification. Were this galaxy not lensed, b…

2017 The Astrophysical Journal
eHST 35
Milky Way Tomography with K and M Dwarf Stars: The Vertical Structure of the Galactic Disk
DOI: 10.3847/1538-4357/aa77fd Bibcode: 2017ApJ...843..141F

Yanny, Brian; Ferguson, Deborah; Gardner, Susan

We use the number density distributions of K and M dwarf stars with vertical height from the Galactic disk, determined using observations from the Sloan Digital Sky Survey, to probe the structure of the Milky Way disk across the survey’s footprint. Using photometric parallax as a distance estimator we analyze a sample of several million disk stars…

2017 The Astrophysical Journal
Gaia 35
A dichotomy between the hard state spectral properties of black hole and neutron star X-ray binaries
DOI: 10.1093/mnras/stw2514 Bibcode: 2017MNRAS.466..194B

Sunyaev, R.; Gilfanov, M.; Burke, M. J.

We analyse the spectra of black hole (BH) and neutron star (NS) X-ray binaries (XBs) in the hard state using archival RXTE observations. We find that there is a clear dichotomy in the strength of Comptonization between NS and BH sources, as measured by both the Compton y-parameter and the amplification factor A, with distinct groups of BH and NS X…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 35