Search Publications

CMB anomalies and the effects of local features of the inflaton potential
DOI: 10.1140/epjc/s10052-017-4797-6 Bibcode: 2017EPJC...77..242C

Gariazzo, Stefano; Cadavid, Alexander Gallego; Romano, Antonio Enea

Recent analysis of the WMAP and Planck data have shown the presence of a dip and a bump in the spectrum of primordial perturbations at the scales k=0.002 Mpc

2017 European Physical Journal C
Planck 19
An Active Galactic Nucleus Caught in the Act of Turning Off and On
DOI: 10.3847/1538-4357/aa8e4b Bibcode: 2017ApJ...849..102C

Greene, Jenny E.; Stern, Daniel; Comerford, Julia M. +5 more

We present the discovery of an active galactic nucleus (AGN) that is turning off and then on again in the z = 0.06 galaxy SDSS J1354+1327. This episodic nuclear activity is the result of discrete accretion events that could have been triggered by a past interaction with the companion galaxy that is currently located 12.5 kpc away. We originally ta…

2017 The Astrophysical Journal
eHST 19
Are Internetwork Magnetic Fields in the Solar Photosphere Horizontal or Vertical?
DOI: 10.3847/1538-4357/835/1/14 Bibcode: 2017ApJ...835...14L

Lites, B. W.; Borrero, J. M.; Danilovic, S. +1 more

Using many observations obtained during 2007 with the Spectro-Polarimeter of the Hinode Solar Optical Telescope, we explore the angular distribution of magnetic fields in the quiet internetwork regions of the solar photosphere. Our work follows from the insight of Stenflo, who examined only linear polarization signals in photospheric lines, thereb…

2017 The Astrophysical Journal
Hinode 19
KELT-18b: Puffy Planet, Hot Host, Probably Perturbed
DOI: 10.3847/1538-3881/aa6d5d Bibcode: 2017AJ....153..263M

Bieryla, Allyson; Latham, David W.; Berlind, Perry +54 more

We report the discovery of KELT-18b, a transiting hot Jupiter in a 2.87-day orbit around the bright (V = 10.1), hot, F4V star BD+60 1538 (TYC 3865-1173-1). We present follow-up photometry, spectroscopy, and adaptive optics imaging that allow a detailed characterization of the system. Our preferred model fits yield a host stellar temperature of 667…

2017 The Astronomical Journal
Gaia 19
Mars Under Primordial Solar Wind Conditions: Mars Express Observations of the Strongest CME Detected at Mars Under Solar Cycle #24 and its Impact on Atmospheric Ion Escape
DOI: 10.1002/2017GL075446 Bibcode: 2017GeoRL..4410805R

Barabash, Stas; Nilsson, Hans; Holmström, Mats +3 more

An extremely strong Coronal Mass Ejection (CME) impacted Mars on 12 July 2011, while the Mars Express spacecraft was present inside the nightside ionosphere. Estimated solar wind density and speed during the event are 39 particles cm-3 and 730 km/s, corresponding to nominal solar wind flux at Mars when the solar system was ∼1.1 Ga old. …

2017 Geophysical Research Letters
MEx 19
X-ray flaring in PDS 456 observed in a high-flux state
DOI: 10.1093/mnras/stw2673 Bibcode: 2017MNRAS.465.2804M

Turner, T. J.; Reeves, J. N.; Braito, V. +3 more

We present an analysis of a 190 ks (net exposure) Suzaku observation, carried out in 2007, of the nearby (z = 0.184) luminous (Lbol ∼ 1047 erg s-1) quasar PDS 456. In this observation, the intrinsically steep bare continuum is revealed compared to subsequent observations, carried out in 2011 and 2013, where the sou…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 19
HADES RV Programme with HARPS-N at TNG. VI. GJ 3942 b behind dominant activity signals
DOI: 10.1051/0004-6361/201731307 Bibcode: 2017A&A...608A..63P

Rebolo, R.; Ribas, I.; Morales, J. C. +29 more

Context. Short- to mid-term magnetic phenomena on the stellar surface of M-type stars can resemble the effects of planets in radial velocity data, and may also hide them.
Aims: We analyze 145 spectroscopic HARPS-N observations of GJ 3942 taken over the past five years and additional photometry in order to disentangle stellar activity effects …

2017 Astronomy and Astrophysics
Gaia 19
XMM-Newton observation of MV Lyr and the sandwiched model confirmation
DOI: 10.1093/mnras/stx513 Bibcode: 2017MNRAS.468.1183D

Ness, J. -U.; Dobrotka, A.; Nucita, A. A. +1 more

We present spectral and timing analyses of simultaneous X-ray and UV observations of the VY Scl system MV Lyr taken by XMM-Newton, containing the longest continuous X-ray + UV light curve and highest signal-to-noise X-ray (EPIC) spectrum to date. The RGS spectrum displays emission lines plus continuum, confirming model approaches to be based on th…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
HD 164492C: a rapidly rotating, Hα-bright, magnetic early B star associated with a 12.5 d spectroscopic binary
DOI: 10.1093/mnras/stw2799 Bibcode: 2017MNRAS.465.2517W

Rivinius, Th.; Wade, G. A.; Alecian, E. +6 more

We employ high-resolution spectroscopy and spectropolarimetry to derive the physical properties and magnetic characteristics of the multiple system HD 164492C, located in the young open cluster M20. The spectrum reveals evidence of three components: a broad-lined early B star (HD 164492C1), a narrow-lined early B star (HD 164492C2) and a late B st…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 19
D/H Ratios on Saturn and Jupiter from Cassini CIRS
DOI: 10.3847/1538-3881/aa899d Bibcode: 2017AJ....154..178P

Fletcher, L. N.; Lellouch, E.; Irwin, P. G. J. +7 more

We present new measurements of the deuterium abundance on Jupiter and Saturn, showing evidence that Saturn's atmosphere contains less deuterium than Jupiter's. We analyzed far-infrared spectra from the Cassini Composite Infrared Spectrometer to measure the abundance of HD on both giant planets. Our estimate of the Jovian D/H = (2.95 ± 0.55) × 10

2017 The Astronomical Journal
ISO 19