Search Publications

X-ray absorption towards high-redshift sources: probing the intergalactic medium with blazars
DOI: 10.1051/0004-6361/201732322 Bibcode: 2018A&A...616A.170A

Campana, S.; Ghisellini, G.; Salvaterra, R. +1 more

The role played by the intergalactic medium (IGM) in the X-ray absorption towards high-redshift sources has recently drawn more attention in spectral analysis studies. Here, we study the X-ray absorption towards 15 flat-spectrum radio quasars at z > 2, relying on high counting statistic (≳10 000 photons) provided by XMM-Newton, with additional …

2018 Astronomy and Astrophysics
XMM-Newton 24
Multi-epoch analysis of the X-ray spectrum of the active galactic nucleus in NGC 5506
DOI: 10.1093/mnras/sty1233 Bibcode: 2018MNRAS.478.1900S

Ni, Qingling; Bambi, Cosimo; Guainazzi, Matteo +5 more

We present a multi-epoch X-ray spectroscopy analysis of the nearby narrow-line Seyfert I galaxy NGC 5506. For the first time, spectra taken by Chandra, XMM-Newton, Suzaku, and NuSTAR- covering the 2000-2014 time span - are analysed simultaneously, using state-of-the-art models to describe reprocessing of the primary continuum by optical thick matt…

2018 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 24
HST imaging of four gravitationally lensed quasars
DOI: 10.1093/mnras/sty1793 Bibcode: 2018MNRAS.479.4796B

King, A. L.; Barone-Nugent, R. L.; Bate, N. F. +7 more

We present new Hubble Space Telescope WFC3 imaging of four gravitationally lensed quasars: MG 0414+0534; RXJ 0911+0551; B 1422+231; WFI J2026-4536. In three of these systems we detect wavelength-dependent microlensing, which we use to place constraints on the sizes and temperature profiles of the accretion discs in each quasar. Accretion disc radi…

2018 Monthly Notices of the Royal Astronomical Society
eHST 24
The Second Data Release of the Beijing-Arizona Sky Survey
DOI: 10.3847/1538-4365/aad502 Bibcode: 2018ApJS..237...37Z

Myers, Adam D.; Fan, Xiaohui; Jiang, Linhua +29 more

This paper describes the second data release (DR2) of the Beijing-Arizona Sky Survey (BASS). BASS is an imaging survey covering a 5400 deg2 footprint in the g and r bands using the 2.3 m Bok telescope. DR2 includes the observations through 2017 July obtained by BASS and by the Mayall z-band Legacy Survey (MzLS), which used the 4 m Mayal…

2018 The Astrophysical Journal Supplement Series
Gaia 24
A direct measure of free electron gas via the kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
DOI: 10.1093/mnras/stx3362 Bibcode: 2018MNRAS.475.3764S

Spergel, David N.; Okumura, Teppei; Sugiyama, Naonori S.

We present the measurement of the kinematic Sunyaev-Zel'dovich (kSZ) effect in Fourier space, rather than in real space. We measure the density-weighted pairwise kSZ power spectrum, the first use of this promising approach, by cross-correlating a cleaned cosmic microwave background (CMB) temperature map, which jointly uses both Planck Release 2 an…

2018 Monthly Notices of the Royal Astronomical Society
Planck 24
An explanation for the gap in the Gaia HRD for M dwarfs
DOI: 10.1093/mnras/sty1888 Bibcode: 2018MNRAS.480.1711M

Gizis, John; MacDonald, James

We show that the recently discovered narrow gap in the Gaia Hertzsprung-Russell Diagram near MG = 10 can be explained by standard stellar evolution models and results from a dip in the luminosity function associated with mixing of 3He during merger of envelope and core convection zones that occurs for a narrow range of masses.

2018 Monthly Notices of the Royal Astronomical Society
Gaia 24
A Solar Stationary Type IV Radio Burst and Its Radiation Mechanism
DOI: 10.1007/s11207-018-1280-y Bibcode: 2018SoPh..293...58L

Koval, Artem; Chen, Yao; Feng, Shiwei +6 more

A stationary Type IV (IVs) radio burst was observed on September 24, 2011. Observations from the Nançay RadioHeliograph (NRH) show that the brightness temperature (TB) of this burst is extremely high, over 1011 K at 150 MHz and over 108 K in general. The degree of circular polarization (q ) is between −60 % ∼−100 %…

2018 Solar Physics
SOHO 23
Discovery of an Extremely Luminous Dust-obscured Galaxy Observed with SDSS, WISE, JCMT, and SMA
DOI: 10.3847/1538-4357/aab3cf Bibcode: 2018ApJ...857...31T

Ueda, Junko; Kawabe, Ryohei; Saito, Toshiki +5 more

We present the discovery of an extremely luminous dust-obscured galaxy (DOG) at z spec = 3.703, WISE J101326.25+611220.1. This DOG is selected as a candidate of extremely luminous infrared (IR) galaxies based on the photometry from the Sloan Digital Sky Survey and Wide-field Infrared Survey Explorer. In order to derive its accurate IR l…

2018 The Astrophysical Journal
AKARI 23
Gaia DR2 view of the Lupus V-VI clouds: The candidate diskless young stellar objects are mainly background contaminants
DOI: 10.1051/0004-6361/201833383 Bibcode: 2018A&A...615L...1M

Prusti, T.; Fedele, D.; Alcalá, J. M. +10 more

Extensive surveys of star-forming regions with Spitzer have revealed populations of disk-bearing young stellar objects. These have provided crucial constraints, such as the timescale of dispersal of protoplanetary disks, obtained by carefully combining infrared data with spectroscopic or X-ray data. While observations in various regions agree with…

2018 Astronomy and Astrophysics
Gaia 23
Comparison of Dust Impact and Solitary Wave Signatures Detected by Multiple Electric Field Antennas Onboard the MMS Spacecraft
DOI: 10.1029/2018JA025380 Bibcode: 2018JGRA..123.6119V

Mann, Ingrid; Vaverka, Jakub; Pellinen-Wannberg, Asta +6 more

Dust impact detection by electric field instruments is a relatively new method. However, the influence of dust impacts on electric field measurements is not completely understood and explained. A better understanding is very important for reliable dust impact identification, especially in environments with low dust impact rate. Using data from Ear…

2018 Journal of Geophysical Research (Space Physics)
Cluster 23