Search Publications

Measurements of Photospheric and Chromospheric Magnetic Fields
DOI: 10.1007/s11214-015-0219-y Bibcode: 2017SSRv..210...37L

Gosain, Sanjay; Lagg, Andreas; Lites, Bruce +2 more

The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active regions, magnetic fields are ubiquitous. To a large extent, their importance for the thermodynamics in the solar photosphere is determined by the total magnetic flux. W…

2017 Space Science Reviews
Hinode SOHO 55
New constraints on the average escape fraction of Lyman continuum radiation in z 4 galaxies from the VIMOS Ultra Deep Survey (VUDS)
DOI: 10.1051/0004-6361/201630054 Bibcode: 2017A&A...601A..73M

Maccagni, D.; Schaerer, D.; Thomas, R. +20 more

Context. Determining the average fraction of Lyman continuum (LyC) photons escaping high redshift galaxies is essential for understanding how reionization proceeded in the z> 6 Universe.
Aims: We want to measure the LyC signal from a sample of sources in the Chandra Deep Field South (CDFS) and COSMOS fields for which ultra-deep VIMOS spect…

2017 Astronomy and Astrophysics
eHST 55
Probing the intra-group medium of a z = 0.28 galaxy group
DOI: 10.1093/mnras/stx528 Bibcode: 2017MNRAS.468.1373B

Tejos, N.; Morris, S. L.; Cantalupo, S. +4 more

We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightline passes between multiple z = 0.28 galaxies, whilst showing at the same redshift low-ionized metal line species, including Ca II, Mg I, Mg II and Fe II. Based on the galaxy redshifts measured from the MUSE data, we estimate the galaxies to be part …

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
Astrometric Calibration and Performance of the Dark Energy Camera
DOI: 10.1088/1538-3873/aa6c55 Bibcode: 2017PASP..129g4503B

Benoit-Lévy, A.; Bechtol, K.; Smith, M. +54 more

We characterize the ability of the Dark Energy Camera (DECam) to perform relative astrometry across its 500 Mpix, 3-deg2 science field of view and across four years of operation. This is done using internal comparisons of ∼4 × 107 measurements of high signal-to-noise ratio stellar images obtained in repeat visits to fields of…

2017 Publications of the Astronomical Society of the Pacific
Gaia 55
Major mergers are not significant drivers of star formation or morphological transformation around the epoch of peak cosmic star formation
DOI: 10.1093/mnras/stw2895 Bibcode: 2017MNRAS.465.2895L

Conselice, C. J.; Hartley, W.; Mortlock, A. +2 more

We investigate the contribution of major mergers (mass ratios >1: 5) to stellar mass growth and morphological transformations around the epoch of peak cosmic star formation (z ∼ 2). We visually classify a complete sample of massive (M > 1010M) galaxies at this epoch, drawn from the Cosmic Assembly Near-infrared Deep Ex…

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
Modeling the Historical Flux of Planetary Impactors
DOI: 10.3847/1538-3881/153/3/103 Bibcode: 2017AJ....153..103N

Nesvorný, David; Roig, Fernando; Bottke, William F.

The impact cratering record of the Moon and the terrestrial planets provides important clues about the formation and evolution of the solar system. Especially intriguing is the epoch ≃3.8-3.9 Gyr ago (Ga), known as the Late Heavy Bombardment (LHB), when the youngest lunar basins such as Imbrium and Orientale formed. The LHB was suggested to origin…

2017 The Astronomical Journal
AKARI 55
VoIgt profile Parameter Estimation Routine (viper): H I photoionization rate at z < 0.5
DOI: 10.1093/mnras/stx248 Bibcode: 2017MNRAS.467.3172G

Khaire, Vikram; Srianand, Raghunathan; Choudhury, Tirthankar Roy +1 more

We have developed a parallel code called the VoIgt profile Parameter Estimation Routine (viper) for automatically fitting the H I Lyα forest seen in the spectra of quasi-stellar objects (QSOs). We obtained the H I column density distribution function (CDDF) and linewidth (b) parameter distribution for z < 0.45 using spectra of 82 QSOs obtained …

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
Cosmic viscosity as a remedy for tension between PLANCK and LSS data
DOI: 10.1088/1475-7516/2017/11/005 Bibcode: 2017JCAP...11..005A

Anand, Sampurn; Chaubal, Prakrut; Mazumdar, Arindam +1 more

Measurements of σ8 from large scale structure observations show a discordance with the extrapolated σ8 from Planck CMB parameters using ΛCDM cosmology. Similar discordance is found in the value of H0 and Ωm. In this paper, we show that the presence of viscosity, shear or bulk or combination of both, can …

2017 Journal of Cosmology and Astroparticle Physics
Planck 54
Elongation of Flare Ribbons
DOI: 10.3847/1538-4357/aa6341 Bibcode: 2017ApJ...838...17Q

Qiu, Jiong; Longcope, Dana W.; Cassak, Paul A. +1 more

We present an analysis of the apparent elongation motion of flare ribbons along the polarity inversion line (PIL), as well as the shear of flare loops in several two-ribbon flares. Flare ribbons and loops spread along the PIL at a speed ranging from a few to a hundred km s-1. The shear measured from conjugate footpoints is consistent wi…

2017 The Astrophysical Journal
SOHO 54
Different Origins or Different Evolutions? Decoding the Spectral Diversity Among C-type Asteroids
DOI: 10.3847/1538-3881/153/2/72 Bibcode: 2017AJ....153...72V

Jorda, L.; Lamy, P.; Groussin, O. +15 more

Anhydrous pyroxene-rich interplanetary dust particles (IDPs) have been proposed as surface analogs for about two-thirds of all C-complex asteroids. However, this suggestion appears to be inconsistent with the presence of hydrated silicates on the surfaces of some of these asteroids, including Ceres. Here, we report the presence of enstatite (pyrox…

2017 The Astronomical Journal
ISO 54