Search Publications

MC2: Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster
DOI: 10.3847/1538-4357/aa667f Bibcode: 2017ApJ...838..110G

Dawson, William A.; Jee, M. James; van Weeren, Reinout J. +2 more

We present and analyze a rich data set including Subaru/SuprimeCam, HST/Advanced Camera for Surveys and Wide Field Camera 3, Keck/DEIMOS, Chandra/ACIS-I, and JVLA/C and D array for the merging cluster of galaxies ZwCl 0008.8+5215. With a joint Subaru+HST weak gravitational lensing analysis, we identify two dominant subclusters and estimate the mas…

2017 The Astrophysical Journal
eHST 37
Constraining the ΛCDM and Galileon models with recent cosmological data
DOI: 10.1051/0004-6361/201628878 Bibcode: 2017A&A...600A..40N

Möller, A.; Astier, P.; Guy, J. +4 more


Aims: The Galileon theory belongs to the class of modified gravity models that can explain the late-time accelerated expansion of the Universe. In previous works, cosmological constraints on the Galileon model were derived, both in the uncoupled case and with a disformal coupling of the Galileon field to matter. There, we showed that these mo…

2017 Astronomy and Astrophysics
Planck 37
IRIS Burst Spectra Co-spatial to a Quiet-Sun Ellerman-like Brightening
DOI: 10.3847/1538-4357/aa7e7a Bibcode: 2017ApJ...845...16N

Erdélyi, R.; Mathioudakis, M.; Oliver, R. +3 more

Ellerman bombs (EBs) have been widely studied over the past two decades; however, only recently have the counterparts of these events been observed in the quiet-Sun. The aim of this article is to further understand small-scale quiet-Sun Ellerman-like brightenings (QSEBs) through research into their spectral signatures, including investigating whet…

2017 The Astrophysical Journal
IRIS 37
Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
DOI: 10.1051/0004-6361/201629666 Bibcode: 2017A&A...599A..34R

Adam, R.; Benoît, A.; Catalano, A. +37 more

Magnetic fields, which play a major role in a large number of astrophysical processes can be traced via observations of dust polarization. In particular, Planck low-resolution observations of dust polarization have demonstrated that Galactic filamentary structures, where star formation takes place, are associated to well organized magnetic fields.…

2017 Astronomy and Astrophysics
Planck 37
Impact of theoretical priors in cosmological analyses: The case of single field quintessence
DOI: 10.1103/PhysRevD.96.063524 Bibcode: 2017PhRvD..96f3524P

Peirone, Simone; Raveri, Marco; Silvestri, Alessandra +1 more

We investigate the impact of general conditions of theoretical stability and cosmological viability on dynamical dark energy models. As a powerful example, we study whether minimally coupled, single field quintessence models that are safe from ghost instabilities, can source the Chevallier-Polarski-Linder (CPL) expansion history recently shown to …

2017 Physical Review D
Planck 37
Modeling the Gravitational Potential of a Cosmological Dark Matter Halo with Stellar Streams
DOI: 10.3847/1538-4357/aa5eb4 Bibcode: 2017ApJ...836..234S

Helmi, Amina; Sanderson, Robyn E.; Hartke, Johanna

Stellar streams result from the tidal disruption of satellites and star clusters as they orbit a host galaxy, and can be very sensitive probes of the gravitational potential of the host system. We select and study narrow stellar streams formed in a Milky-Way-like dark matter halo of the Aquarius suite of cosmological simulations, to determine if t…

2017 The Astrophysical Journal
Gaia 37
A Suzaku, NuSTAR, and XMM-Newton view on variable absorption and relativistic reflection in NGC 4151
DOI: 10.1051/0004-6361/201630293 Bibcode: 2017A&A...603A..50B

Dauser, T.; Wilms, J.; Kadler, M. +6 more

We disentangle X-ray disk reflection from complex line-of-sight absorption in the nearby Seyfert NGC 4151, using a suite of Suzaku, NuSTAR, and XMM-Newton observations. Extending upon earlier published work, we pursue a physically motivated model using the latest angle-resolved version of the lamp-post geometry reflection model relxillCp_lp togeth…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 37
Hierarchical star formation across the grand-design spiral NGC 1566
DOI: 10.1093/mnras/stx445 Bibcode: 2017MNRAS.468..509G

Gouliermis, Dimitrios A.; Grebel, Eva K.; Smith, Linda J. +19 more

We investigate how star formation is spatially organized in the grand-design spiral NGC 1566 from deep Hubble Space Telescope photometry with the Legacy ExtraGalactic UV Survey. Our contour-based clustering analysis reveals 890 distinct stellar conglomerations at various levels of significance. These star-forming complexes are organized in a hiera…

2017 Monthly Notices of the Royal Astronomical Society
eHST 37
Probing cosmological isotropy with Planck Sunyaev-Zeldovich galaxy clusters
DOI: 10.1093/mnras/stw3233 Bibcode: 2017MNRAS.466.2799B

Bernui, A.; Ferreira, I. S.; Alcaniz, J. S. +1 more

We probe the statistical isotropy hypothesis of the large-scale structure with the second Planck Sunyaev-Zeldovich (PSZ2) galaxy clusters data set. Our analysis adopts a statistical-geometrical method that compares the two-point angular-correlation function of objects in antipodal patches of the sky. Given possible observational biases, such as th…

2017 Monthly Notices of the Royal Astronomical Society
Planck 37
A Multi-wavelength Study of the Turbulent Central Engine of the Low-mass AGN Hosted by NGC 404
DOI: 10.3847/1538-4357/aa7ecf Bibcode: 2017ApJ...845...50N

Davis, Timothy A.; Nguyen, Dieu D.; Nyland, Kristina +9 more

The nearby dwarf galaxy NGC 404 harbors a low-luminosity active galactic nucleus powered by the lowest-mass (<150,000 M ) central massive black hole (MBH), with a dynamical mass constraint, currently known, thus providing a rare low-redshift analog to the MBH “seeds” that formed in the early universe. Here, we present new imaging of…

2017 The Astrophysical Journal
eHST 37