Search Publications

Visualization of Multi-mission Astronomical Data with ESASky
DOI: 10.1088/1538-3873/129/972/028001 Bibcode: 2017PASP..129b8001B

de Marchi, Guido; Merín, Bruno; O'Mullane, William +17 more

ESASky is a science-driven discovery portal to explore the multi-wavelength sky and visualize and access multiple astronomical archive holdings. The tool is a web application that requires no prior knowledge of any of the missions involved and gives users world-wide simplified access to the highest-level science data products from multiple astrono…

2017 Publications of the Astronomical Society of the Pacific
INTEGRAL XMM-Newton 20
Constraining scalar-Gauss-Bonnet inflation by reheating, unitarity, and Planck data
DOI: 10.1103/PhysRevD.95.023514 Bibcode: 2017PhRvD..95b3514B

Bhattacharjee, Srijit; Maity, Debaprasad; Mukherjee, Rupak

We revisit the inflationary dynamics in detail for theories with Gauss-Bonnet gravity coupled to scalar functions, in light of the Planck data. Considering the chaotic inflationary scenario, we constrain the parameters of two models involving inflaton-Gauss-Bonnet coupling by current Planck data. For nonzero inflaton-Gauss-Bonnet coupling β , an i…

2017 Physical Review D
Planck 20
Population mixtures and searches of lensed and extended quasars across photometric surveys
DOI: 10.1093/mnras/stw3239 Bibcode: 2017MNRAS.466.3088W

Treu, Tommaso; Agnello, Adriano; Williams, Peter

Wide-field photometric surveys enable searches of rare yet interesting objects, such as strongly lensed quasars or quasars with a bright host galaxy. Past searches for lensed quasars based on their optical and near-infrared properties have relied on photometric cuts and spectroscopic preselection (as in the Sloan Quasar Lens Search), or neural net…

2017 Monthly Notices of the Royal Astronomical Society
eHST 20
Interaction of Two Filaments in a Long Filament Channel Associated with Twin Coronal Mass Ejections
DOI: 10.3847/1538-4357/aa5c38 Bibcode: 2017ApJ...836..160Z

Chen, Yao; Zheng, Ruisheng; Wang, Bing +4 more

Using the high-quality observations of the Solar Dynamics Observatory, we present the interaction of two filaments (F1 and F2) in a long filament channel associated with twin coronal mass ejections (CMEs) on 2016 January 26. Before the eruption, a sequence of rapid cancellation and emergence of the magnetic flux has been observed, which likely tri…

2017 The Astrophysical Journal
SOHO 20
Interplanetary Coronal Mass Ejections Resulting from Earth-Directed CMEs Using SOHO and ACE Combined Data During Solar Cycle 23
DOI: 10.1007/s11207-017-1050-2 Bibcode: 2017SoPh..292...30P

Paouris, Evangelos; Mavromichalaki, Helen

In this work a total of 266 interplanetary coronal mass ejections observed by the Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph (SOHO/LASCO) and then studied by in situ observations from Advanced Composition Explorer (ACE) spacecraft, are presented in a new catalog for the time interval 1996 - 2009 covering Solar Cyc…

2017 Solar Physics
SOHO 20
The Slowest Spinning X-Ray Pulsar in an Extragalactic Globular Cluster
DOI: 10.3847/1538-4357/aa689d Bibcode: 2017ApJ...839..125Z

Sartore, Nicola; Bachetti, Matteo; Webb, Natalie A. +2 more

Neutron stars are thought to be born rapidly rotating and then exhibit a phase of rotation-powered pulsations as they slow down to 1-10 s periods. The significant population of millisecond pulsars observed in our Galaxy is explained by the recycling concept: during an epoch of accretion from a donor star in a binary system, the neutron star is spu…

2017 The Astrophysical Journal
XMM-Newton eHST 20
Probing the Hot X-Ray Gas in the Narrow-line Region of Mrk 3
DOI: 10.3847/1538-4357/aa8c76 Bibcode: 2017ApJ...848...61B

Andrade-Santos, Felipe; Kraft, Ralph P.; Forman, William R. +2 more

We study the prototypical Seyfert 2 galaxy, Markarian 3, based on imaging and high-resolution spectroscopy observations taken by Chandra. We construct a deconvolved X-ray image, which reveals the S-shaped morphology of the hot gas in the narrow-line region (NLR). While this morphology is similar to the radio and [O III] emission, the distribution …

2017 The Astrophysical Journal
eHST 20
Direct Measurement of Anisotropic and Asymmetric Wave Vector Spectrum in Ion-scale Solar Wind Turbulence
DOI: 10.3847/2041-8213/aa9bf3 Bibcode: 2017ApJ...851L..11R

Escoubet, C. P.; Narita, Y.; Roberts, O. W.

This analysis represents the first time that a simultaneous measurement of parallel and perpendicular spectral indices at both inertial and kinetic scales has been made directly in wave vector space, using a single interval of solar wind plasma. An interferometric wave vector analysis method is applied to four-point magnetometer data from the Clus…

2017 The Astrophysical Journal
Cluster 20
Vertical magnetic field gradient in the photospheric layers of sunspots
DOI: 10.1051/0004-6361/201527060 Bibcode: 2017A&A...599A..35J

Joshi, Jayant; Lagg, Andreas; Hirzberger, Johann +2 more


Aims: We investigate the vertical gradient of the magnetic field of sunspots in the photospheric layer.
Methods: Independent observations were obtained with the Solar Optical Telescope/Spectropolarimeter (SOT/SP) on board the Hinode spacecraft and with the Tenrife Infrared Polarimeter-2 (TIP-2) mounted at the German Vacuum Tower Telescop…

2017 Astronomy and Astrophysics
Hinode 20
Searching for Fossil Evidence of AGN Feedback in WISE-selected Stripe-82 Galaxies by Measuring the Thermal Sunyaev-Zel’dovich Effect with the Atacama Cosmology Telescope
DOI: 10.3847/1538-4357/834/2/102 Bibcode: 2017ApJ...834..102S

Cohen, Seth; Joshi, Bhavin; Scannapieco, Evan +2 more

We directly measure the thermal energy of the gas surrounding galaxies through the thermal Sunyaev-Zel’dovich (tSZ) effect. We perform a stacking analysis of microwave background images from the Atacama Cosmology Telescope, around 1179 massive quiescent elliptical galaxies at 0.5 ≤ z ≤ 1.0 (“low-z”) and 3274 galaxies at 1.0 ≤ z ≤ 1.5 (“high-z”), s…

2017 The Astrophysical Journal
Planck eHST 20