Search Publications

Discovery of the First Quadruple Gravitationally Lensed Quasar Candidate with Pan-STARRS
DOI: 10.3847/1538-4357/aa7aa6 Bibcode: 2017ApJ...844...90B

Keeton, C. R.; Berghea, C. T.; Dudik, R. P. +2 more

We report the serendipitous discovery of the first gravitationally lensed quasar candidate from Pan-STARRS. The grizy images reveal four point-like images with magnitudes between 14.9 and 18.1 mag. The colors of the point sources are similar, and they are more consistent with quasars than with stars or galaxies. The lensing galaxy is detected in t…

2017 The Astrophysical Journal
Gaia 27
ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
DOI: 10.1093/mnras/stx1112 Bibcode: 2017MNRAS.469.4683C

Daddi, E.; Elbaz, D.; Rujopakarn, W. +13 more

We present deep ALMA CO(5-4) observations of a main-sequence, clumpy galaxy at z = 1.5 in the HUDF. Thanks to the ∼0{^''.}5 resolution of the ALMA data, we can link stellar population properties to the CO(5-4) emission on scales of a few kiloparsec. We detect strong CO(5-4) emission from the nuclear region of the galaxy, consistent with…

2017 Monthly Notices of the Royal Astronomical Society
eHST 27
Gaia eclipsing binary and multiple systems. Two-Gaussian models applied to OGLE-III eclipsing binary light curves in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201730613 Bibcode: 2017A&A...606A..92M

Audard, M.; Rimoldini, L.; Holl, B. +11 more

Context. The advent of large scale multi-epoch surveys raises the need for automated light curve (LC) processing. This is particularly true for eclipsing binaries (EBs), which form one of the most populated types of variable objects. The Gaia mission, launched at the end of 2013, is expected to detect of the order of few million EBs over a five-ye…

2017 Astronomy and Astrophysics
Gaia 27
Global Energetics of Solar Flares. VI. Refined Energetics of Coronal Mass Ejections
DOI: 10.3847/1538-4357/aa8952 Bibcode: 2017ApJ...847...27A

Aschwanden, Markus J.

In this study, we refine the coronal mass ejection (CME) model that was presented in an earlier study of the global energetics of solar flares and associated CMEs and apply it to all (860) GOES M- and X-class flare events observed during the first seven years (2010-2016) of the Solar Dynamics Observatory (SDO) mission. The model refinements includ…

2017 The Astrophysical Journal
SOHO 27
Scattering Properties of the Venusian Clouds Observed by the UV Imager on board Akatsuki
DOI: 10.3847/1538-3881/aa78a5 Bibcode: 2017AJ....154...44L

Yamada, M.; Imamura, T.; Murakami, S. +6 more

We analyze the albedo of Venus obtained from the UV Imager on board Akatsuki. A relative global mean albedo over phase angle is used in this study, and we confirm the glory feature at 283 and 365 nm in the data acquired in 2016 May. We successfully simulate the observation using a radiative transfer model. Our results show that cloud aerosols of {…

2017 The Astronomical Journal
VenusExpress 27
Alignments of parity even/odd-only multipoles in CMB
DOI: 10.1093/mnras/stx2112 Bibcode: 2017MNRAS.472.2410A

Aluri, Pavan K.; Ralston, John P.; Weltman, Amanda

We compare the statistics of parity even and odd multipoles of the cosmic microwave background (CMB) sky from Planck full mission temperature measurements. An excess power in odd multipoles compared to even multipoles has previously been found on large angular scales. Motivated by this apparent parity asymmetry, we evaluate directional statistics …

2017 Monthly Notices of the Royal Astronomical Society
Planck 27
Hubble Space Telescope Imaging of the Active Dwarf Galaxy RGG 118
DOI: 10.3847/1538-4357/aa9067 Bibcode: 2017ApJ...850..196B

Greene, Jenny E.; Baldassare, Vivienne F.; Reines, Amy E. +1 more

RGG 118 (SDSS 1523+1145) is a nearby (z = 0.0243), dwarf disk galaxy ({M}* ≈ 2× {10}9 {M}) that is found to host an active ∼50,000 solar mass black hole at its core. RGG 118 is one of a growing collective sample of dwarf galaxies known to contain active galactic nuclei (AGNs)—a group that, until recently, contain…

2017 The Astrophysical Journal
eHST 27
Expelled grains from an unseen parent body around AU Microscopii
DOI: 10.1051/0004-6361/201731061 Bibcode: 2017A&A...607A..65S

Augereau, J. -C.; Boccaletti, A.; Sezestre, É. +1 more

Context. Recent observations of the edge-on debris disk of AU Mic have revealed asymmetric, fast outward-moving arch-like structures above the disk midplane. Although asymmetries are frequent in debris disks, no model can readily explain the characteristics of these features.
Aims: We present a model aiming to reproduce the…

2017 Astronomy and Astrophysics
eHST 27
Quasar lenses and galactic streams: outlier selection and Gaia multiplet detection
DOI: 10.1093/mnras/stx1650 Bibcode: 2017MNRAS.471.2013A

Agnello, Adriano

I describe two novel techniques originally devised to select strongly lensed quasar candidates in wide-field surveys. The first relies on outlier selection in optical and mid-infrared magnitude space; the second combines mid-infrared colour selection with Gaia spatial resolution, to identify multiplets of objects with quasar-like colours. Both met…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 27
Sheath-accumulating Propagation of Interplanetary Coronal Mass Ejection
DOI: 10.3847/2041-8213/aa624c Bibcode: 2017ApJ...837L..17T

Shibata, Kazunari; Takahashi, Takuya

Fast interplanetary coronal mass ejections (ICMEs) are the drivers of strong space weather storms such as solar energetic particle events and geomagnetic storms. The connection between the space-weather-impacting solar wind disturbances associated with fast ICMEs at Earth and the characteristics of causative energetic CMEs observed near the Sun is…

2017 The Astrophysical Journal
SOHO 27