Search Publications

Strong Lensing Model of SPT-CL J0356-5337, a Major Merger Candidate at Redshift 1.0359
DOI: 10.3847/1538-4357/ab886b Bibcode: 2020ApJ...894..150M

Mahler, Guillaume; Schrabback, Tim; Sharon, Keren +10 more

We present an analysis of the mass distribution inferred from strong lensing by SPT-CL J0356-5337, a cluster of galaxies at redshift $z=1.0359$ revealed in the follow-up of the SPT-SZ clusters. The cluster has an Einstein radius of ${\theta }_{{\rm{E}}}\simeq $ 14″ for a source at z = 3 and a mass within 500 kpc of ${M}_{500\mathrm{kpc}}=4.0\pm 0.…

2020 The Astrophysical Journal
eHST 10
Reconstructing Solar Wind Inhomogeneous Structures From Stereoscopic Observations in White Light: Solar Wind Transients in 3-D
DOI: 10.1029/2019JA027513 Bibcode: 2020JGRA..12527513L

Wang, Yuming; Shen, Fang; Shen, Chenglong +7 more

White-light images from Heliospheric Imager-1 (HI1) onboard the Solar Terrestrial Relations Observatory (STEREO) provide two-dimensional (2-D) global views of solar wind transients traveling in the inner heliosphere from two perspectives. How to retrieve the hidden three-dimensional (3-D) features of the transients from these 2-D images is intrigu…

2020 Journal of Geophysical Research (Space Physics)
SOHO 10
Inferences About the Magnetic Field Structure of a CME with Both In Situ and Faraday Rotation Constraints
DOI: 10.3847/1538-4357/ab93b8 Bibcode: 2020ApJ...896...99W

Wood, Brian E.; Nieves-Chinchilla, Teresa; Kooi, Jason E. +2 more

On 2012 August 2, two coronal mass ejections (CMEs; CME-1 and CME-2) erupted from the west limb of the Sun as viewed from Earth, and were observed in images from the white-light coronagraphs on the SOlar and Heliospheric Observatory and Solar TErrestrial RElations Observatory (STEREO) spacecraft. These events were also observed by the Very Large A…

2020 The Astrophysical Journal
SOHO 10
Characterization of a local dust storm on Mars with REMS/MSL measurements and MARCI/MRO images
DOI: 10.1016/j.icarus.2019.113521 Bibcode: 2020Icar..33813521O

Hueso, Ricardo; Sánchez-Lavega, Agustín; Ordonez-Etxeberria, Iñaki +1 more

The REMS instrument on board the Curiosity rover has been collecting meteorological data from Gale crater on Mars since August 2012. A dust storm that developed north of Gale crater in sol 852 of the Mars Science Laboratory (MSL) mission spread above the location of the Curiosity rover during sols 853-855 (December 30, 2014 to January 1, 2015, are…

2020 Icarus
MEx 10
Discovery of a thermonuclear Type I X-ray burst in infrared: new limits on the orbital period of 4U 1728-34
DOI: 10.1093/mnrasl/slaa049 Bibcode: 2020MNRAS.495L..37V

Altamirano, D.; Belloni, T.; Vincentelli, F. M. +4 more

We report the detection of an infrared burst lagging a thermonuclear Type I X-ray burst from the accreting neutron star (NS) 4U 1728-34 (GX 354-0). Observations were performed simultaneously with XMM-Newton (0.7-12 keV), NuSTAR (3-79 keV), and HAWK-I@VLT (2.2 µm). We measure a lag of 4.75 ± 0.5 s between the peaks of the emission in the two …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
Photometric investigation on the W-subtype contact binary V1197 Her
DOI: 10.1088/1674-4527/20/1/10 Bibcode: 2020RAA....20...10Z

Soonthornthum, Boonrucksar; Zhou, Xiao

Multi-color light curves of V1197 Her were obtained with the 2.4 meter optical telescope at the Thai National Observatory and the Wilson-Devinney (W-D) program was used to model the observational light curves. The photometric solutions reveal that V1197 Her is a W-subtype shallow contact binary system with a mass ratio of q = 2.61 and a fill-out f…

2020 Research in Astronomy and Astrophysics
Gaia 10
NGTS-8b and NGTS-9b: two non-inflated hot Jupiters
DOI: 10.1093/mnras/stz3140 Bibcode: 2020MNRAS.491.2834C

Jackman, James A. G.; Wheatley, Peter J.; Bayliss, Daniel +36 more

We report the discovery, by the next generation transit survey (NGTS), of two hot Jupiters NGTS-8b and NGTS-9b. These orbit a V = 13.68 K0V star (Teff = 5241 ± 50 K) with a period of 2.49970 d, and a V = 12.80 F8V star (Teff = 6330 ± 130 K) in 4.43527 d, respectively. The transits were independently verified by follow-up phot…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 10
Sunquake with a second bounce, other sunquakes, and emission associated with the X9.3 flare of 6 September 2017. I. Observations
DOI: 10.1051/0004-6361/201936755 Bibcode: 2020A&A...639A..78Z

Dammasch, Ingolf E.; Matthews, Sarah; Inoue, Satoshi +4 more


Aims: The 6 September 2017 X9.3 solar flare produced very unique observations of magnetic field transients and a few seismic responses, or sunquakes, detected by the Helioseismic and Magnetic Imager (HMI) instrument aboard Solar Dynamic Observatory (SDO) spacecraft, including the strongest sunquake ever reported. This flare was one of a few f…

2020 Astronomy and Astrophysics
Hinode 10
Coupled day-night models of exoplanetary atmospheres
DOI: 10.1093/mnras/staa3143 Bibcode: 2020MNRAS.499.4984G

Gandhi, Siddharth; Jermyn, Adam S.

We provide a new framework to model the day side and night side atmospheres of irradiated exoplanets using 1D radiative transfer by incorporating a self-consistent heat flux carried by circulation currents (winds) between the two sides. The advantages of our model are its physical motivation and computational efficiency, which allows for an explor…

2020 Monthly Notices of the Royal Astronomical Society
eHST 10
Searching for volcanic activity and a mercury-like exosphere of the super-Earth HD3167 b
DOI: 10.1093/mnras/stz3288 Bibcode: 2020MNRAS.491.3974G

Guenther, Eike W.; Kislyakova, Kristina G.

HD3167 b is a transiting super-Earth that has a density which is consistent with a rocky composition. The planet is exposed to strong radiation, intense stellar wind, and likely strong tidal forces and induction heating. According to theory, planets that are so close to the star should have an atmosphere like Mercury but much more extended and den…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 10