Search Publications

X-Ray Spectrum of RBS 315: Absorption or Intrinsic Curvature
DOI: 10.3847/1538-4357/ab340f Bibcode: 2019ApJ...882..130B

Behar, Ehud; Mushotzky, Richard F.; Ben Haim, Sivan

X-ray absorption of high-redshift quasars is enigmatic, because it remains unclear where in the universe the absorbing gas is. If absorption occurs near the high-z host, it could help us understand early stages of galaxy formation. If it is in the intergalactic medium (IGM), it provides a unique way to probe this elusive baryon component. We repor…

2019 The Astrophysical Journal
XMM-Newton 4
Lens Model and Source Reconstruction Reveal the Morphology and Star Formation Distribution in the Cool Spiral LIRG SGAS J143845.1+145407
DOI: 10.3847/1538-4357/ab0d7d Bibcode: 2019ApJ...875...18D

Rigby, Jane R.; Whitaker, Katherine E.; Sharon, Keren +8 more

We present Hubble Space Telescope (HST) imaging and grism spectroscopy of a strongly lensed LIRG at z = 0.816, SGAS 143845.1+145407, and use the magnification boost of gravitational lensing to study the distribution of star formation throughout this galaxy. Based on the HST imaging data, we create a lens model for this system; we compute the mass …

2019 The Astrophysical Journal
eHST 4
A Hubble Space Telescope Survey for Novae in the Globular Clusters of M87
DOI: 10.3847/1538-4357/ab0490 Bibcode: 2019ApJ...874...65D

Shara, Michael M.; Zurek, David; Doyle, Trisha F. +1 more

The giant elliptical galaxy M87 has been imaged over 30 consecutive days in 2001, 60 consecutive days in 2005-2006, and every 5 days over a 265-day span in 2016-2017 with the Hubble Space Telescope, leading to the detection of 137 classical novae throughout M87. We have identified 2134 globular clusters (GC) in M87 in these images and carried out …

2019 The Astrophysical Journal
eHST 4
Relation between solar flares and halo coronal mass ejections
DOI: 10.1007/s12036-018-9570-1 Bibcode: 2019JApA...40....1R

Sankarasubramanian, K.; Rao, V. Koteswara; Gopal, K. Rama +2 more

Solar flares and coronal mass ejections (CMEs) are two very important active events from Sun. Inspite of several theoretical and statistical analyses, the relation between solar flares and CMEs is so far not well established, and strong opinions and arguments still continue. Statistical approaches use a lot of data available from many measurements…

2019 Journal of Astrophysics and Astronomy
Hinode SOHO 4
Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
DOI: 10.1016/j.pss.2018.08.001 Bibcode: 2019P&SS..166...59X

Muller, J. -P.; Xiong, S.

Subsurface layers are preserved in polar regions on Mars, which are considered to be a record of past climate changes on Mars. Orbital radar instruments like the SHAllow RADar (SHARAD) on board Mars Reconnaissance Orbiter (MRO) transmit radar signals to Mars and receive a set of signals returned from interfaces having a contrast in dielectric prop…

2019 Planetary and Space Science
MEx 4
Io’s Atmosphere Silhouetted by Jupiter Lyα
DOI: 10.3847/1538-3881/ab3c4c Bibcode: 2019AJ....158..154R

Feaga, L. M.; Roth, L.; Retherford, K. D. +4 more

We report results from a new technique for mapping Io’s SO2 vapor distribution. The Space Telescope Imaging Spectrograph (STIS) instrument on the Hubble Space Telescope observed Io during four Jupiter transit events to obtain medium resolution far-UV spectral images near the Lyα wavelength of 121.6 nm. Jupiter’s bright Lyα dayglow provi…

2019 The Astronomical Journal
eHST 4
AKARI mid-infrared slit-less spectroscopic catalogue
DOI: 10.1093/pasj/psy132 Bibcode: 2019PASJ...71....3Y

Baba, Shunsuke; Onaka, Takashi; Yamamura, Issei +4 more

AKARI/IRC is capable of conducting slit-less spectroscopy in the mid-infrared (5-13 µm) over a 10' × 10' area with a spectral resolution of 50, which is suitable for serendipitous surveys. The data reduction is, however, rather complicated by the confusion of nearby sources after dispersing the spectra. To achieve efficient and reliable data…

2019 Publications of the Astronomical Society of Japan
AKARI 4
Investigating the Pulsar Wind Nebula 3C 58 Using Emission Models
DOI: 10.5303/JKAS.2019.52.5.173 Bibcode: 2019JKAS...52..173K

An, Hongjun; Park, Jaegeun; Kim, Seungjong

We present IR flux density measurements, models of the broadband SED, and results of SED modeling for the Pulsar Wind Nebula (PWN) 3C 58. We find that the Herschel flux density seems to be slightly lower than suggested by interpolation of previous measurements in nearby wavebands, implying that there may be multiple electron populations in 3C 58. …

2019 Journal of Korean Astronomical Society
Herschel 4
Calibration of parent and fragment ion detection rates in Rosettas ROSINA/DFMS mass spectrometer
DOI: 10.1016/j.ijms.2019.116233 Bibcode: 2019IJMSp.44616233D

Altwegg, K.; Balsiger, H.; Fuselier, S. A. +7 more

2019 International Journal of Mass Spectrometry
Rosetta 4
Revisiting the magnetization of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834278 Bibcode: 2019A&A...630A..46H

Richter, I.; Glassmeier, K. H.; Heinisch, P. +1 more

Context. The landing of the Philae probe as part of the ESA Rosetta mission made it possible to study the magnetization of comet 67P/Churyumov-Gerasimenko (67P) by combining observations from the lander and orbiter. In this work, we revisit the magnetic properties with information gained during the progression of the mission for a comprehensive un…

2019 Astronomy and Astrophysics
Rosetta 4