Search Publications

A successful search for intervening 21 cm H I absorption in galaxies at 0.4 < z <1.0 with the Australian square kilometre array pathfinder (ASKAP)
DOI: 10.1093/mnras/staa2390 Bibcode: 2020MNRAS.499.4293S

Ellison, Sara L.; Koribalski, Bärbel S.; Lagos, Claudia del P. +6 more

We have used the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope to search for intervening 21 cm neutral hydrogen (H I) absorption along the line of sight to 53 bright radio continuum sources. Our observations are sensitive to H I column densities typical of Damped Lyman Alpha absorbers (DLAs) in cool gas with an H I spin temp…

2020 Monthly Notices of the Royal Astronomical Society
eHST 24
NuSTAR Discovery of a Compton-thick, Dust-obscured Galaxy: WISE J0825+3002
DOI: 10.3847/1538-4357/ab5718 Bibcode: 2020ApJ...888....8T

Tanimoto, Atsushi; Ueda, Yoshihiro; Kawamuro, Taiki +6 more

We report the discovery of a Compton-thick (CT), dust-obscured galaxy at z = 0.89, WISE J082501.48+300257.2 (WISE 0825+3002), observed by the Nuclear Spectroscopic Telescope Array. X-ray analysis with the XCLUMPY model revealed that hard X-ray luminosity in the rest-frame 2-10 keV band of WISE 0825+3002 is L X (2-10 keV) = {4.2}-1.…

2020 The Astrophysical Journal
XMM-Newton 24
Chandra Observations of NGC 7212: Large-scale Extended Hard X-Ray Emission
DOI: 10.3847/1538-4357/ab76c8 Bibcode: 2020ApJ...891..133J

Elvis, Martin; Fabbiano, G.; Siemiginowska, A. +5 more

Recent observations of nearby Compton thick (CT) active galactic nuclei (AGNs) with Chandra have resolved hard (>3 keV) X-ray emission extending out from the central supermassive black hole to kiloparsec scales, challenging the long-held belief that the characteristic hard X-ray continuum and fluorescent Fe K lines originate in the inner ∼parse…

2020 The Astrophysical Journal
eHST 24
Search for 7Be in the outbursts of four recent novae
DOI: 10.1093/mnras/stz3587 Bibcode: 2020MNRAS.492.4975M

Bonifacio, P.; Hernanz, M.; Molaro, P. +3 more

Following the recent detection of 7Be II in the outburst spectra of classical novae, we report the search for this isotope in the outbursts of four recent bright novae by means of high-resolution Ultraviolet and Visual Echelle Spectrograph (UVES) observations. The 7Be II λλ313.0583, 313.1228 nm doublet resonance lines are det…

2020 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL 24
An Increase in Small-planet Occurrence with Metallicity for Late-type Dwarf Stars in the Kepler Field and Its Implications for Planet Formation
DOI: 10.3847/1538-3881/abb773 Bibcode: 2020AJ....160..253L

Cheng, Sihao; Schlaufman, Kevin C.; Lu, Cicero X.

While it is well-established that giant-planet occurrence rises rapidly with host star metallicity, it is not yet clear if small-planet occurrence around late-type dwarf stars depends on host star metallicity. Using the Kepler Data Release 25 planet candidate list and its completeness data products, we explore planet occurrence as a function of me…

2020 The Astronomical Journal
Gaia 24
TESS light curves of γ Cas stars
DOI: 10.1093/mnras/staa2553 Bibcode: 2020MNRAS.498.3171N

Nazé, Yaël; Rauw, Gregor; Pigulski, Andrzej

γ Cas stars constitute a subgroup of Be stars showing unusually hard and bright X-ray emission. In search for additional peculiarities, we analysed the TESS light curves of 15 γ Cas analogues. Their periodograms display broad frequency groups and/or narrow isolated peaks, often superimposed over red noise. The detected signals appear at low freque…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 24
The orbital phase space of contracted dark matter haloes
DOI: 10.1093/mnras/staa1089 Bibcode: 2020MNRAS.495...12C

Grand, Robert J. J.; Marinacci, Federico; Deason, Alis J. +4 more

We study the orbital phase space of dark matter (DM) haloes in the AURIGA suite of cosmological hydrodynamics simulations of Milky Way (MW) analogues. We characterize haloes by their spherical action distribution, $F\left(J_{{r}},L\right)$ , a function of the specific angular momentum, L, and the radial action, Jr, of the DM particles. …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 24
Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
DOI: 10.1093/mnras/staa2898 Bibcode: 2020MNRAS.499.1154H

Sato, Toshiki; Podsiadlowski, Philipp; Mandel, Ilya +2 more

We explore a new scenario for producing stripped-envelope supernova progenitors. In our scenario, the stripped-envelope supernova is the second supernova of the binary, in which the envelope of the secondary was removed during its red supergiant phase by the impact of the first supernova. Through 2D hydrodynamical simulations, we find that ∼50-90 …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 24
Efficient Methanol Production on the Dark Side of a Prestellar Core
DOI: 10.3847/1538-4357/ab8f93 Bibcode: 2020ApJ...895..101H

Bizzocchi, Luca; Caselli, Paola; Rosolowsky, Erik +23 more

We present Atacama Large Millimeter/submillimeter Array maps of the starless molecular cloud core Ophiuchus/H-MM1 in the lines of deuterated ammonia (ortho- ${\mathrm{NH}}_{2}{\rm{D}}$ ), methanol ( ${\mathrm{CH}}_{3}\mathrm{OH}$ ), and sulfur monoxide (SO). The dense core is seen in ${\mathrm{NH}}_{2}{\rm{D}}$ emission, whereas the ${\mathrm{CH}}…

2020 The Astrophysical Journal
Herschel 24
A catalogue of over 10 million variable source candidates in ZTF Data Release 1
DOI: 10.1093/mnras/staa2814 Bibcode: 2020MNRAS.499.5782O

Gal-Yam, Avishay; Ofek, Eran O.; Masci, Frank +4 more

Variable sources probe a wide range of astrophysical phenomena. We present a catalogue of over 10 million variable source candidates found in Data Release 1 (DR1) of the Zwicky Transient Facility (ZTF). We perform a periodicity search up to a frequency of 160 d-1, and we classify the light curves into erratic and smooth variables. We al…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 24