Search Publications

The Sloan Digital Sky Survey Reverberation Mapping Project: Estimating Masses of Black Holes in Quasars with Single-epoch Spectroscopy
DOI: 10.3847/1538-4357/abbc1c Bibcode: 2020ApJ...903..112D

Brandt, W. N.; Shen, Yue; Peterson, Bradley M. +19 more

It is well known that reverberation mapping of active galactic nuclei (AGNs) reveals a relationship between AGN luminosity and the size of the broad-line region, and that use of this relationship, combined with the Doppler width of the broad emission line, enables an estimate of the mass of the black hole at the center of the active nucleus based …

2020 The Astrophysical Journal
eHST 106
An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz
DOI: 10.1093/mnras/staa2824 Bibcode: 2020MNRAS.499..482N

Campana, S.; Berger, E.; Gromadzki, M. +42 more

At 66 Mpc, AT2019qiz is the closest optical tidal disruption event (TDE) to date, with a luminosity intermediate between the bulk of the population and the faint-and-fast event iPTF16fnl. Its proximity allowed a very early detection and triggering of multiwavelength and spectroscopic follow-up well before maximum light. The velocity dispersion of …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 106
Observing the tail of reionization: neutral islands in the z = 5.5 Lyman-α forest
DOI: 10.1093/mnras/staa894 Bibcode: 2020MNRAS.494.3080N

Nasir, Fahad; D'Aloisio, Anson

Previous studies have noted difficulties in modelling the highest opacities of the z > 5.5 Ly α forest, epitomized by the extreme Lyα trough observed towards quasar ULAS J0148 + 0600. One possibility is that the most opaque regions at these redshifts contain significant amounts of neutral hydrogen. This explanation, which abandons the common as…

2020 Monthly Notices of the Royal Astronomical Society
eHST 105
The CatWISE Preliminary Catalog: Motions from WISE and NEOWISE Data
DOI: 10.3847/1538-4365/ab7f2a Bibcode: 2020ApJS..247...69E

Teplitz, Harry I.; Schlegel, David J.; Mobasher, Bahram +19 more

CatWISE is a program to catalog sources selected from combined WISE and NEOWISE all-sky survey data at 3.4 and 4.6 &mgrm (W1 and W2). The CatWISE Preliminary Catalog consists of 900,849,014 sources measured in data collected from 2010 to 2016. This data set represents four times as many exposures and spans over 10 times as large a time baselin…

2020 The Astrophysical Journal Supplement Series
Gaia 105
The MOSDEF Survey: The Variation of the Dust Attenuation Curve with Metallicity
DOI: 10.3847/1538-4357/aba35e Bibcode: 2020ApJ...899..117S

Siana, Brian; Azadi, Mojegan; Shivaei, Irene +14 more

We derive a UV-optical stellar dust attenuation curve of galaxies at z = 1.4-2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding those with very young or heavily obscured star formation, from the MOSFIRE Deep Evolution Field survey with Hα, Hβ, and [N II]λ 6585 spectroscopic measurements. We constrai…

2020 The Astrophysical Journal
eHST 104
Limit on the LMC mass from a census of its satellites
DOI: 10.1093/mnras/staa1238 Bibcode: 2020MNRAS.495.2554E

Belokurov, Vasily A.; Erkal, Denis

We study the orbits of dwarf galaxies in the combined presence of the Milky Way and Large Magellanic Cloud (LMC) and find six dwarfs that were likely accreted with the LMC (Car 2, Car 3, Hor 1, Hyi 1, Phe 2, and Ret 2), in addition to the Small Magellanic Cloud (SMC), representing strong evidence of dwarf galaxy group infall. This procedure depend…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 104
A radio parallax to the black hole X-ray binary MAXI J1820+070
DOI: 10.1093/mnrasl/slaa010 Bibcode: 2020MNRAS.493L..81A

Maccarone, T. J.; Altamirano, D.; Belloni, T. +18 more

Using the Very Long Baseline Array and the European Very Long Baseline Interferometry Network, we have made a precise measurement of the radio parallax of the black hole X-ray binary MAXI J1820+070, providing a model-independent distance to the source. Our parallax measurement of (0.348 ± 0.033) mas for MAXI J1820+070 translates to a distance of (…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 103
High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations
DOI: 10.1051/0004-6361/202038300 Bibcode: 2020A&A...640A..81N

Christensen-Dalsgaard, J.; Spitoni, E.; Nissen, P. E. +3 more


Aims: Previous high-precision studies of abundances of elements in solar twin stars are extended to a wider metallicity range to see how the trends of element ratios with stellar age depend on [Fe/H].
Methods: HARPS spectra with signal-to-noise ratios S/N ≳ 600 at λ ∼ 6000 Å were analysed with MARCS model atmospheres to obtain 1D LTE abu…

2020 Astronomy and Astrophysics
Gaia 103
The Host Galaxies of Tidal Disruption Events
DOI: 10.1007/s11214-020-00657-y Bibcode: 2020SSRv..216...32F

Zabludoff, Ann I.; French, K. Decker; Graur, Or +2 more

Recent studies of Tidal Disruption Events (TDEs) have revealed unexpected correlations between the TDE rate and the large-scale properties of the host galaxies. In this review, we present the host galaxy properties of all TDE candidates known to date and quantify their distributions. We consider throughout the differences between observationally-i…

2020 Space Science Reviews
eHST 102
A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy
DOI: 10.3847/2041-8213/ab8cc7 Bibcode: 2020ApJ...895L..23C

Lundqvist, P.; Reichart, D. E.; Kochanek, C. S. +35 more

We present X-ray and radio observations of the Fast Blue Optical Transient CRTS-CSS161010 J045834-081803 (CSS161010 hereafter) at t = 69-531 days. CSS161010 shows luminous X-ray (LX ∼ 5 × 1039 erg s-1) and radio (Lν ∼ 1029 erg s-1 Hz-1) emission. The radio emission peaked…

2020 The Astrophysical Journal
INTEGRAL 101