Search Publications

Constraints on Metastable Helium in the Atmospheres of WASP-69b and WASP-52b with Ultranarrowband Photometry
DOI: 10.3847/1538-3881/ab8e34 Bibcode: 2020AJ....159..278V

Tinyanont, Samaporn; Millar-Blanchaer, Maxwell A.; Knutson, Heather A. +7 more

Infrared observations of metastable 23S helium absorption with ground- and space-based spectroscopy are rapidly maturing, as this species is a unique probe of exoplanet atmospheres. Specifically, the transit depth in the triplet feature (with vacuum wavelengths near 1083.3 nm) can be used to constrain the temperature and mass-loss rate …

2020 The Astronomical Journal
eHST 54
Confirmation of water emission in the dayside spectrum of the ultrahot Jupiter WASP-121b
DOI: 10.1093/mnras/staa1628 Bibcode: 2020MNRAS.496.1638M

Mikal-Evans, Thomas; Sing, David K.; Wakeford, Hannah R. +5 more

We present four new secondary eclipse observations for the ultrahot Jupiter WASP-121b acquired using the Hubble Space Telescope Wide Field Camera 3. The eclipse depth is measured to a median precision of 60 ppm across 28 spectroscopic channels spanning the 1.12- $1.64\, \mu {\rm m}$ wavelength range. This is a considerable improvement to the 90 pp…

2020 Monthly Notices of the Royal Astronomical Society
eHST 54
Revealing the intermediate-mass black hole at the heart of the dwarf galaxy NGC 404 with sub-parsec resolution ALMA observations
DOI: 10.1093/mnras/staa1567 Bibcode: 2020MNRAS.496.4061D

Neumayer, Nadine; Barth, Aaron J.; Greene, Jenny E. +15 more

We estimate the mass of the intermediate-mass black hole at the heart of the dwarf elliptical galaxy NGC 404 using Atacama Large Millimetre/submillimetre Array (ALMA) observations of the molecular interstellar medium at an unprecedented linear resolution of ≈0.5 pc, in combination with existing stellar kinematic information. These ALMA observation…

2020 Monthly Notices of the Royal Astronomical Society
eHST 54
Absolute V-band magnitudes and mass-to-light ratios of Galactic globular clusters
DOI: 10.1017/pasa.2020.38 Bibcode: 2020PASA...37...46B

Hilker, M.; Baumgardt, H.; Sollima, A.

We have used Hubble Space Telescope and ground-based photometry to determine total V-band magnitudes and mass-to-light ratios of more than 150 Galactic globular clusters. We do this by summing up the magnitudes of their individual member stars, using colour-magnitude information, Gaia DR2 proper motions, and radial velocities to distinguish cluste…

2020 Publications of the Astronomical Society of Australia
Gaia eHST 54
An all-sky proper-motion map of the Sagittarius stream using Gaia DR2
DOI: 10.1051/0004-6361/201937145 Bibcode: 2020A&A...635L...3A

Jordi, C.; Anders, F.; Helmi, A. +4 more


Aims: We aim to measure the proper motion along the Sagittarius stream, which is the missing piece in determining its full 6D phase space coordinates.
Methods: We conduct a blind search of over-densities in proper motion from the Gaia second data release in a broad region around the Sagittarius stream by applying wavelet transform techni…

2020 Astronomy and Astrophysics
Gaia 54
Chemical Evolution in the Milky Way: Rotation-based Ages for APOGEE-Kepler Cool Dwarf Stars
DOI: 10.3847/1538-4357/ab5c24 Bibcode: 2020ApJ...888...43C

van Saders, Jennifer L.; García, Rafael A.; Claytor, Zachary R. +5 more

We use models of stellar angular momentum evolution to determine ages for ∼500 stars in the APOGEE-Kepler Cool Dwarfs sample. We focus on lower-main-sequence stars, where other age-dating tools become ineffective. Our age distributions are compared to those derived from asteroseismic and giant samples and solar analogs. We are able to recover gyro…

2020 The Astrophysical Journal
Gaia 54
The Magellanic Corona as the key to the formation of the Magellanic Stream.
DOI: 10.1038/s41586-020-2663-4 Bibcode: 2020Natur.585..203L

Bland-Hawthorn, J.; Lucchini, S.; D'Onghia, E. +3 more

The dominant gaseous structure in the Galactic halo is the Magellanic Stream, an extended network of neutral and ionized filaments surrounding the Large and Small Magellanic Clouds (LMC/SMC), the two most massive satellite galaxies of the Milky Way. Recent observations indicate that the Clouds are on their first passage around our Galaxy, the Stre…

2020 Nature
eHST 54
Primordial black holes and oscillating gravitational waves in slow-roll and slow-climb inflation with an intermediate noninflationary phase
DOI: 10.1103/PhysRevD.102.043527 Bibcode: 2020PhRvD.102d3527F

Wu, Puxun; Yu, Hongwei; Fu, Chengjie

We propose a new single field inflation model in which the usual slow-roll inflation is joined to a new period of slow-climb and slow-roll inflation through a short intermediate noninflationary phase. We then show that primordial curvature perturbations can be enhanced at small scales, a sizable amount of primordial black holes (PBHs) can be produ…

2020 Physical Review D
INTEGRAL 54
Cosmological constraints from galaxy-lensing cross-correlations using BOSS galaxies with SDSS and CMB lensing
DOI: 10.1093/mnras/stz2922 Bibcode: 2020MNRAS.491...51S

Mandelbaum, Rachel; Seljak, Uroš; Slosar, Anže +2 more

We present cosmological parameter constraints based on a joint modelling of galaxy-lensing cross-correlations and galaxy clustering measurements in the SDSS, marginalizing over small-scale modelling uncertainties using mock galaxy catalogues, without explicit modelling of galaxy bias. We show that our modelling method is robust to the impact of di…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 53
The ALPINE-ALMA [CII] survey. Circumgalactic medium pollution and gas mixing by tidal stripping in a merging system at z ∼ 4.57
DOI: 10.1051/0004-6361/202038284 Bibcode: 2020A&A...643A...7G

Maiolino, R.; Schaerer, D.; Béthermin, M. +25 more

We present ALMA observations of a merging system at z ∼ 4.57, observed as a part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) survey. Combining ALMA [CII]158 µm and far-infrared continuum data with multi-wavelength ancillary data, we find that the system is composed of two massive (M ≳ 1010 M<…

2020 Astronomy and Astrophysics
eHST 53