Search Publications

The scatter of the M dwarf mass-radius relationship
DOI: 10.1093/mnras/sty2345 Bibcode: 2018MNRAS.481.1083P

Hermes, J. J.; Gänsicke, B. T.; Dhillon, V. S. +14 more

M dwarfs are prime targets in the hunt for habitable worlds around other stars. This is due to their abundance as well as their small radii and low masses and temperatures, which facilitate the detection of temperate, rocky planets in orbit around them. However, the fundamental properties of M dwarfs are difficult to constrain, often limiting our …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 93
The ALMA-PILS survey: the sulphur connection between protostars and comets: IRAS 16293-2422 B and 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/sty462 Bibcode: 2018MNRAS.476.4949D

van Dishoeck, Ewine F.; Drozdovskaya, Maria N.; Jørgensen, Jes K. +9 more

The evolutionary past of our Solar system can be pieced together by comparing analogous low-mass protostars with remnants of our Protosolar Nebula - comets. Sulphur-bearing molecules may be unique tracers of the joint evolution of the volatile and refractory components. ALMA Band 7 data from the large unbiased Protostellar Interferometric Line Sur…

2018 Monthly Notices of the Royal Astronomical Society
Rosetta 93
Lost but not forgotten: intracluster light in galaxy groups and clusters
DOI: 10.1093/mnras/stx2946 Bibcode: 2018MNRAS.474.3009D

Donahue, Megan; Mulchaey, John S.; Connor, Thomas +4 more

With Hubble Space Telescope imaging, we investigate the progenitor population and formation mechanisms of the intracluster light (ICL) for 23 galaxy groups and clusters at 0.29 ≤ z ≤ 0.89. The colour gradients of the BCG+ICL become bluer with increasing radius out to 53-100 kpc for all but one system, suggesting that violent relaxation after major…

2018 Monthly Notices of the Royal Astronomical Society
eHST 92
Fast and Slow Paths to Quiescence: Ages and Sizes of 400 Quiescent Galaxies from the LEGA-C Survey
DOI: 10.3847/1538-4357/aae822 Bibcode: 2018ApJ...868...37W

Bell, Eric F.; Franx, Marijn; Muzzin, Adam +11 more

We analyze the stellar age indicators (D n 4000 and EW(Hδ)) and sizes of 467 quiescent galaxies with M * ≥ 1010 M at z ∼ 0.7 drawn from DR2 of the LEGA-C survey. Interpreting index variations in terms of equivalent single stellar population age, we find that the median stellar population is younger for…

2018 The Astrophysical Journal
eHST 92
Gaia Data Release 2. Observations of solar system objects
DOI: 10.1051/0004-6361/201832900 Bibcode: 2018A&A...616A..13G

Prusti, T.; Mazeh, T.; Zucker, S. +449 more

Context. The Gaia spacecraft of the European Space Agency (ESA) has been securing observations of solar system objects (SSOs) since the beginning of its operations. Data Release 2 (DR2) contains the observations of a selected sample of 14,099 SSOs. These asteroids have been already identified and have been numbered by the Minor Planet Center repos…

2018 Astronomy and Astrophysics
Gaia 92
On the Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars
DOI: 10.3847/1538-4357/aaa9be Bibcode: 2018ApJ...854..158S

Ho, Luis C.; Shangguan, Jinyi; Xie, Yanxia

The interstellar medium is crucial to understanding the physics of active galaxies and the coevolution between supermassive black holes and their host galaxies. However, direct gas measurements are limited by sensitivity and other uncertainties. Dust provides an efficient indirect probe of the total gas. We apply this technique to a large sample o…

2018 The Astrophysical Journal
Herschel 92
Homogeneous Analysis of the Dust Morphology of Transition Disks Observed with ALMA: Investigating Dust Trapping and the Origin of the Cavities
DOI: 10.3847/1538-4357/aabf94 Bibcode: 2018ApJ...859...32P

van der Plas, G.; Pascucci, I.; Garufi, A. +11 more

We analyze the dust morphology of 29 transition disks (TDs) observed with Atacama Large (sub-)Millimeter Array (ALMA) at (sub-)millimeter emission. We perform the analysis in the visibility plane to characterize the total flux, cavity size, and shape of the ring-like structure. First, we found that the M dust-M relation is …

2018 The Astrophysical Journal
Gaia 92
Non-negative Matrix Factorization: Robust Extraction of Extended Structures
DOI: 10.3847/1538-4357/aaa1f2 Bibcode: 2018ApJ...852..104R

Duchêne, Gaspard; Pueyo, Laurent; Debes, John +2 more

We apply the vectorized non-negative matrix factorization (NMF) method to the post-processing of the direct imaging data of exoplanetary systems such as circumstellar disks. NMF is an iterative approach, which first creates a nonorthogonal and non-negative basis of components using the given reference images and then models a target with the compo…

2018 The Astrophysical Journal
eHST 92
Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet
DOI: 10.3847/1538-3881/aa9791 Bibcode: 2018AJ....155....4M

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +11 more

Planets in young clusters are powerful probes of the evolution of planetary systems. Here we report the discovery of three planets transiting EPIC 247589423, a late-K dwarf in the Hyades (≃800 Myr) cluster, and robust detection limits for additional planets in the system. The planets were identified from their K2 light curves as part of our survey…

2018 The Astronomical Journal
Gaia 91
Molecular outflow and feedback in the obscured quasar XID2028 revealed by ALMA
DOI: 10.1051/0004-6361/201731641 Bibcode: 2018A&A...612A..29B

Lutz, D.; Daddi, E.; Sargent, M. T. +29 more

We imaged, with ALMA and ARGOS/LUCI, the molecular gas and dust and stellar continuum in XID2028, which is an obscured quasi-stellar object (QSO) at z = 1.593, where the presence of a massive outflow in the ionised gas component traced by the [OIII]5007 emission has been resolved up to 10 kpc. This target represents a unique test case to study QSO…

2018 Astronomy and Astrophysics
eHST 91