Search Publications

A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2
DOI: 10.3847/1538-3881/ab1cbd Bibcode: 2019AJ....158...20M

Brown, A. G. A.; Messineo, M.

We investigate individual distances and luminosities of a sample of 889 nearby candidate red supergiants (RSGs) with reliable parallaxes (ϖ/σ ϖ > 4 and RUWE < 2.7) from Gaia Data Release 2 (DR2). The sample was extracted from the historical compilation of spectroscopically derived spectral types by Skiff, and consists of K-M sta…

2019 The Astronomical Journal
Gaia eHST 26
Search for Nearby Earth Analogs. I. 15 Planet Candidates Found in PFS Data
DOI: 10.3847/1538-4365/ab1b16 Bibcode: 2019ApJS..242...25F

Butler, R. Paul; Crane, Jeffrey D.; Thompson, Ian B. +6 more

The radial velocity (RV) method plays a major role in the discovery of nearby exoplanets. To efficiently find planet candidates from the data obtained in high-precision RV surveys, we apply a signal diagnostic framework to detect RV signals that are statistically significant, consistent in time, robust in the choice of noise models, and do not cor…

2019 The Astrophysical Journal Supplement Series
Gaia 26
Simulating MOS science on the ELT: Lyα forest tomography
DOI: 10.1051/0004-6361/201936048 Bibcode: 2019A&A...632A..94J

Kaper, L.; Yang, Y.; Gendron, E. +14 more

Mapping the large-scale structure through cosmic time has numerous applications in studies of cosmology and galaxy evolution. At z ≳ 2, the structure can be traced by the neutral intergalactic medium (IGM) by way of observing the Lyα forest towards densely sampled lines of sight of bright background sources, such as quasars and star-forming galaxi…

2019 Astronomy and Astrophysics
eHST 26
An Enormous Molecular Gas Flow in the RX J0821+0752 Galaxy Cluster
DOI: 10.3847/1538-4357/aaf1b4 Bibcode: 2019ApJ...870...57V

Fabian, A. C.; Combes, F.; McDonald, M. +6 more

We present recent Chandra X-ray observations of the RX J0821.0+0752 galaxy cluster, in addition to ALMA observations of the CO(1-0) and CO(3-2) line emission tracing the molecular gas in its central galaxy. All of the CO line emission, originating from a {10}10 {M} molecular gas reservoir, is located several kiloparsecs awa…

2019 The Astrophysical Journal
eHST 26
SDSS-IV/SPIDERS: A catalogue of X-ray selected AGN properties. Spectral properties and black hole mass estimates for SPIDERS SDSS DR14 type 1 AGN
DOI: 10.1051/0004-6361/201833996 Bibcode: 2019A&A...625A.123C

Salvato, M.; Schulze, A.; Nandra, K. +7 more

This work presents the catalogue of optical spectral properties for all X-ray selected SPIDERS active galactic nuclei (AGN) up to SDSS DR14. SPIDERS (SPectroscopic IDentification of eROSITA Sources) is an SDSS-IV programme that is currently conducting optical spectroscopy of the counterparts to the X-ray selected sources detected in the ROSAT all-…

2019 Astronomy and Astrophysics
XMM-Newton eHST 26
New photometric analysis of five exoplanets: CoRoT-2b, HAT-P-12b, TrES-2b, WASP-12b, and WASP-52b
DOI: 10.1093/mnras/stz747 Bibcode: 2019MNRAS.486.2290O

Erdem, Ahmet; Öztürk, Oǧuz

We report 12, 11, 9, 10, and 8 new transit light curves of CoRoT-2b, HAT-P-12b, TrES-2b, WASP-12b, and WASP-52b, respectively, obtained at Çanakkale Onsekiz Mart University Observatory and TÜBİTAK National Observatory in 2016 and 2017. These transit light curves were analysed using JKTEBOP code. Planetary radii of CoRoT-2b, HAT-P-12b, TrES-2b, WAS…

2019 Monthly Notices of the Royal Astronomical Society
CoRoT 26
The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state
DOI: 10.1051/0004-6361/201935984 Bibcode: 2019A&A...628A..86B

Arnaud, M.; Pratt, G. W.; Bartalucci, I. +2 more

We study the dynamical state and the integrated total mass profiles of 75 massive (M500 > 5 × 1014 M) Sunyaev-Zeldovich(SZ)-selected clusters at 0.08 < z < 1.1. The sample is built from the Planck catalogue, with the addition of four SPT clusters at z > 0.9. Using XMM-Newton imaging observations, we ch…

2019 Astronomy and Astrophysics
XMM-Newton 26
The Planet Formation Potential around a 45 Myr Old Accreting M Dwarf
DOI: 10.3847/1538-4357/aaf794 Bibcode: 2019ApJ...872...92F

Hughes, A. Meredith; Murphy, Simon J.; Mamajek, Eric E. +1 more

Debris disk detections around M dwarfs are rare, and so far no gas emission has been detected from an M dwarf debris disk. This makes the 45 Myr old M dwarf WISE J080822.18-644357.3 a bit of a curiosity; it has a strong infrared excess at an age beyond the lifetime of a typical planet-forming disk, and also exhibits broad Hα emission consistent wi…

2019 The Astrophysical Journal
Gaia 26
Weak-lensing shear measurement with machine learning. Teaching artificial neural networks about feature noise
DOI: 10.1051/0004-6361/201833775 Bibcode: 2019A&A...621A..36T

Schrabback, T.; Hildebrandt, H.; Courbin, F. +3 more

Cosmic shear, that is weak gravitational lensing by the large-scale matter structure of the Universe, is a primary cosmological probe for several present and upcoming surveys investigating dark matter and dark energy, such as Euclid or WFIRST. The probe requires an extremely accurate measurement of the shapes of millions of galaxies based on imagi…

2019 Astronomy and Astrophysics
eHST 26
Linking surface morphology, composition, and activity on the nucleus of 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201833803 Bibcode: 2019A&A...630A...7F

Lamy, P. L.; Bertaux, J. -L.; Shi, X. +37 more


Aims: The Rosetta space probe accompanied comet 67P/Churyumov-Gerasimenko for more than two years, obtaining an unprecedented amount of unique data of the comet nucleus and inner coma. This has enabled us to study its activity almost continuously from 4 au inbound to 3.6 au outbound, including the perihelion passage at 1.24 au. This work focu…

2019 Astronomy and Astrophysics
Rosetta 26