Search Publications

Background Short-period Eclipsing Binaries in the Original Kepler Field
DOI: 10.3847/1538-4365/ac10c0 Bibcode: 2021ApJS..256...11B

Bódi, Attila; Szabó, Róbert; Forró, Adrienn +2 more

During the primary Kepler mission, between 2009 and 2013, about 150,000 preselected targets were observed with a 29.42 minute long cadence. However, a survey of background stars that fall within the field of view (FOV) of the downloaded apertures of the primary targets has revealed a number of interesting objects. In this paper, we present the res…

2021 The Astrophysical Journal Supplement Series
Gaia 8
Resolving the inner accretion flow towards the central supermassive black hole in SDSS J1339+1310
DOI: 10.1051/0004-6361/202038770 Bibcode: 2021A&A...646A.165S

Goicoechea, L. J.; Sergeyev, A. V.; Shalyapin, V. N. +2 more

We studied the accretion disc structure in the doubly imaged lensed quasar SDSS J1339+1310 using r-band light curves and UV-visible to near-IR spectra from the first 11 observational seasons after its discovery. The 2009-2019 light curves displayed pronounced microlensing variations on different timescales, and this microlensing signal permitted u…

2021 Astronomy and Astrophysics
eHST 8
X-Ray Evidence Against the Hypothesis that the Hyperluminous z = 6.3 Quasar J0100+2802 is Lensed
DOI: 10.3847/2041-8213/ac37b5 Bibcode: 2021ApJ...922L..24C

Connor, Thomas; Stern, Daniel; Bañados, Eduardo +1 more

The z = 6.327 quasar SDSS J010013.02+280225.8 (hereafter J0100+2802) is believed to be powered by a black hole more massive than 1010 M , making it the most massive black hole known in the first billion years of the universe. However, recent high-resolution ALMA imaging shows four structures at the location of this quasar, p…

2021 The Astrophysical Journal
XMM-Newton 8
Diagnosing Open Cluster Stock 2: Member Candidates and Mass Distribution with Gaia DR2 and LAMOST
DOI: 10.3847/1538-3881/abc61a Bibcode: 2021AJ....161....8Y

Bird, Sarah A.; Zhao, Gang; Liu, Chao +5 more

We identify 1325 member candidates of the open cluster (OC) Stock 2 using data from Gaia DR2. We use the algorithms Clusterix 2.0 and HDBSCAN to select cluster candidates and further refine the final cluster membership by defining neighbors in 5D phase space (Xcp, Ycp, ${Z}_{\mathrm{cp}},\kappa \cdot {\mu }_{\alpha }^{* }$ /ϖ…

2021 The Astronomical Journal
Gaia 8
Observational constraints to the dynamics of dust particles in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stab1152 Bibcode: 2021MNRAS.504.4687F

Sierks, H.; Fulle, M.; Güttler, C. +18 more

In this work, we aim to characterize the dust motion in the inner coma of comet 67P/Churyumov-Gerasimenko to provide constraints for theoretical 3D coma models. The OSIRIS camera on-board the Rosetta mission was able for the first time to acquire images of single dust particles from inside the cometary coma, very close to the nucleus. We analyse a…

2021 Monthly Notices of the Royal Astronomical Society
Rosetta 8
The VVV open cluster project. Near-infrared sequences of NGC 6067, NGC 6259, NGC 4815, Pismis 18, Trumpler 23, and Trumpler 20
DOI: 10.1093/mnras/stab328 Bibcode: 2021MNRAS.503.1864P

Peña Ramírez, K.; Chené, A. -N.; Ramírez Alegría, S. +1 more

Open clusters are central elements of our understanding of the Galactic disc evolution, as an accurate determination of their parameters leads to an unbiased picture of our Galaxy's structure. Extending the analysis towards fainter magnitudes in cluster sequences has a significant impact on the derived fundamental parameters, such as extinction an…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 8
Associated Molecular and Atomic Clouds with X-Ray Shell of Superbubble 30 Doradus C in the LMC
DOI: 10.3847/1538-4357/ac0adb Bibcode: 2021ApJ...918...36Y

Filipović, M. D.; Aharonian, F.; Rowell, G. +20 more

30 Doradus C is a superbubble that emits the brightest non-thermal X- and TeV gamma-rays in the Local Group. To explore the detailed connection between the high-energy radiation and the interstellar medium, we have carried out new CO and HI observations using the Atacama Large Millimeter/Submillimeter Array (ALMA), Atacama Submillimeter Telescope …

2021 The Astrophysical Journal
XMM-Newton 8
The Hubble PanCET program: Transit and Eclipse Spectroscopy of the Hot-Jupiter WASP-74b
DOI: 10.3847/1538-3881/ac3008 Bibcode: 2021AJ....162..271F

Deming, Drake; Nikolov, Nikolay; Mikal-Evans, Thomas +12 more

Planets are like children with each one being unique and special. A better understanding of their collective properties requires a deeper understanding of each planet. Here we add the transit and eclipse spectra of hot-Jupiter WASP-74b into the ever growing data set of exoplanet atmosphere spectral library. With six transits and three eclipses usi…

2021 The Astronomical Journal
eHST 8
Candidate z ∼ 2.5 Lyman Continuum Sources in the GOODS Fields
DOI: 10.3847/1538-4357/abd5b8 Bibcode: 2021ApJ...908..222J

Barger, A. J.; Cowie, L. L.; Jones, L. H.

We use the wealth of deep archival optical spectroscopy on the GOODS-South field from Keck, the VLT, and other facilities to select candidate high-redshift Lyman continuum (LyC) leakers in the Hubble Deep UV Legacy Survey (HDUV) data set. We select sources at $2.35\lt z\lt 3.05$ , where the HST/WFC3 F275W filter probes only the redshifted LyC. We …

2021 The Astrophysical Journal
eHST 8
Revisiting the formation mechanism for coronal rain from previous studies
DOI: 10.1088/1674-4527/21/10/255 Bibcode: 2021RAA....21..255L

Peter, Hardi; Chitta, Lakshmi Pradeep; Li, Le-Ping +1 more

Solar coronal rain is classified generally into two categories: flare-driven and quiescent coronal rain. Th latter is observed to form along both closed and open magnetic field structures. Recently, we proposed that some of the quiescent coronal rain events, detected in the transition region and chromospheric diagnostics, along loop-like paths cou…

2021 Research in Astronomy and Astrophysics
IRIS 8