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Differentiating modern and prebiotic Earth scenarios for TRAPPIST-1e: high-resolution transmission spectra and predictions for JWST
DOI: 10.1093/mnras/stab1486 Bibcode: 2021MNRAS.505.3562L

MacDonald, Ryan J.; Lin, Zifan; Kaltenegger, Lisa +1 more

The TRAPPIST-1 system is a priority target for terrestrial exoplanet characterization. TRAPPIST-1e, residing in the habitable zone, will be observed during the James Webb Space Telescope (JWST) GTO Program. Here, we assess the prospects of differentiating between prebiotic and modern Earth scenarios for TRAPPIST-1e via transmission spectroscopy. U…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 32
Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
DOI: 10.3847/1538-4357/abeb71 Bibcode: 2021ApJ...912..128P

Gabor, P.; Smith, N.; Rest, A. +35 more

With the conclusion of the third observing run for Advanced LIGO/Virgo (O3), we present a detailed analysis of both triggered and serendipitous observations of 17 gravitational-wave (GW) events (7 triggered and 10 purely serendipitous) from the Searches After Gravitational-waves Using ARizona Observatories (SAGUARO) program. We searched a total of…

2021 The Astrophysical Journal
Gaia 32
Towards a volumetric census of close white dwarf binaries - I. Reference samples
DOI: 10.1093/mnras/stab753 Bibcode: 2021MNRAS.504.2420I

Pala, A. F.; Breedt, E.; Marsh, T. R. +3 more

Close white dwarf binaries play an important role across a range of astrophysics, including thermonuclear supernovae, the Galactic low-frequency gravitational wave signal, and the chemical evolution of the Galaxy. Progress in developing a detailed understanding of the complex, multithreaded evolutionary pathways of these systems is limited by the …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 32
The origin of reconnection-mediated transient brightenings in the solar transition region
DOI: 10.1038/s41550-020-01263-2 Bibcode: 2021NatAs...5..237B

Winebarger, Amy R.; Bahauddin, Shah Mohammad; Bradshaw, Stephen J.

The ultraviolet emission from the solar transition region is dominated by dynamic, low-lying magnetic loops. The enhanced spatial and temporal resolution of the solar observation satellite Interface Region Imaging Spectrograph (IRIS) has made it possible to study these structures in fine detail. IRIS has observed `transient brightenings' in these …

2021 Nature Astronomy
IRIS 32
Hot Subdwarf Atmospheric Parameters, Kinematics, and Origins Based on 1587 Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR7
DOI: 10.3847/1538-4365/ac11f6 Bibcode: 2021ApJS..256...28L

Han, Zhanwen; Luo, Yangping; Németh, Péter +2 more

Based on the Gaia DR2 catalog of hot subdwarf star candidates, we identified 1587 hot subdwarf stars with spectra in LAMOST DR7. We present atmospheric parameters for these stars by fitting the LAMOST spectra with TLUSTY/SYNSPEC non-LTE synthetic spectra. Combining LAMOST radial velocities and Gaia Early Data Release 3 (EDR3) parallaxes and proper…

2021 The Astrophysical Journal Supplement Series
Gaia 32
TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes
DOI: 10.3847/1538-3881/ac02bd Bibcode: 2021AJ....162...62D

Batalha, Natalie M.; Latham, David W.; Rice, Malena +48 more

We report the discovery of TOI-1444b, a 1.4 R super-Earth on a 0.47 day orbit around a Sun-like star discovered by TESS. Precise radial velocities from Keck/HIRES confirmed the planet and constrained the mass to be 3.87 ± 0.71M. The RV data set also indicates a possible nontransiting, 16 day planet (11.8 ± 2.9M)…

2021 The Astronomical Journal
Gaia 32
The GAPS Programme at TNG. XXVIII. A pair of hot-Neptunes orbiting the young star TOI-942
DOI: 10.1051/0004-6361/202039042 Bibcode: 2021A&A...645A..71C

Baratella, M.; Mallonn, M.; Scandariato, G. +48 more

Context. Young stars and multi-planet systems are two types of primary objects that allow us to study, understand, and constrain planetary formation and evolution theories.
Aims: We validate the physical nature of two Neptune-sized planets transiting TOI-942 (TYC 5909-319-1), a previously unacknowledged young star (50-20+30

2021 Astronomy and Astrophysics
Gaia Hipparcos 32
The Complex Organic Molecular Content in the L1498 Starless Core
DOI: 10.3847/1538-4357/ac024c Bibcode: 2021ApJ...917...44J

Caselli, Paola; Viti, Serena; Jiménez-Serra, Izaskun +3 more

Observations carried out toward starless and prestellar cores have revealed that complex organic molecules are prevalent in these objects, but it is unclear what chemical processes are involved in their formation. Recently, it has been shown that complex organics are preferentially produced at an intermediate-density shell within the L1544 prestel…

2021 The Astrophysical Journal
Herschel 32
Galaxy Mergers up to z < 2.5. II. AGN Incidence in Merging Galaxies at Separations of 3-15 kpc
DOI: 10.3847/1538-4357/abdbb1 Bibcode: 2021ApJ...909..124S

Marchesini, Danilo; Iono, Daisuke; Silverman, John D. +4 more

We present a study of the incidence of active galactic nucleus (AGN) in a sample of major merging systems at 0.3 < z < 2.5. Galaxies in this merger sample have projected separations between 3 and 15 kpc and are selected from the CANDELS/3D-Hubble Space Telescope catalogs using a peak-finding algorithm. AGNs in mergers and non-mergers are ide…

2021 The Astrophysical Journal
eHST 32
WISDOM Project - IX. Giant molecular clouds in the lenticular galaxy NGC 4429: effects of shear and tidal forces on clouds
DOI: 10.1093/mnras/stab1537 Bibcode: 2021MNRAS.505.4048L

Davis, Timothy A.; Bureau, Martin; Iguchi, Satoru +5 more

We present high spatial resolution (≈12 pc) Atacama Large Millimeter/submillimeter Array 12CO(J = 3-2) observations of the nearby lenticular galaxy NGC 4429. We identify 217 giant molecular clouds within the 450 pc radius molecular gas disc. The clouds generally have smaller sizes and masses but higher surface densities and observed lin…

2021 Monthly Notices of the Royal Astronomical Society
eHST 32