Search Publications

DIAmante TESS AutoRegressive Planet Search (DTARPS). I. Analysis of 0.9 Million Light Curves
DOI: 10.3847/1538-3881/ad29f0 Bibcode: 2024AJ....167..202M

Feigelson, Eric D.; Montalto, Marco; Melton, Elizabeth J. +3 more

Nearly one million light curves from the TESS Year 1 southern hemisphere extracted from Full Field Images with the DIAmante pipeline are processed through the AutoRegressive Planet Search statistical procedure. ARIMA models remove lingering autocorrelated noise, the Transit Comb Filter identifies the strongest periodic signal in the light curve, a…

2024 The Astronomical Journal
Gaia 7
Effects of density and temperature variations on the metallicity of Mrk 71
DOI: 10.1038/s41550-024-02198-8 Bibcode: 2024NatAs...8..275M

Kreckel, Kathryn; Esteban, César; García-Rojas, Jorge +2 more

In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII] collisional excited lines (CELs) and the OII recombination lines (RLs) in the star forming galaxy Mrk71. In t…

2024 Nature Astronomy
Herschel 7
First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA
DOI: 10.1051/0004-6361/202348868 Bibcode: 2024A&A...692A.237Z

Maitra, Chandreyee; Koribalski, Bärbel S.; Sasaki, Manami +11 more

Aims. The all-sky survey carried out by the extended Roentgen Survey with an Imaging Telescope Array (eROSITA) on board Spektrum-Roentgen-Gamma (Spektr-RG, SRG) has provided spatially and spectrally resolved X-ray data of the entire Large Magellanic Cloud (LMC) and its immediate surroundings in the soft X-ray band down to 0.2 keV, with an average …

2024 Astronomy and Astrophysics
XMM-Newton 7
Host-star Properties of Hot, Warm, and Cold Jupiters in the Solar Neighborhood from Gaia Data Release 3: Clues to Formation Pathways
DOI: 10.3847/1538-3881/ad429f Bibcode: 2024AJ....168....7B

Henning, Thomas; Manoj, P.; Narang, Mayank +5 more

Giant planets exhibit diverse orbital properties, hinting at their distinct formation and dynamic histories. In this paper, using Gaia Data Release 3 (DR3), we investigate if and how the orbital properties of Jupiters are linked to their host star properties, particularly their metallicity and age. We obtain metallicities for main-sequence stars o…

2024 The Astronomical Journal
Gaia 7
NOEMA reveals the true nature of luminous red JWST z > 10 galaxy candidates
DOI: 10.1051/0004-6361/202348306 Bibcode: 2024A&A...681L...3M

Walter, F.; Oesch, P. A.; Barrufet, L. +3 more

The first year of JWST has revealed a surprisingly large number of luminous galaxy candidates beyond z > 10. While some galaxies have already been spectroscopically confirmed, there is mounting evidence that a subsample of the candidates with particularly red inferred UV colours are, in fact, lower redshift contaminants. These interlopers are o…

2024 Astronomy and Astrophysics
eHST JWST 7
Not-so-fast Kepler-1513: a perturbing planetary interloper in the exomoon corridor
DOI: 10.1093/mnras/stad3070 Bibcode: 2024MNRAS.527..620Y

Dalba, Paul A.; McLeod, Kim K.; Nesvorný, David +9 more

Transit timing variations (TTVs) can be induced by a range of physical phenomena, including planet-planet interactions, planet-moon interactions, and stellar activity. Recent work has shown that roughly half of moons would induce fast TTVs with a short period in the range of 2-4 orbits of its host planet around the star. An investigation of the Ke…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Characterizing the Rapid Hydrogen Disappearance in SN 2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
DOI: 10.3847/1538-4357/ad710e Bibcode: 2024ApJ...974..316D

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Modjaz, Maryam +52 more

We present optical and near-infrared (NIR) observations of SN 2022crv, a stripped-envelope supernova in NGC 3054, discovered within 12 hr of explosion by the Distance Less Than 40 Mpc Survey. We suggest that SN 2022crv is a transitional object on the continuum between Type Ib supernovae (SNe Ib) and Type IIb supernovae (SNe IIb). A high-velocity h…

2024 The Astrophysical Journal
eHST 7
Extended Lyman-α emission towards the SPT2349-56 protocluster at z = 4.3
DOI: 10.1051/0004-6361/202245785 Bibcode: 2024A&A...683A..64A

Anguita, Timo; Spilker, Justin; Aravena, Manuel +20 more

Context. Deep spectroscopic surveys with the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed that some of the brightest infrared sources in the sky correspond to concentrations of submillimeter galaxies (SMGs) at high redshift. Among these, the SPT2349-56 protocluster system is amongst the most extreme examples given its high sou…

2024 Astronomy and Astrophysics
eHST 7
The GALAH survey: tracing the Milky Way's formation and evolution through RR Lyrae stars
DOI: 10.1093/mnras/stae1149 Bibcode: 2024MNRAS.531..137D

Lewis, Geraint F.; Casey, Andrew R.; Matsunaga, Noriyuki +39 more

Stellar mergers and accretion events have been crucial in shaping the evolution of the Milky Way (MW). These events have been dynamically identified and chemically characterized using red giants and main-sequence stars. RR Lyrae (RRL) variables can play a crucial role in tracing the early formation of the MW since they are ubiquitous, old (t ≥ 10 …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
ALMA Lensing Cluster Survey: Full Spectral Energy Distribution Analysis of z ∼ 0.5–6 Lensed Galaxies Detected with millimeter Observations
DOI: 10.3847/1538-4357/ad26f7 Bibcode: 2024ApJ...965..108U

Koekemoer, Anton M.; Smail, Ian; Fujimoto, Seiji +17 more

Sub/millimeter galaxies are a key population for the study of galaxy evolution because the majority of star formation at high redshifts occurred in galaxies deeply embedded in dust. To search for this population, we have performed an extensive survey with Atacama Large Millimeter/submillimeter Array (ALMA), called the ALMA Lensing Cluster Survey (…

2024 The Astrophysical Journal
Herschel eHST 7