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Stellar-reddening-based Extinction Maps for Cosmological Applications
DOI: 10.3847/1538-4357/acc32c Bibcode: 2023ApJ...949...47M

Finkbeiner, Douglas P.; Mudur, Nayantara; Park, Core Francisco

Cosmological surveys must correct their observations for the reddening of extragalactic objects by Galactic dust. Existing dust maps, however, have been found to have spatial correlations with the large-scale structure of the Universe. Errors in extinction maps can propagate systematic biases into samples of dereddened extragalactic objects and in…

2023 The Astrophysical Journal
Gaia 5
The Large Deficit of HMXB Emission from Luminous Infrared Galaxies: The Case of the Circumnuclear Starburst Ring in NGC 7552
DOI: 10.3847/1538-4357/acd9aa Bibcode: 2023ApJ...952...22W

Zezas, Andreas; Roberts, Timothy P.; West, Lacey +5 more

Luminous infrared galaxies (LIRGs), the most extreme star-forming galaxies in the nearby (D < 30 Mpc) universe, show a notable X-ray emission deficiency (up to a factor of ~10) compared with predictions from scaling relations of galaxy-wide high-mass X-ray binary (HMXB) luminosity with star formation rate. In the nearby (≈20 Mpc) LIRG NGC 7552,…

2023 The Astrophysical Journal
eHST 5
Intriguing Plasma Composition Pattern in a Solar Active Region: A Result of Nonresonant Alfvén Waves?
DOI: 10.3847/1538-4357/ad05bf Bibcode: 2023ApJ...959...72M

Stangalini, Marco; Long, David M.; Brooks, David H. +6 more

The plasma composition of the solar corona is different from that of the solar photosphere. Elements that have a low first ionization potential (FIP) are preferentially transported to the corona and therefore show enhanced abundances in the corona compared to the photosphere. The level of enhancement is measured using the FIP bias parameter. In th…

2023 The Astrophysical Journal
Hinode 5
How Magnetic Reconnection May Affect the Coherence of Interplanetary Coronal Mass Ejections
DOI: 10.3847/1538-4357/acdcf7 Bibcode: 2023ApJ...953...15F

Farrugia, C. J.; Galvin, A. B.; Davies, E. E. +12 more

On 2020 April 19-20, a solar ejection was seen by spacecraft in a radial alignment that included Solar Orbiter and Wind. The ejection contained a magnetic flux rope where magnetic field and plasma parameters were well correlated between spacecraft. This structure is called an "unperturbed magnetic flux rope" (UMFR). Ahead of the UMFR is a portion …

2023 The Astrophysical Journal
SolarOrbiter 5
Internal Calibration of LAMOST and Gaia DR3 GSP-Spec Stellar Abundances
DOI: 10.3847/1538-4357/accf8b Bibcode: 2023ApJ...950..104N

Niu, Zexi; Liu, Jifeng; Yuan, Haibo

Stellar chemical abundances are crucial and fundamental in astrophysics. However, they could suffer from substantial systematic errors according to several investigations but still lack calibrations in bulk. By using Gaia wide binaries, we find the temperature-dependent bias between the two binary components for [Fe/H] and [α/Fe] measurements from…

2023 The Astrophysical Journal
Gaia 5
The Binary and the Disk: The Beauty is Found within NGC3132 with JWST
DOI: 10.3847/1538-4357/aca7ba Bibcode: 2023ApJ...943..110S

Sahai, Raghvendra; Bujarrabal, Valentin; Quintana-Lacaci, Guillermo +4 more

The planetary nebula (PN) NGC 3132 is a striking example of the dramatic but poorly understood mass-loss phenomena that (1-8) M stars undergo during their death throes as they evolve into white dwarfs (WDs). From an analysis of JWST multiwavelength (0.9-18 µm) imaging of NGC 3132, we report the discovery of an extended dust clou…

2023 The Astrophysical Journal
Gaia eHST JWST 5
The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO/SWAN
DOI: 10.3847/1538-4357/acda8c Bibcode: 2023ApJ...952....2B

Bzowski, M.; Quémerais, E.; Kubiak, M. A. +3 more

Interstellar neutral hydrogen flows into the heliosphere as a mixture of the primary and secondary populations from two somewhat different directions due to splitting occurring in the magnetized outer heliosheath. The direction of the inflow of interstellar neutral H observed in the inner heliosphere, confronted with that of the unperturbed flow o…

2023 The Astrophysical Journal
SOHO 5
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei
DOI: 10.3847/1538-4357/acb4e9 Bibcode: 2023ApJ...945..121U

Fujimoto, Seiji; Kohno, Kotaro; Sun, Fengwu +10 more

We report the multiwavelength properties of millimeter galaxies hosting X-ray detected active galactic nuclei (AGNs) from the ALMA Lensing Cluster Survey (ALCS). ALCS is an extensive survey of well-studied lensing clusters with ALMA, covering an area of 133 arcmin2 over 33 clusters with a 1.2 mm flux-density limit of ~60 µJy (1σ).…

2023 The Astrophysical Journal
Herschel eHST 5
NuSTAR Observations of a Heavily X-Ray-obscured AGN in the Dwarf Galaxy J144013+024744
DOI: 10.3847/1538-4357/ac9382 Bibcode: 2023ApJ...942...82A

Trump, Jonathan R.; Brandt, W. N.; Swartz, Douglas A. +10 more

We present a multiwavelength analysis of the dwarf Seyfert 2 galaxy J144013+024744, a candidate obscured active galactic nucleus (AGN) thought to be powered by an intermediate-mass black hole (IMBH, M ≈ 104-106 M ) of mass M ~ 105.2 M . To study its X-ray properties…

2023 The Astrophysical Journal
XMM-Newton 5
Modulation of Cosmic-Ray Antiprotons in the Heliosphere: Simulations for a Solar Cycle
DOI: 10.3847/1538-4357/ace31e Bibcode: 2023ApJ...953..101A

Luo, Xi; Potgieter, M. S.; Aslam, O. P. M. +1 more

The precision measurements of galactic cosmic-ray protons from the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics and the Alpha Magnetic Spectrometer are reproduced using a well-established three-dimensional numerical model for the period 2006 July-2019 November. The resulting modulation parameters are applied to simulate …

2023 The Astrophysical Journal
Ulysses 5