Search Publications

GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
DOI: 10.1051/0004-6361/202346894 Bibcode: 2023A&A...680A..53M

Sturm, E.; Marconi, A.; Vignali, C. +44 more

The Gaia Multipeak (GMP) technique can be used to identify large numbers of dual or lensed active galactic nucleus (AGN) candidates at subarcsec separation, allowing us to study both multiple supermassive black holes (SMBHs) in the same galaxy and rare, compact lensed systems. The observed samples can be used to test the predictions of the models …

2023 Astronomy and Astrophysics
Gaia 13
Are JWST/NIRCam Color Gradients in the Lensed z = 2.3 Dusty Star-forming Galaxy El Anzuelo Due to Central Dust Attenuation or Inside-out Galaxy Growth?
DOI: 10.3847/1538-4357/aceb4a Bibcode: 2023ApJ...955...91K

Grogin, Norman A.; Koekemoer, Anton M.; Pirzkal, Nor +25 more

Gradients in the mass-to-light ratio of distant galaxies impede our ability to characterize their size and compactness. The long-wavelength filters of JWST's NIRCam offer a significant step forward. For galaxies at Cosmic Noon (z ~ 2), this regime corresponds to the rest-frame near-infrared, which is less biased toward young stars and captures emi…

2023 The Astrophysical Journal
Gaia eHST JWST 13
Ongoing hierarchical massive cluster assembly: The LISCA II structure in the Perseus complex
DOI: 10.1051/0004-6361/202346095 Bibcode: 2023A&A...674A..93D

Dalessandro, E.; Bellazzini, M.; Sanna, N. +7 more

We report on the identification of a massive (∼105 M) substructured stellar system in the Galactic Perseus complex likely undergoing hierarchical cluster assembly. This system comprises nine star clusters (including the well-known clusters NGC 654 and NGC 663) and an extended and low-density stellar halo. Gaia-DR3 and availa…

2023 Astronomy and Astrophysics
Gaia 13
Debris disk color with the Hubble Space Telescope
DOI: 10.1051/0004-6361/202245458 Bibcode: 2023A&A...672A.114R

Debes, John H.; Roberge, Aki; Schneider, Glenn +14 more

Context. Multiwavelength scattered light imaging of debris disks may inform dust properties including typical size and mineral composition. Existing studies have investigated a small set of individual systems across a variety of imaging instruments and filters, calling for uniform comparison studies to systematically investigate dust properties. <…

2023 Astronomy and Astrophysics
Gaia eHST 13
Investigating the M GCS-M h Relation in the Most Massive Galaxies
DOI: 10.3847/1538-4357/accbc3 Bibcode: 2023ApJ...950..179D

Harris, William E.; Dornan, Veronika

The relation between the total mass contained in the globular clusters of a galaxy and the mass of its dark-matter halo has been found observationally to be nearly linear over five decades of mass. However, the high-mass end of this relation is not well determined from previous data and shows large scatter. We analyze the globular cluster systems …

2023 The Astrophysical Journal
eHST 13
WIYN Open Cluster Study. LXXXVII. Hubble Space Telescope Ultraviolet Detection of Hot White Dwarf Companions to Blue Lurkers in M67
DOI: 10.3847/1538-4357/acb046 Bibcode: 2023ApJ...944..145N

Mathieu, Robert D.; Nine, Andrew C.; Gosnell, Natalie M. +1 more

We present the results of our Hubble Space Telescope far-ultraviolet survey of the blue lurkers (BLs) in M67. We find evidence for two white dwarf (WD) companions among the BLs that are indicative of mass transfer from an evolved companion, one in WOCS 14020 and the other in WOCS 3001. The cooling ages of the WDs suggest that mass transfer in thes…

2023 The Astrophysical Journal
Gaia eHST 13
Testing super-eddington accretion on to a supermassive black hole: reverberation mapping of PG 1119+120
DOI: 10.1093/mnras/stad1409 Bibcode: 2023MNRAS.523..545D

Ho, Luis C.; Horne, Keith; Du, Pu +11 more

We measure the black hole mass and investigate the accretion flow around the local (z = 0.0502) quasar PG 1119+120. Spectroscopic monitoring with Calar Alto provides H β lags and linewidths from which we estimate a black hole mass of log (M/M) = 7.0, uncertain by ~0.4 dex. High cadence photometric monitoring over 2 yr with …

2023 Monthly Notices of the Royal Astronomical Society
eHST 13
Improvement of Pan-STARRS Photometric Calibration with LAMOST and Gaia
DOI: 10.3847/1538-4365/acee73 Bibcode: 2023ApJS..268...53X

Huang, Bowen; Yuan, Haibo; Xiao, Kai +3 more

In this work, we perform the recalibration of Pan-STARRS1 (PS1) photometry by correcting for position-dependent systematic errors using the spectroscopy-based stellar color regression (SCR) method, the photometry-based SCR method, and the Gaia BP/RP synthetic photometry method. We confirm the significant large-scale and small-scale spatial variati…

2023 The Astrophysical Journal Supplement Series
Gaia 13
Linear Mode Decomposition in Magnetohydrodynamics Revisited
DOI: 10.3847/1538-4365/acdf5d Bibcode: 2023ApJS..268...18Z

Zank, G. P.; Zhao, L. -L.; Telloni, D. +4 more

Small-amplitude fluctuations in the magnetized solar wind are measured typically by a single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically expressed in terms of the fundamental modes admitted by the system. An important question is how to resolve an observed set of fluctuations, typically plasma moments such…

2023 The Astrophysical Journal Supplement Series
SolarOrbiter 13
A Single Ejection Model of the DART/Dimorphos Debris Trail
DOI: 10.3847/2041-8213/acfd1d Bibcode: 2023ApJ...956L..26K

Jewitt, David; Kim, Yoonyoung

The collision of the NASA DART spacecraft with asteroid Dimorphos resulted in the formation of a distinctive and long-lived debris trail, formed by the action of solar radiation pressure on ejected particles. This trail briefly displayed a double appearance, which has been interpreted as the result of a double ejection. We present a model that can…

2023 The Astrophysical Journal
eHST 13