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From the 1 of 7 papers with an AI index.

most citedRobust AGN and host-galaxy decomposition in optical spectral fitting

1 citations

7 papers

astro-ph.EP2026

SaNDi-SHoP: Searching for Satellites'N'Disks with a Star-Hopping Program II. Spectrophotometric analysis and orbital monitoring of directly imaged companions

Andrea Bernardi, Alice Zurlo, Cecilia Lazzoni +7

The paper presents new near‑infrared photometry, low‑resolution spectra, and high‑precision astrometry for thirteen directly imaged planetary and brown‑dwarf companions observed wi…

astro-ph.EP2026

Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66

Jinghuai Yao, Ke Zhang, Andrea Banzatti +10

We present JWST/MIRI Medium Resolution Spectrometer spectra of the wide-separation (projected separation au) binary protoplanetary disks Sz 65 (K7; ) and Sz…

astro-ph.GA2026

Seeing through the dust: Unraveling near-infrared variability in type 2 active galactic nuclei

J. Cerón-Meneses, P. Arévalo, P. Sánchez-Sáez +3

Near-infrared (NIR) variability studies of active galactic nuclei (AGNs) are still limited, as long-term multiepoch monitoring in the NIR is observationally challenging. The depth,…

astro-ph.SR2026

First Detection of HC5N in a Class II Disk around TW Hya

Steven C. Wampler, Ryan A. Loomis, Amina Diop +9

Over the last decade of ALMA's operation the molecular inventory of protoplanetary disks has expanded rapidly, revealing a diverse set of nitrogen-bearing organics and carbon-chain…

astro-ph.GA2026

ODIN: Clustering Properties of Ly Blobs at 2.4 and 3.1

Byeongha Moon, Yujin Yang, Eric Gawiser +18

Spatially extended Ly nebulae, known as Ly blobs (LABs), are a rare population at that are thought to trace proto-groups or the progenitors of massive galaxies in t…

astro-ph.EP2026

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) XI: Gas-dust interactions and radial offsets between micron and millimetre-sized grains

J. Olofsson, M. R. Jankovic, S. Marino +22

The dust observed in debris disks is the result of a collisional cascade initiated from km-sized parent bodies. Using near-infrared to sub-millimeter observations, we can pr…