8k citations · 8.8k across the 13 of their papers we have counts for
13 papers
SPIRITS 19q: Dust Production by a Subsolar-metallicity Carbon-rich Wolf-Rayet Star in NGC 2403
Sam Rose, Ryan M. Lau, Jacob E. Jencson +20
We present JWST/NIRSpec IFU observations of SPIRITS 19q, the highly dust-producing carbon-rich (WC) binary candidate located in a subsolar-metallicity region of the nearby spiral g…
Protoplanetary Disk Evolution in a Low-Metallicity Environment: JWST's First Mid-Infrared Census of Low-Mass Stars
Chikako Yasui, Natsuko Izumi, Masao Saito +3
This study presents the first high-resolution, high-sensitivity mid-infrared (MIR) investigation of protoplanetary disks in a low-metallicity environment, using JWST/NIRCam and MIR…
Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of Cen A. I. Observations, Orbital and Physical Properties, and Exozodi Upper Limits
Charles Beichman, Aniket Sanghi, Dimitri Mawet +27
We report on coronagraphic observations of the nearest solar-type star, Cen A, using the MIRI instrument on the James Webb Space Telescope. With three epochs of observation (Au…
Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of Cen A. II. Binary Star Modeling, Planet and Exozodi Search, and Sensitivity Analysis
Aniket Sanghi, Charles Beichman, Dimitri Mawet +14
JWST observed our closest solar twin, Cen A, with the MIRI coronagraph in F1550C (15.5 m) at three distinct epochs between August 2024 and April 2025. For the first time wit…
Rising from the Ashes: Mid-Infrared Re-Brightening of the Impostor SN 2010da in NGC 300
Ryan M. Lau, Mansi M. Kasliwal, Howard E. Bond +16
We present multi-epoch mid-infrared (IR) photometry and the optical discovery observations of the "impostor" supernova (SN) 2010da in NGC 300 using new and archival Spitzer Space T…
The Mid-Infrared Instrument for the James Webb Space Telescope, IX: Predicted Sensitivity
Alistair Glasse, G. H. Rieke, E. Bauwens +6
We present an estimate of the performance that will be achieved during on orbit operations of the JWST Mid Infrared Instrument, MIRI. The efficiency of the main imager and spectrom…
Thermal Model Calibration for Minor Planets Observed with WISE/NEOWISE: Comparison with IRAS
A. Mainzer, T. Grav, J. Masiero +5
With thermal infrared observations detected by the NEOWISE project, we have measured diameters for 1742 minor planets that were also observed by the Infrared Astronomical Satellite…
New Young Star Candidates in the Taurus-Auriga Region as Selected From WISE
L. M. Rebull, X. P. Koenig, D. L. Padgett +11
The Taurus Molecular Cloud subtends a large solid angle on the sky, in excess of 250 square degrees. The search for legitimate Taurus members to date has been limited by sky covera…
The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
Edward L. Wright, Peter R. M. Eisenhardt, Amy Mainzer +35
The all sky surveys done by the Palomar Observatory Schmidt, the European Southern Observatory Schmidt, and the United Kingdom Schmidt, the InfraRed Astronomical Satellite and the…
High Spatial Resolution Imaging of NGC 1068 in the Mid Infrared
J. J. Bock, G. Neugebauer, K. Matthews +6
Mid-infrared observations of the central source of NGC 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1" (~ 7pc). The central source is extended by…
APM 08279+5255: Keck Near- and Mid-IR High-Resolution Imaging
E. Egami, G. Neugebauer, B. T. Soifer +5
We present Keck high-resolution near-IR (2.2 microns; FWHM~0.15") and mid-IR (12.5 microns; FWHM~0.4") images of APM08279+5255, a z=3.91 IR-luminous BALQSO with a prodigious appare…
High Resolution Mid-Infrared Imaging of Ultraluminous Infrared Galaxies
B. T. Soifer, G. Neugebauer, K. Matthews +9
Observations of ultraluminous infrared galaxies (ULIRGs) with an achieved resolution approaching the diffraction limit in the mid-infrared from 8 - 25 m using the Keck Telescope…
High Resolution Infrared Imaging of the Compact Nuclear Source in NGC4258
R. Chary, E. E. Becklin, A. S. Evans +4
We present high resolution imaging of the nucleus of NGC4258 from 1 micron to 18 microns. Our observations reveal that the previously discovered compact source of emission is unres…