Results 111 to 120 of about 3,877 (212)
We present follow-up SCExAO/CHARIS H- and K -band ( R ∼ 70) high-contrast integral field spectroscopy and Keck/NIRC2 photometry of directly imaged brown dwarf companion HD 33632 Ab and new radial-velocity data for the system from the SOPHIE spectrograph,
Mona El Morsy +19 more
doaj +1 more source
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images. [PDF]
Seaton DB +7 more
europepmc +1 more source
The Apodized Pupil Lyot Coronagraph (APLC) is a diffraction suppression system installed in the recently deployed instruments Palomar/P1640, Gemini/GPI, and VLT/SPHERE to allow direct imaging and spectroscopy of circumstellar environments.
N'Diaye, Mamadou +2 more
core +2 more sources
Prototyping liquid-crystal coronagraphs for exo-Earth imaging
14 pages, 10 ...
Laginja, I. +14 more
openaire +3 more sources
Deepest Limits on Scattered Light Emission from the Epsilon Eridani Inner Debris Disk with HST/STIS
Epsilon Eridani is one of the first debris disk systems detected by the Infrared Astronomical Satellite. However, the system has thus far eluded detection in scattered light with no components having been directly imaged.
Sai Krishanth P. M. +11 more
doaj +1 more source
HPIC: The Habitable Worlds Observatory Preliminary Input Catalog
The Habitable Worlds Observatory Preliminary Input Catalog (HPIC) is a list of ∼13,000 nearby bright stars that will be potential targets for the Habitable Worlds Observatory (HWO) in its search for Earth-sized planets around Sun-like stars. We construct
Noah W. Tuchow +2 more
doaj +1 more source
"Troponinosis", the Cardiologist's Curse-When Clinic-Laboratory Interaction Unveils the Mystery: A Case Report. [PDF]
Bosi D +7 more
europepmc +1 more source
Imaging low-mass planets within the habitable zone of α Centauri. [PDF]
Wagner K +41 more
europepmc +1 more source
JWST/NIRCam Detection of the Fomalhaut C Debris Disk in Scattered Light
Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M dwarf debris disks have been studied in detail—making it unclear how or if ...
Kellen Lawson +22 more
doaj +1 more source

