Results 11 to 20 of about 2,141 (221)

Macular pigment optical density measured by heterochromatic modulation photometry. [PDF]

open access: yesPLoS ONE, 2014
PURPOSE:To psychophysically determine macular pigment optical density (MPOD) employing the heterochromatic modulation photometry (HMP) paradigm by estimating 460 nm absorption at central and peripheral retinal locations. METHODS:For the HMP measurements,
Cord Huchzermeyer   +5 more
doaj   +7 more sources

Optical and Infrared Photometry of SN 2005df* [PDF]

open access: yesResearch Notes of the AAS, 2017
12 pages, 3 figures, to be published in Research Notes of the ...
Kevin Krisciunas   +5 more
openaire   +2 more sources

Modeling and Analysis of an Echo Laser Pulse Waveform for the Orientation Determination of Space Debris

open access: yesRemote Sensing, 2020
Orientation information of space debris is required to improve the orbital prediction accuracy for mitigation or elimination of a significant threat to not only human space activities but also operational satellites.
Hyung-Chul Lim   +6 more
doaj   +1 more source

Optical Photometry of GRB 021004: The First Month [PDF]

open access: yesThe Astronomical Journal, 2003
21 pages with five figures. Uses AASTEX 5.02. To appear in AJ.
Holland, S.T.   +19 more
openaire   +3 more sources

Optical and Infrared Photometry of the nearby SN 2017cbv [PDF]

open access: yesThe Astrophysical Journal, 2018
Abstract On 2017 March 11, the DLT40 Transient Discovery Survey discovered SN 2017cbv in NGC 5643, a Type 2 Seyfert Galaxy in the Lupus Constellation. SN 2017cbv went on to become a bright Type Ia supernova, with a V max of 11.51 ± 0.05 mag.
Jerrick Wee   +3 more
openaire   +2 more sources

Stellar Photometry with the Optical Monitors [PDF]

open access: yesInternational Astronomical Union Colloquium, 1993
AbstractThe Optical Monitors are small optical telescopes which will fly on board of the X-ray satellites SPECTRUM-X-GAMMA (JET-X experiment) and XMM. Their main scientific applications are the simultaneous observations (imaging) in the optical and UV band of the optical counterparts of X-ray sources, with limiting magnitudes of aboutmv=22(JET-X) and ...
E. Antonello, M. Cropper
openaire   +1 more source

DDO68 C: The Actual Appearance of a Ghost Satellite Dwarf through Adaptive Optics at the Large Binocular Telescope

open access: yesThe Astrophysical Journal Letters, 2023
Through adaptive optics (AO) imaging with the SOUL+LUCI instrument at the Large Binocular Telescope we were able to resolve, for the first time, individual stars in the gas-rich galaxy DDO68 C. This system was already suggested to be interacting with the
Francesca Annibali   +9 more
doaj   +1 more source

Optical and Radio Surface Photometry of NGC 891 [PDF]

open access: yesSymposium - International Astronomical Union, 1990
A general correlation between the radio and optical continuum surface brightness has been found in the edge-on galaxy NGC 891. This suggests that the relativistic electrons are produced/accelerated in the vicinity of evolved stars or stellar remnants which have a spatial distribution similar to old disk stars.
ALLEN, RJ   +3 more
openaire   +2 more sources

Multicolor photometry of the GRB970508 optical remnant [PDF]

open access: yesFourth Huntsville gamma-ray burst symposium, 1998
We report results of follow-up multicolor photometry of the optical variable source that is a probable remnant of the gamma-ray burst GRB970508 discovered by the BeppoSAX satellite (IAUC 6649). Observations were carried out in Johnson-Kron-Cousins $ BVR_cI_c system with the 1-m and 6-m telescopes of SAO RAS.
Sokolov, V. V.   +6 more
openaire   +2 more sources

The photometry of optical instruments [PDF]

open access: yesTransactions of the Optical Society, 1922
The use of a portable surface-brightness photometer of the polarisation type for the measurement of the fraction of the incident light transmitted by an optical instrument or reflected by a mirror or system of mirrors, and for the measurement of the relative brightness of different parts of the field of view of an optical instrument, is described.
openaire   +1 more source

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