6533b883fe1ef96bd12ddf4f

RESEARCH PRODUCT

OMC: An Optical Monitoring Camera for INTEGRAL - Instrument description and performance

J. M. Mas-hesseA. GimenezJ. L. CulhaneClaude JamarB. McbreenJ. TorraR. HudecJ. FabregatE. MeursJean-pierre SwingsM. A. AlcaceraA. BaladoR. BeizteguiT. BelenguerL. BradleyM. D. CaballeroP. CaboJean-marc DefiseE. DiazA. DomingoF. FiguerasI. FigueroaL. HanlonF. HrochV. HudcovaT. GarciaB. JordanC. JordiP. KretschmarC. LaviadaM. MarchE. MartinEmmanuel MazyM. MenendezJ. M. MiE. De MiguelT. MunozK. NolanR. OlmedoJean-yves PlesseriaJ. PolcarM. ReinaEtienne RenottePierre RochusA. SanchezJ. C. San MartinA. SmithJ. SoldanPierre ThomasV. TimonD. Walton

subject

Physical chemical mathematical & earth Sciencesstars : variables : generalPhysique chimie mathématiques & sciences de la terreEarth sciences & physical geographyinstrumentation : photometerstechniques : photometricspace vehicles : instrumentsSciences de la terre & géographie physique

description

The Optical Monitoring Camera (OMC) will observe the optical emission from the prime targets of the gammaray instruments onboard the ESA mission INTEGRAL, with the support of the JEM-X monitor in the X-ray domain. This capability will provide invaluable diagnostic information on the nature and the physics of the sources over a broad wavelength range. Its main scientific objectives are: ( 1) to monitor the optical emission from the sources observed by the gamma- and X-ray instruments, measuring the time and intensity structure of the optical emission for comparison with variability at high energies, and ( 2) to provide the brightness and position of the optical counterpart of any gamma- or X-ray transient taking place within its field of view. The OMC is based on a refractive optics with an aperture of 50 mm focused onto a large format CCD (1024 x 2048 pixels) working in frame transfer mode (1024 x 1024 pixels imaging area). With a field of view of 5degrees x 5degrees it will be able to monitor sources down to magnitude V = 18. Typical observations will perform a sequence of different integration times, allowing for photometric uncertainties below 0.1 mag for objects with V less than or equal to 16.

10.1051/0004-6361:20031418https://hdl.handle.net/2268/18170