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

被引:154
作者
Mas-Hesse, JM [1 ]
Giménez, A
Culhane, JL
Jamar, C
McBreen, B
Torra, J
Hudec, R
Fabregat, J
Meurs, E
Swings, JP
Alcacera, MA
Balado, A
Beiztegui, R
Belenguer, T
Bradley, L
Caballero, MD
Cabo, P
Defise, JM
Díaz, E
Domingo, A
Figueras, F
Figueroa, I
Hanlon, L
Hroch, F
Hudcova, V
García, T
Jordan, B
Jordi, C
Kretschmar, P
Laviada, C
March, M
Martín, E
Mazy, E
Menéndez, M
Mi, JM
de Miguel, E
Muñoz, T
Nolan, K
Olmedo, R
Plesseria, JY
Polcar, J
Reina, M
Renotte, E
Rochus, P
Sánchez, A
San Martín, JC
Smith, A
Soldan, J
Thomas, P
Timón, V
机构
[1] CSIC, INTA, Ctr Astrobiol, Torrejon De Ardoz 28850, Spain
[2] INTA, Lab Astrofis Espacial & Fis Fundamental, Madrid 28080, Spain
[3] European Space Agcy, Estec, Res & Sci Support Dept, NL-2200 AG Noordwijk, Netherlands
[4] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[5] Univ Liege, Ctr Spatial Liege, B-4031 Angleur, Belgium
[6] Natl Univ Ireland Univ Coll Dublin, Dept Expt Phys, Dublin 4, Ireland
[7] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
[8] Acad Sci Czech Republic, Inst Astron, CS-25165 Ondrejov, Czech Republic
[9] Univ Valencia, Dept Astron & Astrofis, E-46100 Burjassot, Spain
[10] Dublin Inst Adv Studies, Dunsink Observ, Dublin 15, Ireland
[11] Inst Estudis Espacials Catalunya, Barcelona 08034, Spain
[12] INTEGRAL Sci Data Ctr, CH-1290 Versoix, Switzerland
[13] Univ Liege, Inst Astron & Geophys, B-4000 Liege, Belgium
来源
ASTRONOMY & ASTROPHYSICS | 2003年 / 411卷 / 01期
关键词
instrumentation : photometers; space vehicles : instruments; techniques : photometric; stars : variables : general;
D O I
10.1051/0004-6361:20031418
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:L261 / L268
页数:8
相关论文
共 7 条
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