... Create small regions of about 100 sq. arcmin sort all objects within these regions by magnitude create an histogram index of these regions, i.e., pointer to first object and number of objects within a magnitude bin. ...
... We selected mB , b ecause: (i) it yields good correlation with GSC magnitudes, (ii) it is more representative in RC3 than other magnitudes, and (iii) it is close to the system used in the stellar distribution. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/malkovo.pdf -- 961.7 Кб -- 14.01.1998 Похожие документы
... The goal is to get positions accurate to 20 mas for stars in the 8-14 m magnitude range, and about 70 mas at the limiting magnitude (Zacharias 1997). ...
... Figure 1 shows how scat was used iteratively by searching the PPM catalog to get 2000 positions, the 2MASS Point Source Catalog to get JHK infrared magnitudes, and the Hipparcos Catalog (ESA 1997) to get distance and V magnitudes. ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/O8-5.pdf -- 206.8 Кб -- 11.03.2003 Похожие документы
... 3. First Experiments . 3.1. Magnitude/Jansky Converter . 3.2. Archive Data Preview . 4. ... As a working example, we developed the Magnitude/Flux/Jansky Converter. ...
... The stellar B magnitudes are indicated. ... the plates by using a number of stars in the field with known broadband magnitudes ... The derived blue continuum magnitude of HBV 475 is indicated. 2. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P1-4.pdf -- 113.9 Кб -- 27.08.2004 Похожие документы
... Time to Photometric Magnitude To compute a limiting magnitude without reprocessing ... or LMC for Limiting Magnitude Calculator) is able to convert magnitude between bands ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-2.pdf -- 74.8 Кб -- 27.08.2004 Похожие документы