PHOTOMETRY OF CENTRAL PARTS OF M33 GALAXY IN NEAR INFRARED

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NIKZAT FATEME; MIRTORABI MOHAMMAD TAGHI

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Journal: JOURNAL OF SCIENCE (KHARAZMI UNIVERSITY) Year:2011 | Volume:11 | Issue:3 Page(s): 187-196

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Information Journal Paper

Title

PHOTOMETRY OF CENTRAL PARTS OF M33 GALAXY IN NEAR INFRARED

Author(s)

NIKZAT FATEME | MIRTORABI MOHAMMAD TAGHI | Issue Writer Certificate

Keywords

M33 GALAXYQ2

PHOTOMETRYQ2

POINT SPREAD FUNCTIONQ2

Abstract

In this paper, we analyze, near infra-red images of the central region of the local group galaxy M33. These images were obtained in K band with the UFTI instrument, installed on the UKIRT telescope. This is a part of a bigger project started in 2003 with an aim to investigate RGB and AGB stars in M33. K band magnitude was obtained for 18509 stars by fitting appropriate PSF models to stellar profiles in the images. ‎The ‎final ‎catalogue ‎was ‎obtained ‎by calibrating ‎instrumental ‎magnitude ‎to ‎standard‎ ‎system.‎ Cross correlation methods was manipulated to assign J-K color index to each star. A color magnitude diagram was plotted which represents population of RGB, AGB and Carbon stars in the core of M33 GALAXY.

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APA: Copy

NIKZAT, FATEME, & MIRTORABI, MOHAMMAD TAGHI. (2011). PHOTOMETRY OF CENTRAL PARTS OF M33 GALAXY IN NEAR INFRARED. JOURNAL OF SCIENCE (KHARAZMI UNIVERSITY), 11(3), 187-196. SID. https://sid.ir/paper/43964/en

Vancouver: Copy

NIKZAT FATEME, MIRTORABI MOHAMMAD TAGHI. PHOTOMETRY OF CENTRAL PARTS OF M33 GALAXY IN NEAR INFRARED. JOURNAL OF SCIENCE (KHARAZMI UNIVERSITY)[Internet]. 2011;11(3):187-196. Available from: https://sid.ir/paper/43964/en

IEEE: Copy

FATEME NIKZAT, and MOHAMMAD TAGHI MIRTORABI, “PHOTOMETRY OF CENTRAL PARTS OF M33 GALAXY IN NEAR INFRARED,” JOURNAL OF SCIENCE (KHARAZMI UNIVERSITY), vol. 11, no. 3, pp. 187–196, 2011, [Online]. Available: https://sid.ir/paper/43964/en

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