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Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

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Page 1: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Fan Zhou

Profs Jun Ma and Xu Zhou

BATC Group,NAOC

The BATC Multicolor Photometric Study of M31 Globular Clusters

Page 2: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The BATC Multicolor Photometry System

The Bejing-Arizona-Taiwan-Connecticut (BATC) group was created by Academician Chen J.-S. 15 years ago.

60/90 cm f/3 Schmidt Telescope at Xionglong.

>12e

<4e

RON

<5%15um/pixel 1.7"/pixel

58’×58’2K × 2KOld Thick

 92.2%12um/pixel 1.3"/pixel

90’×90’4K × 4KNew E2V

BQE(~400nm)Pixel ScaleFOVSize

Page 3: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The BATC intermediate band filters

• The BATC multicolor photometric system includes 15 intermediate band filters, covering the total optical wavelength range from ~3000 to ~10000Å.

• The filters are designed to avoid the brightest and most variable night sky emission lines.

Page 4: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The BATC multicolor photometry of M31

• The central 1o×1o field in 15 intermediate bands

• 1995 Sep.-1999 Dec.

• Total EXP:37hr20min

Page 5: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The ages of M31 GCs

• Jiang & Ma (2003) use the Battistini et al. (1987) to obtain BATC SEDs of 172 GCs

• Using the BC96 SSP model to derive the ages and metallicities

• Nearly all the GCs are older than 1 Gyr

• Metal-poor ->old• Metal-rich->young

Page 6: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Break the degeneracy!

• One big problem in the SSP model: age~metallcity degeneracy! Reddening also affects it!

• Idea: use the known metallicty and reddening to derive the age.

Page 7: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Our data for our sample GCs

• BATC(13) + Broadband(5) + 2MASS(3) JHKs photometry (Galleti et al. 2004).

• Spectroscopic [Fe/H] obtained: Perrett et al. (2002) and Barmby et al. (2000)

• The reddening data: Barmby priv. comm.

Page 8: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

BC03 SSP model

• Age: 0.1Myr ~ 20 Gyr

• Wavelength: 91 Å-160 μm

• Track: Padova 1994 (Z=0.0001-0.10)

• IMF:Salpeter 1955

2.5log 48.6AB

dF R

md

R

Page 9: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The SED fitting with BC03 model

Page 10: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The age distribution of our sample GCs in M31

Page 11: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

The metallicity ~age relationship in M31

• Old metal-poor

• Young metal-rich

Page 12: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Future Work

9o×9o field with >1000 GCs and candidates

Green boxes:Observed already

White boxes: to be observed in the future

15 intermediate-band

Page 13: Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters

Thanks very much!

http://batc.bao.ac.cn/~fanzhou