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38 M31X [163] M3130%XXL X ≥ 5 × 10 37 erg s −1 X [151, 164] Di Stefano (2003) [165] Chadra XM104 SombreroXXXXXXX [166] Bellazzini et al.(1995) [167] M31LMXBsTrudolyubov & Priedhorsky (2004) [149] Bellazzini etal. (1995) [167] BATCFan et al. 1996 [99] , Zheng et al. 1999 [168] M311358 ′ × 58 ′ X4.24.3X4.462X4.54.64.2 M31XXTrudolyubov & Priedhorsky(2004) [149] XMM − NewtonChandra XM31 ∼ 6100arcmin 2 XM3143X M31X Trinchieri & Fabbiano (1991) [156] Primini, Forman & Jones (1993) [157] Trinchieri et al. (1999) [158] Supper et al. (2001) [148] Kaaret (2002) [160] Konget al. (2002) [161] Williams et al. (2004) [162] Trinchieri & Fabbiano(1991) [156] Einstein M31 108X0.2 − 4.0 keVForman & Jones (1993) [157] ROSAT HRI1990M31∼ 34 ′ 48,00086XL X > 1.4 × 10 36 erg s −1 X18Trinchieriet al. (1999) [158] M31X0.110 keV
M31X 39XXXXSupper et al. (2001) [148] ROSAT M31∼ 10.7 deg 2 96X560X55331610ChandraHigh Resolution Camera HRC [169] M31Kaaret (2002) [160] 143X20199920018Chandra ACIS-IKong et al. (2002) [161] M31 ∼ 17 ′ × 17 ′ 204X452299supersoftsources23Williams et al. (2004) [162] ChandraHRC17166X28171BL63M3154XTrinchieri & Fabbiano (1991) [156] Primini et al. (1993) [157] Trinchieriet al. (1999) [158] Kaaret (2002) [160] Kong et al. (2002) [161] Williams et al. (2004)[162]M31XBATC X4.3 BATCM31M31BATC 60/90f/3seeing∼ 3 ′′ CCD2k×2k CCD13BATC03−BATC15∼ 4000 − 10000 Å199511151999121637 Oke & Gunn (1983) [101] FHD 19445, HD 84937, BD+26 ◦ 2606BD +17 ◦ 4708 BATCABm BATC = −2.5 log ˜F ν − 48.60 (4.1)
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UDCM31 2009562009526
Page 3:
The Multi-color Photometric Studyof
Page 6 and 7: iiM314RBC V.3.5BATC 1530RBC V.3.5M3
Page 8 and 9: ivM31for M31 GCs. Using the photome
Page 11 and 12: vii5.2.4 2MASS . . . . . . . . . .
Page 13 and 14: 2.1 BATCCCD . . . . . . . . . . . .
Page 15 and 16: 1.1 BATC60/90f/3M31 . . . 51.2 HST
Page 17: xiii7.3 BATCV Caldwell et al. (2009
Page 20 and 21: 2 M31 [10] [8] HST Advanced Camera
Page 22 and 23: 4 M311.3 WMAPΛ (ΛCDM) [18] 6 < z
Page 24 and 25: 6 M311.5 1.5.1 Globular Clusters GC
Page 26 and 27: 8 M31Gerssen et al. (2002) [36] HST
Page 28 and 29: 10 M311.5 pc10 pc50 pc [29] 2mass s
Page 30 and 31: 12 M31Crampton et al. (1985) [63] M
Page 32 and 33: 14 M31cDNGC 4874IC 4051Kalirai et a
Page 34 and 35: 16 M31CCD 2.2: BATC1520064096 × 40
Page 36 and 37: 18 M31100GSC84CCD567CCD82.4 Pipelin
Page 38 and 39: 20 M313CCD45b. :1tv look1.1more 1.1
Page 40 and 41: 22 M315: p1731925T518o023.fit 24.4
Page 42 and 43: 24 M31D. pip21 PipelineIICCDPSFpip2
Page 44 and 45: 26 M316. *.als2 ′′ 7. BATCABe8.
Page 46 and 47: 28 M314. (m inst )BATC(m BATC )Km i
Page 49 and 50: 3.1 M31NGC 5128HSTM31M87HST 3.2 Sin
Page 51 and 52: 333.3 BC03GALAXEVBruzual & Charlot
Page 53 and 54: 35t ∼ 0.1 Gyr1 GyrAGBt = 1 Gyr4 G
Page 55: M31X4.1 Local GroupM31∼ 780 kpc [
Page 59 and 60: M31X 41XKong et al. (2002) [161] Ka
Page 61 and 62: M31X 43 4.2: M3149X4.4.3 8XXDAOPHOT
Page 63 and 64: M31X 454.5 62X62XX4.5.1 62X58X43 Tr
Page 65 and 66: M31X 47(1987) [64] 5V B−V 58V B
Page 67 and 68: M31X 49 4.6: M31XB − V V B − V
Page 69 and 70: M31X 51 4.8: M31XXV B − V XV M31X
Page 71 and 72: M31X 53 4.2: 49XBATC 13NameBATC Fil
Page 73 and 74: M31X 55 4.2: -NameBATC Filter No.03
Page 75 and 76: M31X 57 4.3: -Optical Name FWHMs (G
Page 77 and 78: M31X 59 4.6: M3162XXSource Optical
Page 79 and 80: 5.1 M31∼780 kpc [19, 20] Galleti
Page 81 and 82: 63−− 5.2BATCUBV RI2MASS5.35.45.
Page 83 and 84: 6525% − 50%[Fe/H]= −0.6 − −
Page 85 and 86: 675.2.4 2MASSWorthey (1994) [135]
Page 87 and 88: 69Barmby et al. (2000) [4] 5.4.1 5.
Page 89 and 90: 71 5.3: χ 2 5.4.4 Jiang et al.
Page 91 and 92: 73 5.5: Jiang et al. (2003) [66] Ji
Page 93 and 94: 75∼ 3σ Gyr 5.8: 91M31 5.5BC03 Gy
Page 95 and 96: 77M315.8M31Fusi Pecci et al.2005 [2
Page 97 and 98: 79 [66] (5.3) √ 2biassystematic o
Page 99 and 100: 81 5.1: - χ 2 min(Gyr) [Fe/H] ()
Page 101: 83 5.2: Name(Gyr) 0.5 2Bo015 1.43
Page 104 and 105: 86 M31M31M31M31Frogel et al. (1980)
Page 106 and 107:
88 M31et al. (2004) [25] Carpenter
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90 M31−(X − Y ) 0 = a[Fe/H] + b
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92 M31 6.2: H036.3.3 M31Barmby et a
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94 M31 6.4: M31Racine (1991)[256]
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96 M31(B − V ) 0 = 0.66 ± 0.02 6
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98 M314D max = 0.0616.8KS 6.7: M31
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100 M31KMMP −6.6KMM P −M3199.6%
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102 M31 6.10: M312 kpc 3 M31Perrett
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104 M31 6.12: M310.000 ± 0.001 dex
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106 M31 6.13: V 0 6.5 Barmb
Page 126 and 127:
108 M31−Q−Barmby et al. (2000)
Page 128 and 129:
110 M31 6.1: -Name [Fe/H] S Name [F
Page 130 and 131:
112 M31 6.3: Q−Q XY Z (X − Y )
Page 132 and 133:
114 M31 6.4: -Name E(B − V ) Name
Page 134 and 135:
116 M31 6.5: −M31Name [Fe/H] Name
Page 137 and 138:
M317.1 ω CenNGC 2808NGC 1851HST Yi
Page 139 and 140:
M31 121547.13024Caldwell etal. (200
Page 141 and 142:
M31 123 7.1: BATC M3158 ′ × 58
Page 143 and 144:
M31 125B189D B193D G289 G295 NB34 N
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M31 1277.4.2 RBC V.3.57.57.4M31UBV
Page 147 and 148:
M31 129 7.5: M31RBCV.3.57.57.4.3 bl
Page 149 and 150:
M31 131 7.7: M31−V 7.6RBC V.3.57.
Page 151 and 152:
M31 133 7.9: 7.8RBC V.3.57.5LAMOSTV
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M31 135 7.3: BATC M31-2 - M31-7Fiel
Page 155 and 156:
M31 137 7.3: -Field Filter C. W. Ba
Page 157 and 158:
M31 139 7.4: -ID a b c d e f g h i
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−M311M3149XX8EinsteinROSAT HRICha
Page 161 and 162:
143KMM3−0.006 ± 0.001 −0.007
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[1] Steidel, C. C., Giavalisco, M.
Page 165 and 166:
147[31] Strom, S. E., Strom, K. M.,
Page 167 and 168:
149[62] Battistini, P., Bònoli, F.
Page 169 and 170:
151[93] Baum, W. A., et al. 1995, A
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153[129] Allard, F., Hauschildt, P.
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155[165] Di Stefano, R., Kong, A. K
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157[200] Leitherer, C., Heckman, T.
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159[232] Sarajedini, A., King, C. R
Page 179:
161[273] Parmentier, G., Jehin, E.,
Page 182 and 183:
164 M31[10] Ma, J., de Grijs, R., F
Page 185 and 186:
BATCAstronomerBATCBATCBATCSchmidt B
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