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Calibrators at 610 MHz

Based on our criteria for a calibrator ( Flux density $>$ 0.75 Jy, flat $uv$-distance plot and no secondary source greater than 10% of the calibrator), we identified 102 sources which could be used as GMRT calibrators at 610MHz. These are presented in Table 4.1, List 1 as Class A calibrators.

To increase the number of calibrators and give the astronomer a larger choice, we have also defined a list of Class B calibrators where we have relaxed the limit on the secondary sources in the field allowing it to be as high as 25%. While the class B calibrators will be inferior to the Class A, they could be used with some care in the situation demanded. There are 9 source in this category which are listed in Table 4.2, List 2 as Class B calibrators.


Table 4.1: (Class A - List 1) : Identified Calibrators for GMRT at 610 MHz (Flux Density of Secondary Source is $<$ 10% of that of Primary Source.)
(Class A - List 1) : Identified Calibrators for GMRT at 610 MHz (Flux Density of Secondary Source is $<$ 10% of that of Primary Source.)
Sr. Source Flux Sr. Source Flux Sr. Source Flux
No. Name Density No. Name Density No. Name Density
  (J2000) (Jy.)   (J2000) (Jy.)   (J2000) (Jy.)
1. 0022+002 3.62 26. 0447-220 4.21 51. 1154-350 8.82
2. 0024-420 1.19 27. 0453-281 3.09 52. 1219+484 0.76
3. 0029+349 1.92 28. 0459+024 1.09 53. 1227+365 1.77
4. 0059+001 3.66 29. 0503+020 1.20 54. 1248-199 7.77
5. 0102+584 1.19 30. 0530+135 1.43 55. 1313+675 4.55
6. 0119+321 3.69 31. 0541-056 1.29 56. 1323-448 4.29
7. 0136+478 1.23 32. 0604+442 1.43 57. 1330+251 11.9
8. 0155-408 2.66 33. 0607-085 2.58 58. 1347+122 8.12
9. 0204-170 0.99 34. 0609-157 2.75 59. 1351-148 1.48
10. 0217+738 2.24 35. 0632+103 2.80 60. 1400+621 6.93
11. 0237+288 2.03 36. 0713+438 1.50 61. 1432-180 1.18
12. 0238+166 1.25 37. 0735-175 3.01 62. 1435+760 2.05
13. 0240-231 5.27 38. 0739+016 2.15 63. 1445+099 2.48
14. 0321+123 2.40 39. 0741+312 1.44 64. 1448-163 1.82
15. 0323+055 5.17 40. 0745+101 1.83 65. 1545+478 0.85
16. 0329+279 1.33 41. 0828-375 1.41 66. 1602+334 2.94
17. 0336+323 2.46 42. 0837-198 8.95 67. 1609+266 4.40
18. 0403+260 0.82 43. 0842+185 1.16 68. 1613+342 4.41
19. 0410+769 7.89 44. 0854+201 1.16 69. 1629+679 1.40
20. 0414+343 2.09 45. 0943-083 4.10 70. 1635+381 3.00
21. 0423-013 2.00 46. 1035+564 1.95 71. 1653+397 1.82
22. 0424+020 1.40 47. 1107-448 1.85 72. 1743-038 0.90
23. 0432+416 13.8 48. 1120+143 3.76 73. 1800+784 1.76
24. 0438+488 2.34 49. 1130-148 5.77 74. 1845+401 1.21
25. 0440-435 6.65 50. 1150-003 3.85 75. 1923-210 1.68



Table 4.1: (Class A - List 1) : Identified Calibrators for GMRT at 610 MHz (Flux Density of Secondary Source is $<$ 10% of that of Primary Source.)
Continued... (Class A - List 1) : Identified Calibrators for GMRT at 610 MHz (Flux Density of Secondary Source is $<$ 10% of that of Primary Source.)
Sr. Source Flux Sr. Source Flux Sr. Source Flux
No. Name Density No. Name Density No. Name Density
  (J2000) (Jy.)   (J2000) (Jy.)   (J2000) (Jy.)
76. 1924+334 6.10 85. 2035+109 1.27 94. 2202+422 2.35
77. 1925+211 1.08 86. 2035+189 2.42 95. 2212+018 4.42
78. 1944+548 1.84 87. 2050+314 0.83 96. 2214-385 2.90
79. 2007-445 0.99 88. 2052+365 4.87 97. 2236+284 0.82
80. 2011-067 2.15 89. 2101-423 1.09 98. 2246-121 1.76
81. 2015+371 1.47 90. 2130+050 4.60 99. 2254+247 2.64
82. 2022+616 1.61 91. 2136+006 1.53 100. 2314-449 3.20
83. 2023+544 1.01 92. 2139+143 1.03 101. 2344+824 5.67
84. 2025+337 0.87 93. 2148+069 3.43 102. 2355+498 2.91



Table 4.2: (Class B - List 2) : Identified Calibrators for GMRT at 610 MHz (Flux Density of Secondary Source is $>$ 10% and $<$ 25% of that of Primary Source.)
Sr. Source Flux Sr. Source Flux Sr. Source Flux
No. Name Density No. Name Density No. Name Density
  (J2000) (Jy.)   (J2000) (Jy.)   (J2000) (Jy.)
1. 0334-401 0.76 4. 1316-336 1.23 7. 1751-253 0.75
2. 0614+607 1.53 5. 1513+236 2.34 8. 1937-399 0.79
3. 1111+199 1.13 6. 1751+096 0.75 9. 2005+778 0.84



next up previous contents
Next: Calibrators at 235 MHz Up: Calibrators, their Identifications Previous: Calibrators, their Identifications   Contents
Manisha Jangam 2007-06-19