The finder charts have been constructed only for the primary standard star candidates and for some aditional fields, supposed to contain red AND blue stars.
Each image was constructed by averaging 2-4 frames in order to eliminate cosmic rays and bad columns, not always succesfully.
On each chart I have marked the primary stars by red arrows. In some of the SA fields there's more than one primary.
The stars have been identified using finder charts in Landolt 1992 paper (Landolt, A., AJ 104,pg 340, plates 21 to 76), finder charts for HST photometric and spectrophotometric stars (Turnshek et al., AJ, 99, 1243, plates 45 to 78).
For the brightest of the candidates, Hipparcos coordinates have been used for generating a small finder chart. Many of these stars have noticeable proper motions and I could actually see them moving since the first generation Palomar plates have been taken.
Most of the SA stars are now in the second release of the Tycho catalogue, available online from Simbad.
So, here's the list of stars for which finder charts have been constructed so far. Please click on the star name for a jpg image of the field. The finder charts have N up and E to the left.
The charts cover about 121 primary stars and 3 Red-Blue fields by now.(Sept 25, 2000). There's more to come.
| PT target list star name
Large format (40'x40')finding chart |
Close up (10x10') finding chart | Notes |
| 23_15 | red-blue pairs | |
| 38_270 | red-blue pairs | |
| 38_273 | red-blue pairs | |
| Hilt31 | Hilt31 | |
| 92_235
92_322 |
||
| 92_276
92_342 92_263 92_282 92_288 |
||
| 92_263
92_276 92_282 92_342 |
||
| 93_317
93_333 93_424 |
||
| G3-33 | ||
| LHS-0149 | ||
| LHS-0014 | ||
| Hilt233 | Hilt233 | |
| Feige22 | ||
| 94_242
94_251 |
||
| Ross34 | high proper motion (PA ~ 220) | |
| GD50 | ||
| 95_190
95_301 95_302 95_96 95_193 |
||
| 95_218
95_330 95_132 95_142 95_149 |
||
| 95_74
95_132 95_142 95_218 |
||
| 95_236
95_74 95_142 95_149 |
||
| BD+21o607 | fundamental | |
| BD-21o910 | ||
| 96_36 | ||
| 96_737 | ||
| 96_83
96_36 96_235 |
||
| Ross49 | Ross49 is almost "blended" with a field star and has very high proper motion (PA ~ 190). According to the Hipparcos catalogue, the stars formed an optical double at the epoch of the survey(J1991.25)- separation = 0.946 arcsec, PA 170, deltamag=0.98 (Hp V magnitudes). The pair designation is HP27111 = CCDM 05449+0915). Due to the rapid proper motion of Ross49 - aprox 704 mass/yr - the integrated magnitude of the pair is likely to vary fast. The field also contains Cederblad 59 - Ced59, an HII region surrounding FU Ori-the bright star about 17' SE of Ross49-, the dark nebulae B35-the large void area S and W of Ross49 and scores of HH objects... | |
| 97_249
97_75 97_351 97_345 |
||
| 97_351
97_249 97_345 97_284 97_288 |
||
| 97_284
97_75 97_249 97_288 97_345 97_351 |
||
| Hilt566 | ||
| LHS-1858 | high proper motion | |
| 98_185
98_978 98_618 (red) 98_193 98_653 98_685 |
||
| Ru149B
Ru149D Ru149F |
||
| LHS-0033 | ||
| 99_438
99_447 |
||
| BD+75o325 | ||
| BD+8o2015 | ||
| BD+25o1981 | ||
| 100_280
100_241 100_394 |
||
| PG0918+029D | ||
| BD-12o2918 | noticeable proper motion (PA ~ 270) | |
| 101_316
101_315 |
||
| 101_282
101_281 101_207 (southern edge of the chip) |
||
| Feige34 | ||
| BD+29o2091 | high proper motion (PA ~ 200) | |
| G163_50
G163_51 |
G163_50
G163_51 |
|
| Wolf365 | Wolf365 | High proper motion |
| 103_626
103_526 |
103_526
103_626 |
|
| Feige66 | ||
| 104_598 | 104_598 | |
| PG1323-086D | field mislabeled(?) by Landolt = PG1323-085 field | |
| G14-55 | G14-55 | Very close physical double. Very high pm. |
| BD+30o2428B | the fainter, western component | |
| BD+2o2711 | ||
| HD121968 | ||
| Ross838 | Ross838 | High proper motion, nice galaxy field |
| BD+26o2606 | fundamental | |
| GCRV8758 | GCRV8758 | |
| LHS-0394 | LHS-0394 | |
| PG1528+062B | PG1528+062B | |
| G15-24 | G15-24 | |
| 107_1006 | 107_1006 | |
| 107_351 | 107_351 | |
| BD+33o2642 | BD+33o2642 | |
| Ross530 | Ross530 | High proper motion |
| GCRV9483 | GCRV9483 | |
| 107_351 | 107_351 | |
| 108_551
108_475 |
||
| BD+18o3407 | BD+18o3407 | Extremely close double (~ 10"). Also v. high proper motion. |
| BD+2o3375 | BD+2o3375 | |
| 109_71
109_381 109_231 |
109_71
109_381 109_231 |
|
| 109_231
109_71 109_381 109_537 |
109_231
109_71 109_381 109_537 |
|
| Hilt760 | Hilt760 | |
| Ross711 | Ross711 | Noticeable proper motion |
| 110_232
110_340 |
110_232
110_340 |
|
| 110_503
110_499 |
110_503
110_499 |
|
| GJ745A GJ745B |
GJ745A GJ745B |
Wide binary, shared large proper motion |
| BD+35o3659 | BD+35o3659 | Beautiful-and very dense- Milky Way field |
| 111_775
111_1925 111_1969 |
111_775
111_1969 111_1925 |
|
| 111_1969
111_1925 |
111_1969
111_1925 |
|
| 112_250
112_223 112_805 112_822 |
||
| 113_260
113_259 113_339 113_466 113_475 |
||
| BD+25o4655 | BD+25o4655 | |
| BD+17o4708 | fundamental | |
| 114_531
114_548 |
||
| 114_656
114_548 114_654 114_750 |
||
| Ross786 | Ross786 | |
| BD+33o4737 | noticeable proper motion (PA ~ 270) | |
| 115_516 | ||
| LHS-0550 |
