# Last edited on 2025-08-17 21:58:08 by stolfi # # Table of stars in the SPS and their properties. # # Columns: # # SN: the star serial number in the page, from S01 # # CORE: type of the star's core, drawn in normal ink. Either of: # "no": no core. # "dot": single dot. # "ring": ring with blank interior (none in the SPS). # "--": cannot tell type be determined because of opaque paint. # # PAINT: kind of paint job aplied to the star: # "no": unpainted. # "splot": a round spot contained in the body of the star. # "grub": for irregular and gritty smear of paint # "fill": tries to fill most of the outline, including # most of the rays. # "frub": like fill but very rough partial, as for "grub". # # COLOR: the color of the paint applied to the star. Either: # "yel": the semi-transparent yellow of the Light Painter. # "RED": an opaque dark red paint. # "WHT": an uncertain semi-transparent off-white paint that may be # just bleached yel paint. # "--": not painted. # # R: number of rays, including any that becomes a fat tail. # # T: presence and type of the "tail", a thin wavy trace # emanating from the star. Either: # "-": no tail. # "1": a single tail, # "2": a "fat" tail, with two strokes that converge at the end. # # OBS: an observation with no embedded blanks, or "--". # # In general the tail of a star extends or starts from a ray tip near # 05:00. But sometimes it starts at a notch between two rays. # # There doesn't seem to be a sharp boundary between fat and thin tails. # The difference is only how far the fat part of the tail extends. # # In some thin-tailed stars, the outline was drawn first and the tail # was added as a separate stroke. In other cases the drawing of the # outline apparently started at a ray tip around 05:00, went CW all # around, then instead of stopping at the starting point continued out # to form the (single) tail. # # In the case of stars with fat tails, sometimes the star outline is # drawn as two or more strokes in opposite directions, starting at a ray # tip in the general NW area, until a ray tip around around 05:00, and # each stroke is then extended to make one edge of the tail. See S13 in # f113r for example. # # Other times a star with fat tail is drawn by drawing a thin-tail star # first (in either of the pssible ways), and then adding the left edge # of the tail as a separate stroke. See the tail of S06 in f114v for # example. # PAGE ! SN ! VPOS ! CORE ! PAINT ! CLR ! R ! T ! OBS ------+-----+--------+------+-------+-----+---+---+--------------- # f103r | S01 | 01+0.0 | -- | fill | RED | 7 | - | -- f103r | S02 | 05+0.0 | no | splot | yel | 8 | - | -- f103r | S03 | 08+0.2 | dot | splot | yel | 8 | - | -- f103r | S04 | 09-0.2 | -- | fill | RED | 6 | - | small_star f103r | S05 | 13+0.5 | dot | splot | yel | 8 | - | -- f103r | S06 | 16+0.0 | -- | fill | RED | 8 | - | -- f103r | S07 | 18+0.0 | no | splot | yel | 7 | - | -- f103r | S08 | 21+0.3 | no | no | -- | 7 | - | -- f103r | S09 | 24+0.0 | -- | fill | RED | 7 | - | -- f103r | S10 | 27-0.2 | no | splot | yel | 7 | - | -- f103r | S11 | 30+0.0 | dot | no | -- | 8 | - | -- f103r | S12 | 33+0.4 | -- | fill | RED | 7 | - | -- f103r | S13 | 35+0.0 | no | splot | yel | 7 | - | -- f103r | S14 | 37+0.0 | -- | grub | RED | 7 | - | -- f103r | S15 | 40+0.0 | no | splot | yel | 8 | - | -- f103r | S16 | 43+1.0 | no | no | -- | 7 | - | -- f103r | S17 | 45+1.0 | -- | fill | RED | 7 | - | -- f103r | S18 | 48+0.0 | dot | splot | yel | 8 | - | -- f103r | S19 | 52+0.0 | dot | splot | yel | 8 | 1 | tail_up # f103v | S01 | 01+0.0 | -- | splot | RED | 7 | - | -- f103v | S02 | 05+0.0 | no | splot | yel | 7 | - | -- f103v | S03 | 09+0.0 | -- | splot | RED | 7 | - | -- f103v | S04 | 12+0.5 | dot | splot | yel | 7 | - | -- f103v | S05 | 14+0.0 | -- | splot | RED | 7 | - | -- f103v | S06 | 17+0.0 | dot | splot | yel | 7 | - | -- f103v | S07 | 20+0.0 | -- | splot | RED | 7 | - | -- f103v | S08 | 21+0.0 | dot | splot | yel | 6 | - | small_star f103v | S09 | 27+0.0 | -- | splot | RED | 6 | - | small_star f103v | S10 | 30+0.0 | dot | splot | yel | 8 | - | -- f103v | S11 | 33+0.0 | -- | splot | RED | 8 | - | -- f103v | S12 | 37+0.0 | dot | splot | yel | 8 | - | -- f103v | S13 | 39+0.0 | -- | splot | RED | 7 | - | -- f103v | S14 | 43+0.0 | no | splot | yel | 8 | - | -- # # On this page the red-painted stars are initially grubbed with a # half-dry pen in a clumsy attempt to fill them. At star S10 they # suddenly the technique changes to a red splot, confined to the star's # body, seemingly applied with a brush. The yel paint, on the other hand, # is always a roundish splot, apparently applied with a brush. # Star S10 has apparently was drawn as an 8-ray star and then # the double tail was added as an extra ray that starts at 04:00, between # two previous rays. # # The (thin) tail of star S11 starts in the notch at 04:30, not at a ray tip. # f104r | S01 | 01-0.9 | -- | frub | RED | 7 | 1 | -- f104r | S02 | 05+0.0 | no | splot | yel | 7 | 1 | -- f104r | S03 | 10+0.5 | -- | frub | RED | 8 | 1 | -- f104r | S04 | 12+0.3 | -- | frub | RED | 7 | 1 | -- f104r | S05 | 16+0.3 | no | splot | yel | 7 | 1 | -- f104r | S06 | 19+0.0 | -- | frub | RED | 8 | 1 | -- f104r | S07 | 22+0.0 | no | splot | yel | 8 | 1 | -- f104r | S08 | 27+0.8 | -- | frub | RED | 7 | 1 | -- f104r | S09 | 30-0.3 | dot | splot | yel | 9 | 1 | -- f104r | S10 | 34+0.5 | -- | splot | RED | 9 | 2 | -- f104r | S11 | 36+0.0 | no | splot | yel | 7 | 1 | -- f104r | S12 | 39+0.2 | -- | splot | RED | 7 | 1 | -- f104r | S13 | 43+0.5 | no | splot | yel | 8 | 1 | -- # f104v | S01 | 01+0.0 | -- | splot | RED | 8 | 1 | -- f104v | S02 | 06+0.5 | no | splot | yel | 8 | 1 | -- f104v | S03 | 08+0.0 | -- | splot | RED | 7 | 1 | -- f104v | S04 | 12+1.0 | no | splot | yel | 7 | 1 | -- f104v | S05 | 15+0.5 | -- | splot | RED | 8 | 1 | -- f104v | S06 | 19+0.0 | no | splot | yel | 8 | 1 | -- f104v | S07 | 22+0.0 | -- | splot | RED | 8 | 1 | -- f104v | S08 | 27+0.2 | dot | splot | yel | 8 | 1 | -- f104v | S09 | 29+0.0 | -- | splot | RED | 8 | 1 | -- f104v | S10 | 32+0.5 | no | splot | yel | 8 | 1 | -- f104v | S11 | 35+0.0 | -- | splot | RED | 8 | 1 | -- f104v | S12 | 37+0.0 | no | splot | yel | 8 | 1 | -- f104v | S13 | 41+0.6 | -- | splot | RED | 8 | 1 | -- # # The double tail of star S05 starts at the core like an extra ray; # counted as such. # # The tails of stars S07 and S08 are double only for a while, then # revert to single; maybe they are just fat and slightly bent rays, not # tails. # # The red paint of S04 was apparently a splot applied with a brush, # a clumsy attempt was made to fill the rays by pulling the fresh paint # into them with a pen or other sharp object. # f105r | S01 | 01+1.0 | -- | splot | RED | 8 | 1 | above_1st_word f105r | S02 | 06+0.7 | -- | splot | RED | 7 | 2 | -- f105r | S03 | 10+0.9 | no | splot | yel | 7 | 1 | -- f105r | S04 | 13+0.0 | -- | grub | RED | 7 | 1 | -- f105r | S05 | 16+0.3 | no | splot | yel | 8 | 2 | -- f105r | S06 | 23+0.9 | -- | splot | RED | 7 | 2 | -- f105r | S07 | 25+0.9 | no | splot | yel | 7 | 2 | -- f105r | S08 | 27+0.9 | -- | splot | RED | 7 | 2 | -- f105r | S09 | 30+0.9 | no | splot | yel | 7 | 1 | -- f105r | S10 | 34+1.3 | -- | splot | RED | 7 | 2 | -- # f105v | S01 | 01+0.0 | -- | splot | RED | 7 | 2 | -- f105v | S02 | 03-0.5 | no | splot | yel | 7 | 2 | -- f105v | S03 | 08+0.5 | -- | splot | RED | 7 | 2 | -- f105v | S04 | 14+1.3 | no | splot | yel | 7 | 2 | -- f105v | S05 | 18+0.9 | -- | splot | RED | 7 | 1 | -- f105v | S06 | 20+0.9 | no | splot | yel | 7 | 1 | -- f105v | S07 | 23+0.0 | -- | splot | RED | 7 | 1 | -- f105v | S08 | 25+0.0 | no | splot | yel | 8 | 1 | -- f105v | S09 | 29+0.7 | -- | splot | RED | 7 | 1 | -- f105v | S10 | 32+0.0 | no | splot | yel | 7 | 2 | -- # # Star S03 shares the tip of one ray a tiny "companion" star, with vpos # 07+0.0 and 7 rays. That tiny starlet seems to have a dot core in # normal ink and also a red dot (not splot!) inside the body but off to # one side, avoiding the dot core. # f106r | S01 | 01-0.5 | -- | splot | RED | 7 | 1 | -- f106r | S02 | 04-0.5 | no | splot | yel | 8 | 1 | -- f106r | S03 | 08+0.0 | -- | splot | RED | 7 | 1 | w_tiny_star f106r | S04 | 10+0.0 | no | splot | yel | 8 | 2 | -- f106r | S05 | 13+0.0 | -- | splot | RED | 7 | 1 | -- f106r | S06 | 15+0.0 | ?? | splot | yel | 7 | 1 | -- f106r | S07 | 18+0.3 | -- | splot | RED | 7 | 1 | -- f106r | S08 | 22+0.7 | no | splot | yel | 8 | 1 | -- f106r | S09 | 24+0.0 | -- | splot | RED | 8 | 1 | -- f106r | S10 | 27+0.0 | no | splot | yel | 7 | 1 | -- f106r | S11 | 32+0.0 | -- | splot | RED | 8 | 1 | -- f106r | S12 | 34-0.6 | no | splot | yel | 8 | 1 | -- f106r | S13 | 36-0.5 | -- | splot | RED | 8 | 1 | -- f106r | S14 | 38+0.0 | no | splot | yel | 7 | 1 | -- f106r | S15 | 42+0.0 | -- | splot | RED | 8 | 1 | -- # # The splot of star S14 seems to have been applied with brush, like the # other red splots, but it is off-center and irreular, overflowing the # outline. # f106v | S01 | 01+0.0 | no | splot | yel | 7 | 1 | -- f106v | S02 | 05+0.5 | -- | splot | RED | 8 | 1 | -- f106v | S03 | 09+0.0 | no | splot | yel | 8 | 1 | -- f106v | S04 | 11+0.0 | -- | splot | RED | 8 | 1 | -- f106v | S05 | 15+0.8 | no | splot | yel | 8 | 1 | -- f106v | S06 | 18+0.0 | -- | splot | RED | 7 | 1 | -- f106v | S07 | 20+0.0 | dot | splot | yel | 9 | 1 | -- f106v | S08 | 26+0.0 | -- | splot | RED | 8 | 1 | -- f106v | S09 | 28-0.2 | dot | splot | yel | 8 | 1 | faint_core f106v | S10 | 32+0.0 | -- | splot | RED | 8 | 1 | -- f106v | S11 | 34-0.2 | no | splot | yel | 7 | 1 | -- f106v | S12 | 37+0.0 | -- | splot | RED | 8 | 1 | -- f106v | S13 | 40+0.0 | no | splot | yel | 8 | 1 | -- f106v | S14 | 42+0.0 | -- | splot | RED | 7 | 1 | grubbish # # Star S11 has three dots at its left, in the dark-gray Retracer ink. # # The splot of star S14 is a bit smeared and wanders off from the body. # f107r | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f107r | S02 | 04+0.5 | no | splot | yel | 7 | 1 | -- f107r | S03 | 08+0.0 | -- | splot | RED | 7 | 1 | -- f107r | S04 | 13+0.0 | no | splot | yel | 7 | 1 | -- f107r | S05 | 16+0.0 | -- | splot | RED | 7 | 1 | short_tail f107r | S06 | 18-0.2 | no | splot | yel | 8 | 1 | -- f107r | S07 | 21+0.5 | -- | splot | RED | 7 | 1 | -- f107r | S08 | 24+0.3 | no | splot | yel | 7 | 1 | -- f107r | S09 | 27-0.5 | -- | splot | RED | 7 | 1 | -- f107r | S10 | 30+0.0 | no | splot | yel | 7 | 1 | -- f107r | S11 | 34+0.0 | -- | splot | RED | 7 | 1 | three_dots f107r | S12 | 38-0.2 | dot | splot | yel | 7 | 1 | -- f107r | S13 | 42+0.0 | -- | splot | RED | 7 | 1 | -- f107r | S14 | 45+0.0 | no | splot | yel | 8 | 2 | smeared_splot f107r | S15 | 48+0.0 | -- | splot | RED | 8 | 1 | short_tail # # Star S01 has three reverse-comma marks on each side, aligned with two # rays at 02:00 and 08:00. They seem to be in normal ink. # f107v | S01 | 01+0.0 | -- | splot | RED | 6 | 1 | triple_quotes. f107v | S02 | 05+0.0 | dot | splot | yel | 7 | 1 | -- f107v | S03 | 08+0.0 | -- | splot | RED | 8 | 1 | -- f107v | S04 | 11+0.0 | dot | splot | yel | 8 | 1 | short_tail f107v | S05 | 16+0.0 | -- | splot | RED | 8 | 1 | -- f107v | S06 | 20-0.2 | no | splot | yel | 7 | 1 | -- f107v | S07 | 23-0.2 | -- | splot | RED | 7 | 1 | -- f107v | S08 | 25-0.2 | no | splot | yel | 7 | 1 | -- f107v | S09 | 29+0.0 | -- | splot | RED | 8 | 1 | -- f107v | S10 | 32+0.0 | dot | splot | yel | 9 | 1 | -- f107v | S11 | 35+0.0 | -- | grub | RED | 8 | 1 | -- f107v | S12 | 37+0.0 | no | splot | yel | 7 | 1 | -- f107v | S13 | 41+0.2 | -- | splot | RED | 7 | 1 | -- f107v | S14 | 43+0.5 | dot | splot | yel | 8 | 1 | -- f107v | S15 | 45-0.7 | -- | splot | RED | 8 | 1 | short_tail # # Star S01 is within a light brown stain that obscueres the shape of the # yel paint. But seems to be a splot. # # In star S02, the splot seems to be smeared into and over the 05:00 ray. # # The fill of star S03 leaves 3 rays almost unpainted. # # Stars S02, S03, and S04 seem to have been shifted by ~2.5 lines from # the correct position. Maybe the scribe did not notice a parag break on # line 02 (see puff) and instead thought that line 11 was a parag head. # f108r | S01 | 01-0.2 | no | splot | yel | 7 | 1 | stain f108r | S02 | 02+2.3 | no | splot | yel | 7 | 1 | -- f108r | S03 | 05+2.5 | -- | frub | RED | 7 | 1 | -- f108r | S04 | 08+2.7 | no | frub | yel | 7 | 1 | -- f108r | S05 | 14+0.0 | no | grub | yel | 7 | 1 | -- f108r | S06 | 17+0.0 | dot | frub | yel | 7 | 1 | -- f108r | S07 | 21+0.0 | -- | frub | RED | 7 | 1 | -- f108r | S08 | 24+0.0 | no | splot | yel | 7 | 1 | grubbish f108r | S09 | 29+0.0 | no | no | -- | 7 | 1 | -- f108r | S10 | 31+0.0 | -- | frub | RED | 7 | 1 | -- f108r | S11 | 35+0.0 | no | splot | yel | 7 | 1 | -- f108r | S12 | 37+0.0 | -- | fill | RED | 7 | 1 | -- f108r | S13 | 39+0.0 | no | no | -- | 7 | 1 | -- f108r | S14 | 41-0.7 | dot | splot | yel | 7 | 1 | -- f108r | S15 | 45+0.5 | dot | no | -- | 7 | 1 | -- f108r | S16 | 48+0.0 | -- | fill | RED | 7 | 1 | -- # # Stars on f108v vary a lot in size. # # The VPOS of stars S04 and S05 depends on how one splits lines 07-19, # which is a conflict between "starlet nearby" and "no puffs" criteria. # f108v | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f108v | S02 | 05+0.6 | no | splot | yel | 7 | 1 | -- f108v | S03 | 07+0.0 | -- | splot | RED | 8 | 1 | -- f108v | S04 | 15+3.0 | dot | splot | yel | 8 | 1 | -- f108v | S05 | 17+2.0 | -- | splot | RED | 7 | 1 | -- f108v | S06 | 20+0.0 | no | splot | yel | 7 | 1 | -- f108v | S07 | 23+0.0 | -- | splot | RED | 8 | 1 | -- f108v | S08 | 28+2.0 | no | splot | yel | 7 | 1 | -- f108v | S09 | 30+0.5 | dot | splot | yel | 8 | 1 | -- f108v | S10 | 34+0.0 | -- | splot | RED | 8 | 1 | -- f108v | S11 | 37+0.0 | no | splot | yel | 8 | 1 | -- f108v | S12 | 40+0.5 | -- | splot | RED | 7 | 1 | -- f108v | S13 | 43+0.5 | dot | splot | yel | 8 | 1 | -- f108v | S14 | 46+0.5 | -- | splot | RED | 7 | 1 | -- f108v | S15 | 48+0.0 | no | splot | yel | 7 | 1 | -- f108v | S16 | 50-0.2 | -- | splot | RED | 7 | 1 | -- # # The core of star S08 may have been a small dot that was erased by the # paint applied over it. # f111r | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f111r | S02 | 06+0.0 | no | splot | yel | 8 | 1 | brownish_yel f111r | S03 | 08+0.0 | -- | splot | RED | 8 | 1 | -- f111r | S04 | 10+0.0 | dot | splot | yel | 8 | 1 | -- f111r | S05 | 13+0.0 | -- | splot | RED | 8 | 1 | -- f111r | S06 | 17+0.0 | dot | splot | yel | 8 | 1 | -- f111r | S07 | 20+0.5 | -- | splot | RED | 9 | 1 | bifurc_tail f111r | S08 | 23+0.0 | no | splot | yel | 8 | 1 | lost_dot? f111r | S09 | 25-0.7 | -- | splot | RED | 8 | 1 | -- f111r | S10 | 29+0.0 | no | splot | yel | 8 | 1 | -- f111r | S11 | 32+0.5 | -- | splot | RED | 8 | 1 | -- f111r | S12 | 34+0.0 | no | splot | yel | 8 | 1 | -- f111r | S13 | 36+0.0 | -- | splot | RED | 7 | 1 | -- f111r | S14 | 39+0.0 | no | splot | yel | 7 | 1 | -- f111r | S15 | 44+0.0 | -- | splot | RED | 7 | 1 | -- f111r | S16 | 48+0.0 | no | splot | yel | 7 | 1 | -- f111r | S17 | 51+0.0 | -- | splot | RED | 8 | 2 | bifurc_tail # # # The dot of star S10 is a thin and short vertical dash, off-center, and # very dark; maybe added by the Retracer? Or just a parch defect? # # The tail of star S09 comes off from a wide gap between rays, rather # than from the tip of ray. # # The 04:00 ray of star S18 seem to have been partly retraced in dark # ink. # f111v | S01 | 01+0.0 | -- | splot | RED | 8 | 1 | -- f111v | S02 | 04+0.0 | no | splot | yel | 7 | - | -- f111v | S03 | 06+0.2 | -- | splot | RED | 7 | 1 | -- f111v | S04 | 07+1.0 | no | splot | yel | 7 | 1 | -- f111v | S05 | 10-0.7 | -- | splot | RED | 7 | - | -- f111v | S06 | 13+0.0 | dot | splot | yel | 8 | - | -- f111v | S07 | 16+0.5 | -- | splot | RED | 7 | - | -- f111v | S08 | 18+0.0 | dot | splot | yel | 7 | - | -- f111v | S09 | 20-0.7 | -- | splot | RED | 7 | 1 | -- f111v | S10 | 24+0.5 | dot | no | -- | 8 | - | retraced_dot? f111v | S11 | 26+0.0 | -- | splot | RED | 7 | - | -- f111v | S12 | 29+0.5 | no | splot | yel | 7 | - | -- f111v | S13 | 31+0.7 | -- | splot | RED | 7 | - | -- f111v | S14 | 32+0.0 | dot | splot | yel | 7 | - | -- f111v | S15 | 34+0.5 | -- | splot | RED | 8 | 1 | -- f111v | S16 | 37+0.5 | dot | splot | yel | 8 | - | -- f111v | S17 | 39-0.5 | -- | splot | RED | 7 | - | -- f111v | S18 | 45+0.5 | no | splot | yel | 7 | - | ray_retraced? f111v | S19 | 48+0.5 | -- | splot | RED | 8 | - | -- # f112r | S01 | 01+0.3 | -- | splot | RED | 7 | 1 | -- f112r | S02 | 05+0.0 | no | splot | yel | 7 | 1 | -- f112r | S03 | 11+0.0 | -- | splot | RED | 7 | 1 | -- f112r | S04 | 15+0.0 | no | splot | yel | 7 | 1 | -- f112r | S05 | 19+0.0 | -- | splot | RED | 7 | 1 | -- f112r | S06 | 23+0.0 | no | splot | yel | 7 | 1 | -- f112r | S07 | 27+0.0 | -- | splot | RED | 8 | 1 | -- f112r | S08 | 31+0.0 | no | splot | yel | 7 | 1 | -- f112r | S09 | 33+0.5 | -- | splot | RED | 7 | 1 | -- f112r | S10 | 37+0.5 | dot | splot | yel | 8 | 1 | -- f112r | S11 | 39+0.0 | -- | splot | RED | 7 | 1 | -- f112r | S12 | 42+0.0 | no | splot | yel | 7 | 1 | -- # # The stars of f112v lie roughly on a straight line but that line is # significantly tilted, apparently to avoid some area of bad parch at # the top left corner, adjacent to the big indentation on the edge. That # hypothesis is suported by the tilt and two steps of indentation of the # left rail of the text. Perhaps the parch in that part was oily and # did not hold the ink? # # The outlines and tails of stars S02 and S06 are quite faint. The # outlines of red-painted stars apparently escaped the fading, except # for S13. The red paint in the splots does not show any sign of fading, # not even on S13. # # The tail of star S01 is blurry. # # Star S02 may have been backtraced (rays 01:00 and 06:00) but even those # backtraced strokes are faint. # # Star S02 perhaps had a dot or ring core, but it is almost invisible because # of fading and yel paint-over. # # Strokes at 10:30, 04:00 and 05:00 of tar S13 may have been backtraced, # but even those strokes are fainter and blurry. # # The core of star S06, if it existed, has faded almost to invisibility; # if what we see is indeed the core, it seem to hav been a ring rather # than a dot. # # Star S06 has only a stub at 05:00 where a ray should have been. The # tail of S11 leaves between two rays 04:00 and 06:00 instead of from a # ray tip. # f112v | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f112v | S02 | 07+1.1 | no? | splot | yel | 7 | 1 | very_faint f112v | S03 | 11+0.0 | -- | splot | RED | 7 | 2 | -- f112v | S04 | 15+0.0 | no | splot | yel | 7 | 1 | -- f112v | S05 | 20+0.0 | -- | splot | RED | 7 | 1 | -- f112v | S06 | 23-0.2 | ring | splot | yel | 7 | 1 | ray_stub f112v | S07 | 27+0.0 | -- | splot | RED | 8 | 1 | -- f112v | S08 | 30+0.0 | no | splot | yel | 7 | 1 | -- f112v | S09 | 32+0.0 | -- | splot | RED | 7 | 1 | -- f112v | S10 | 36+0.0 | no | splot | yel | 8 | 2 | -- f112v | S11 | 39+0.5 | -- | splot | RED | 7 | 1 | -- f112v | S12 | 42+0.0 | no | splot | yel | 6 | 1 | -- f112v | S13 | 45+0.0 | -- | splot | RED | 7 | 1 | -- # # Stars on f113r lie rather close to the binding edge and are distorted # in scans by the curvature of the parch there. # # The splot of star 14 has sharp edges but is elongated NS and does not # fill the body of the star. # # The body of S13 is extra wide and so it its splot. # # The outline of S13 appears to have been drawn in at least twho # strokes. The first one started at the ray tip at 11:00 and went CW to # the notch at 05:00, then continued to make the right edge of the # double tail. The second stroke started as the same ray tip as the # first, and went CCW to the notch at 06:00, then continued to make the # left edge of the tail. f113r | S01 | 01+0.0 | no | splot | yel | 7 | 1 | -- f113r | S02 | 04+0.5 | -- | splot | RED | 7 | 1 | -- f113r | S03 | 08+0.5 | no | splot | yel | 7 | 1 | -- f113r | S04 | 10+0.0 | -- | splot | RED | 7 | 1 | -- f113r | S05 | 13+0.0 | no | splot | yel | 7 | 1 | -- f113r | S06 | 16+0.0 | -- | splot | RED | 8 | 1 | -- f113r | S07 | 20+0.0 | no | splot | yel | 7 | 1 | -- f113r | S08 | 22-0.7 | -- | splot | RED | 8 | 1 | -- f113r | S09 | 27+0.0 | no | splot | yel | 8 | 1 | -- f113r | S10 | 30-0.3 | -- | splot | RED | 7 | 1 | -- f113r | S11 | 34+0.0 | no | splot | yel | 7 | 1 | -- f113r | S12 | 37+0.0 | -- | splot | RED | 8 | 1 | -- f113r | S13 | 39+0.0 | no | splot | yel | 8 | 2 | -- f113r | S14 | 42-0.2 | -- | splot | RED | 7 | 1 | grushish f113r | S15 | 45+0.0 | no | fill | yel | 8 | 1 | -- f113r | S16 | 48-0.5 | -- | splot | RED | 8 | 1 | -- # # Star S01 seems to have an extra short troke inside th ray at 10:30. # # Star S10 may have had a core, but if so it is too fiant now to be sure. # # Star S11 has a short stroke extending from tip of ray at 01:30. # f113v | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S02 | 04+0.0 | no | splot | yel | 8 | 1 | -- f113v | S03 | 07+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S04 | 10+0.0 | dot | splot | yel | 7 | 1 | -- f113v | S05 | 13+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S06 | 18+0.0 | dot | splot | yel | 7 | 1 | -- f113v | S07 | 21+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S08 | 25+0.0 | dot | splot | yel | 8 | 1 | -- f113v | S09 | 28+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S10 | 33+0.0 | no | splot | yel | 7 | 1 | -- f113v | S11 | 36+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S12 | 38+0.0 | dot | splot | yel | 8 | 1 | -- f113v | S13 | 42+0.0 | -- | splot | RED | 7 | 1 | -- f113v | S14 | 45+0.0 | no | splot | yel | 8 | 1 | -- f113v | S15 | 47+0.0 | -- | splot | RED | 7 | 1 | -- # # Stars on f114r lie rather close to the binding edge and are distorted # in scans by the curvature of the parch there. # f114r | S01 | 01+0.0 | -- | splot | RED | 7 | 1 | -- f114r | S02 | 04+0.0 | no | splot | yel | 8 | 2 | -- f114r | S03 | 08+0.0 | -- | splot | RED | 7 | 1 | -- f114r | S04 | 11+0.0 | no | splot | yel | 8 | 1 | -- f114r | S05 | 14+0.0 | -- | splot | RED | 7 | 1 | -- f114r | S06 | 19+0.0 | no | splot | yel | 7 | 1 | -- f114r | S07 | 22-0.2 | -- | splot | RED | 7 | 1 | -- f114r | S08 | 24-1.0 | no | splot | yel | 8 | 2 | -- f114r | S09 | 28-0.5 | -- | splot | RED | 7 | 1 | -- f114r | S10 | 32+0.0 | no | splot | yel | 7 | 1 | -- f114r | S11 | 35+0.2 | -- | splot | RED | 8 | 1 | -- f114r | S12 | 39+0.9 | no | splot | yel | 8 | 1 | -- f114r | S13 | 42+0.7 | -- | splot | RED | 8 | 1 | -- # # The double tail of S05 is an extension of a ray that was inserted into # the notch at 04:30 after a 7-ray outline had been drawn. The two edges # of the tail are separate strokes. # f114v | S01 | 01+0.0 | no | splot | yel | 7 | 1 | -- f114v | S02 | 06+0.7 | -- | splot | RED | 7 | 1 | -- f114v | S03 | 08+0.0 | no | splot | yel | 7 | 1 | -- f114v | S04 | 11+0.0 | -- | splot | RED | 7 | 1 | -- f114v | S05 | 14+0.0 | no | splot | yel | 8 | 2 | grafted_ray f114v | S06 | 18+0.0 | -- | splot | RED | 7 | 2 | -- f114v | S07 | 20-0.4 | no | splot | yel | 7 | 2 | -- f114v | S08 | 23+0.3 | -- | splot | RED | 7 | 1 | -- f114v | S09 | 26+0.4 | no | splot | yel | 7 | 1 | -- f114v | S10 | 29+0.0 | -- | splot | RED | 7 | 1 | -- f114v | S11 | 33+0.0 | no | splot | yel | 7 | 2 | -- f114v | S12 | 36+0.3 | -- | splot | RED | 8 | 1 | -- # # Stars S01--S05 are mostly drawn in dark ink, like the first 16.7 lines # of the text, and may have been retraced. See comments in the SPS # transcription file and the verbal description file.# # # The red splots of S01, S03, and S03 apparently cover and obscure the # dark ink of the outline. This would be evidence that the Dark Painter # operated after the Retracer. # # The CCW edge of the 01:00 ray of star S02, and the 01:00 and 02:00 # rays of S04, are much fainter than the rest of the respective star # outlines, and may be instances of the original state before retracing # (if it occurred). # # There are some wormholes in the margin, and one of them may or may not # have eaten an entire ray of S04. Assuming that it did. # # The double tail of S05 is filled in with the dark ink. Accident? # f115r | S01 | 01-0.2 | -- | splot | RED | 7 | 1 | -- f115r | S02 | 04+0.0 | dot | splot | yel | 8 | - | -- f115r | S03 | 08+0.0 | -- | splot | RED | 7 | 1 | -- f115r | S04 | 10+0.0 | no | splot | yel | 8 | 1 | wormhole f115r | S05 | 13+0.0 | -- | splot | RED | 8 | 2 | filled_tail f115r | S06 | 19+0.7 | -- | splot | RED | 9 | 1 | -- f115r | S07 | 22-0.2 | no | splot | yel | 8 | 1 | -- f115r | S08 | 26+0.0 | -- | splot | RED | 8 | 1 | -- f115r | S09 | 29+0.0 | no | splot | yel | 8 | 1 | -- f115r | S10 | 35+0.0 | -- | splot | RED | 8 | 1 | -- f115r | S11 | 37+0.0 | no | splot | yel | 8 | 1 | -- f115r | S12 | 40+0.0 | -- | splot | RED | 8 | 1 | -- f115r | S13 | 42+0.0 | no | splot | yel | 8 | 1 | -- # # The color of the yel splots on this page seem to have faded so that # their presence is barely visible in some stars as a change of the # normal parch collor to an more off-white tone (denoted WHT below), a # slight smoothing of the parch texture. Some of the stars listed below # as "unpainted" may in fact have had a yel splot which became # completely invisible. It may be visible in IR transmission scans, # perhaps. # # The red paint shows no sign of fading. # # The left edge of the parch was damaged by a huge wormhole (see scan # of f115r) and was aparently restored by pasting on f115v a patch of # new parch, ~10 mm wide and ~18 mm tall, that partly obscured star S07 # (near text line 21). Still visible are 8 rays, and one more probably # exists but is hidden under the patch. # f115v | S01 | 01+0.0 | -- | splot | RED | 8 | 1 | -- f115v | S02 | 06+0.9 | no | no | -- | 8 | 1 | -- f115v | S03 | 08+0.8 | -- | splot | RED | 8 | 1 | -- f115v | S04 | 11+0.0 | no | splot | WHT | 8 | 1 | -- f115v | S05 | 13-0.3 | -- | splot | RED | 8 | 1 | -- f115v | S06 | 18+0.0 | no | splot | WHT | 8 | 1 | -- f115v | S07 | 21+0.0 | -- | splot | RED | 9 | 1 | patch f115v | S08 | 24+0.6 | no | no | -- | 8 | 1 | -- f115v | S09 | 29+1.0 | -- | splot | RED | 7 | 1 | -- f115v | S10 | 31+0.7 | no | no | -- | 7 | 1 | -- f115v | S11 | 34+0.0 | -- | splot | RED | 8 | 1 | -- f115v | S12 | 37+0.5 | dot | no | -- | 8 | 1 | -- f115v | S13 | 41+0.5 | -- | splot | RED | 8 | 1 | -- # # The 04:30 ray of star S09 is almost entirely filled with dark ink, as # if it had been clumsily retraced. There is a @'qo' just to the right of # it whose @o is almost certainly retraced with the same ink. However, # the transtion from dark strokes to strong strokes along the star's # outlne may not be sharp. Perhaps it is just strong normal ink that # happened to have a higher concentration of black particles. # # The strokes of the two rays of S07 at 04:30 and 06:00 too are thicker # and darker, and appear to be retraced. # # There are several wormholes near the left edge of the page # around lines 10--13 of f116r. One of these may or may not have # eaten the complete 12:00 ray of S05, if it existed. Assuming that # it did. # # Star S07 is smaller than the others (~5 mm diam instead of ~7 mm) but # has similar or bigger body, and thus has shorter and chubbier rays. # f116r | S01 | 01+0.0 | no | splot | yel | 7 | - | -- f116r | S02 | 04+0.0 | -- | splot | RED | 7 | - | -- f116r | S03 | 07+0.0 | no | splot | yel | 7 | - | -- f116r | S04 | 10+0.0 | -- | splot | RED | 7 | - | -- f116r | S05 | 15+2.1 | no | splot | yel | 8 | - | wormhole f116r | S06 | 18+3.0 | -- | splot | RED | 7 | - | -- f116r | S07 | 19+1.0 | dot | splot | yel | 8 | - | small_chubby f116r | S08 | 20-1.0 | -- | splot | RED | 7 | - | -- f116r | S09 | 25+1.0 | no | splot | yel | 8 | - | -- f116r | S10 | 27+0.0 | -- | splot | RED | 7 | - | --