Aton Resources Inc. (AAN: TSX-V) (“Aton” or the “Company") is very
pleased to update investors on the latest assay results from the
Phase 2 diamond drilling programme at its advanced Rodruin gold
exploration project. Rodruin is located in the Company’s 100% owned
Abu Marawat Concession (“Abu Marawat” or the “Concession”), in the
Eastern Desert of Egypt.
Highlights:
- Diamond
drilling is ongoing at Rodruin, with 35 drill holes now having been
completed to date, ROD-048 and ROD-051 to ROD-084, for a total of
3,862 metres;
- Drill
holes ROD-048, ROD-070, and ROD-071 were drilled to test for
potential deep sulphide mineralisation to the north of the
Aladdin’s Hill zone;
- Drill
hole ROD-071 returned a mineralised intersection grading
5.76 g/t Au, 42.0 g/t Ag, 0.31% Cu and 2.40% Zn over
88.6m, from 117.2m down hole depth, which included
a very high grade zone grading 39.4 g/t Au, 261.7 g/t Ag,
0.84% Cu and 3.55% Zn over 9.9m;
- The
Au-Ag-Cu-Zn sulphide mineralisation in hole ROD-071 is hosted
within heavily siliceous and phyllic altered tuffogenic
sediments;
- Other
drill holes also returned significant mineralised intersections
including 17.1m grading 1.07 g/t Au and 15.7 g/t Ag (hole ROD-048),
and 5.7m grading 4.21 g/t Au and 14.6 g/t Ag (hole ROD-070);
- These
latest results indicate the potential for the development of
significant high grade polymetallic sulphide gold resources at
Rodruin.
“To say that we are happy with these latest
drilling results from Rodruin would frankly be a bit of an
understatement” said Tonno Vahk, Interim CEO. “The sulphide
intersection from hole ROD-071 is by some distance the best
intersection Aton has ever drilled in Egypt, and is hugely
encouraging for the deeper sulphide potential at Rodruin. The
mineralisation is hosted in very strongly altered sediments,
associated with significant copper and zinc sulphides, and appears
to be the fresh unweathered precursor to the high grade
mineralisation that we intersected in the discovery hole ROP-003 at
Aladdin’s Hill in 2018. Everything that we are seeing is backing up
our long held belief that the Rodruin deposit comprises zones of
bulk mineralisation, containing discrete very high grade zones.
There are at least two distinct mineralisation styles at Rodruin –
the first hosted in sulphidic carbonates, which weather to gossans,
and a second style of coarse gold bearing mineralisation hosted in
heavily altered sediments. The identification of high grade primary
sulphide-rich altered sediment hosted mineralisation at depth is
very important, and indicates the potential for Rodruin to become a
really significant sized deposit. The mineralisation at Rodruin is
rather unusual, but its association with silver, zinc and copper
indicates a polymetallic association that is similar to what we see
at the Abu Marawat and Hamama deposits, and it is our belief that
while apparently quite different, these three deposits are all
genetically related. Rodruin is clearly structurally complex, but
we are very much moving in the right direction with the
identification of the high grade sulphide mineralisation, and we
also continue to be very encouraged by the identification of coarse
visible gold in holes which we are currently drilling at Aladdin’s
Hill.”
Rodruin diamond drilling
programme
The Rodruin prospect was discovered in December
2017 by Aton geologists (see news release dated December 14, 2017),
and is located approximately 18km east of the Company’s Hamama West
mineral deposit (Figure 1). During 2018 Aton constructed a c. 4.5km
access road to the prospect, and undertook a highly successful 50
hole Phase 1 reverse circulation percussion (“RC”) drilling
programme at Rodruin, which returned numerous mineralised
intersections including 36m grading 12.47 g/t Au and 9.3 g/t Ag,
from 5m downhole depth (hole ROP-003, see news release dated
October 1, 2018).
The Phase 2 diamond drilling programme at
Rodruin commenced in late November 2021, and results reported to
date include 48.0m grading 1.97 g/t Au and 5.3 g/t Ag, from 27.0m,
in hole ROD-052 (see news release dated January 25, 2022), and
88.25m grading 1.74 g/t Au and 9.7 g/t Ag, from 25.75m, in hole
ROD-055 (see news release dated March 1, 2022).
After the completion of hole ROD-069 the drill
rig was converted over to its standard steep hole configuration,
and holes ROD-070 and ROD-071 (Figure 2) were drilled to follow up
on the primary carbonate-hosted mineralisation intersected in RC
hole ROP-050 (61m grading 1.55 g/t Au and 8.9 g/t Ag, from 111m,
see news release dated January 29, 2019). Additionally, the
vertical RC hole ROP-048 was re-entered and deepened, and
re-numbered as hole ROD-048. Collar and survey details of these
holes are provided in Table 1.
Hole ID |
Collar co-ordinates 1 |
Dip 2 |
Grid azimuth 2 |
EOH depth (m) |
Comments |
X |
Y |
Z |
ROD-048 |
552453 |
2913057 |
748 |
-88.1 |
125.0 |
219.60 |
Re-entry of RC hole ROP-048 |
ROD-070 |
552454 |
2913051 |
748 |
-55.4 |
183.8 |
177.20 |
Aladdin’s Hill North sulphides |
ROD-071 |
552455 |
2913158 |
740 |
-68.0 |
188.0 |
246.40 |
Aladdin’s Hill North sulphides |
Notes: 1) Collar
co-ordinates as laid out using handheld
GPS 2) Collar
surveys of drill holes undertaken at c. 5-6m depth, using Reflex
EZ-Trac survey
tool 3) All
co-ordinates are UTM (WGS84) Zone 36R |
Table 1: Collar details of diamond
drill holes ROD-048, ROD-070, and ROD-071
Discussion of results
All 3 drillholes were drilled on the north-south
552450E section at Rodruin (Figure 3). Hole ROD-070 was drilled to
test above the mineralised carbonate intercepted in RC hole
ROP-050, whereas holes ROP-048 and ROD-071 were designed to test
under this zone. Hole ROD-074 and ROD-075 have also been
subsequently completed on this section, and assay results from
these 2 holes are pending. Hole ROD-048 intersected a wide zone of
heavily sulphidic carbonate, similar to that identified in RC hole
ROP-050, whereas neither ROD-070 nor ROD-071 intersected this
carbonate unit. ROD-071 intersected wide zones of heavily
quartz-sericite-pyrite (“phyllic”) altered rocks (Figure 3).
Holes ROD-048 and ROD-070 intersected
carbonate-hosted gold-silver-zinc oxide mineralisation from
surface, with ROD-048 also intersecting deeper carbonate-hosted
mineralisation at depth. Hole ROD-071 returned a long
gold-silver-copper-zinc intersection associated with heavily
sulphidic and silicified phyllic altered sediments. Details of
intersections are provided in Table 2.
Hole ID |
Intersection (m) 1 |
Au (g/t) |
Ag (g/t) |
Cu (%) |
Pb (%) |
Zn (%) |
Comments |
From |
To |
Interval |
ROD-048 |
0.0 2 |
17.0 |
17.0 |
2.21 |
6.8 |
0.43 |
- |
5.98 |
Re-entry of RC hole ROP-048, coring started at 65.5m |
48.0 |
53.0 |
5.0 |
0.78 |
2.8 |
0.02 |
- |
0.26 |
116.7 |
133.8 |
17.1 |
1.07 |
15.7 |
0.01 |
0.03 |
0.33 |
178.8 |
183.9 |
5.1 |
0.64 |
22.2 |
0.83 |
0.03 |
7.45 |
ROD-070 |
0.00 |
5.7 |
5.7 |
4.21 |
14.6 |
0.11 |
0.07 |
1.64 |
|
18.4 |
20.6 |
2.2 |
3.35 |
8.5 |
0.03 |
0.14 |
0.96 |
ROD-071 |
58.9 |
75.3 |
16.4 |
1.20 |
23.2 |
0.03 |
0.10 |
0.09 |
|
|
117.2 |
205.8 |
88.6 |
5.76 |
42.0 |
0.31 |
0.03 |
2.40 |
|
incl. |
138.1 |
148.0 |
9.9 |
39.40 |
261.7 |
0.84 |
0.02 |
3.55 |
|
Notes: 1) Intersections
calculated at a nominal cutoff grade of 0.3 g/t Au in runs of
continuous
mineralisation 2) Intersection
previously reported – see news release dated January 29, 2019 |
Table 2: Mineralised intersections
from diamond drill holes ROD-048, ROD-070, and ROD-071
ROD-071
Hole ROD-071 returned an intersection of
88.6m grading 5.76 g/t Au, 42.0 g/t Ag, 0.31% Cu and 2.40%
Zn from 117.2m depth, including a bonanza grade interval
from 138.1m, grading 39.4 g/t Au, 261.7 g/t Ag, 0.84% Cu
and 3.55% Zn over 9.9m. All the assays from this
intersection are provided in Appendix A. This polymetallic
mineralisation is associated with a unit of dark grey, highly
altered and siliceous rock, consisting primarily of quartz,
sericite and sulphide and sulphosalt minerals. All original texture
in the rock has been destroyed, but this unit is interpreted as
consisting of very heavily altered sedimentary rocks. The
mineralised interval is not believed to represent true thickness,
but the orientation of the mineralised zone is not yet
determined.
The mineralised interval is strongly sulphidic,
carrying approximately 10% pyrite, and up to 20% very pale grey
sphalerite in places, with locally very high concentrations (Figure
4). The highest bonanza grade intersection is notably elevated in
both copper and zinc (Appendix A), and there appears to be a good
correlation between copper with the highest grades of gold (up to
140.5 g/t, between 140.1-142.1m) and silver (up to 1105 g/t, over
the same interval). It is noted that the strongest gold
mineralisation appears to be associated with an increase in the
level of silicification of the rock, as well as copper. It is also
noted that coarse visible gold is typically associated with copper
and lead/arsenic oxide minerals from the near-surface Aladdin’s
Hill zone in drill core and outcrop, eg. in hole ROD-055 (see news
release dated March 1, 2022).
The heavily phyllic altered unit that hosts the
mineralised intersection is fault-bounded to both the south and the
north, and also above by the South Ridge Thrust (“SRT”), a
prominent structural feature which outcrops along the south side of
the South Ridge and which dips to the north at about 40°. Hole
ROD-071 intersected a separate sequence of heavily foliated
quartz-sericite-pyrite rock above the SRT, which also returned a
mineralised intersection grading 1.20 g/t Au and 23.2 g/t
Ag over 16.4m, from 58.9m down hole on its northern
faulted margin.
ROD-048 and ROD-070
Both holes ROD-048 and ROD-070 intersected
gold-silver-zinc mineralisation immediately from surface, with
ROD-048 returning 2.21 g/t Ag, 6.8 g/t Ag and 5.98% Zn over 17m
(see news release dated January 29, 2019), and ROD-070 returning
4.21 g/t Ag, 14.6 g/t Ag and 1.64% Zn over 5.7m, in gossanous
carbonate host rocks. Hole ROD-070 passed into unmineralised
sediments above and below the SRT, and did not intersect further
mineralisation below 20m depth. Hole ROD-048 also intersected
several deeper zones of mineralisation including 1.07 g/t Au and
15.7 g/t Ag over 17.1m, from 116.7m downhole depth, in a
sulphide-rich carbonate-silica-talc unit.
Discussion
The sulphide mineralisation intersected in hole
ROD-071 appears to be the primary sulphide equivalent of the block
of fault-bounded coarse gold bearing oxide mineralisation seen at
Aladdin’s Hill. The deep sulphide mineralisation intersected in
ROD-071 is hosted within a fault-bounded block of highly siliceous
and altered rock, which is apparently bounded above by the SRT.
This block is open at depth and along strike, and is effectively
‘blind’ as it is located directly under both the SRT and Upper
Thrust (“UT”) structures (Figure 3). These blocks of heavily
phyllic altered rocks, and the associated polymetallic
mineralisation, are interpreted as being fault-bounded and
controlled.
The regional stratigraphy consists of a sequence
of predominantly tuffogenic sedimentary rocks (slates and
tuffogenic sandstones), and carbonate-silica-sulphide(±talc) rocks,
of undetermined origin, which host much of the gossanous
mineralisation that outcrops over wide areas of the South Ridge at
Rodruin. Mapping of this stratigraphy indicates that it has been
heavily folded and faulted, as well as being cut by at least 2
shallow north-dipping structures – the SRT and the UT. The UT,
which is roughly parallel to and controls the mountain slope on the
northern flank of the South Ridge (Figure 3), appears to be a
significant structure, and outcrops to the northwest of and bounds
the main mineralised area at Rodruin. Its hangingwall sequence
appears to consist predominantly of a series of unmineralised
carbonate altered sediments. It is likely that the mineralised
sequence in the footwall of the UT, which is exposed at surface on
the South Ridge at Rodruin, continues to the northwest, and could
be continuous at very shallow depths beneath the hangingwall
sequence of rocks above the UT.
Aton believes that there is potential to
identify very significant volumes of additional mineralisation at
Rodruin, as the current drilling continues to indicate that it is
effectively open in all directions, at depth and along strike, as
well as there being potential for further blind mineralisation
under the UT. The identification of the high grade primary
polymetallic sulphide mineralisation associated with the phyllic
altered sediments at depth is particularly significant.
The current diamond drilling programme at
Rodruin was designed with the objective of testing and quantifying
the potential near surface open pittable resources at Rodruin, as
well as testing the deeper primary mineralisation identified during
the Phase 1 RC drilling programme. The original programme has now
been extended beyond its original planned meterage. Additional
drilling (holes ROD-074 and ROD-075, Figure 3) has intersected
further Cu-Zn sulphide mineralisation at depth, and Aton will
continue to release new drill results as the assays become
available.
Sample processing and analytical
procedures
Drill core was logged by Aton geologists, and
marked up for cutting and sampling at the Rodruin core farm.
Samples were typically selected over nominal 1m intervals, but as
determined by the logged lithologies. The core was half-cut by Aton
staff at the onsite Rodruin sample preparation facility.
The split half-core samples were collected and
bagged up in cloth bags, weighed and crushed to -4mm onsite, and
split to a nominal c. 250-500g sample size. The coarse crushed
reject samples are retained onsite at the Rodruin sample prep
facility.
QAQC samples are inserted at a rate of
approximately 1 certified reference material (or “standard” sample)
every 30 samples, 1 blank sample every 15 samples, and 1 duplicate
split sample every 15 samples.
The c. 250-500g dried, crushed and split samples
were shipped to ALS Minerals sample preparation laboratory at Marsa
Alam, Egypt where they were pulverised to a size fraction of better
than 85% passing 75 microns. From this pulverised material a
further sub-sample was split off with a nominal c. 50g size, which
was shipped on to ALS Minerals at Rosia Montana, Romania for
analysis.
Samples were analysed for gold by fire assay
with an atomic absorption spectroscopy (“AAS”) finish (analytical
code Au-AA23), and for silver, copper, lead and zinc using an aqua
regia digest followed by an AAS finish (analytical code AA45). Any
high grade gold samples (>10 g/t Au) were re-analysed using
analytical code Au-GRA21 (also fire assay, but with a gravimetric
finish). Any high grade Ag and base metal samples (Ag >100 g/t,
and Cu, Pb and Zn >10,000ppm or >1%) were re-analysed using
the ore grade technique AA46 (also an aqua regia digest followed by
an AAS finish).
About Aton Resources Inc.
Aton Resources Inc. (AAN: TSX-V) is focused on
its 100% owned Abu Marawat Concession (“Abu Marawat”), located in
Egypt’s Arabian-Nubian Shield, approximately 200 km north of
Centamin’s world-class Sukari gold mine. Aton has identified
numerous gold and base metal exploration targets at Abu Marawat,
including the Hamama deposit in the west, the Abu Marawat deposit
in the northeast, and the advanced Rodruin exploration prospect in
the south of the Concession. Two historic British gold mines are
also located on the Concession at Sir Bakis and Semna. Aton has
identified several distinct geological trends within Abu Marawat,
which display potential for the development of a variety of styles
of precious and base metal mineralisation. Abu Marawat is 447.7 km2
in size and is located in an area of excellent infrastructure; a
four-lane highway, a 220kV power line, and a water pipeline are in
close proximity, as are the international airports at Hurghada and
Luxor.
Qualified person
The technical information contained in this News
Release was prepared by Javier Orduña BSc (hons), MSc, MCSM, DIC,
MAIG, SEG(M), Exploration Manager of Aton Resources Inc. Mr. Orduña
is a qualified person (QP) under National Instrument 43-101
Standards of Disclosure for Mineral Projects.
For further information regarding Aton Resources
Inc., please visit us at www.atonresources.com or contact:
TONNO VAHK
Interim CEOTel: +1 604 318 0390Email:
info@atonresources.com
Note Regarding Forward-Looking
Statements Some of the statements contained in this
release are forward-looking statements. Since forward-looking
statements address future events and conditions; by their very
nature they involve inherent risks and uncertainties. Actual
results in each case could differ materially from those currently
anticipated in such statements. Neither TSX Venture Exchange nor
its Regulation Services Provider (as that term is defined in
policies of the TSX Venture Exchange) accepts responsibility for
the adequacy or accuracy of this release.
Appendix A – Assay results of the
ROD-071 Au-Ag-Cu-Zn sulphide intersection
Sample No. |
From (m) |
To (m) |
Interval (m) |
Au (g/t) |
Ag (g/t) |
Cu (ppm) |
Pb (ppm |
Zn (ppm) |
AHA-37745 |
117.20 |
118.15 |
0.95 |
0.51 |
6.4 |
1650 |
361 |
59900 |
AHA-37746 |
118.15 |
119.70 |
1.55 |
4.51 |
27 |
6400 |
407 |
88100 |
AHA-37748 |
119.70 |
120.65 |
0.95 |
0.19 |
1.5 |
1040 |
19 |
12150 |
AHA-37749 |
120.65 |
121.50 |
0.85 |
1.54 |
11.6 |
5350 |
186 |
90700 |
AHA-37750 |
121.50 |
122.50 |
1.00 |
1.65 |
2.9 |
207 |
43 |
2380 |
AHA-37751 |
122.50 |
123.50 |
1.00 |
0.94 |
22.6 |
2920 |
185 |
23800 |
AHA-37752 |
123.50 |
124.50 |
1.00 |
1.92 |
5.9 |
844 |
75 |
6400 |
AHA-37753 |
124.50 |
125.50 |
1.00 |
2.13 |
10.9 |
2300 |
281 |
17700 |
AHA-37755 |
125.50 |
126.50 |
1.00 |
0.70 |
4.2 |
1300 |
94 |
6630 |
AHA-37756 |
126.50 |
127.50 |
1.00 |
0.31 |
3.4 |
1210 |
40 |
11950 |
AHA-37757 |
127.50 |
128.50 |
1.00 |
4.21 |
17.4 |
3080 |
101 |
37600 |
AHA-37758 |
128.50 |
129.50 |
1.00 |
0.67 |
4 |
431 |
41 |
6610 |
AHA-37759 |
129.50 |
130.50 |
1.00 |
0.24 |
1.2 |
43 |
34 |
448 |
AHA-37760 |
130.50 |
131.50 |
1.00 |
0.31 |
1.6 |
95 |
64 |
1855 |
AHA-37761 |
131.50 |
132.50 |
1.00 |
0.20 |
1.3 |
42 |
44 |
821 |
AHA-37763 |
132.50 |
133.50 |
1.00 |
1.51 |
4.3 |
183 |
131 |
14650 |
AHA-37764 |
133.50 |
134.50 |
1.00 |
0.30 |
11.2 |
954 |
63 |
8550 |
AHA-37765 |
134.50 |
135.30 |
0.80 |
0.50 |
22.4 |
1940 |
82 |
18650 |
AHA-37766 |
135.30 |
136.10 |
0.80 |
0.81 |
31.1 |
2730 |
273 |
47200 |
AHA-37767 |
136.10 |
137.10 |
1.00 |
0.32 |
5.5 |
396 |
58 |
6500 |
AHA-37769 |
137.10 |
138.10 |
1.00 |
0.20 |
3 |
202 |
30 |
3220 |
AHA-37770 |
138.10 |
139.10 |
1.00 |
12.6 |
15.3 |
4050 |
48 |
42700 |
AHA-37771 |
139.10 |
140.10 |
1.00 |
17.4 |
61.1 |
19550 |
368 |
120000 |
AHA-37772 |
140.10 |
141.10 |
1.00 |
113.0 |
710 |
21610 |
283 |
65000 |
AHA-37773 |
141.10 |
142.10 |
1.00 |
140.5 |
1105 |
10840 |
195 |
25000 |
AHA-37775 |
142.10 |
143.10 |
1.00 |
2.57 |
22.2 |
5440 |
47 |
9770 |
AHA-37776 |
143.10 |
144.10 |
1.00 |
0.34 |
11.2 |
3240 |
131 |
13050 |
AHA-37777 |
144.10 |
145.10 |
1.00 |
0.44 |
17.5 |
2120 |
74 |
7780 |
AHA-37778 |
145.10 |
146.00 |
0.90 |
0.35 |
7.7 |
1690 |
106 |
4340 |
AHA-37779 |
146.00 |
147.00 |
1.00 |
82.0 |
529 |
7860 |
355 |
43900 |
AHA-37780 |
147.00 |
148.00 |
1.00 |
20.9 |
113 |
6750 |
434 |
20500 |
AHA-37782 |
148.00 |
149.00 |
1.00 |
0.18 |
5.8 |
1320 |
65 |
3210 |
AHA-37783 |
149.00 |
150.00 |
1.00 |
0.25 |
4 |
568 |
52 |
1170 |
AHA-37784 |
150.00 |
151.00 |
1.00 |
0.38 |
6 |
696 |
74 |
4740 |
AHA-37785 |
151.00 |
152.00 |
1.00 |
2.12 |
23.3 |
2030 |
158 |
5410 |
AHA-37786 |
152.00 |
153.00 |
1.00 |
0.32 |
2 |
159 |
101 |
1490 |
AHA-37788 |
153.00 |
154.00 |
1.00 |
0.21 |
4 |
761 |
975 |
4830 |
AHA-37789 |
154.00 |
155.00 |
1.00 |
0.30 |
3.5 |
610 |
411 |
4140 |
AHA-37790 |
155.00 |
156.00 |
1.00 |
0.36 |
3.8 |
1110 |
88 |
1595 |
AHA-37791 |
156.00 |
157.00 |
1.00 |
0.36 |
1.6 |
107 |
90 |
855 |
AHA-37792 |
157.00 |
158.00 |
1.00 |
0.84 |
4.5 |
1090 |
40 |
1610 |
AHA-37793 |
158.00 |
159.00 |
1.00 |
0.39 |
1.3 |
194 |
21 |
428 |
AHA-37794 |
159.00 |
160.00 |
1.00 |
0.30 |
1.4 |
197 |
35 |
434 |
AHA-37795 |
160.00 |
161.00 |
1.00 |
0.21 |
1.2 |
178 |
48 |
487 |
AHA-37796 |
161.00 |
162.00 |
1.00 |
0.37 |
1.9 |
237 |
61 |
3240 |
Sample No. |
From (m) |
To (m) |
Interval (m) |
Au (g/t) |
Ag (g/t) |
Cu (ppm) |
Pb (ppm |
Zn (ppm) |
AHA-37797 |
162.00 |
163.00 |
1.00 |
13.45 |
86.1 |
5140 |
278 |
44300 |
AHA-37799 |
163.00 |
164.00 |
1.00 |
4.29 |
26.6 |
3570 |
246 |
36700 |
AHA-37800 |
164.00 |
165.00 |
1.00 |
1.42 |
14.3 |
2540 |
281 |
53600 |
AHA-37801 |
165.00 |
166.00 |
1.00 |
1.51 |
15.7 |
2280 |
704 |
76200 |
AHA-37803 |
166.00 |
167.00 |
1.00 |
1.05 |
10.2 |
4120 |
358 |
54800 |
AHA-37804 |
167.00 |
168.00 |
1.00 |
0.86 |
6.9 |
1570 |
21 |
5300 |
AHA-37805 |
168.00 |
169.00 |
1.00 |
0.76 |
6.3 |
900 |
61 |
3970 |
AHA-37806 |
169.00 |
170.00 |
1.00 |
0.59 |
3.1 |
305 |
95 |
3100 |
AHA-37807 |
170.00 |
171.00 |
1.00 |
0.46 |
5.6 |
1120 |
47 |
5160 |
AHA-37808 |
171.00 |
172.00 |
1.00 |
2.92 |
33.1 |
8120 |
27 |
14200 |
AHA-37809 |
172.00 |
173.00 |
1.00 |
1.65 |
18.6 |
5560 |
102 |
8740 |
AHA-37810 |
173.00 |
174.00 |
1.00 |
0.72 |
8.6 |
2010 |
89 |
7450 |
AHA-37811 |
174.00 |
175.00 |
1.00 |
1.59 |
13.4 |
1245 |
51 |
17000 |
AHA-37812 |
175.00 |
176.00 |
1.00 |
2.83 |
27.1 |
2510 |
119 |
8320 |
AHA-37813 |
176.00 |
177.00 |
1.00 |
0.34 |
7.9 |
3300 |
27 |
1655 |
AHA-37815 |
177.00 |
178.00 |
1.00 |
0.35 |
7.3 |
2620 |
145 |
9700 |
AHA-37816 |
178.00 |
179.00 |
1.00 |
2.26 |
19.1 |
1615 |
67 |
20400 |
AHA-37817 |
179.00 |
180.00 |
1.00 |
0.20 |
2.7 |
474 |
16 |
3010 |
AHA-37818 |
180.00 |
181.00 |
1.00 |
2.65 |
27.5 |
3460 |
548 |
100500 |
AHA-37819 |
181.00 |
182.00 |
1.00 |
1.19 |
14.1 |
1335 |
184 |
17000 |
AHA-37821 |
182.00 |
183.00 |
1.00 |
3.46 |
37.1 |
6360 |
281 |
72000 |
AHA-37822 |
183.00 |
184.00 |
1.00 |
3.31 |
22.5 |
4560 |
277 |
46400 |
AHA-37823 |
184.00 |
185.00 |
1.00 |
1.50 |
16.3 |
3300 |
226 |
41000 |
AHA-37824 |
185.00 |
186.00 |
1.00 |
1.88 |
29.1 |
9060 |
885 |
137500 |
AHA-37825 |
186.00 |
187.00 |
1.00 |
1.21 |
17 |
4130 |
224 |
64600 |
AHA-37826 |
187.00 |
188.00 |
1.00 |
0.28 |
7 |
1825 |
15 |
3860 |
AHA-37828 |
188.00 |
189.00 |
1.00 |
0.15 |
4.3 |
1420 |
9 |
1210 |
AHA-37829 |
189.00 |
190.00 |
1.00 |
0.44 |
7.2 |
1680 |
16 |
12300 |
AHA-37830 |
190.00 |
191.00 |
1.00 |
1.64 |
19 |
5620 |
17 |
10500 |
AHA-37831 |
191.00 |
192.00 |
1.00 |
1.09 |
14.1 |
6340 |
105 |
24900 |
AHA-37833 |
192.00 |
193.00 |
1.00 |
2.86 |
25.3 |
4300 |
721 |
60400 |
AHA-37834 |
193.00 |
194.00 |
1.00 |
0.76 |
5.4 |
609 |
30 |
9640 |
AHA-37835 |
194.00 |
195.00 |
1.00 |
1.69 |
24.2 |
5590 |
4290 |
42300 |
AHA-37837 |
195.00 |
196.00 |
1.00 |
2.10 |
21.8 |
4420 |
416 |
28600 |
AHA-37839 |
196.00 |
197.00 |
1.00 |
1.99 |
16.5 |
3170 |
199 |
41100 |
AHA-37841 |
197.00 |
198.00 |
1.00 |
1.22 |
8.8 |
2080 |
31 |
4000 |
AHA-37842 |
198.00 |
199.00 |
1.00 |
0.85 |
8.3 |
4010 |
236 |
12650 |
AHA-37843 |
199.00 |
199.90 |
0.90 |
1.58 |
27.6 |
6090 |
3690 |
26600 |
AHA-37844 |
199.90 |
200.90 |
1.00 |
2.57 |
14.6 |
3300 |
225 |
42400 |
AHA-37845 |
200.90 |
202.00 |
1.10 |
1.13 |
14.8 |
5120 |
1015 |
10700 |
AHA-37846 |
202.00 |
203.00 |
1.00 |
13.00 |
116 |
7920 |
160 |
37700 |
AHA-37848 |
203.00 |
204.00 |
1.00 |
0.56 |
11.9 |
3570 |
104 |
17250 |
AHA-37849 |
204.00 |
205.00 |
1.00 |
0.30 |
3.4 |
694 |
92 |
3300 |
AHA-37850 |
205.00 |
205.80 |
0.80 |
2.31 |
44.4 |
1430 |
56 |
16100 |
Photos accompanying this announcement are available at:
https://www.globenewswire.com/NewsRoom/AttachmentNg/2e1806ae-5656-4a80-b0db-6dc532743dbf
https://www.globenewswire.com/NewsRoom/AttachmentNg/510920e3-67fe-40c5-8299-5592f72c34c4
https://www.globenewswire.com/NewsRoom/AttachmentNg/200c6b64-13d6-4450-aca5-1cf8e9c5e69b
https://www.globenewswire.com/NewsRoom/AttachmentNg/07129da3-4d6d-4ccc-8c9f-76d7ba8716fa
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