-- High-grade, visible-gold bearing mineralization
intersected more than 250 metres (“m”) north of Lantern
Deposit
- Key intercepts: 1,624 grams per tonne (“g/t”) gold (“Au”)
over 0.91 m, including 4,750 g/t Au over 0.31 m; 198 g/t Au
over 3.0 m, including 1,577 g/t Au over 0.35; 40.8 g/t Au over 18.7
m
-- Mineralization identified over 500 m strike
length and 1,200 m down-plunge (to 1,000 m below surface); Lantern
Deposit remains open in multiple directions
-- Underground exploration development into Lantern
Deposit to commence in early 2018 in support of upgrading and
expanding Mineral Resources
-- Lantern exploration program key component of
plan to establish economic Mineral Reserve leading to resumption of
operations at Cosmo Mine in Northern Territory of
Australia.
Kirkland Lake Gold Ltd. (“Kirkland Lake
Gold” or the “Company”) (TSX:KL)
(NYSE:KL) (ASX:KLA) today announced positive drilling results at
the Cosmo Mine (“Cosmo”) in the Northern Territory (“NT”),
Australia. A total of 65 holes for 23,553 m from underground
diamond drilling and nine holes for 4,184 m from surface drilling
were completed to test the expansion potential of the Lantern
Deposit (“Lantern”). The results substantially increase the deposit
footprint, particularly to the north, and demonstrate the potential
for significant growth in Mineral Resources. The high-grade gold
mineralization intersected from recent drilling exhibits a change
from fine-grained free gold in Cosmo Deposit to coarser-grained
free gold in narrow quartz veins within Lantern.
Included in the new results is the highest-grade
gold assay ever reported at Cosmo, totaling 4,750 g/t Au over 0.31
m (estimated true width “ETW” 0.2 m) in hole LU73020, which is
located more than 250 m north of the current main Lantern Mineral
Resource (see Figure 3). For details of the Lantern Mineral
Resource see the NI43-101 Technical Report, entitled, “Report on
the Mineral Resources & Mineral Reserves of the Northern
Territory Operations, Northern Territory, Australia,” dated March
30, 2017 (the “Technical Report”).
Tony Makuch, President and CEO of Kirkland Lake
Gold, commented: “After suspending production at Cosmo on June 30,
2017, we expanded our extensive exploration program at the Lantern
Deposit, recognizing the significant potential that exists to
identify new Mineral Resources. The results being reported today
are very encouraging, as they demonstrate that Lantern is much
larger than previously identified with the potential for
substantially higher grades. Based on the latest drilling, we have
extended Lantern to over 500 m along strike, more than 1,200 m
down-plunge and over 1,000 m vertically from surface, with a
significant number of high-grade intersections and multiple
occurrences of visible gold.
“The progress being made at Lantern increases
our confidence that we can establish an economic deposit or
deposits in the Northern Territory and resume mining and milling
operations at the Cosmo Mine and Union Reefs Mill. In support of
this goal, we are initiating an underground exploration development
program on two levels, 320 m vertically apart, to access Lantern
underground from the existing Cosmo ramp. This development will
provide the first underground exposures of the Lantern
mineralization, deliver improved drilling access and provide
initial production platforms for the potential restart of
operations in 2018. Five diamond drill rigs (three underground and
two surface) and a reverse-circulation (“RC”) percussion drill rig
are currently operating at the Cosmo Mine to further define and
expand the Lantern mineralization.”
Drilling Highlights within the Lantern
Deposit at the Cosmo Mine
Drill results reported today include 74 new
drill holes for a total of 27,737 m. The drilling was completed as
part of an extensive program of underground infill & extension
diamond drilling, with results demonstrating the significant
high-grade potential and down-plunge extent of the Lantern
Deposit.
Key intercepts are listed below, with further
details provided in the commentary that follows.
Highlight Drilling Intercepts:
- 1,624 g/t Au over 0.91 m (ETW 0.6 m), including 4,750 g/t Au
over 0.31 m (ETW 0.2 m) in hole LU73020 (3600 Lode)
- 198 g/t Au over 3.0 m (ETW 1.0 m), including 1,577 g/t Au over
0.35 m (ETW 0.1 m) in hole LU73017 (3800 Lode)
- 89.7 g/t Au over 1.0 m (ETW 0.8 m) in hole DS001 (3600
Lode)
- 40.8 g/t Au over 18.7 m (ETW 5.2 m), in hole LU101020 (3400
Lode)
- 22.6 g/t Au over 8.8 m (ETW 4.4 m), in hole LU101014 (3900
Lode)
- 14.6 g/t Au over 5.9 m (ETW 2.8 m) in hole LU101014 (3400
Lode), and
- 11.7 g/t Au over 19.1 m (ETW 6.5 m) in hole LU101026 (3600
Lode).
ETW – Estimated True Width, all drill results
are presented in Table 1 and all drill collars are listed in Table
2.
A total of 16 holes intersected significant
Lantern gold mineralization of over 30 Gram-m (gold grade
(g/t Au) x estimated true width (m)). Results above 100 Gram‑m
were also recorded for four holes, including: 1,624 g/t Au over
0.91 m (ETW 0.6 m), including 4,750 g/t Au over 0.31 m (ETW 0.2 m)
in hole LU73020, 198 g/t Au over 3.0 m (ETW 1.0 m), including 1,577
g/t Au over 0.35 m (ETW 0.1m) in hole LU73017, 40.8 g/t Au over
18.7 m (ETW 5.2 m), in hole LU101020 and 22.6 g/t Au over 8.8 m
(ETW 4.4 m), in hole LU101014.
Of the four 100 Gram-m holes, Hole LU73017 is
the second deepest drill intercept recorded to date at the Lantern
Deposit (Figure 8). Hole DS001, drilled from surface, intersected
89.7 g/t Au over 1.0 m (ETW 0.5m) and is the most southern drill
intercept to date at Lantern (Figure 6). Based on current drilling,
the Company believes that considerable potential exists for
continued expansion of the Lantern mineralization both down-plunge
to the north and up-plunge to the south.
There are currently six drill rigs drilling at
the Lantern Deposit; comprising three underground diamond drill
rigs, two surface diamond drill rigs and one RC percussion drill
rig. The RC percussion drill rig commenced in December to
potentially define near-surface Lantern Mineral Resources.
Underground exploration development to access the Lantern
mineralization on two levels is expected to start in the first
quarter of 2018 with the first mineralization to be exposed during
the second quarter. Each level of geological mapping and sampling
will determine the character and continuity of gold grades,
including any controlling structures, which will be used to refine
the Mineral Resource models and underpin Mineral Reserve estimates
and mine production designs. The ongoing exploration program is
being conducted to increase Mineral Resources and establish an
economic Mineral Reserve base which would facilitate the resumption
of mining at Cosmo with a defined and sustainable five-year mine
plan.
Lantern Mineralization – Background
The Lantern mineralization was subject to
open-pit mining of oxide areas to a depth of 110 m during 1991-1992
by Dominion Mining. Production during this period totaled 1.37
million tonnes (“Mt”) at an average grade of 2.04 g/t Au for
approximately 90 thousand ounces (“kozs”). Studies in early 2016
revealed potential for the underlying Lantern metasediments in the
core of the Cosmo-Howley fold to host gold mineralization similar
to the Callie Deposit in the Tanami region of the NT. On March 6,
2017, the Company announced the discovery of the Lantern Deposit
based on historical information as well as the result of 25
underground drill holes completed in 2016 to test the down-plunge
extension of the Cosmo open pit (see Kirkland Lake Gold News
Release dated March 6, 2017). On March 28, 2017, an initial Mineral
Resource for the Lantern Deposit was announced, totaling 55.5 kozs
Au (566 thousand tonnes at an average grade of 3.1 g/t Au) in the
Indicated category and 104.0 kozs (1.12 Mt at an average grade
of 2.9 g/t Au) in the Inferred category, using a 2.0 g/t Au cut-off
(see Kirkland Lake Gold News Release dated March 28, 2017, and the
Technical Report dated March 30, 2017).
Since the March 6, 2017 Kirkland Lake Gold News
Release, underground diamond drilling of the Lantern targets has
been accelerated to expand and then infill the Mineral Resources.
It is likely that over 100 additional diamond holes will be
included in the year-end 2017 Lantern Mineral Resource estimate,
which is expected to result in an increase in Mineral Resource
ounces and a higher average grade compared to the previous
estimate.
The additional drilling completed in 2017 has
expanded the previous 6 mineralized lodes to more than 30 lodes,
which comprise Lantern Deposit, with those in the combined Western
Lantern Lode-set being the most continuous and gold endowed (see
Figure 2 and Figures 4 to 9 for Lantern Lodes 3400 to 3900). A
mineralized strike extent of over 500 m, and vertical extent
of 1,000 m is now defined. The mineralization for most lodes is
still untested up‑plunge (shallower) to the south on the western
limb, and down‑plunge (deeper) to the north. Study of the Lantern
and Cosmo alteration zoning suggests that the western fold limb
acted as the main conduit for gold-bearing fluids to become trapped
in the fold hinge and eastern limb effectively against a blanket of
thick and highly-sulfidic carbonaceous black mudstone.
The Lantern mineralization is hosted within
iron-rich, weakly-carbonaceous, siltstones and dolomitic siltstones
with common intense carbonate, sericite-pyrite-chlorite and
blood-red Fe-oxy-hydroxide hypogene alteration, associated with
quartz-carbonate veining. Geological studies strongly suggest
most gold was introduced to the rock after the metamorphic peak,
which has produced a chlorite-biotite-magnetite-tourmaline-garnet
mineral assemblage. Although partly stratabound, gold
mineralization occurs in a quartz-sulfide-carbonate vein network of
steeply-dipping sub-linear shear veins, and associated
sub-horizontal dipping tensile vein arrays.
The Lantern sequence is structurally thickened
by local folding and shears with a moderate 40o to 55o plunge to
the north for the overall mineralized zone, and hosts internal
local steeply-plunging high-grade corridors where quartz veins are
locally at an oblique angle to overall Lantern structure and are
likely to have high gold content.
To view a PDF of the tables and figures as referenced in
this News Release, visit the links below:
Tables – http://resource.globenewswire.com/Resource/Download/f9bc80b0-6d13-428d-a411-2dc0bc868e1f
Figure 1. Location Plan of Cosmo
Mine – http://www.globenewswire.com/NewsRoom/AttachmentNg/813e95ef-245e-4926-9086-18dfcd2d52c6
Figure 2. Schematic Geological Cross
Section of Lantern Deposit, Cosmo Gold
Mine – http://www.globenewswire.com/NewsRoom/AttachmentNg/e5b21720-9270-484f-beb7-eeef603ce796
Figure 3. Long Projection of Lantern
Mineralization – http://www.globenewswire.com/NewsRoom/AttachmentNg/1656b355-8f4a-40cf-b9e8-458ad31766dc
Figure 4. Long Projection of Lantern
3400
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/75afe846-0257-4505-8b93-fee44f119170
Figure 5. Long Projection of Lantern
3500
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/4e1c4a3b-32fb-414d-87e2-723c5342a1d3
Figure 6. Long Projection of Lantern
3600
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/8c166c74-8b5f-43f0-93c5-7dbf238af2b9
Figure 7. Long Projection of Lantern
3700
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/4a23f4df-cd8d-41ab-ad7f-4d74b70fa062
Figure 8. Long Projection of Lantern
3800
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/d2e5fa82-5645-4fa0-9666-a7c9a4b4fcaa
Figure 9. Long Projection of Lantern
3900
Lode – http://www.globenewswire.com/NewsRoom/AttachmentNg/2a3b12b2-c796-4514-910b-b225ae6b964c
Qualified Person
Mark Edwards, FAusIMM (CP), MAIG, Geology
Manager, NT Operations, is a "qualified person" as such term is
defined in National Instrument 43-101 and has reviewed and approved
the technical information and data included in this News
Release.
Drilling and Assay QAQC
Kirkland Lake Gold has in place quality-control
systems to ensure best practice in drilling, sampling and analysis
of drill core. All diamond drill hole collars (Table 2) are
accurately surveyed using a Leica Total Stations instrument and
down hole deviations are measured using a down-hole Gyro
instrument.
All reported drill intercepts are from NQ2 or
HQ3 sized diamond drill core that was sampled from core cut
longitudinally in half with a diamond saw. One-half of the drill
core was sent for assay and the other half retained for reference.
Drill core sample intervals vary between 0.2 and 1.4m in length and
were determined from logging of sulfide and visible gold and
conform to logged lithological and alteration geological
boundaries.
Assay results are based on 50-gram charge fire
assay. Intercepts are constrained with wireframe envelopes,
generally based on a 2 g/t Au cut-off (where possible) and having a
maximum 3 m internal dilution. However, narrower intercepts are
reported to highlight lengths of higher gold grade or where
mineralization is limited. No upper gold grade cap has been applied
to the data. However, during mineral resource work the requirement
for capping assay grades will be assessed.
Drill samples from the Lantern Deposit are
routinely assayed at North Australian Laboratories Pty Ltd, an
independent laboratory in Pine Creek, Northern Territory. Site
audits and reviews of the laboratory are conducted from time to
time as well as routine assessment of intra-laboratory analyses to
ensure quality of reported results.
About Kirkland Lake Gold
Ltd.
Kirkland Lake Gold Ltd. is a mid-tier gold
producer with 2017 target production of 580,000 to 595,000 ounces
from mines in Canada and Australia. The production profile of the
company is anchored from two high-grade, low-cost operations,
including the Macassa Mine located in northeastern Ontario and the
Fosterville Mine located in the state of Victoria, Australia.
Kirkland Lake Gold's solid base of quality assets is complemented
by district scale exploration potential, supported by a strong
financial position with extensive management and operational
expertise.
Cautionary Note Regarding
Forward-Looking Information
This News Release includes certain
"forward-looking statements". All statements other than statements
of historical fact included in this release are forward-looking
statements that involve various risks and uncertainties. These
forward-looking statements include, but are not limited to,
statements with respect to planned exploration programs, costs and
expenditures, changes in mineral resources and conversion of
mineral resources to proven and probable reserves, and other
information that is based on forecasts of future operational or
financial results, estimates of amounts not yet determinable and
assumptions of management. These forward-looking statements
include, but are not limited to, statements with respect to future
exploration potential, project economics, timing and scope of
future exploration, anticipated costs and expenditures, changes in
mineral resources and conversion of mineral resources to proven and
probable reserves, and other information that is based on forecasts
of future operational or financial results, estimates of amounts
not yet determinable and assumptions of management.
Any statements that express or involve
discussions with respect to predictions, expectations, beliefs,
plans, projections, objectives, assumptions or future events or
performance (often, but not always, using words or phrases such as
"expects" or "does not expect", "is expected", "anticipates" or
"does not anticipate", "plans", "estimates" or "intends", or
stating that certain actions, events or results "may", "could",
"would", "might" or "will" be taken, occur or be achieved) are not
statements of historical fact and may be "forward-looking
statements." Forward-looking statements are subject to a variety of
risks and uncertainties that could cause actual events or results
to differ from those reflected in the forward-looking statements.
Exploration results that include geophysics, sampling, and drill
results on wide spacings may not be indicative of the occurrence of
a mineral deposit. Such results do not provide assurance that
further work will establish sufficient grade, continuity,
metallurgical characteristics and economic potential to be classed
as a category of mineral resource. A mineral resource that is
classified as "inferred" or "indicated" has a great amount of
uncertainty as to its existence and economic and legal feasibility.
It cannot be assumed that any or part of an "indicated mineral
resource" or "inferred mineral resource" will ever be upgraded to a
higher category of resource. Investors are cautioned not to assume
that all or any part of mineral deposits in these categories will
ever be converted into proven and probable reserves.
There can be no assurance that forward-looking
statements will prove to be accurate and actual results and future
events could differ materially from those anticipated in such
statements. Important factors that could cause actual results to
differ materially from the Company’s expectations include, among
others, risks related to international operations, risks related to
obtaining the permits required to carry out planned exploration or
development work, the actual results of current exploration
activities, conclusions of economic evaluations and changes in
project parameters as plans continue to be refined as well as
future prices of gold, as well as those factors discussed in the
section entitled "Risk Factors" in the Company’s Annual Information
Form and other disclosures of "Risk Factors" by the Company and its
predecessors, available on SEDAR. Although Kirkland Lake Gold has
attempted to identify important factors that could cause actual
results to differ materially, there may be other factors that cause
results not to be as anticipated, estimated or intended. There can
be no assurance that such statements will prove to be accurate as
actual results and future events could differ materially from those
anticipated in such statements. Accordingly, readers should not
place undue reliance on forward-looking statements.
Cautionary Note to U.S. Investors -
Mineral Reserve and Resource Estimates
All resource and reserve estimates included in
this news release or documents referenced in this news release have
been prepared in accordance with Canadian National Instrument
43-101 - Standards of Disclosure for Mineral Projects ("NI 43-101")
and the Canadian Institute of Mining, Metallurgy and Petroleum (the
"CIM") - CIM Definition Standards on Mineral Resources and Mineral
Reserves, adopted by the CIM Council, as amended (the "CIM
Standards"). NI 43-101 is a rule developed by the Canadian
Securities Administrators, which established standards for all
public disclosure an issuer makes of scientific and technical
information concerning mineral projects. The terms "mineral
reserve", "proven mineral reserve" and "probable mineral reserve"
are Canadian mining terms as defined in accordance with NI 43-101
and the CIM Standards. These definitions differ materially from the
definitions in SEC Industry Guide 7 ("SEC Industry Guide 7") under
the United States Securities Act of 1933, as amended, and the
Exchange Act.
In addition, the terms "mineral resource",
"measured mineral resource", "indicated mineral resource" and
"inferred mineral resource" are defined in and required to be
disclosed by NI 43-101 and the CIM Standards; however, these terms
are not defined terms under SEC Industry Guide 7 and are normally
not permitted to be used in reports and registration statements
filed with the U.S. Securities and Exchange Commission (the "SEC").
Investors are cautioned not to assume that all or any part of
mineral deposits in these categories will ever be converted into
reserves. "Inferred mineral resources" have a great amount of
uncertainty as to their existence, and great uncertainty as to
their economic and legal feasibility. It cannot be assumed that all
or any part of an inferred mineral resource will ever be upgraded
to a higher category. Under Canadian rules, estimates of inferred
mineral resources may not form the basis of feasibility or
pre-feasibility studies, except in very limited circumstances.
Investors are cautioned not to assume that all or any part of a
mineral resource exists, will ever be converted into a mineral
reserve or is or will ever be economically or legally mineable or
recovered.
FOR FURTHER INFORMATION PLEASE CONTACT
Anthony Makuch, President, Chief Executive
Officer & DirectorPhone: +1 416-840-7884E-mail:
tmakuch@klgold.com
Mark Utting, Vice-President, Investor Relations Phone: +1
416-840-7884 E-mail: mutting@klgold.com
Table 1: Drill Assay Intercepts for Surface and
Underground Drilling for the Lantern Deposit
(The Lantern Results are an update to those reported in March 6,
2017 Kirkland Lake Gold News Release)
Hole ID |
From (m) |
To (m) |
Downhole Interval (m) |
Gold Grade (g/t Au) |
Estimated True Width (m) |
Geological Structure |
Lantern 3400 Lode Results |
CW101001A |
No Significant Intercept |
3400 Lode |
CW101002 |
218.90 |
221.75 |
2.85 |
16.2 |
1.4 |
3400 Lode |
CW101003 |
178.15 |
183.90 |
5.75 |
3.9 |
2.5 |
3400 Lode |
CW101004 |
271.50 |
274.50 |
3.00 |
2.6 |
1.3 |
3400 Lode |
CW101005 |
198.60 |
206.00 |
7.40 |
1.3 |
3.1 |
3400 Lode |
CW101006 |
224.70 |
227.95 |
3.25 |
0.7 |
1.4 |
3400 Lode |
CW101010 |
158.00 |
183.30 |
25.30 |
1.4 |
9.4 |
3400 Lode |
CW101011 |
128.00 |
131.00 |
3.00 |
1.3 |
1.6 |
3400 Lode |
CW101012 |
129.30 |
141.10 |
11.80 |
11.9 |
4.9 |
3400 Lode |
And |
152.60 |
167.70 |
15.10 |
12.3 |
8.6 |
3400 Lode |
CW101013 |
No Significant Intercept |
3400 Lode |
CW93515 |
327.00 |
328.00 |
1.00 |
3.9 |
0.6 |
3400 Lode |
DS001 |
202.30 |
213.10 |
10.80 |
0.3 |
7.9 |
3400 Lode |
LS005 |
No Significant Intercept |
3400 Lode |
LS006 |
270.90 |
275.00 |
4.10 |
0.5 |
2.2 |
3400 Lode |
LS007 |
232.00 |
240.00 |
8.00 |
0.3 |
6.9 |
3400 Lode |
LS008 |
215.00 |
217.00 |
2.00 |
1.6 |
1.9 |
3400 Lode |
LU101003 |
85.00 |
89.24 |
4.24 |
1.3 |
2.2 |
3400 Lode |
And |
95.92 |
97.00 |
1.08 |
22.1 |
0.5 |
3400 Lode |
And |
122.00 |
123.00 |
1.00 |
7.9 |
0.6 |
3400 Lode |
LU101004 |
138.30 |
140.00 |
1.70 |
5.1 |
0.8 |
3400 Lode |
LU101009 |
76.20 |
79.55 |
3.35 |
0.8 |
1.8 |
3400 Lode |
LU101013 |
105.00 |
108.00 |
3.00 |
1.8 |
1.8 |
3400 Lode |
LU101014 |
135.30 |
141.20 |
5.90 |
14.6 |
2.8 |
3400 Lode |
LU101015 |
No Significant Intercept |
3400 Lode |
LU101016 |
145.75 |
159.40 |
13.65 |
3.0 |
6.3 |
3400 Lode |
LU101017 |
166.00 |
195.90 |
29.90 |
4.3 |
9.2 |
3400 Lode |
LU101018 |
206.50 |
209.50 |
3.00 |
2.3 |
1.6 |
3400 Lode |
LU101019 |
No Significant Intercept |
3400 Lode |
LU101020 |
174.50 |
193.20 |
18.70 |
40.8 |
5.2 |
3400 Lode |
LU101021 |
No Significant Intercept |
3400 Lode |
LU101022 |
No Significant Intercept |
3400 Lode |
LU101023 |
No Significant Intercept |
3400 Lode |
LU101024 |
267.00 |
272.00 |
5.00 |
0.7 |
2.0 |
3400 Lode |
LU101025 |
193.80 |
196.80 |
3.00 |
1.7 |
1.1 |
3400 Lode |
LU101025 |
No Significant Intercept |
3400 Lode |
LU101026 |
226.30 |
233.90 |
7.60 |
2.4 |
2.0 |
3400 Lode |
LU64001 |
494.20 |
494.80 |
0.60 |
90.9 |
0.2 |
3400 Lode |
LU73011A |
149.00 |
156.00 |
7.00 |
1.5 |
3.3 |
3400 Lode |
LU73012 |
No Significant Intercept |
3400 Lode |
LU73014 |
365.70 |
366.10 |
0.40 |
5.0 |
0.3 |
3400 Lode |
LU73015 |
No Significant Intercept |
3400 Lode |
LU73020 |
265.00 |
267.24 |
2.24 |
3.0 |
1.4 |
3400 Lode |
LU86006 |
No Significant Intercept |
3400 Lode |
LU92001 |
364.50 |
366.80 |
2.30 |
1.0 |
1.2 |
3400 Lode |
LU92002 |
330.40 |
333.10 |
2.70 |
0.9 |
1.4 |
3400 Lode |
LU92003 |
No Significant Intercept |
3400 Lode |
LU92004 |
No Significant Intercept |
3400 Lode |
Lantern 3500 Lode Results |
CW101001A |
No Significant Intercept |
3500 Lode |
CW101002 |
228.80 |
248.20 |
19.40 |
3.7 |
10.1 |
3500 Lode |
CW101003 |
No Significant Intercept |
3500 Lode |
CW101003 |
No Significant Intercept |
3500 Lode |
CW101004 |
284.45 |
286.50 |
2.05 |
2.9 |
0.7 |
3500 Lode |
CW101005 |
219.70 |
221.00 |
1.30 |
70.3 |
0.6 |
3500 Lode |
CW101006 |
238.30 |
253.50 |
15.20 |
2.2 |
6.5 |
3500 Lode |
CW101010 |
194.00 |
203.20 |
9.20 |
4.1 |
3.6 |
3500 Lode |
CW101011 |
142.00 |
148.00 |
6.00 |
1.7 |
3.1 |
3500 Lode |
CW101012 |
173.70 |
178.30 |
4.60 |
2.8 |
2.1 |
3500 Lode |
CW101013 |
No Significant Intercept |
3500 Lode |
CW93513 |
288.10 |
290.55 |
2.45 |
3.7 |
1.3 |
3500 Lode |
CW93515 |
349.00 |
354.00 |
5.00 |
0.7 |
3.0 |
3500 Lode |
CW93516 |
No Significant Intercept |
3500 Lode |
LS001 |
No Significant Intercept |
3500 Lode |
LS005 |
210.00 |
211.00 |
1.00 |
3.2 |
1.0 |
3500 Lode |
LS006 |
No Significant Intercept |
3500 Lode |
LS007 |
224.00 |
226.00 |
2.00 |
1.8 |
1.9 |
3500 Lode |
LS008 |
No Significant Intercept |
3500 Lode |
And |
205.00 |
210.00 |
5.00 |
1.8 |
4.9 |
3500 Lode |
LU101001 |
74.10 |
87.10 |
13.00 |
9.0 |
7.3 |
3500 Lode |
LU101001 |
106.00 |
109.00 |
3.00 |
1.9 |
2.1 |
3500 Lode |
LU101003 |
128.00 |
130.00 |
2.00 |
3.3 |
1.1 |
3500 Lode |
LU101004 |
160.00 |
162.00 |
2.00 |
1.6 |
1.0 |
3500 Lode |
LU101005 |
71.00 |
78.00 |
7.00 |
3.1 |
5.4 |
3500 Lode |
LU101008 |
72.90 |
76.00 |
3.10 |
3.9 |
2.3 |
3500 Lode |
LU101009 |
102.18 |
108.25 |
6.07 |
4.1 |
3.7 |
3500 Lode |
And |
132.72 |
133.13 |
0.41 |
5.7 |
0.3 |
3500 Lode |
LU101010 |
89.00 |
92.70 |
3.70 |
3.8 |
2.1 |
3500 Lode |
LU101013 |
126.30 |
127.60 |
1.30 |
5.9 |
0.7 |
3500 Lode |
And |
132.70 |
144.90 |
12.20 |
2.8 |
7.0 |
3500 Lode |
LU101014 |
171.10 |
174.70 |
3.60 |
4.8 |
1.4 |
3500 Lode |
LU101015 |
137.40 |
143.60 |
6.20 |
0.7 |
3.7 |
3500 Lode |
And |
149.30 |
151.90 |
2.60 |
2.3 |
1.2 |
3500 Lode |
LU101016 |
171.78 |
174.54 |
2.76 |
1.8 |
1.0 |
3500 Lode |
LU101017 |
201.30 |
212.80 |
11.50 |
3.3 |
5.0 |
3500 Lode |
LU101018 |
222.00 |
225.50 |
3.50 |
4.9 |
0.3 |
3500 Lode |
LU101019 |
252.60 |
254.50 |
1.90 |
11.8 |
0.2 |
3500 Lode |
LU101020 |
207.00 |
222.50 |
15.50 |
8.5 |
6.8 |
3500 Lode |
LU101021 |
No Significant Intercept |
3500 Lode |
LU101022 |
199.70 |
203.00 |
3.30 |
3.5 |
1.3 |
3500 Lode |
LU101023 |
246.60 |
248.60 |
2.00 |
2.4 |
0.7 |
3500 Lode |
LU101024 |
No Significant Intercept |
3500 Lode |
LU101025 |
226.30 |
231.50 |
5.20 |
1.0 |
1.8 |
3500 Lode |
LU101026 |
275.00 |
289.00 |
14.00 |
0.7 |
3.6 |
3500 Lode |
LU64001 |
305.60 |
308.60 |
3.00 |
10.8 |
1.2 |
3500 Lode |
LU73011A |
193.10 |
195.30 |
2.20 |
2.8 |
1.0 |
3500 Lode |
LU73012 |
No Significant Intercept |
3500 Lode |
LU73014 |
444.00 |
464.00 |
20.00 |
0.6 |
4.8 |
3500 Lode |
LU73015 |
304.80 |
308.00 |
3.20 |
2.4 |
1.1 |
3500 Lode |
LU73020 |
273.00 |
273.50 |
0.50 |
57.9 |
0.3 |
3500 Lode |
LU86006 |
274.00 |
278.15 |
4.15 |
1.4 |
1.6 |
3500 Lode |
LU92001 |
377.50 |
379.50 |
2.00 |
1.0 |
1.0 |
3500 Lode |
LU92002 |
No Significant Intercept |
3500 Lode |
LU92003 |
No Significant Intercept |
3500 Lode |
LU92004 |
No Significant Intercept |
3500 Lode |
LU93501 |
No Significant Intercept |
3500 Lode |
LU93504 |
207.10 |
212.80 |
5.70 |
0.9 |
3.8 |
3500 Lode |
Lantern 3600 Lode Results |
CW101001A |
250.80 |
273.50 |
22.70 |
0.4 |
9.8 |
3600 Lode |
CW101002 |
253.00 |
258.00 |
5.00 |
1.9 |
2.2 |
3600 Lode |
CW101003 |
No Significant Intercept |
3600 Lode |
CW101004 |
314.10 |
321.85 |
7.75 |
1.2 |
3.0 |
3600 Lode |
CW101005 |
235.90 |
263.00 |
27.10 |
1.6 |
10.4 |
3600 Lode |
CW101006 |
261.80 |
273.60 |
11.80 |
3.4 |
6.2 |
3600 Lode |
CW101010 |
217.00 |
223.00 |
6.00 |
2.7 |
2.7 |
3600 Lode |
CW101011 |
165.00 |
166.00 |
1.00 |
4.5 |
0.7 |
3600 Lode |
CW101012 |
No Significant Intercept |
3600 Lode |
CW101013 |
No Significant Intercept |
3600 Lode |
CW93513 |
312.20 |
317.90 |
5.70 |
0.3 |
4.0 |
3600 Lode |
CW93515 |
358.00 |
382.00 |
24.00 |
1.0 |
12.8 |
3600 Lode |
DS001 |
184.20 |
185.20 |
1.00 |
89.7 |
0.8 |
3600 Lode |
LS001 |
No Significant Intercept |
3600 Lode |
LS005 |
193.00 |
195.80 |
2.80 |
3.1 |
2.6 |
3600 Lode |
LS006 |
239.00 |
239.72 |
0.72 |
32.4 |
0.7 |
3600 Lode |
LS007 |
214.00 |
219.00 |
5.00 |
3.2 |
3.5 |
3600 Lode |
LS008 |
184.00 |
186.00 |
2.00 |
1.3 |
1.9 |
3600 Lode |
LU101001 |
128.50 |
132.65 |
4.15 |
1.1 |
2.9 |
3600 Lode |
LU101003 |
160.00 |
160.64 |
0.64 |
4.7 |
0.4 |
3600 Lode |
LU101004 |
No Significant Intercept |
3600 Lode |
LU101005 |
109.50 |
112.00 |
2.50 |
5.4 |
1.9 |
3600 Lode |
And |
119.50 |
120.85 |
1.35 |
6.1 |
1.1 |
3600 Lode |
LU101008 |
98.00 |
105.40 |
7.40 |
8.4 |
6.4 |
3600 Lode |
LU101009 |
142.40 |
143.54 |
1.14 |
3.5 |
0.8 |
3600 Lode |
LU101010 |
115.00 |
119.35 |
4.35 |
2.5 |
3.4 |
3600 Lode |
LU101011 |
100.00 |
102.00 |
2.00 |
1.5 |
1.4 |
3600 Lode |
LU101013 |
151.40 |
158.10 |
6.70 |
3.8 |
3.9 |
3600 Lode |
LU101014 |
180.20 |
187.00 |
6.80 |
4.9 |
3.5 |
3600 Lode |
LU101015 |
171.50 |
173.40 |
1.90 |
6.3 |
1.0 |
3600 Lode |
LU101016 |
No Significant Intercept |
3600 Lode |
LU101017 |
225.90 |
231.00 |
5.10 |
3.3 |
1.4 |
3600 Lode |
LU101018 |
255.40 |
262.50 |
7.10 |
3.3 |
1.8 |
3600 Lode |
LU101019 |
282.90 |
284.90 |
2.00 |
3.0 |
0.6 |
3600 Lode |
LU101020 |
No Significant Intercept |
3600 Lode |
LU101021 |
286.70 |
293.70 |
7.00 |
2.4 |
3.6 |
3600 Lode |
LU101022 |
No Significant Intercept |
3600 Lode |
LU101023 |
293.00 |
305.00 |
12.00 |
1.8 |
4.5 |
3600 Lode |
LU101024 |
322.00 |
341.00 |
19.00 |
1.5 |
3.1 |
3600 Lode |
LU101025 |
No Significant Intercept |
3600 Lode |
LU101026 |
300.60 |
319.70 |
19.10 |
11.7 |
6.5 |
3600 Lode |
LU64001 |
180.40 |
181.10 |
0.70 |
16.1 |
0.3 |
3600 Lode |
LU64003 |
130.00 |
137.00 |
7.00 |
5.1 |
4.2 |
3600 Lode |
LU73011A |
223.20 |
254.90 |
31.70 |
0.1 |
13.0 |
3600 Lode |
LU73012 |
344.00 |
352.00 |
8.00 |
1.9 |
3.2 |
3600 Lode |
LU73014 |
No Significant Intercept |
3600 Lode |
LU73015 |
No Significant Intercept |
3600 Lode |
LU73016 |
No Significant Intercept |
3600 Lode |
LU73017 |
No Significant Intercept |
3600 Lode |
LU73020 |
277.42 |
278.33 |
0.91 |
1,624 |
0.6 |
3600 Lode |
Including |
277.42 |
277.73 |
0.31 |
4,750 |
0.2 |
3600 Lode |
LU86006 |
324.00 |
328.20 |
4.20 |
2.6 |
1.3 |
3600 Lode |
LU92001 |
395.60 |
398.70 |
3.10 |
1.0 |
1.6 |
3600 Lode |
LU92002 |
No Significant Intercept |
3600 Lode |
LU92003 |
No Significant Intercept |
3600 Lode |
LU92004 |
No Significant Intercept |
3600 Lode |
LU93501 |
No Significant Intercept |
3600 Lode |
LU93504 |
No Significant Intercept |
3600 Lode |
Lantern 3700 Lode Results |
CP009W1 |
722.28 |
724.38 |
2.10 |
7.0 |
0.9 |
3700 Lode |
CW101001A |
296.45 |
298.20 |
1.75 |
37.0 |
0.8 |
3700 Lode |
CW101002 |
No Significant Intercept |
3700 Lode |
CW101003 |
258.60 |
259.65 |
1.05 |
170 |
0.5 |
3700 Lode |
CW101005 |
No Significant Intercept |
3700 Lode |
CW101006 |
329.30 |
331.50 |
2.20 |
2.1 |
0.9 |
3700 Lode |
CW101010 |
272.10 |
274.00 |
1.90 |
5.3 |
0.8 |
3700 Lode |
CW101011 |
189.00 |
190.00 |
1.00 |
0.7 |
0.5 |
3700 Lode |
CW101012 |
236.30 |
237.00 |
0.70 |
4.9 |
0.3 |
3700 Lode |
CW101013 |
No Significant Intercept |
3700 Lode |
CW93513 |
No Significant Intercept |
3700 Lode |
CW93515 |
No Significant Intercept |
3700 Lode |
CW93516 |
360.90 |
366.80 |
5.90 |
2.8 |
2.6 |
3700 Lode |
DS001 |
No Significant Intercept |
3700 Lode |
LS005 |
183.00 |
185.00 |
2.00 |
1.9 |
1.9 |
3700 Lode |
LS006 |
205.00 |
206.00 |
1.00 |
1.9 |
0.9 |
3700 Lode |
LS007 |
195.00 |
197.00 |
2.00 |
3.9 |
1.6 |
3700 Lode |
LS008 |
173.00 |
176.00 |
3.00 |
4.8 |
2.9 |
3700 Lode |
LU101001 |
136.00 |
137.75 |
1.75 |
1.4 |
1.2 |
3700 Lode |
LU101002 |
No Significant Intercept |
3700 Lode |
LU101003 |
171.00 |
172.50 |
1.50 |
1.1 |
1.0 |
3700 Lode |
LU101004 |
No Significant Intercept |
3700 Lode |
LU101005 |
No Significant Intercept |
3700 Lode |
LU101006A |
No Significant Intercept |
3700 Lode |
LU101008 |
114.00 |
117.15 |
3.15 |
4.3 |
2.3 |
3700 Lode |
LU101009 |
149.97 |
151.80 |
1.83 |
6.6 |
1.2 |
3700 Lode |
LU101010 |
152.00 |
155.25 |
3.25 |
2.7 |
1.9 |
3700 Lode |
And |
161.10 |
164.15 |
3.05 |
2.4 |
1.9 |
3700 Lode |
LU101013 |
179.10 |
180.90 |
1.80 |
1.8 |
1.0 |
3700 Lode |
LU101014 |
231.30 |
234.00 |
2.70 |
3.3 |
1.3 |
3700 Lode |
LU101015 |
195.50 |
197.10 |
1.60 |
6.4 |
0.8 |
3700 Lode |
LU101016 |
234.05 |
237.30 |
3.25 |
0.7 |
1.6 |
3700 Lode |
LU101017 |
No Significant Intercept |
3700 Lode |
LU101018 |
No Significant Intercept |
3700 Lode |
LU101019 |
304.60 |
307.20 |
2.60 |
1.5 |
1.0 |
3700 Lode |
LU101020 |
291.00 |
292.00 |
1.00 |
10.5 |
0.5 |
3700 Lode |
LU101021 |
362.00 |
364.00 |
2.00 |
1.5 |
0.9 |
3700 Lode |
LU101022 |
272.70 |
274.60 |
1.90 |
3.7 |
0.8 |
3700 Lode |
LU101023 |
357.80 |
363.00 |
5.20 |
0.2 |
2.4 |
3700 Lode |
LU101024 |
419.20 |
433.20 |
14.00 |
0.1 |
4.8 |
3700 Lode |
LU101025 |
314.00 |
315.00 |
1.00 |
3.7 |
0.3 |
3700 Lode |
LU101026 |
332.70 |
359.00 |
26.30 |
2.7 |
15.0 |
3700 Lode |
LU63003 |
224.00 |
225.90 |
1.90 |
1.9 |
1.2 |
3700 Lode |
LU64001 |
129.90 |
138.00 |
8.10 |
4.7 |
3.2 |
3700 Lode |
LU64003 |
122.00 |
125.00 |
3.00 |
10.5 |
1.8 |
3700 Lode |
LU73005 |
323.00 |
338.50 |
15.50 |
0.3 |
7.6 |
3700 Lode |
LU73007 |
219.00 |
220.00 |
1.00 |
3.0 |
0.7 |
3700 Lode |
LU73009 |
266.00 |
267.00 |
1.00 |
2.2 |
0.5 |
3700 Lode |
LU73011A |
No Significant Intercept |
3700 Lode |
LU73012 |
397.20 |
400.00 |
2.80 |
1.2 |
1.1 |
3700 Lode |
LU73014 |
549.00 |
574.00 |
25.00 |
0.3 |
6.6 |
3700 Lode |
LU73015 |
412.00 |
415.20 |
3.20 |
2.8 |
1.3 |
3700 Lode |
LU73016 |
No Significant Intercept |
3700 Lode |
LU73017 |
378.20 |
411.00 |
32.80 |
0.2 |
15.5 |
3700 Lode |
LU73020 |
286.00 |
288.06 |
2.06 |
9.9 |
1.3 |
3700 Lode |
LU92001 |
434.90 |
436.70 |
1.80 |
1.7 |
1.0 |
3700 Lode |
LU92002 |
365.50 |
380.00 |
14.50 |
0.6 |
7.6 |
3700 Lode |
LU92003 |
488.00 |
507.00 |
19.00 |
1.8 |
7.6 |
3700 Lode |
LU92004 |
368.00 |
372.00 |
4.00 |
0.7 |
2.7 |
3700 Lode |
Lantern 3800 Lode Results |
CP009W1 |
802.39 |
806.30 |
3.91 |
3.4 |
1.7 |
3800 Lode |
CW101001A |
318.40 |
322.00 |
3.60 |
2.0 |
1.5 |
3800 Lode |
CW101002 |
No Significant Intercept |
3800 Lode |
CW101003 |
286.40 |
289.30 |
2.90 |
3.4 |
1.5 |
3800 Lode |
CW101006 |
No Significant Intercept |
3800 Lode |
CW101010 |
No Significant Intercept |
3800 Lode |
CW101011 |
No Significant Intercept |
3800 Lode |
CW101012 |
No Significant Intercept |
3800 Lode |
CW101013 |
304.50 |
306.00 |
1.50 |
3.4 |
0.7 |
3800 Lode |
CW93513 |
364.70 |
369.50 |
4.80 |
3.7 |
2.4 |
3800 Lode |
CW93515 |
435.60 |
439.30 |
3.70 |
1.5 |
1.8 |
3800 Lode |
CW93516 |
381.60 |
384.00 |
2.40 |
2.6 |
1.2 |
3800 Lode |
DS001 |
150.00 |
151.05 |
1.05 |
2.6 |
0.8 |
3800 Lode |
GFG001W1 |
No Significant Intercept |
3800 Lode |
LS001 |
No Significant Intercept |
3800 Lode |
LS003 |
No Significant Intercept |
3800 Lode |
LS005 |
160.00 |
161.00 |
1.00 |
1.9 |
0.9 |
3800 Lode |
LS006 |
189.00 |
191.00 |
2.00 |
1.0 |
1.6 |
3800 Lode |
LS007 |
No Significant Intercept |
3800 Lode |
LS008 |
156.00 |
159.00 |
3.00 |
0.4 |
2.9 |
3800 Lode |
LU101001 |
167.00 |
170.00 |
3.00 |
4.3 |
2.2 |
3800 Lode |
LU101003 |
No Significant Intercept |
3800 Lode |
LU101004 |
No Significant Intercept |
3800 Lode |
LU101005 |
155.00 |
159.00 |
4.00 |
1.1 |
3.0 |
3800 Lode |
LU101008 |
No Significant Intercept |
3800 Lode |
LU101009 |
173.30 |
174.30 |
1.00 |
2.2 |
0.8 |
3800 Lode |
LU101010 |
171.75 |
173.40 |
1.65 |
3.0 |
1.2 |
3800 Lode |
LU101011 |
No Significant Intercept |
3800 Lode |
LU101013 |
189.90 |
191.80 |
1.90 |
1.6 |
1.2 |
3800 Lode |
LU101014 |
247.70 |
248.70 |
1.00 |
2.6 |
0.5 |
3800 Lode |
LU101015 |
No Significant Intercept |
3800 Lode |
LU101016 |
247.75 |
248.70 |
0.95 |
2.4 |
0.4 |
3800 Lode |
LU101017 |
325.00 |
326.00 |
1.00 |
1.2 |
0.4 |
3800 Lode |
LU101018 |
No Significant Intercept |
3800 Lode |
LU101019 |
350.50 |
352.10 |
1.60 |
2.0 |
0.6 |
3800 Lode |
LU101021 |
No Significant Intercept |
3800 Lode |
LU101022 |
293.70 |
297.10 |
3.40 |
1.8 |
1.1 |
3800 Lode |
LU101023 |
No Significant Intercept |
3800 Lode |
LU101024 |
441.00 |
445.00 |
4.00 |
2.1 |
1.3 |
3800 Lode |
LU101025 |
352.30 |
355.30 |
3.00 |
2.7 |
0.6 |
3800 Lode |
LU101026 |
No Significant Intercept |
3800 Lode |
LU63001 |
182.80 |
183.70 |
0.90 |
26.9 |
0.7 |
3800 Lode |
LU63002 |
206.50 |
207.30 |
0.80 |
2.3 |
0.6 |
3800 Lode |
LU63003 |
249.30 |
250.40 |
1.10 |
0.5 |
0.8 |
3800 Lode |
LU63004 |
175.60 |
176.60 |
1.00 |
5.9 |
0.9 |
3800 Lode |
LU63005 |
228.00 |
231.00 |
3.00 |
0.5 |
2.1 |
3800 Lode |
LU63006 |
283.60 |
285.30 |
1.70 |
2.4 |
0.9 |
3800 Lode |
LU63007 |
215.00 |
217.50 |
2.50 |
4.6 |
1.8 |
3800 Lode |
LU64001 |
123.00 |
125.95 |
2.95 |
9.5 |
1.2 |
3800 Lode |
LU64003 |
98.80 |
104.30 |
5.50 |
3.6 |
3.3 |
3800 Lode |
LU73001 |
126.40 |
130.00 |
3.60 |
0.9 |
2.8 |
3800 Lode |
LU73002 |
191.00 |
193.00 |
2.00 |
5.5 |
1.2 |
3800 Lode |
And |
No Significant Intercept |
3800 Lode |
LU73003 |
158.30 |
159.30 |
1.00 |
10.7 |
0.6 |
3800 Lode |
LU73004 |
238.20 |
241.00 |
2.80 |
0.8 |
1.8 |
3800 Lode |
LU73005 |
No Significant Intercept |
3800 Lode |
LU73006 |
No Significant Intercept |
3800 Lode |
LU73007 |
No Significant Intercept |
3800 Lode |
LU73008 |
191.90 |
192.80 |
0.90 |
4.5 |
0.5 |
3800 Lode |
LU73009 |
No Significant Intercept |
3800 Lode |
LU73010 |
No Significant Intercept |
3800 Lode |
LU73011A |
No Significant Intercept |
3800 Lode |
LU73012 |
445.10 |
456.10 |
11.00 |
0.5 |
5.1 |
3800 Lode |
LU73014 |
604.00 |
611.00 |
7.00 |
0.4 |
3.8 |
3800 Lode |
LU73015 |
No Significant Intercept |
3800 Lode |
LU73016 |
313.00 |
316.10 |
3.10 |
0.7 |
2.1 |
3800 Lode |
LU73017 |
493.00 |
496.00 |
3.00 |
198 |
1.0 |
3800 Lode |
Including |
493.00 |
493.35 |
0.35 |
98.7 |
0.1 |
3800 Lode |
And including |
493.35 |
493.70 |
0.35 |
1,577 |
0.1 |
3800 Lode |
LU86001 |
219.00 |
226.60 |
7.60 |
1.4 |
4.4 |
3800 Lode |
And |
No Significant Intercept |
3800 Lode |
LU86002 |
No Significant Intercept |
3800 Lode |
And |
250.00 |
251.00 |
1.00 |
5.9 |
0.8 |
3800 Lode |
LU86006 |
No Significant Intercept |
3800 Lode |
LU92001 |
No Significant Intercept |
3800 Lode |
LU92002 |
388.00 |
393.00 |
5.00 |
1.4 |
2.6 |
3800 Lode |
LU92004 |
No Significant Intercept |
3800 Lode |
LU93501 |
267.00 |
269.00 |
2.00 |
2.4 |
1.4 |
3800 Lode |
LU93504 |
272.00 |
275.70 |
3.70 |
1.0 |
2.6 |
3800 Lode |
Lantern 3900 Lode Results |
CP009W1 |
821.43 |
832.76 |
11.33 |
3.1 |
3.0 |
3900 Lode |
CW101001A |
375.00 |
377.70 |
2.70 |
1.2 |
1.4 |
3900 Lode |
CW101002 |
378.00 |
380.30 |
2.30 |
7.7 |
0.9 |
3900 Lode |
CW101006 |
No Significant Intercept |
3900 Lode |
CW101010 |
No Significant Intercept |
3900 Lode |
CW101011 |
No Significant Intercept |
3900 Lode |
CW101012 |
287.00 |
291.00 |
4.00 |
6.9 |
1.9 |
3900 Lode |
CW101013 |
324.40 |
333.00 |
8.60 |
3.5 |
3.4 |
3900 Lode |
CW93513 |
398.50 |
407.45 |
8.95 |
1.7 |
3.8 |
3900 Lode |
CW93515 |
462.00 |
467.40 |
5.40 |
4.7 |
2.7 |
3900 Lode |
CW93516 |
400.30 |
405.10 |
4.80 |
2.6 |
2.1 |
3900 Lode |
DS001 |
121.60 |
123.60 |
2.00 |
1.6 |
1.6 |
3900 Lode |
LS001 |
No Significant Intercept |
3900 Lode |
LS005 |
138.00 |
141.00 |
3.00 |
13.7 |
2.8 |
3900 Lode |
LS006 |
170.00 |
173.00 |
3.00 |
5.1 |
2.4 |
3900 Lode |
LS007 |
No Significant Intercept |
3900 Lode |
LS008 |
130.00 |
132.20 |
2.20 |
4.6 |
1.9 |
3900 Lode |
LU101001 |
178.45 |
181.00 |
2.55 |
3.2 |
1.9 |
3900 Lode |
LU101002 |
106.00 |
107.00 |
1.00 |
2.6 |
1.0 |
3900 Lode |
LU101003 |
No Significant Intercept |
3900 Lode |
LU101004 |
287.18 |
294.00 |
6.82 |
2.1 |
3.3 |
3900 Lode |
LU101005 |
No Significant Intercept |
3900 Lode |
LU101006A |
No Significant Intercept |
3900 Lode |
LU101008 |
176.30 |
183.00 |
6.70 |
1.4 |
5.2 |
3900 Lode |
LU101009 |
193.97 |
195.80 |
1.83 |
1.9 |
1.3 |
3900 Lode |
LU101010 |
215.00 |
216.00 |
1.00 |
5.4 |
0.7 |
3900 Lode |
LU101011 |
No Significant Intercept |
3900 Lode |
LU101013 |
No Significant Intercept |
3900 Lode |
LU101014 |
278.00 |
286.80 |
8.80 |
22.6 |
4.4 |
3900 Lode |
LU101015 |
245.50 |
248.00 |
2.50 |
5.1 |
1.6 |
3900 Lode |
LU101016 |
272.20 |
279.20 |
7.00 |
1.0 |
3.3 |
3900 Lode |
LU101017 |
No Significant Intercept |
3900 Lode |
LU101018 |
364.20 |
375.60 |
11.40 |
1.5 |
4.6 |
3900 Lode |
LU101019 |
382.00 |
385.10 |
3.10 |
6.1 |
1.5 |
3900 Lode |
LU101020 |
353.00 |
357.00 |
4.00 |
1.6 |
1.2 |
3900 Lode |
LU101021 |
388.80 |
399.80 |
11.00 |
1.9 |
4.3 |
3900 Lode |
LU101022 |
351.40 |
354.50 |
3.10 |
26.3 |
1.2 |
3900 Lode |
LU101023 |
419.20 |
427.50 |
8.30 |
1.7 |
2.9 |
3900 Lode |
LU101024 |
480.80 |
484.00 |
3.20 |
12.2 |
1.1 |
3900 Lode |
LU101025 |
447.80 |
452.60 |
4.80 |
3.8 |
0.9 |
3900 Lode |
LU101026 |
563.70 |
566.70 |
3.00 |
1.6 |
0.8 |
3900 Lode |
LU63001 |
192.10 |
194.30 |
2.20 |
2.0 |
1.6 |
3900 Lode |
LU63003 |
266.00 |
268.00 |
2.00 |
2.0 |
1.4 |
3900 Lode |
LU63005 |
251.90 |
260.00 |
8.10 |
5.9 |
6.0 |
3900 Lode |
LU63006 |
353.80 |
354.80 |
1.00 |
6.5 |
0.5 |
3900 Lode |
LU63007 |
240.60 |
241.60 |
1.00 |
2.0 |
0.7 |
3900 Lode |
LU64001 |
88.50 |
93.10 |
4.60 |
6.7 |
1.8 |
3900 Lode |
LU64003 |
61.00 |
62.00 |
1.00 |
8.3 |
0.6 |
3900 Lode |
LU73001 |
153.55 |
158.20 |
4.65 |
3.2 |
3.8 |
3900 Lode |
LU73002 |
No Significant Intercept |
3900 Lode |
LU73003 |
174.10 |
179.90 |
5.80 |
1.1 |
4.4 |
3900 Lode |
LU73004 |
No Significant Intercept |
3900 Lode |
LU73005 |
No Significant Intercept |
3900 Lode |
LU73006 |
168.50 |
174.80 |
6.30 |
0.8 |
4.5 |
3900 Lode |
LU73007 |
254.20 |
257.00 |
2.80 |
1.3 |
1.7 |
3900 Lode |
LU73008 |
No Significant Intercept |
3900 Lode |
And |
219.50 |
221.50 |
2.00 |
1.6 |
1.4 |
3900 Lode |
LU73009 |
350.20 |
353.00 |
2.80 |
4.7 |
1.2 |
3900 Lode |
LU73010 |
195.00 |
198.00 |
3.00 |
2.9 |
2.0 |
3900 Lode |
LU73011A |
396.80 |
400.00 |
3.20 |
1.4 |
1.5 |
3900 Lode |
LU73012 |
483.10 |
485.00 |
1.90 |
4.7 |
1.0 |
3900 Lode |
LU73014 |
No Significant Intercept |
3900 Lode |
LU73015 |
488.00 |
489.00 |
1.00 |
2.0 |
0.5 |
3900 Lode |
LU73016 |
345.90 |
347.50 |
1.60 |
2.0 |
0.6 |
3900 Lode |
LU73017 |
No Significant Intercept |
3900 Lode |
LU73020 |
364.00 |
365.00 |
1.00 |
5.1 |
0.6 |
3900 Lode |
LU86001 |
281.90 |
288.90 |
7.00 |
3.1 |
4.6 |
3900 Lode |
LU86002 |
243.00 |
249.00 |
6.00 |
2.1 |
3.2 |
3900 Lode |
And |
272.00 |
280.90 |
8.90 |
2.3 |
5.7 |
3900 Lode |
LU86004 |
No Significant Intercept |
3900 Lode |
LU86005 |
No Significant Intercept |
3900 Lode |
LU86006 |
No Significant Intercept |
3900 Lode |
LU92001 |
No Significant Intercept |
3900 Lode |
LU92002 |
No Significant Intercept |
3900 Lode |
LU92003 |
618.00 |
619.70 |
1.70 |
2.1 |
0.8 |
3900 Lode |
LU92004 |
No Significant Intercept |
3900 Lode |
LU93501 |
312.00 |
315.00 |
3.00 |
3.0 |
2.2 |
3900 Lode |
LU93502 |
No Significant Intercept |
3900 Lode |
LU93503 |
No Significant Intercept |
3900 Lode |
LU93504 |
293.00 |
296.25 |
3.25 |
0.6 |
2.6 |
3900 Lode |
And |
306.50 |
323.00 |
16.50 |
3.4 |
12.3 |
3900 Lode |
Drill Intercept Notes:
- Intercepts with >30 Gram-Metres (gold grade (g/t Au) x
estimated true width (m)) are in bold text.
- Intercepts are constrained with wireframe envelopes, generally
based on a 2 g/t Au cut-off (where possible) and having a maximum 3
m internal dilution. However, narrower intercepts are reported to
highlight lengths of higher gold grade or where mineralization is
limited.
- Drillholes that were reported in previous News Releases are
shown in italics, and may have different reported intercepts due to
changes in the geological understanding of mineralized structures
and application of reporting criteria previously applied.
Table 2: Surface and Underground Diamond
Drill Hole Collar Locations, Lantern Deposit.
Hole ID |
Northing (m) |
Easting (m) |
Elevation (m) |
Collar Azimuth (°) |
Collar Plunge (°) |
Hole Length (m) |
Surface Drilling |
DS001 |
971 |
4,825 |
1,141 |
87.5 |
-65.3 |
766.0 |
LS001 |
1,329 |
4,753 |
1,144 |
85.1 |
-61.1 |
586.0 |
LS003 |
1,385 |
4,672 |
1,145 |
84.5 |
-63.0 |
677.7 |
LS004 |
1,385 |
4,672 |
1,145 |
84.2 |
-51.8 |
552.4 |
LS005 |
1,117 |
4,787 |
1,145 |
89.0 |
-52.0 |
252.9 |
LS006 |
1,117 |
4,787 |
1,145 |
89.5 |
-67.1 |
303.6 |
LS007 |
1,273 |
4,796 |
1,145 |
90.5 |
-64.0 |
384.6 |
LS008 |
1,273 |
4,796 |
1,145 |
90.5 |
-53.1 |
498.9 |
LS009 |
1,102 |
5,171 |
1,156 |
270.0 |
-50.6 |
162.3 |
Underground Drilling |
LU101001 |
1,335 |
5,020 |
1,016 |
222.8 |
13.7 |
440.8 |
LU101002 |
1,336 |
5,019 |
1,017 |
252.2 |
29.5 |
160.0 |
LU101003 |
1,335 |
5,020 |
1,015 |
222.3 |
-2.7 |
263.9 |
LU101004 |
1,335 |
5,020 |
1,015 |
209.7 |
2.3 |
350.5 |
LU101005 |
1,336 |
5,019 |
1,015 |
234.8 |
6.2 |
200.9 |
LU101006A |
1,335 |
5,021 |
1,014 |
255.2 |
6.0 |
179.1 |
LU101007 |
1,337 |
5,019 |
1,016 |
272.7 |
20.2 |
231.0 |
LU101008 |
1,337 |
5,019 |
1,014 |
249.3 |
-8.9 |
311.0 |
LU101009 |
1,336 |
5,019 |
1,014 |
235.8 |
-12.3 |
313.0 |
LU101010 |
1,336 |
5,020 |
1,014 |
248.3 |
-21.1 |
331.0 |
LU101011 |
1,337 |
5,019 |
1,014 |
262.1 |
-20.1 |
233.6 |
LU101012 |
1,337 |
5,019 |
1,014 |
274.6 |
-1.8 |
170.7 |
LU101013 |
1,336 |
5,019 |
1,014 |
234.3 |
-18.1 |
236.6 |
LU101014 |
1,336 |
5,020 |
1,014 |
223.3 |
-14.8 |
305.6 |
LU101015 |
1,336 |
5,020 |
1,014 |
240.8 |
-26.2 |
275.0 |
LU101016 |
1,336 |
5,020 |
1,014 |
234.6 |
-28.0 |
302.7 |
LU101017 |
1,336 |
5,020 |
1,014 |
231.2 |
-30.4 |
383.0 |
LU101018 |
1,336 |
5,020 |
1,014 |
226.7 |
-29.9 |
446.5 |
LU101019 |
1,336 |
5,020 |
1,014 |
222.3 |
-28.2 |
419.7 |
LU101020 |
1,336 |
5,020 |
1,014 |
236.8 |
-35.5 |
416.0 |
LU101021 |
1,336 |
5,020 |
1,014 |
226.2 |
-34.1 |
417.0 |
LU101022 |
1,336 |
5,020 |
1,014 |
242.2 |
-40.4 |
407.0 |
LU101023 |
1,337 |
5,019 |
1,014 |
233.9 |
-40.1 |
503.9 |
LU101024 |
1,336 |
5,020 |
1,014 |
226.0 |
-38.4 |
533.8 |
LU101025 |
1,337 |
5,019 |
1,014 |
250.6 |
-45.1 |
452.6 |
LU101026 |
1,337 |
5,019 |
1,014 |
246.0 |
-47.1 |
617.6 |
LU63001 |
1,550 |
4,875 |
635 |
249.0 |
1.8 |
220.0 |
LU63002 |
1,550 |
4,875 |
634 |
249.6 |
-9.0 |
248.0 |
LU63003 |
1,550 |
4,875 |
634 |
250.9 |
-17.8 |
282.2 |
LU63004 |
1,550 |
4,875 |
635 |
265.1 |
6.3 |
230.7 |
LU63005 |
1,550 |
4,875 |
634 |
257.4 |
-12.5 |
284.0 |
LU63006 |
1,550 |
4,875 |
634 |
254.6 |
-24.2 |
378.1 |
LU63007 |
1,550 |
4,875 |
634 |
271.2 |
-6.4 |
275.7 |
LU64001 |
1,842 |
4,629 |
624 |
273.5 |
-83.1 |
587.0 |
LU64003 |
1,841 |
4,629 |
624 |
166.1 |
-51.1 |
389.0 |
LU73001 |
1,495 |
4,920 |
734 |
237.5 |
15.7 |
203.1 |
LU73002 |
1,495 |
4,920 |
733 |
240.6 |
-11.2 |
248.0 |
LU73003 |
1,495 |
4,920 |
733 |
256.2 |
-5.5 |
200.0 |
LU73004 |
1,495 |
4,921 |
732 |
258.7 |
-24.4 |
284.2 |
LU73005 |
1,496 |
4,921 |
732 |
259.1 |
-36.4 |
484.4 |
LU73006 |
1,495 |
4,920 |
733 |
246.8 |
-1.8 |
200.0 |
LU73007 |
1,495 |
4,921 |
732 |
243.1 |
-23.0 |
287.2 |
LU73008 |
1,495 |
4,920 |
733 |
251.5 |
-14.7 |
242.1 |
LU73009 |
1,495 |
4,921 |
732 |
248.8 |
-31.1 |
368.0 |
LU73010 |
1,496 |
4,921 |
733 |
267.4 |
-12.5 |
227.4 |
LU73011A |
1,494 |
4,922 |
732 |
226.9 |
-21.2 |
445.0 |
LU73012 |
1,495 |
4,922 |
732 |
229.1 |
-34.4 |
545.4 |
LU73014 |
1,494 |
4,922 |
732 |
221.9 |
-35.6 |
650.0 |
LU73015 |
1,495 |
4,922 |
732 |
239.3 |
-41.9 |
567.0 |
LU73016 |
1,496 |
4,922 |
732 |
249.9 |
-38.4 |
427.0 |
LU73017 |
1,496 |
4,921 |
732 |
260.9 |
-42.6 |
572.0 |
LU73020 |
1,499 |
4,922 |
732 |
389.9 |
-13.9 |
303.0 |
LU86001 |
1,502 |
4,987 |
859 |
219.9 |
-2.0 |
314.5 |
LU86002 |
1,501 |
4,986 |
858 |
226.5 |
-11.3 |
368.0 |
LU86004 |
1,502 |
4,986 |
859 |
229.1 |
0.5 |
368.0 |
LU86005 |
1,502 |
4,986 |
858 |
232.2 |
-9.4 |
236.6 |
LU86006 |
1,501 |
4,986 |
858 |
221.5 |
-25.1 |
480.0 |
LU92001 |
1,305 |
5,079 |
920 |
235.8 |
-32.1 |
536.2 |
LU92002 |
1,305 |
5,079 |
920 |
253.4 |
-36.2 |
506.0 |
LU92003 |
1,305 |
5,079 |
920 |
251.6 |
-43.7 |
773.0 |
LU92004 |
1,305 |
5,078 |
920 |
246.3 |
-28.9 |
490.0 |
LU93501 |
1,460 |
5,074 |
939 |
231.6 |
-5.5 |
333.0 |
LU93502 |
1,460 |
5,074 |
939 |
239.3 |
-2.2 |
281.8 |
LU93503 |
1,460 |
5,074 |
939 |
241.1 |
-9.4 |
473.0 |
LU93504 |
1,460 |
5,074 |
939 |
234.1 |
-13.2 |
341.9 |
Total - Surface and Underground
Drilling |
74 holes |
27,737 m |
Previously Reported Drilling |
Surface Drilling |
|
|
|
|
|
|
CP009W1 |
1,617 |
5,270 |
1,155 |
241.0 |
-54.0 |
950.1 |
GFG001W1 |
1,840 |
5,195 |
1,159 |
240.0 |
-60.0 |
1,019.3 |
Underground Drilling |
|
|
|
|
|
|
CW101001 |
1,346 |
5,038 |
1,013 |
256.8 |
-40.4 |
72.6 |
CW101001A |
1,345 |
5,038 |
1,013 |
253.6 |
-42.1 |
441.0 |
CW101002 |
1,345 |
5,038 |
1,013 |
239.2 |
-35.5 |
431.8 |
CW101003 |
1,345 |
5,038 |
1,013 |
247.8 |
-36.6 |
308.0 |
CW101004 |
1,345 |
5,038 |
1,013 |
240.1 |
-42.8 |
340.8 |
CW101005 |
1,344 |
5,039 |
1,014 |
221.3 |
-22.5 |
303.0 |
CW101006 |
1,345 |
5,040 |
1,013 |
233.8 |
-31.1 |
425.9 |
CW101007A |
1,321 |
5,038 |
1,015 |
99.7 |
-4.7 |
72.0 |
CW101008 |
1,320 |
5,038 |
1,014 |
112.0 |
-23.5 |
92.4 |
CW101009 |
1,320 |
5,038 |
1,015 |
118.6 |
-3.5 |
98.7 |
CW101010 |
1,335 |
5,020 |
1,014 |
229.8 |
-28.5 |
368.9 |
CW101011 |
1,335 |
5,020 |
1,014 |
228.1 |
-14.0 |
386.3 |
CW101012 |
1,336 |
5,020 |
1,014 |
239.7 |
-31.0 |
329.9 |
CW101013 |
1,335 |
5,020 |
1,014 |
214.2 |
-17.5 |
373.3 |
CW93501 |
1,456 |
5,076 |
940 |
201.6 |
7.4 |
284.8 |
CW93502 |
1,457 |
5,075 |
940 |
217.4 |
-0.3 |
143.4 |
CW93503 |
1,457 |
5,075 |
941 |
223.6 |
27.0 |
170.1 |
CW93504 |
1,457 |
5,075 |
939 |
211.6 |
-9.2 |
155.8 |
CW93505 |
1,456 |
5,076 |
941 |
193.2 |
20.2 |
185.0 |
CW93506 |
1,456 |
5,076 |
939 |
193.7 |
-7.0 |
183.0 |
CW93507 |
1,457 |
5,075 |
940 |
210.2 |
9.1 |
140.2 |
CW93508 |
1,458 |
5,075 |
940 |
223.1 |
9.8 |
128.3 |
CW93509 |
1,459 |
5,074 |
940 |
236.8 |
9.8 |
156.6 |
CW93510 |
1,458 |
5,075 |
939 |
222.9 |
-9.0 |
130.9 |
CW93511 |
1,459 |
5,074 |
939 |
237.3 |
-8.7 |
146.1 |
CW93513 |
1,459 |
5,075 |
939 |
236.9 |
-24.5 |
441.6 |
CW93515 |
1,458 |
5,075 |
939 |
219.9 |
-13.3 |
491.2 |
CW93516 |
1,459 |
5,075 |
939 |
243.8 |
-29.9 |
409.5 |
- Holes previously reported are in italics
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