Kirkland Lake Gold Ltd. (“
Kirkland Lake
Gold” or the “
Company”) (TSX:KL)
(NYSE:KL) (ASX:KLA) today announced new high-grade results from
surface and underground drilling at the Fosterville Mine in
Victoria, Australia. Recent infill drilling in the Swan Zone has
returned intercepts with higher than anticipated grades and
visible-gold near the intersection of the Swan Fault and the Swan
Splay structure. Surface drilling has continued to target
additional growth in the Robbin’s Hill gold system to assess the
potential of further Mineral Reserve expansion. Underground growth
drilling programs have also progressed in the Lower Phoenix gold
system targeting the Cygnet Fault, and in the Harrier gold system
targeting the Harrier Base Fault, where encouraging results have
been returned. Drill results reported are from 44 holes (6,803 m)
from the Swan infill drilling program and 111 holes (59,311 m) from
step out, extension and infill drilling at Robbin’s Hill, Cygnet
and Harrier (Figures 1 & 2).
Tony Makuch, President and CEO of Kirkland Lake
Gold, commented: “Drilling at Fosterville continues to demonstrate
the significant size and scale of the mineralized structures, all
of which contain quartz veining with visible-gold and all of which
have the potential to host additional Swan or Swan-like zones. At
the Swan Zone, results from new infill drilling include higher than
expected grades, which is encouraging as we work towards our next
Mineral Reserve and Mineral Resource update. In particular, the
infill results confirm that the area where the Swan Fault and Swan
Footwall Splay intersect contains more gold than currently
modelled.
“At Robbin’s Hill, exploration activities are
progressing well with recent surface drill results significantly
expanding the size of the mineralized system and demonstrating the
potential for continued Mineral Resource and Mineral Reserve growth
along both the Curie and surrounding mineralized structures.
Encouragingly, drilling and recent modelling of newly-acquired 3D
seismic data clearly establish the potential for other mineralized
structures within the Robbin’s Hill area, where there are
several historical open pits with plunge extents to be
investigated. The new twin underground exploration ramp we are
developing will be extremely important for the future exploration
of these areas as well as Robbin’s Hill itself. The ramp is
advancing well, having been driven over 1,330 m to the end of
June.
“Drill results at Cygnet and Harrier also
continue to return encouraging results. At the Cygnet structure,
approximately 125 m footwall to Swan, new drilling returned
multiple significant intercepts beyond the northern extent of the
existing Mineral Resource. There are several high-grade
intersections with visible-gold in the Cygnet system, which extends
over a 750 m strike length and 300 m vertically. At Harrier, new
drilling returned high-grade mineralization outside of the existing
Mineral Reserves, and also demonstrated the continuity of the
Harrier structure for an additional 400 metres down-plunge-plunge,
with the system remaining open for further expansion. As with Lower
Phoenix and Robbin’s Hill, the exploration potential at both Cygnet
and Harrier is substantial and we are increasingly confident that
significant new Mineral Reserves and Mineral Resources can be
identified with further drilling.”
Exploration activities at Fosterville ceased in
late March as part of the Company’s COVID-19 response, which
included the suspension of all non-essential work. Prior to this
time, work on the exploration program was advancing with four
surface drills and nine underground drills at Fosterville on the
mine lease and three surface drills on regional projects. With the
suspension of exploration work, all surface drilling was
discontinued and underground drilling was reduced to three drills,
all being dedicated to supporting operations and sustaining capital
drill requirements. Discussions and proactive planning with
drilling contractors were undertaken in early April to manage
COVID-19 risks with strict control measures being implemented to
support a resumption of exploration drilling. By the middle of the
month, two underground drills and two surface drills were deployed.
The ramp up of operating drills has continued, with the current
fleet standing at four surface drills at Robbin’s Hill and six
underground drills active at the Fosterville mine. Regional
exploration drilling remains suspended as part of the Company’s
ongoing response to COVID-19.
Swan Infill Drilling
Programs
Infill drilling into the Swan Mineral Reserves
since the December 2019 Mineral Resource and Reserve update has
returned results with higher than expected grades, demonstrating
the potential to increase the mine’s Mineral Reserves in this zone
with further model updates. Intercepts of significant high-grade,
visible-gold mineralization of substantial width were returned in a
zone where the Swan Footwall Splay intersects the Swan (Figure 3).
Two infill holes into this zone returned gram-meter (gold grade x
estimated true width) intercepts greater than 5000 gram-m, with a
further three intercepts returning greater than 1000 gram-m, with
the key intercepts listed below:
- 976 g/t Au over 7.4 m (ETW 7.0 m) in hole UDH3167, incl. 5,710
g/t Au over 1.3m (ETW 1.2 m);
- 933 g/t Au over 6.4 m (ETW 5.8 m) in hole UDH3405, incl. 6,202
g/t Au over 1.0 m (ETW 0.9 m);
- 416 g/t Au over 6.8 m (ETW 5.6 m) in hole UDH3392, incl. 3,510
g/t Au over 0.8 m (ETW 0.7 m);
- 222 g/t Au over 8.1 m (ETW 7.3 m) in hole UDH3169, incl. 1,684
g/t Au over 1.0 m (ETW 0.9 m); and
- 156 g/t Au over 9.2 m (ETW 8.6 m) in hole UDH3360, incl. 307
g/t Au over 1.7m (ETW 1.6 m)
These results demonstrate the continuity of
extremely high-grade, visible-gold mineralization along the
structural intersection of the Swan Fault and Swan Footwall Splay,
which plunges gently towards the south. Recent mine development
into this zone also confirms the continuity of this mineralization,
with this new information expected to result in the addition of new
ounces in this area as part of future Mineral Resource model
updates. Mine production in the zone of current infill drilling and
development is expected to extend through the 2020 – 2023
period.
Further infill drilling targeting this
intersection area is scheduled for the second half of 2020, which
will establish increased drill density and has the potential to
support Mineral Reserve growth. In addition, recent drill platform
development has been completed and will support continued infill
drilling of the down-plunge Swan Inferred Mineral Resources.
Drilling using the new platform infrastructure has commenced with
three rigs currently in operation.
Robbin’s Hill Drilling
Programs
The drill results reported were drilled from
late Q4 2019 and through the first half of 2020 by up to six
surface diamond drills operating in the Robbin’s Hill area. The
primary target was gold mineralization along the west-dipping Curie
Fault, one of the controlling structures for mineralization at
Robbins’s Hill. Programs have included infill drilling within the
existing Mineral Resource, and extension and step out drilling
along the Robbin’s Hill Curie Fault mineralization trend. Four
surface drills are currently operating at Robbins Hill focused on
Mineral Resource extension including identifying the potential
high-grade shoot down-plunge. Drilling programs in the second half
of the year will expand to cover targets generated from the
interpretation of 3D seismic data integrated with other geophysical
data sets (Figure 4).
Extension Drilling
Twenty-seven surface drill holes for a total of
23,173 m were drilled targeting the down-plunge extensions of
existing Mineral Resources and Mineral Reserves on the Curie Fault.
The objective of this surface program is to obtain sufficient drill
coverage to assess Mineral Resource potential down-plunge
southwards to the ~11500mN before the end of 2020. The results of
this drilling to date support the potential extension of Curie
Fault mineralization approximately 950 m down-plunge from current
Mineral Reserves (Figure 5). Additional drilling is required to
establish continuity over this 950 m area.
Key sulfide-gold bearing intercepts include:
- 30.8 g/t Au over 3.6 m (ETW 2.9 m) in hole RHD355;
- 9.6 g/t Au over 4.6 m (ETW 3.7 m) in hole RHD365;
- 7.7 g/t Au over 3.7 m (ETW 2.8 m) in hole RHD387B;
- 10.6 g/t Au over 1.6 m (ETW 1.6 m) in hole RHD374; and
- 4.9g/t Au over 17.8m (ETW 11.7m) in hole RHD400A
Results down-plunge of the current Mineral
Reserves show southerly plunging zones of high-grade gold
mineralization within the broader, lower grade mineralized Curie
Fault system. The main zone of high‑grade mineralization that
supported the Robbin’s Hill maiden Mineral Reserve is located where
the west dipping Curie Fault structure transects and offsets a
felsic dyke that has intruded along an anticlinal fold axis. Other
zones of dilation and high-grade mineralization are emerging along
the Curie Fault as it transects the folded sequence, as represented
by a grouping of higher-grade results including RHD408 and RHD387B
(Figure 5). These zones are typically represented by zones of
extensional veining and disseminated sulfide gold mineralization,
but often have stibnite-enriched quartz veins indicating a high
potential for visible-gold mineralization.
Two recent diamond drill holes in RHD413 and
RHD411A have intersected visible-gold mineralization at depth as
part of this program, further reinforcing the growth potential in
this area.
RHD413 intersects the Curie Fault approximately
950 m down-plunge from Mineral Reserves where the hole transects
the eastern limb of an anticline. The structure hosts a 0.6 m wide
brecciated to massive quartz vein containing 2-3mm slugs and specs
of visible-gold which run parallel to a stylolite approximately 50
mm from the lower vein contact. The vein is surrounded by
disseminated sulfide mineralization and tension veining, which is
more prevalent in the sandstone dominated footwall, extending for
approximately 2 m from the vein. This visible-gold occurrence is
the deepest and southernmost observed occurrence on the Curie Fault
to date (Figure 5).
Further to this, visible-gold mineralization has
been intersected in other structures adjacent to the Curie Fault.
RHD411A intercepted two westerly dipping quartz veins of 150-200 mm
thickness approximately 60 m hangingwall of the Curie Fault (Figure
5). The two veins contain strong laminations and stylolitic
textures, the lower of which contained a spec of visible-gold.
Disseminated stockwork veining and sulfide mineralization, whilst
relatively constrained on the hangingwall, extends at least 3 m
into the footwall of the structure.
A significant part of the planned drill programs
at Robbin’s Hill for the remainder of 2020 will aim to further
define the continuity and extent of these high-grade mineralized
shoots down-plunge, which are open for expansion at
depth.
In addition to results returned from the
continued expansion drilling targeting the Curie Fault at Robbin’s
Hill, a significant intercept containing visible-gold on the
adjacent Herschel Fault was returned. Hole RHD408 contained an
approximate 100 mm wide quartz interval containing a quartz vein
bearing visible‑gold and stylolitic textures surrounded by a halo
of disseminated sulfide mineralization with an estimated true width
of 3.2 m.
Key visible-gold bearing intercept:
- 68.1 g/t Au over 4.4 m (ETW 3.2 m) in hole RHD408, incl. 747
g/t Au over 0.35 m (ETW 0.3m)
The Herschel Fault occurs approximately 200 m
hangingwall to the Curie Fault at the northing of intersection
(Figure 6) Surface drilling targeting Curie has incidentally
intersected the Herschel Fault through recent drill programs.
Initial interpretations suggest that mineralization is orientated
on the north-south trending west-dipping fault and requires further
drilling to determine its strike, dip and down‑plunge
lengths. There is potential connectivity with mineralization
associated with the Robbin’s Hill pit towards the north, which also
has occurrences of visible-gold mineralization, However, further
drilling and interpretation work is required to confirm this. The
intercept for RHD408 demonstrates the potential for high-grade
visible‑gold mineralization along the structure, and vectoring in
on its location and determining its extent will form part of future
drill programs in the Robbin’s Hill area.
Step out drilling
Six step-out drill holes, totaling 7,343m
demonstrate that mineralization on the Curie Fault persists over a
2 km distance to the south of the existing Robbins Hill Mineral
Reserves (Figure 5). Intercepts from this drilling demonstrate the
scale and growth potential of the Robbin’s Hill mineralized system
which has the potential to similar in size and scale to the Phoenix
system (approximately 3.5 km in strike length) at Fosterville.
Drill holes RHD395, RHD376 and RHD379 targeted the Curie Fault
beyond 1.5 km to the south of Mineral Resources, and each hole
intersected significant quartz-dominant stockwork disseminated
sulfide mineralization. The intercepts for RHD395 and RHD376 were
characterized by increased sulfide mineralization at a fault in an
oblique-oblique structural setting on the eastern limb of a
parasitic anticlinal fold. Drill hole RHD379 intersected the
Curie Fault, adjacent to an up-dip syncline axial plane, with east
dipping mineralized structures also identified in the hanging-wall
(Figure 5).
The most southern sulfide-gold bearing
intercepts include:
- 2.9 g/t Au over 2.6 m (ETW 2.0 m) in hole RHD395;
- 2.5 g/t Au over 5.3 m (ETW 4.6 m) in hole RHD376; and
- 1.8 g/t Au over 7.9 m (ETW 7.6 m) in hole RHD379
The demonstrated extent and scale of the system highlights the
opportunity through further drilling to realize substantial Mineral
Resource growth.
High-Resolution 3D Seismic
Survey
The Company completed a high-resolution 3D
Seismic survey in the northern part of the Fosterville Mining
License over the Robbin’s Hill mineralization trend. The survey was
the first of its kind to be undertaken in Victoria for gold
exploration and provides a high-resolution 3D dataset to a depth of
over 1 km for detailed planning of future of underground
development.
The survey area was approximately 6 km2 with
data collected along 12.5 m spaced east‑west lines (Figure 4).
Initial processing of the 3D seismic data was completed in April
with fold resolution defined to 30 m and significant structural
trends identified. Interpretation of this data is underway and
combined with other geophysical datasets target generation work is
progressing. The seismic data will contribute to the geological
understanding and aid future exploration and development of the
Robbin’s Hill area.
Robbin’s Hill Underground Decline
Development
Underground development of the Robbin’s Hill
ramp commenced in January this year and has progressed ahead of
schedule, advancing a total of 1,336 m to the end of June. The
recent arrival of a smart jumbo will provide increased development
capacity and we will be targeting a total of 3,380 m of development
at Robbin’s Hill in 2020. The development will be used as an
underground drill platform for exploration diamond drilling
activities as the ramp progresses.
Cygnet Drilling Programs
Recent drilling exploring the northern
extensions of the Cygnet Mineral Resources have returned
encouraging results with three returning intercepts greater than 30
gram-meters (Figure 7). The Cygnet Fault key intercepts
include:
- 13.6 g/t Au over 6.6 m (ETW 5.9 m) in hole UDH3398;
- 10.8 g/t Au over 2.9 m (ETW 2.9 m) in hole UDH3207A; and
- 5.4 g/t Au over 9.7 m (ETW 8.0 m) in hole UDH3206
These results demonstrate the potential for
further expansion of Cygnet Mineral Resources to the north and
exploration drill programs during the second half of 2020 will
initially target up to 250 m beyond existing Mineral Resources.
In addition, infill drill results into the
Cygnet Mineral Resources continue to return encouraging results and
both Cygnet and subsidiary structures Cygnet Hangingwall and
Footwall Splays contain significant mineralization(Figure 7 &
8) including key intercepts:
Cygnet Infill
- 12.7 g/t Au over 2.1 m (ETW 2.1 m) in hole UDH3196;
- 11.0 g/t Au over 8.5 m (ETW 5.7 m) in hole UDH3492;
- 8.1 g/t Au over 4.9 (ETW 4.2 m) in hole UDH3485;
- 9.4 g/t Au over 3.1 m (ETW 2.0 m) in hole UDH3417A; and
- 6.1 g/t Au over 6.0 m (ETW 5.6m) in hole UDE279
Cygnet Splays
- 36.6 g/t Au over 2.2 m (ETW 1.9 m) in hole UDH3492, incl. 168
g/t Au over 0.4 m (ETW 0.3 m); and
- 4.2 g/t Au over 4.3 m (ETW 4.1 m) in hole UDH3206
Infill drill programs into Cygnet will continue
throughout the second half of 2020, with the objective to increase
resource confidence to enable mineral reserve evaluation in this
zone at the end of the year.
Harrier Drilling Programs
Recent drilling exploring the down dip and
southern extensions of the Harrier Base Fault have returned
encouraging results, demonstrating continued growth opportunity in
the Harrier system.
High-grade sulfide mineralization has been
intersected on the Harrier Base Fault between the 4150 and 4250mRLs
(Figure 9), displaying grades and widths with significant potential
to support further Mineral Reserve expansion in this zone.
The Harrier Base Fault key intercepts outside of December 2019
Mineral Reserves include:
- 20.9 g/t Au over 5.9 m (ETW 5.5 m) in hole UDH3045 incl. 295
g/t Au over 0.3 m (ETW 0.3 m);
- 22.8 g/t Au(1) over 4.3 m (ETW 3.7 m) in hole UDH3474A;
- 24.5 g/t Au over 3.8 m (ETW 3.8 m) in hole UDH3497;
- 12.0 g/t Au over 3.8 m (ETW 3.7 m) in hole UDH3498;
- 8.3 g/t Au over 9.4 m (ETW 9.3 m) in hole UDH3510; and
- 5.2 g/t Au over 6.9 m (ETW 6.8 m) in hole UDH3499
In addition, drilling targeting the Harrier Base
Fault down-plunge demonstrates that continuity of mineralization
extends a distance of approximately 400 m down-plunge of the lowest
Mineral Reserves and is open for further exploration targeting.
Mineralization grades and widths of significance occur along this
plunge extent and include:
- 8.1 g/t Au over 4.5 m (ETW 3.9 m) in hole UDE239;
Further to this, drilling extended below the
Harrier Base fault has outlined the stratigraphic and structural
framework to assist with further target generation in the Harrier
zone (Figure 10). Structures footwall to the Harrier Base have
displayed evidence of sulfide mineralization (Wagtail) and present
future targets at depth.
The Harrier gold system has now been defined
over a down-plunge extent of approximately 3.4 km and remains open
for expansion. Future drilling in the Harrier zone will test target
strike and dip extensions of known mineralized structures such as
the Harrier Base Fault as well as adjacent trends of known and
interpreted mineralization.
Qualified Persons
Troy Fuller, MAIG, Director of Exploration,
Australia, 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.
For further information regarding the Company’s
2019 Mineral Reserves and Mineral Resources estimates for the
Fosterville Gold Mine, please refer to the Company’s News Release
dated February 29, 2020 and the Technical Report entitled “Updated
NI 43-101 Technical Report Fosterville Gold Mine In the State of
Victoria, Australia” effective December 31, 2018.
Drilling and Underground Sampling 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 TS16 Total Station instrument and
down-hole deviations are measured by either electronic gyro or
single-shot instruments.
Sampling consisted of diamond drill core that
was either full core (i.e. for Swan drill samples) or half core
sampled. Half core samples were cut longitudinally in half with a
diamond saw; one-half of the drill core was sent to an independent
laboratory for analysis and the other drill core half retained for
reference. Sample pulps are returned from the
assay laboratory for reference and future geological or
metallurgical studies. Drill core sample intervals vary between 0.3
and 1.2m in length and were determined from logging of sulfide and
visible-gold to geological boundaries.
Samples containing visible-gold or considered
likely to contain visible-gold were separated from sulfide gold
samples and dispatched independently for assaying. At the
laboratory “visible-gold” jobs were processed through a single
pulverizer and material barren of gold (‘quartz wash’) was crushed
before and after each sample to minimize the potential for gold to
contaminate successive samples.
Assays are either based on 25-gram fire assay.
Mean grades are calculated using a variable lower grade cut-off
(generally 2 g/t Au) and maximum 2 m internal dilution. No upper
gold grade cut is applied to the data. However, during future
Mineral Resource studies the requirement for assay top cutting will
be assessed.
The samples were assayed at On Site Laboratory
Services, an independent laboratory in Bendigo, Victoria. The
facility is registered under ISO 9001:2015 (CERT-40147) and
operates in accordance with ISO/IEC17025 (accreditation no. 20456)
under National Association of Testing Authorities, Australia
(NATA).
About Kirkland Lake Gold Ltd.
Kirkland Lake Gold Ltd. is a growing gold
producer operating in Canada and Australia that produced 974,615
ounces in 2019. The production profile of the Company is anchored
by three high-quality operations, including the Macassa Mine and
Detour Lake Mine, both located in Northern 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 expertise.
For further information on Kirkland Lake Gold
and to receive news releases by email, visit the website at
www.kl.gold.
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 Resource estimates, potential
growth in Mineral Resources, conversion of Mineral Resources to
proven and probable Mineral 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, financial statements and related MD&A for the periods
ended December 31, 2019 and March 31, 2020 and other disclosures of
"Risk Factors" by the Company and its predecessors, which are filed
with the securities regulatory authorities in certain provinces in
Canada and available on SEDAR. Although the Company has attempted
to identify key factors that could cause actual results to differ
materially, there may be other factors that cause unanticipated and
unintended results. 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@kl.gold
Mark Utting, Senior Vice President, Investor Relations Phone: +1
416-840-7884 E-mail: mutting@kl.gold
Table 1:Drill Assay Intercepts for the
Swan Fault, Curie Fault, Curie Hangingwall Fault, Curie Footwall
Fault, Herschel Fault, Cygnet Fault, Cygnet Hangingwall Splay,
Cygnet Footwall Splay and Harrier Base Fault at Fosterville Gold
Mine.
(The results are later than those used for the December 31, 2019
Mineral Resources and Mineral Reserves update of The Fosterville
Gold Mine)
Hole ID |
From (m) |
To (m) |
Downhole Interval (m) |
Estimated True Width (m) |
Gold Grade (g/t Au) |
Geological Structure |
Swan Fault Mineralization |
UDE285 |
654.6 |
657.5 |
2.9 |
1.9 |
2.9 |
Swan Fault |
UDH3167(1) |
74.35 |
81.7 |
7.35 |
7.0 |
976 |
Swan Fault |
Including(1) |
74.75 |
76 |
1.25 |
1.2 |
5,710 |
Swan Fault |
UDH3168(1) |
87.45 |
91.9 |
4.45 |
4.0 |
99.2 |
Swan Fault |
Including(1) |
89.35 |
89.65 |
0.3 |
0.3 |
1,270 |
Swan Fault |
UDH3169(1) |
82.6 |
90.7 |
8.1 |
7.3 |
222 |
Swan Fault |
Including(1) |
83.1 |
84.1 |
1.0 |
0.9 |
1,684 |
Swan Fault |
UDH3185(1) |
135 |
141.45 |
6.45 |
4.1 |
50.9 |
Swan Fault |
Including(1) |
140.25 |
140.75 |
0.5 |
0.3 |
546 |
Swan Fault |
UDH3267(1) |
108 |
113.8 |
5.8 |
5.3 |
53.0 |
Swan Fault |
Including(1) |
111.35 |
111.65 |
0.3 |
0.3 |
890 |
Swan Fault |
UDH3269(1) |
101.2 |
113.05 |
11.85 |
10.7 |
55.1 |
Swan Fault |
Including(1) |
111.3 |
111.65 |
0.35 |
0.3 |
1,520 |
Swan Fault |
UDH3271 |
102.9 |
119.35 |
16.45 |
14.3 |
9.1 |
Swan Fault |
UDH3272(1) |
107 |
117.3 |
10.3 |
9.3 |
157 |
Swan Fault |
Including(1) |
107.7 |
109.1 |
1.4 |
1.3 |
1,122 |
Swan Fault |
UDH3274(1) |
115.9 |
119 |
3.1 |
2.7 |
31.4 |
Swan Fault |
Including(1) |
117.8 |
118.15 |
0.35 |
0.3 |
243 |
Swan Fault |
UDH3276(1) |
106.5 |
110.2 |
3.7 |
3.6 |
551 |
Swan Fault |
Including(1) |
107.85 |
108.25 |
0.4 |
0.4 |
5,010 |
Swan Fault |
UDH3278(1) |
116.2 |
123.7 |
7.5 |
6.8 |
67.6 |
Swan Fault |
Including(1) |
116.5 |
117.4 |
0.9 |
0.8 |
479 |
Swan Fault |
UDH3279(1) |
125.15 |
129.55 |
4.4 |
3.7 |
35.5 |
Swan Fault |
Including(1) |
125.45 |
125.75 |
0.3 |
0.3 |
374 |
Swan Fault |
UDH3280(1) |
110.2 |
121.8 |
11.6 |
10.9 |
28.9 |
Swan Fault |
Including(1) |
116.8 |
117.3 |
0.5 |
0.5 |
425 |
Swan Fault |
UDH3281(1) |
116.4 |
126.86 |
10.46 |
10.0 |
17.3 |
Swan Fault |
Including(1) |
122.5 |
122.9 |
0.4 |
0.4 |
123 |
Swan Fault |
UDH3282(1) |
132.1 |
141.15 |
9.05 |
5.8 |
9.5 |
Swan Fault |
UDH3283 |
107.1 |
120.75 |
13.65 |
12.5 |
16.7 |
Swan Fault |
Including |
112.3 |
113 |
0.7 |
0.6 |
122 |
Swan Fault |
UDH3284 |
102.5 |
116.9 |
14.4 |
14.1 |
7.4 |
Swan Fault |
UDH3320 |
113.4 |
118.05 |
4.65 |
3.8 |
12.8 |
Swan Fault |
UDH3322 |
124.7 |
127.95 |
3.25 |
2.8 |
28.3 |
Swan Fault |
UDH3324 |
124.8 |
130.7 |
5.9 |
4.8 |
7.3 |
Swan Fault |
UDH3326(1) |
122.8 |
124.6 |
1.8 |
1.6 |
228 |
Swan Fault |
Including(1) |
123.7 |
124 |
0.3 |
0.3 |
1,310 |
Swan Fault |
UDH3328 |
136.7 |
137.1 |
0.4 |
0.3 |
3.9 |
Swan Fault |
UDH3332 |
134.5 |
136.7 |
2.2 |
2.0 |
21.5 |
Swan Fault |
UDH3334 |
142.75 |
144.7 |
1.95 |
1.3 |
17.3 |
Swan Fault |
UDH3360(1) |
115.05 |
124.2 |
9.15 |
8.6 |
156 |
Swan Fault |
Including(1) |
115.05 |
116.7 |
1.65 |
1.6 |
307 |
Swan Fault |
UDH3361(1) |
104.7 |
116.55 |
11.85 |
10.3 |
68.9 |
Swan Fault |
Including(1) |
109.2 |
110.5 |
1.3 |
1.1 |
530 |
Swan Fault |
UDH3362(1) |
110.7 |
125.05 |
14.35 |
10.2 |
54.6 |
Swan Fault |
Including(1) |
112.9 |
114 |
1.1 |
0.8 |
581 |
Swan Fault |
UDH3364(1) |
98.85 |
115.1 |
16.25 |
15.3 |
18.2 |
Swan Fault |
Including(1) |
106.8 |
107.85 |
1.05 |
1.0 |
200 |
Swan Fault |
UDH3365(1) |
99.4 |
113.3 |
13.9 |
11.3 |
40.8 |
Swan Fault |
Including(1) |
108.1 |
109 |
0.9 |
0.7 |
515 |
Swan Fault |
UDH3367(1) |
103 |
114.1 |
11.1 |
10.1 |
13.9 |
Swan Fault |
Including(1) |
104.9 |
105.6 |
0.7 |
0.6 |
114 |
Swan Fault |
UDH3384(1) |
76.1 |
83.05 |
6.95 |
6.5 |
70.0 |
Swan Fault |
Including(1) |
79.5 |
79.95 |
0.45 |
0.4 |
870 |
Swan Fault |
UDH3385(1) |
79.3 |
87.25 |
7.95 |
7.5 |
13.8 |
Swan Fault |
UDH3386(1) |
71.7 |
74.4 |
2.7 |
2.7 |
63.7 |
Swan Fault |
Including(1) |
71.7 |
72.1 |
0.4 |
0.4 |
351 |
Swan Fault |
UDH3387 |
84.4 |
90.5 |
6.1 |
5.3 |
7.6 |
Swan Fault |
UDH3389(1) |
65.5 |
72.15 |
6.65 |
5.8 |
94.2 |
Swan Fault |
Including(1) |
70.35 |
71.85 |
1.5 |
1.3 |
400 |
Swan Fault |
UDH3390(1) |
75.3 |
81.1 |
5.8 |
5.7 |
89.6 |
Swan Fault |
Including(1) |
78.75 |
79.65 |
0.9 |
0.9 |
518 |
Swan Fault |
UDH3391(1) |
74.7 |
85.45 |
10.75 |
10.8 |
9.6 |
Swan Fault |
UDH3392(1) |
81.8 |
88.6 |
6.8 |
5.6 |
416 |
Swan Fault |
Including(1) |
86.4 |
87.2 |
0.8 |
0.7 |
3,510 |
Swan Fault |
UDH3393 |
87.4 |
92 |
4.6 |
4.6 |
11.9 |
Swan Fault |
UDH3405(1) |
125.6 |
131.95 |
6.35 |
5.8 |
933 |
Swan Fault |
Including(1) |
127.65 |
128.6 |
0.95 |
0.9 |
6,202 |
Swan Fault |
UDH3406(1) |
122.75 |
128 |
5.25 |
3.7 |
55.3 |
Swan Fault |
Including(1) |
123.9 |
124.4 |
0.5 |
0.4 |
296 |
Swan Fault |
And(1) |
125.5 |
126 |
0.5 |
0.4 |
251 |
Swan Fault |
UDH3407 |
115 |
119 |
4.0 |
2.8 |
2.7 |
Swan Fault |
UDH3408(1) |
108.45 |
114.3 |
5.85 |
5.8 |
74.2 |
Swan Fault |
Including(1) |
109 |
109.3 |
0.3 |
0.3 |
1,080 |
Swan Fault |
Curie Fault
Mineralization |
RHD327 |
450.20 |
453.50 |
3.3 |
3.2 |
7.3 |
Curie Fault |
RHD355 |
760.95 |
764.50 |
3.55 |
2.9 |
30.8 |
Curie Fault |
RHD357 |
1,500.35 |
1,500.85 |
0.5 |
0.5 |
5.2 |
Curie Fault |
RHD358 |
744.90 |
748.85 |
3.95 |
3.0 |
1.4 |
Curie Fault |
RHD360 |
671.50 |
674.85 |
3.35 |
3.1 |
0.4 |
Curie Fault |
RHD361 |
716.05 |
718.35 |
2.3 |
1.7 |
0.8 |
Curie Fault |
RHD362 |
368.40 |
370.50 |
2.1 |
2.0 |
0.1 |
Curie Fault |
RHD364 |
754.45 |
759.85 |
5.4 |
4.7 |
4.5 |
Curie Fault |
RHD365 |
780.90 |
785.50 |
4.6 |
3.7 |
9.6 |
Curie Fault |
Including |
782.10 |
782.60 |
0.5 |
0.4 |
19.9 |
Curie Fault |
RHD366A |
825.30 |
826.70 |
1.4 |
1.2 |
1.4 |
Curie Fault |
RHD366D |
873.70 |
874.40 |
0.7 |
0.6 |
4.7 |
Curie Fault |
RHD367 |
755.85 |
760.00 |
4.15 |
3.3 |
3.3 |
Curie Fault |
RHD369 |
796.05 |
797.15 |
1.1 |
1.0 |
0.5 |
Curie Fault |
RHD374 |
1,252.30 |
1,253.90 |
1.6 |
1.6 |
10.6 |
Curie Fault |
RHD375 |
771.60 |
774.00 |
2.4 |
1.6 |
10.8 |
Curie Fault |
RHD376 |
1,107.90 |
1,113.15 |
5.25 |
4.6 |
2.5 |
Curie Fault |
RHD378 |
844.25 |
849.35 |
5.1 |
3.6 |
2.4 |
Curie Fault |
RHD379 |
795.90 |
803.75 |
7.85 |
7.6 |
1.8 |
Curie Fault |
RHD386 |
822.70 |
827.10 |
4.4 |
2.8 |
4.3 |
Curie Fault |
RHD387B |
804.35 |
808.00 |
3.65 |
2.8 |
7.7 |
Curie Fault |
RHD392 |
862.55 |
864.35 |
1.8 |
1.2 |
2.8 |
Curie Fault |
RHD394 |
745.85 |
747.10 |
1.25 |
0.9 |
0.7 |
Curie Fault |
RHD395 |
1,181.15 |
1,183.75 |
2.6 |
2.0 |
2.9 |
Curie Fault |
RHD397 |
773.50 |
775.20 |
1.7 |
1.6 |
4.5 |
Curie Fault |
RHD398 |
803.20 |
807.45 |
4.25 |
3.4 |
0.9 |
Curie Fault |
RHD398A |
834.25 |
835.20 |
0.95 |
0.8 |
1.1 |
Curie Fault |
RHD400 |
823.40 |
835.60 |
12.2 |
7.6 |
2.2 |
Curie Fault |
RHD400A |
816.25 |
820.20 |
3.95 |
2.5 |
2.0 |
Curie Fault |
And |
828.25 |
846.00 |
17.75 |
11.7 |
5.0 |
Curie Fault |
RHD402 |
715.45 |
717.20 |
1.75 |
1.5 |
8.2 |
Curie Fault |
RHD402B |
681.65 |
684.50 |
2.85 |
2.6 |
5.3 |
Curie Fault |
RHD408 |
756.10 |
760.65 |
4.55 |
3.8 |
4.3 |
Curie Fault |
RHD413 (1) |
Visible-gold observed at 114m downhole. Results
pending |
Curie Fault |
Curie Hangingwall Fault |
RHD411A (1) |
Visible-gold observed at 829m downhole. Results
pending |
Curie HW Fault |
Herschel Fault Mineralization |
RHD408(1) |
309.20 |
313.55 |
4.35 |
3.2 |
68.1 |
Herschel Fault |
Including(1) |
309.60 |
309.95 |
0.35 |
0.3 |
747 |
Herschel Fault |
Cygnet Fault Mineralization |
UDE279 |
259.70 |
265.65 |
5.95 |
5.6 |
6.1 |
Cygnet |
UDE283 |
343.25 |
343.55 |
0.3 |
0.2 |
11.4 |
Cygnet |
UDE284 |
350.70 |
352.60 |
1.9 |
1.4 |
2.6 |
Cygnet |
UDH3196 |
404.10 |
406.20 |
2.1 |
2.1 |
12.7 |
Cygnet |
UDH3204A |
375.95 |
378.30 |
2.35 |
2.0 |
5.6 |
Cygnet |
UDH3205 |
378.75 |
383.30 |
4.55 |
3.7 |
5.4 |
Cygnet |
UDH3206 |
296.80 |
306.50 |
9.7 |
8.0 |
5.4 |
Cygnet |
UDH3207A |
271.10 |
274.00 |
2.9 |
2.9 |
10.8 |
Cygnet |
UDH3208 |
410.50 |
410.80 |
0.3 |
0.2 |
1.9 |
Cygnet |
UDH3398 |
288.30 |
294.90 |
6.6 |
5.9 |
13.6 |
Cygnet |
UDH3399 |
274.15 |
274.45 |
0.3 |
0.3 |
0.1 |
Cygnet |
UDH3402 |
268.40 |
270.40 |
2.3 |
2.2 |
13.1 |
Cygnet |
UDH3404 |
308.70 |
310.20 |
1.5 |
1.2 |
5.7 |
Cygnet |
UDH3414 |
364.40 |
367.75 |
3.35 |
3.1 |
6.4 |
Cygnet |
UDH3415 |
371.40 |
372.10 |
0.7 |
0.7 |
0.1 |
Cygnet |
UDH3417A |
351.20 |
354.30 |
3.1 |
2.0 |
9.4 |
Cygnet |
UDH3441 |
378.90 |
381.60 |
2.7 |
2.6 |
5.6 |
Cygnet |
UDH3479 |
215.30 |
215.70 |
0.4 |
0.4 |
0.7 |
Cygnet |
UDH3480 |
222.20 |
222.70 |
0.5 |
0.2 |
2.0 |
Cygnet |
UDH3482 |
226.00 |
227.25 |
1.25 |
1.1 |
4.2 |
Cygnet |
UDH3484 |
260.20 |
265.80 |
5.6 |
5.1 |
5.0 |
Cygnet |
UDH3485 |
284.05 |
288.90 |
4.85 |
4.2 |
8.1 |
Cygnet |
UDH3486 |
243.00 |
243.40 |
0.4 |
0.4 |
0.6 |
Cygnet |
UDH3492 |
48.00 |
56.50 |
8.5 |
5.7 |
11.0 |
Cygnet |
Cygnet Hangingwall Splay
Mineralization |
UDH3482 |
208.25 |
210.45 |
2.2 |
1.9 |
36.6 |
Cygnet Hangingwall Splay |
Including |
208.25 |
208.60 |
0.35 |
0.3 |
168.0 |
Cygnet Hangingwall Splay |
Cygnet Footwall Splay Mineralization |
UDE281 |
336.50 |
337.20 |
0.7 |
0.6 |
2.4 |
Cygnet Footwall Splay |
UDH3206 |
343.55 |
347.80 |
4.25 |
4.1 |
4.2 |
Cygnet Footwall Splay |
UDH3207A |
283.80 |
285.20 |
1.4 |
1.4 |
6.9 |
Cygnet Footwall Splay |
UDH3162 |
329.35 |
330.90 |
1.55 |
1.3 |
3.6 |
Cygnet Footwall Splay |
UDH3400 |
280.40 |
280.90 |
0.5 |
0.5 |
0.0 |
Cygnet Footwall Splay |
UDH3401 |
273.80 |
274.10 |
0.3 |
0.3 |
12.1 |
Cygnet Footwall Splay |
UDH3485 |
316.10 |
319.40 |
3.3 |
2.1 |
3.3 |
Cygnet Footwall Splay |
Harrier Base Fault Mineralization |
UDE214 |
244.60 |
247.30 |
2.7 |
1.8 |
2.7 |
Harrier Base |
UDE222 |
262.30 |
264.10 |
1.8 |
1.7 |
0.5 |
Harrier Base |
UDE239 |
382.85 |
387.30 |
4.45 |
3.9 |
8.1 |
Harrier Base |
UDE268 |
408.50 |
409.80 |
1.3 |
0.8 |
6.0 |
Harrier Base |
UDE292 |
385.00 |
388.60 |
3.6 |
3.4 |
2.3 |
Harrier Base |
UDE295 |
387.25 |
390.00 |
2.75 |
2.5 |
2.6 |
Harrier Base |
UDE298 |
395.25 |
396.05 |
0.8 |
0.7 |
4.7 |
Harrier Base |
UDE300 |
260.30 |
264.20 |
3.9 |
3.1 |
6.7 |
Harrier Base |
UDE301 |
287.60 |
298.00 |
10.4 |
6.0 |
2.0 |
Harrier Base |
UDE302A |
310.65 |
311.75 |
1.1 |
0.6 |
0.0 |
Harrier Base |
UDE308 |
521.00 |
521.70 |
0.7 |
0.5 |
3.9 |
Harrier Base |
UDE310 |
458.60 |
459.20 |
0.6 |
0.6 |
7.6 |
Harrier Base |
UDE316 |
476.70 |
477.65 |
0.95 |
0.8 |
4.5 |
Harrier Base |
UDE320 |
440.40 |
443.65 |
3.25 |
1.4 |
4.0 |
Harrier Base |
UDE321 |
465.00 |
465.90 |
0.9 |
0.8 |
4.0 |
Harrier Base |
UDE325 |
489.30 |
491.00 |
1.7 |
1.6 |
3.8 |
Harrier Base |
UDE329 |
555.95 |
563.45 |
7.5 |
5.8 |
0.3 |
Harrier Base |
UDE339A |
409.70 |
411.85 |
2.15 |
2.0 |
2.6 |
Harrier Base |
UDH3000 |
214.90 |
216.00 |
1.1 |
1.0 |
3.1 |
Harrier Base |
UDH3001 |
202.60 |
208.00 |
5.4 |
5.4 |
4.0 |
Harrier Base |
UDH3002 |
207.45 |
207.80 |
0.35 |
0.3 |
2.0 |
Harrier Base |
UDH3003 |
217.90 |
218.35 |
0.45 |
0.4 |
11.7 |
Harrier Base |
UDH3004 |
210.80 |
214.00 |
3.2 |
3.2 |
6.2 |
Harrier Base |
UDH3005 |
219.00 |
219.60 |
0.6 |
0.6 |
7.1 |
Harrier Base |
UDH3006 |
226.75 |
228.75 |
2.0 |
1.9 |
8.4 |
Harrier Base |
UDH3007 |
215.30 |
216.40 |
1.1 |
0.8 |
5.4 |
Harrier Base |
UDH3029 |
230.45 |
232.60 |
2.15 |
2.1 |
11.6 |
Harrier Base |
UDH3042 |
233.25 |
233.80 |
0.55 |
0.5 |
2.9 |
Harrier Base |
UDH3043 |
245.90 |
247.10 |
1.2 |
1.1 |
3.8 |
Harrier Base |
UDH3045 |
230.50 |
236.40 |
5.9 |
5.5 |
20.9 |
Harrier Base |
Including |
232.20 |
232.50 |
0.3 |
0.3 |
295 |
Harrier Base |
UDH3046 |
248.45 |
249.50 |
1.05 |
1.0 |
3.2 |
Harrier Base |
UDH3048 |
234.25 |
234.80 |
0.55 |
0.5 |
3.5 |
Harrier Base |
UDH3050 |
244.00 |
244.95 |
0.95 |
0.9 |
6.2 |
Harrier Base |
UDH3052 |
238.85 |
240.60 |
1.75 |
1.7 |
5.0 |
Harrier Base |
UDH3053 |
243.55 |
244.00 |
0.45 |
0.4 |
2.5 |
Harrier Base |
UDH3474 |
245.70 |
246.10 |
0.4 |
0.4 |
3.5 |
Harrier Base |
UDH3474A |
250.70 |
255.00 |
4.3 |
3.7 |
22.8 |
Harrier Base |
UDH3488 |
222.50 |
223.40 |
0.9 |
0.9 |
0.6 |
Harrier Base |
UDH3489 |
222.90 |
228.35 |
5.45 |
4.1 |
4.4 |
Harrier Base |
UDH3490 |
253.25 |
254.20 |
0.95 |
0.7 |
4.5 |
Harrier Base |
UDH3491 |
246.45 |
246.80 |
0.35 |
0.3 |
3.9 |
Harrier Base |
UDH3494 |
241.25 |
249.10 |
7.85 |
7.6 |
3.8 |
Harrier Base |
UDH3495 |
256.60 |
260.80 |
4.2 |
4.2 |
5.6 |
Harrier Base |
UDH3496 |
260.70 |
266.35 |
5.65 |
5.7 |
4.1 |
Harrier Base |
UDH3497 |
289.50 |
293.30 |
3.8 |
3.8 |
24.5 |
Harrier Base |
UDH3498 |
253.10 |
256.85 |
3.75 |
3.7 |
12.0 |
Harrier Base |
UDH3499 |
272.85 |
279.70 |
6.85 |
6.8 |
5.2 |
Harrier Base |
UDH3500 |
268.95 |
269.61 |
0.66 |
0.6 |
6.4 |
Harrier Base |
UDH3510 |
237.50 |
246.90 |
9.4 |
9.3 |
8.3 |
Harrier Base |
UDH3512 |
254.08 |
254.23 |
0.15 |
0.15 |
18.5 |
Harrier Base |
Notes: (1) – Visible-gold
observed in drill intercept. Swan drill intercepts greater than
1,000 Gram-Meter (gold grade x estimated true width) are shown in
bold text; Non-Swan drill intercepts greater than 15 Gram-Meter are
shown in bold text.
To view the figures associated with this release, please visit
the following links:
https://www.globenewswire.com/NewsRoom/AttachmentNg/912e2ccb-42ad-4944-91d3-9020824f5a75
https://www.globenewswire.com/NewsRoom/AttachmentNg/15e16e4b-1b88-41f2-8fa4-bd68d312f2e3
https://www.globenewswire.com/NewsRoom/AttachmentNg/4e853b79-e916-4756-8612-8eb84988aa72
https://www.globenewswire.com/NewsRoom/AttachmentNg/f46d96d0-0c62-4a38-8aeb-8f41a2fb6f99
https://www.globenewswire.com/NewsRoom/AttachmentNg/8ab33af3-6c0b-4db6-835f-7ae7a968b7b7
https://www.globenewswire.com/NewsRoom/AttachmentNg/1d1aa967-1b47-4419-b543-bb495e41bb3f
https://www.globenewswire.com/NewsRoom/AttachmentNg/6f6d08da-7697-467e-a4d4-198b31ee1abd
https://www.globenewswire.com/NewsRoom/AttachmentNg/c0126dbe-998f-4ea1-888e-f23ac820fc03
https://www.globenewswire.com/NewsRoom/AttachmentNg/9a2cbbf9-7169-4673-9625-7851d65cfa06
https://www.globenewswire.com/NewsRoom/AttachmentNg/89ef17c2-e3e0-47b9-bcc2-0e17c592c87b
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