S. Campana Additional docs - Osservatorio Astronomico di Brera

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S. Campana
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Additional docs
All docs can be found at the EVENT web site
!http://www.brera.inaf.it/~campana/EVENT
/Welcome.html
S. Campana
Additional docs
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SCIENTIFIC SUPPORT LETTERS
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Centre de Physique des Particules de Marseille
163, Avenue de Luminy – Case 902 – 13288 Marseille Cedex 9
Tél. : (33) 04 91 82 72 00 – Fax : (33) 04 91 82 72 99
http://marwww.in2p3.fr
Marseille, 19 Nov 2012
Dear Sir,
I have been asked to write a letter of support for the EVENT project and its request for an
ERC advanced grant.
ANTARES is an international collaboration of many European laboratories that have
constructed a deep-sea neutrino telescope located in the Mediterranean Sea, 42km offshore
from the town of Toulon in the south of France. It comprises an array of 900 optical modules
attached to detector lines fixed on the seabed. An angular resolution better than 0.3 degrees on
the direction of the incident neutrino is achieved allowing precision neutrino astronomy to be
performed.
ANTARES has implemented an important multi-messenger program looking for neutrinos
correlated with other cosmic messengers (optical, gamma-rays, cosmic-rays). In particular, we
have the TAToO project, in which ‘special’ neutrino events produce triggers that are sent to a
number of fast robotic optical telescopes around the world. The optical images are then
studied searching for transient optical sources such as GRBs and Supernovae, which are
potential sources of neutrinos. Since 2009 we have generated triggers for the ROTSE,
TAROT, SKYMAPPER and ZADKO optical telescopes. The neutrino triggers are based on
doublets of two neutrinos within 3 degrees and 15 minutes or a single high-energy neutrino
(E>5 TeV). The neutrino alert is generated in less than 20 seconds and has an angular
precision on the neutrino direction less than 1 degree. Typically we generate about 1 alert per
month.
The addition of the EVENT network of robotic telescopes will be of great interest for our
physics program, especially considered that the ROTSE telescopes are soon to be
decommissioned. The timescale of EVENT matches well the planned operation of the
ANTARES (until at least 2016). After 2016 the next generation neutrino telescope, KM3NeT,
will come online and will also want to make use of the EVENT telescopes.
In summary then, the EVENT proposal matches a clear need for neutrino telescopes such as
ANTARES, IceCube and KM3NeT to search for transient optical sources correlated with
neutrinos. The ANTARES and KM3NeT Collaborations will certainly provide neutrino
triggers and provide the manpower to analyse any optical images associated to these triggers.
Yours sincerely,
Dr. Paschal Coyle (Director of research-CNRS, ANTARES Spokesperson)
S. Campana
Additional docs
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SITE SUPPORT LETTERS
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S. Campana
Additional docs
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INSTRUMENTS QUOTATIONS
I.N.A.F. - Astronomical Overvatory of Brera
E.Bianchi 46
23807 MERATE (LC)
ITALIEN
Offer 296/2012
Offer date:
Customer no.:
06.08.2012
905
Page 1 of 1
Contact:
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The offer will be converted into an acknowledgment on receipt of a 30% down payment. Payment follows: 60% on
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Pos. Article
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prime mirror f3, design like the AZ800
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We hope that our offer meets your expectations and remain
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ASA Astrosysteme GmbH
1.260.000,00
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Oggetto:AW: AW: ASA information after SPIE 2012
Data:Tue, 7 Aug 2012 07:25:12 +0000
Mittente:Dietmar Weinzinger <d.weinzinger@astrosysteme.at>
A:Marco Riva <marco.riva@brera.inaf.it>
Dear Mr. Riva,
We also could manage telescope with 1,2m, the price will be approx. 680.000 Euro for one.
We also can manage a telescope with 2m, the price will be approx. 3 Mio. Euro.
This prices depends very strong of the technical speciation’s and equipment.
As already mentioned, we can offer you an extensive study design.
Should you have any further questions, please do not hesitate to contact us.
Mit freundlichen Grüßen / Best regards
Dietmar Weinzinger
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Take a look inside ASA here!
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760 McMurray Road, Buellton CA 93427 Voice (805) 693-9600 Fax (805) 693-9668
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Pagina 1 di 4
Da: L.O.T. ORIEL ITALIA
A: Osservatorio Astronomico di Brera
Ufficio di Roma
Via F. Sapori, 27
00143 Roma
Tel.: 06 5004204
Fax: 06 5010389
E-mail: Baratti@Lot-Oriel.it
Internet: www.Lot-Oriel.it
Oggetto: Nostra Offerta n°
Via E. Bianchi, 46
23807, Merate (LC)
Tel.: +39 +39-039-5971018
C. Att.: Dr. Sergio Campana
68412/AB
Gentile Dr. Campana,
buongiorno.
RingraziandoVi per la cortese richiesta, inviamo alla Vostra attenzione nostra migliore offerta relativa a:
P/N
DESCRIZIONE
Andor CCD iDus model DU401A-BR-DD:
x Sensor: 1024x127 pixels
x BR-DD: Back Illuminated CCD, Deep Depletion with
fringe suppression.
x Pixels size: 26µm
x Multiple Readout Rate: 100, 50 and 33 KHz
x Digitization: 16-bit
DU401A-BR-DD
x Minimum temperature air cooled: -80ºC
x Minimum temperature with coolant chiller: -100ºC
(chiller not included)
x Max spectra per second:
81 (Full Vertical Bin)
88 (Crop Mode - 10 rows)
x USB Interface
Q.TA'
PREZZO
UNITARIO EURO
1
17.500,00
Garanziadiriservatezza
IltrattamentodeidatipersonalicheLariguardanovienesvoltonell’ambitodellabancadatidellaSocietàLOTOrielItaliaLaserOptikTechnologies.r.l.enelrispettodiquantostabilitodallalegge
675/96sullatuteladeidatipersonali.Iltrattamentodeidati,dicuiLegarantiamolamassimariservatezza,èeffettuatoalfinediaggiornarLasuiniziativeedoffertedelgruppo.ISuoidatinon
sarannocomunicatiodiffusiaterzieperessiLeipotràrichiedere,inqualsiasimomento,lamodificaolacancellazionescrivendoall’attenzionedelResponsabileDatidelGruppo
22 novembre 2012
Pagina 2 di 4
P/N
DESCRIZIONE
Q.TA'
PREZZO
UNITARIO EURO
DU401A-BV
Andor CCD model DU401A-BV:
x BV: Back Illuminated CCD, Vis optimized + antifringing
x USB Interface
1
14.300,00
DV401A-BV
Andor CCD model DV401A-BV:
x BV: Back Illuminated CCD, Vis optimized + antifringing
x USB Interface
1
12.800,00
Software
La camera Andor va acquista con almeno uno dei software Andor Technology
P/N
Andor-Solis
DESCRIZIONE
A 32-bit application compatible with 32 and 64-bit
Windows (XP, Vista and 7) offering rich functionality for
data acquisition and processing. AndorBasic provides
macro language control of data acquisition, processing,
display and export.
Q.TA'
PREZZO
UNITARIO EURO
1
1.450,00
22 novembre 2012
Pagina 3 di 4
P/N
DESCRIZIONE
Q.TA'
PREZZO
UNITARIO EURO
Andor-SDK
Andor SDK.
A software development kit that allows you to control the
Andor range of cameras from your own application.
Available as 32 and 64-bit libraries for Windows (XP, Vista
and 7) and Linux. Compatible with C/C++, C#, Delphi,
VB6, VB.NET, LabVIEW and Matlab.
1
490,00
TERMINI E CONDIZIONI
CONSEGNA:_____________ Circa 8-10 settimane dalla data di ricevimento dell’ordine (da
confermare al ricevimento dello stesso).
PAGAMENTO:___________
B. B.30gg D.F.
SPEDIZIONE E IMBALLO:__ Inclusi
VALIDITA’ OFFERTA:_____
30 gg
GARANZIA:_____________
12 Mesi
5 anni di garanzia sulle condizioni di vuoto del sensore.
NOTE:_________________
I prezzi si intendono IVA esclusa
Si accettano ordini a mezzo fax 06.5010389 o via mail info@lot-oriel.it.
A disposizione per qualsiasi ulteriore chiarimento, porgiamo i nostri migliori saluti.
LOT ORIEL ITALIA
Ing. Alessandro Baratti
Sales Manager
S. Campana
Additional docs
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COMPUTER QUOTATIONS
Ciao Giuseppe,
SERVER E STORAGE:
SERVER DOPPIO PER IL CLUSTER DI ALTA AFFIDABILITA' PER LA STAZIONE
REMOTA E MERATE
Key Features
Two hot-pluggable systems (nodes) in a 2U form factor. Each node supports the following:
1. Intel® Xeon® processor E5-2600
family; QPI up to 8GT/s
2. Up to 256GB DDR3 1600MHz ECC
Registered DIMM; 8x DIMM sockets
3. 3x PCI-E 3.0 (x8) slots (1x low-profile
and 2x full-height full-length)
4. Intel® i350 Dual port Gigabit Ethernet
5. 6x Hot-swap 3.5" SATA3
HDD Bays
6. 1280W Redundant Power Supplies
80 PLUS, Platinum Level (94%)
-
SupererServer 2U TWINS 1280W Redundant High-efficiency Digital Power Supplies w/
PMBus 1.2 80 PLUS, Platinum Level (94%), Two hot-pluggable systems (nodes) in a 2U
form factor QPI up to 8GT/s, ciascuno dei due sistemi configurato con due processori Intel
XEON E5-2620 2.00GHZ 15MB CACHE Socket R LGA-2011 Hexa core (6 Core), 16GB
RAM DDR3 1600 ECC REG CL11 DIMM DR X8 (up to 256MB), Controller integrato
SATA 2.0 & 3.0 with RAID 0, 1, 5, 10 – N.6 Hard disk 2TB 7200rpm SATA3 64MB cache,
Intel® i350 Dual Port Gigabit Ethernet, IPMI 2.0 with virtual media over LAN and KVMover-LAN support con porta Gigabit dedicate (3a porta RJ45) + Support for Intelligent
Platform Management Interface v.2.0 *, VGA Matrox G200eW integrata, Scientific Linux
preinstallato, garanzia 3 anni carry-in parti…Euro 6.500,00 + IVA
*gestione complete del sistema da remote, con accesso allo stato del sistema in BIOS e possibilità di
accendere e spegnere il sistema da remoto.
Con questo sistema potresti pensare di gestire l’alta affidabilità nella stazione remota e a Merate, dove
comunque secondo me è necessaria un’affidabilità ed una continuità di servizio.
Nella versione per Merate possiamo utilizzare le porte Gigabit esistenti, aggiungerne altre o installare
delle porte a 10GbE per avere un canale privilegiato verso lo storage che sarà presente con una
tecnologia iSCSI e quindi collegabile direttamente ai due server o via switch Ethernbet (o 10GbE).
Per la parte di dischi, si possono fare 3 RAID1 per sistema, per una capacità di 2TB per RAID1 e 6TB
totali (considerando che il secondo server in cluster è una copia
STORAGE AD ALTA AFFIDABILITA’ ED ALTA CAPACITA’ CON 288GB LORDI PER
MERATE
Codice
QF.0P400Q.
D4240
J300Q-D424
HDD3TSS2QS
Descrizione
Prezzi single
Sistema raid iSCSI ,rack-mount 4U, 24 bay , 6G SAS/SATA drive , Controller 2
x P400H-24 , CPU Intel C3500 , cache 2.0GB/Ctrl, RAID level:
0,1,0+1,3,5,6,10,30,50, 60 and JBOD , Read 1200 MB/s - Write 1000MB/s , canali
host 6x 1GbE iSCSI/Controller , PSU 3 x 500W. Built-in Snapshot , On-line
Migration , RAID Roaming , Windows Clustering , Windows VSS , Windwos MPIO ,
SSL , Trunking/LACP , MC/S , Full iSCSI offload, VMWare ESX 5.1 , Citrix XEN
!
Server, Microsoft Hyper V. Battery Backup Module Built-in 2pcs , Controller ,
Power/Fan , Monitor ,Swappable. Include VD Clone , Qreplica ,(Q-Thin) ,
VAAI support. Espansione fino a 192
HDD.
Garanzia 3 anni - ( Battery backup garanzia 1 anno )
JBOD 4U 24 bay , formato HD 3,5" , 6GB SAS/SATA channel , tre alimentatori 500 W
, due moduli di raffreddamento, dual controller con 2 porte x 6GB SAS per
!
controller. Applicabile a P500Q series ,P300Q series , F300Q series ,S300Q
series. Web UI , UPS&Console Serial , LCM Display.
Hard Disk 3TB 7200rpm SAS2 6Gb in caddy QSAN
!
QT
Y
TOT
7.500,00
1
!
7.500,00
3.500,00
3
!
10.500,00
310,00
96
!
29.760,00
estensione garanzia 3 anni on-site NBD RAID System P400 Dual Controller
!
2.250,00
1
!
2.250,00
estensione garanzia 3 anni on-site NBD JBOD J300 Dual Controller
!
750,00
3
!
2.250,00
Installazione on-site e configurazione
!
500,00
1
!
500,00
TOTALE OFFERTA STORAGE IVA ESCLUSA
!
Questo Storage RAID iSCSI ha 6 canali iSCSI OFF-LOAD per controller per un totale di 12 canali che
si usano in load balancing e per la ridondanza. Se non hai uno Switch con una buona banda interna e
porte disponibili, bisogna aggiungerlo al progetto, un 48 porte Giagbit + 4 SFP diciamo altri 1500/2000
euro (parliamo di qualità e performance non di un prodotto economico).
Totale offerta N.2 Server Dual System Euro 13.000,00 + Storage 52.760,00= Euro 65.760,00 +
IVA
Rimango a disposizione per valutare insieme la proposta e per effettuare eventuali modifiche e
ciao
Enzo Romeo Marro
Active Solution & Systems
BeActive!
52.760,00
S. Campana
Additional docs
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INFRASTUCTURAL QUOTATIONS
I.N.A.F. - Astronomical Overvatory of Brera
E.Bianchi 46
23807 MERATE (LC)
ITALIEN
Offer 297/2012
Offer date:
Customer no.:
06.08.2012
905
Page 1 of 1
Contact:
Phone:
Email:
Dietmar Weinzinger
0043 (0) 7942 77811-50
d.weinzinger@astrosysteme.at
The offer will be converted into an acknowledgment on receipt of a 30% down payment. Payment follows: 60% on
completion, 10% on receipt of goods. Delivery time is 12 months(without shipping time) from time of acknowledgment.
Pos. Article
1 SD5000 / 5.5M dome with complete electronics and mechanics
devices, wireless ScopeDome v. 2.0 USB Card system, Plug&Play
wiring, weather proof box for electronics, encoder module, home
sensor, RAL9007 colour o
2 SONB / dome assembly
Quantity
3 Pcs
Price/Unit
28.000,00
Net (EUR)
1 Pcs
0,00
0,00
1 Pcs
0,00
0,00
84.000,00
to be determined
3 TRANS / Packaging, shipping & insurance
to be determined
Total amount net: EUR
20% VAT: EUR
Total amount gross: EUR
Terms of payment:
Terms of delivery:
Payment due after receipt of the invoice without deduction
Delivery ex factory
We hope that our offer meets your expectations and remain
with best regards
84.000,00
16.800,00
100.800,00
S. Campana
Additional docs
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INAF DELEGATES BRERA OBSERVATORY
S. Campana
Additional docs
!
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iDus 401 Series
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
Spectroscopy
Features and Benefits
Workhorse laboratory and OEM CCD platform
t 1FBL2&VQUP
Visible-optimized ‘BV’ & infrared-optimized
‘BR-DD’ model
The USB2.0-based iDus series is a compact, yet feature-rich platform suitable for demanding
spectroscopy applications such as low-light UV/NIR Photoluminence or Raman spectroscopy,
as well as day-to-day routine laboratory operation and integration into industry-grade
systems.
The iDus 401 boasts market-leading deep thermo-electric cooling to -100°C, complemented
by Andor’s UltravacTM technology with its un-matched reliability track record in the scientific
and industrial community. The iDus low-noise electronics allows seamless access to the best
signal-to-noise ratio performance for the widest range of photon detection regimes.
Anti-fringing comes as standard on back-thinned & back-illuminated sensors for this
1024 x 127, 26 µm pixels array optimized for high dynamic range, high resolution and rapid
data acquisition from Far UV to NIR.
t Fringe suppression technology as standard
Fringing eliminated (Deep-Depletion) or greatly
minimized (Back-Thinned)
t 5&DPPMJOHEPXOUPoC
Critical for elimination of dark current detection
limit - no inconvenience associated with LN2
t UltravacTM
Critical for sustained vacuum integrity and
to maintain unequalled cooling and QE
performance, year after year
t Single UV-grade silica window
Best UV-NIR throughput performance, specific
AR coating and wedge options available
t USB 2.0 connection
Universal plug-and-play capability, ideal for
laptop operation
Seamless operation alongside USB-based
Shamrock spectrograph family
t 26 x 26 µm pixels
Optimized pixel format for high dynamic range
and resolution
Specifications Summary
Active pixels
1024 x 127
Pixel size (W x H)
26 x 26 μm
Image area
26.6 x 3.3 mm
Register well depth (typical)
1,000,000 e-
t Software-selectable pre-amplifier gain
Choice of best SNR performance of dynamic
range at the touch of a button
Maximum cooling
-100ºC
t Compact and rugged platform
Ideal for OEM integration & laboratory setups
Maximum spectra per sec
88
Read noise
As low as 3 e-
Dark current
As low as 0.0005 e-/pixel/sec
t Solis software for Spectroscopy
Comprehensive, user-friendly interface for
simultaneous detector & spectrograph control
t Software Development Kit (SDK)
Ease of control integration into complex
setups: Matlab, Labview, Visual Basic or C/C++
andor.com
Page 1 of 6
discover new ways of seeing™
iDus 401 Series
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
Key Specifications t
Model number
Sensor options
DV401A
DU401A
tBV: Back Illuminated CCD,
Vis optimized + anti-fringing
tFI: Front Illuminated CCD
DU401A BR-DD
tBV: Back Illuminated CCD,
Vis optimized + anti-fringing
tFI: Front Illuminated CCD
Active pixels t
1024 x 127
Pixel size
26 x 26 μm
Image area
tBR-DD: Back Illuminated CCD,
Deep Depletion with fringe
suppression.
Optimum sensor for Near IR
applications
26.6 x 3.3 mm with 100% fill factor
Cooler type
DV
DU
DU
-55ºC
-65ºC
-70ºC
-80ºC
-95ºC
-100ºC
-80ºC
-95ºC
-100ºC
t
Minimum temperatures
Air cooled
Coolant recirculator
Coolant chiller, coolant @ 10ºC, 0.75l/min
88 (10 row crop mode), 81 (Full Vertical Bin)
Max spectra per second t
System window type
Single quartz window, uncoated.
Various AR coatings & MgF2 options
available
Single quartz window, uncoated.
Various AR coatings & MgF2 options
available
Blemish specifications
Single quartz window; 1° wedge,
AR coated on both sides, optimized
at 900 nm
Grade 1 as per sensor manufacturer definition
Advanced Specifications t
Dark current, e-/pixel/sec @ max cooling
FI
BV / BR-DD
0.002
0.004
0.0005
0.001
Register well depth
0.006
1,000,000 e-
Read noise (e-) t
33 kHz
50 kHz
100 kHz
33 kHz
50 kHz
100 kHz
FI: Typ (Max)
BV: Typ (Max)
BR-DD: Typ (Max)
3 (5)
7 (8)
4 (6)
10 (12)
8 (12)
12 (15)
3 (5)
6 (8)
4 (6)
10 (12)
9 (12)
12 (15)
Sensitivity (e-/count)
High Dynamic Range mode
High Sensitivity mode
50 kHz
100 kHz
5 (8)
6 (12)
12 (15)
33 kHz
50 kHz
100 kHz
33 kHz
50 kHz
100 kHz
33 kHz
50 kHz
100 kHz
2
-
3.5
2.5
14
9
2.5
-
3.5
2.5
16
11
2.5
-
3.5
2.5
20
12
Linearity t
Better than 99%
Digitization
16 bit
Vertical clock speed
33 kHz
8, 16, 32, 64 μs (software selectable)
t
Have you found what you are looking for?
Need a larger sensor? The iDus 420 series is similar to the 401 series with 26.6 x 6.6 mm format with 1024 x 255 pixels.
Need to work further into the NIR? The iDus InGaAs series, with up to 1024 pixel linear array with transmission to 2.2 µm.
Need a faster or more sensitive CCD? The Newton series offers over 1,600 spectra per second and EM technology.
Need more UV sensitivity? The iDus 420 series is similar to the 401 series with a range of UV optimized sensors.
Need a customized version? Please contact us to discuss our Customer Special Request options.
The iDus series combines seamlessly with Andor’s research grade Shamrock Czerny-Turner spectrographs.
andor.com
Page 2 of 6
iDus 401 Series
Dark Current
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
Quantum Efficiency Curves
t
t
25°C
Typical Setup
Quantum Efficiency Curves
t
-100ºC
iDus CCD
Power Supply
Alternative Detector
(e.g. iDus InGaAs)
Spectrograph
USB 2.0
PC
Software CD
andor.com
Page 3 of 6
iDus 401 Series
Creating The Optimum
Product for You
How to customize the iDus 401A :
Step 1.
Simply select from the 2 cooler types
that best suit your needs from the
selection opposite.
Step 2.
The iDus 401A comes with 3 options
for sensor types. Please select the
sensor which best suits your needs.
Step 3.
Please indicate if you wish to select
an alternative window and which
software you require.
Step 4.
For compatibility, please indicate
which accessories are required.
DV
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
401A-
BV
example shown
Step 1.
Step 2.
Choose cooler type
Choose sensor type
DV: Standard cooling, to -75ºC
(not a valid option with the BR-DD model)
BR-DD: Back Illuminated, Deep Depletion CCD
with fringe suppression
BV: Back Illuminated CCD, Vis optimized
FI: Front Illuminated CCD
DU: Deep cooling, to -100ºC
Step 3.
5IF'*#7NPEFMTBSFTVQQMJFEXJUIBOVODPBUFE2VBSU[XJOEPXBTTUBOEBSE#3%%
models are provided with an NIR optimized AR coating. The following alternative window
choices are available and must be ordered at time of build (if selected):
OPTION-C1-AR1 AR coated quartz window (optimized broadband visible 400-900nm).
50% transmission at 180 nm
OPTION-C1-MGF2 Magnesium Fluoride window for transmission in the VUV.
50% transmission at 120 nm
The iDus CCD also requires at least one of the following software options:
Solis for Spectroscopy A 32-bit application compatible with 32 and 64-bit Windows (XP, Vista
and 7) offering rich functionality for data acquisition and processing. AndorBasic provides
macro language control of data acquisition, processing, display and export. Control of Andor
Shamrock spectrographs and a very wide range of 3rd party spectrographs is also available, see
list below.
Andor SDK A software development kit that allows you to control the Andor range of cameras
from your own application. Available as 32 and 64-bit libraries for Windows (XP, Vista and 7)
and Linux. Compatible with C/C++, C#, Delphi, VB6, VB.NET, LabVIEW and Matlab.
Step 4.
The following accessories are available:
iDus CCD mounted on a
Shamrock 500 mm triple grating
imaging spectrograph, ideal for high
resolution spectroscopy.
983&$3 Coolant re-circulator for enhanced cooling performance
ACC-XW-CHIL-160 Oasis 160 Ultra Compact Chiller Unit (tubing to be ordered separately)
ACC-6MM-TUBING-2xxxxM 6 mm tubing option for ACC-XW-CHIL-160
LM-C C-mount lens adaptor
LM-NIKON-F C-mount lens adaptor
LMS-NIKON-F-NS25B Nikon F-mount lens adaptor with shutter
ACC-SD-VDM1000 Shutter Driver for NS25B Bistable Shutter (not needed for Shamrock
spectrographs)
ACC-SHT-NS25B Bistable Shutter, Standalone (not needed for Shamrock spectrographs)
Spectrograph Compatibility
The iDus series is fully compatible with Andor’s Shamrock spectrograph (163 - 750 nm focal
lengths) family. Spectrograph mounting flanges and software control are available for a wide
variety of 3rd party spectrographs including McPherson (including 1 m and greater focal length
option), JY/Horiba (excluding USB models), PI/Acton, Chromex/Bruker, Oriel/Newport, Photon
Design, Dongwoo, Bentham, Solar TII and others.
andor.com
Page 4 of 6
iDus 401 Series
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
Product Drawings
Dimensions in mm [inches]
Third-angle projection

=
position of pixel 1,1
Weight: 2 kg [4 lb 8 oz]
NOTE: There are 2x holes:
1x on top and 1x on the
bottom of the camera head
Connecting to the iDus
Camera Control
Connector type: USB 2.0
TTL / Logic
Connector type: SMB, provided with SMB - BNC cable
1 = Fire (Output), 2 = External Trigger (Input), 3 = Shutter (Output)
Mounting hole locations
I2C connector
Compatible with Fischer SC102A054-130
1 = Shutter (TTL), 2 = I2C Clock, 3 = I2C Data, 4 = +5 Vdc, 5 = Ground
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Minimum cable clearance required at rear of camera
90 mm
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Rear connector panel
Applications Guide
DV 401 FI
DV 401 BV
DU 401 FI
DU 401 BV
DU 401 BR-DD
Absorption/Transmittance/Reflection
Atomic Emission Spectroscopy
Fluorescence & Luminescence
NIR Spectroscopy
Raman Spectroscopy (244 – 488 nm)
Raman Spectroscopy (514, 532, 633 nm)
Raman Spectroscopy (785, 830 nm)
= Suitable
= Optimum
andor.com
Page 5 of 6
iDus 401 Series
26.6 x 3.3 mm / 1024 x 127 pixel
Spectroscopy CCD
Order Today
Need more information? At Andor we are committed to finding
the correct solution for you. With a dedicated team of technical
advisors, we are able to offer you one-to-one guidance and
technical support on all Andor products. For a full listing of our
andor.com/contact
local sales offices, please see:
Our regional headquarters are:
Items shipped with your camera:
&VSPQF
Belfast, Northern Ireland
Phone +44 (28) 9023 7126
Fax +44 (28) 9031 0792
Japan
Tokyo
Phone +81 (3) 3518 6488
Fax +81 (3) 3518 6489
North America
Connecticut, USA
Phone +1 (860) 290 9211
Fax +1 (860) 290 9566
China
Beijing
Phone +86 (10) 5129 4977
Fax +86 (10) 6445 5401
Footnotes: Specifications are subject to change without notice
1x 2m BNC - SMB conection cable
1x 3m USB 2.0 cable Type A Æ Type B
1x Set of Allen keys (7/64” & 3/32”)
1x Power supply with mains cable
1x Quick launch guide
1x CD containing Andor user guides
1x Individual system performance booklet
1x CD containing either Solis software or SDK
(if ordered)
1.
Minimum Computer Requirements:
Operating & Storage Conditions
t()[TJOHMFDPSFPS()[NVMUJDPSFQSPDFTTPS
Operating Temperature 0°C to 30°C ambient
t(#3".
Relative Humidity < 70% (non-condensing)
t.#GSFFIBSEEJTDUPJOTUBMMTPGUXBSFBUMFBTU
Storage Temperature -25°C to 50°C
Assembled in a state-of-the-art facility, Andor’s UltraVac™ vacuum process combines a
permanent hermetic vacuum seal (no o-rings), with a stringent protocol and proprietary
materials to minimize outgassing. Outgassing is the release of trapped gases that would
otherwise degrade cooling performance and potentially cause sensor failure.
2. Figures are typical unless otherwise stated.
3
Edge pixels may exhibit a partial response.
4. Minimum temperatures listed are typical values with ambient temperature of 20°C.
5. Based on a Horizontal Pixel Readout of 100 kHz and a vertical pixel shift of 8 μs.
6. System Readout Noise is for the entire system. It is a combination of CCD readout noise
and A/D noise. Measurement is for Single Pixel readout with the CCD at a temperature of
-50°C (BR-DD models tested at -80°C) and minimum exposure time under dark conditions.
Noise is measured at the highest available pre-amplifier gain for each speed.
7. Linearity is measured from a plot of counts vs exposure time under constant photon flux up
to the saturation point of the system.
8. Vertical speeds are software selectable. All sensors are designed to give optimum
ChargeTransfer Efficiency (CTE) at 16 μs vertical pixel shift, some decrease in CTE may be
observed at faster shift speeds.
9. The graph shows typical dark current level as a function of temperature. The dark current
measurement is averaged over the CCD area excluding any regions of blemishes.
10. Quantum efficiency of the sensor as measured by the sensor manufacturer.
1 GB recommended for data spooling)
t64#)JHI4QFFE)PTU$POUSPMMFSDBQBCMFPG
sustained rate of 40 MB/s
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PS-JOVY
Power Requirements
110 - 240 Vac, 50 - 60 Hz
Windows is a registered trademark of Microsoft Corporation.
Labview is a registered trademark of National Instruments.
Matlab is a registered trademark of The MathWorks Inc.
SiDus401SS 0912 R1
andor.com
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