2019/7/27 50

&+042#"$@5;=87:<6) ,* , '())(, ! ( ,-%
" SEICA[Second-generation
Exoplanet Imager with Coronagraphic Ao].370m+9<>++12m

 3.8m
1/3/&+)SEICA: 1
• SEICA– " .'.
– 8696 1 .!1)– # )- ()• Woofer AO– 7=4>#: (' ()– )-?-059:<>5;=• Tweeter AO– 7=4>#: SHWFS,7=40DM1$2 3/– 7=4>#: PDI,7=4 ()– &%: FPGA+ (*)1

SEICA (Second-generation Exoplanet Imager with Coronagraphic Adaptive Optics)

Note. — Confidence limits at which two pairs of planets’ (scaled) photometry diffe- 2 for scaled photometry, Ndata -1 for non-scaled photometry – and the χ2 value. F
different rows indicate the nominal case, using photometry listed in Table 4, the Cu
The two entries (enclosed by parentheses) list the correlation from scaling the planespectra) (right entry). A value closer to one means that the photometry significantly

enclose the scaling factor applied to the second planet in each listed pair that minimu *):0+'

TABLE 6
Atmospheric Model

1. 0’’.2.6;(2AU@10pc)E8=HH/N`bOWcVgSaf
2. 41(for TMT)G9DL:3?(u FPGA controller for ExAO
ExAO
u +,7%#@UfR
Qe[Pb\ u [cfP$71’(60’’)^TZu T]XOd[cfP
HR8799 (Currie+2014)
Qe[Pb\ u -<1c 10M
1’’.1b 7M
u A  1’’.7u
>FKEIH
e 9M+0’’.4
AQfZbTZ3 /....
"
10-5u &:3.8m;>J9d 10M0’’.7– ;>JHMOUTCFigurePanel

PlanetTef f (K)log(g)

Cloud8

top-leftmiddle-leftbottom-left
top-right
middle-rightbottom-right
top-leftbottom-left
top-right
bottom-right

HR 8799 b””
HR 8799 d””
HR 8799 b
HR 8799 c
HR 8799 d
HR 8799 e

900
850
850
1000
975
1000
900
1000
1000
1000

4.0
4.0
4.3
4.0
4.0
4.0
4.0
4.0
4.0
4.0

A
AAAA
A
0.85×A60
0.7×A60
0.9×A60,
0.75×A60

9Note. — References: 1) Burrows et al. (2006), 2) Currie et al. (2011(2012), 5) this work.

JJJJ_fY[fTB2B5%....

Fig. 1.— Keck/NIRC2 L′ images of HR 8799 from 2012 data (left)2
are all easily identifiable.

FY.2021 F.L.*!

3.8m

: u: 3.8m (6+12 ) F/6u$!'!2 8– ()#)": ()7(+– $!'! : 1(SEICA)

+& %)
()#)"()6& %)63

41813.8m+,: &#!
A>B>(.)u #!GSEICAH
A>B>(()
u 0*#!
u ( #!
u " =CD#!'!(2F)
u 3<70 GGAOESH (1F)
u %/#!GKOOLS-IFUHu )(u %0

u KOOLS-IFU6 /-&2201929:>?E@FFu /;42$51&/#!

4

SEICA: %/LHKV[X

Title: C-RED 2 USER MANUAL
Document: C-RED 2 User Manual_20190109
Issue: 005
Classification: PUBLICu#]2021>FLB#;Page : 1
Date : 09/01/201– ’19. ExAO&Woofer?=(9Tweeter*)9C-RED 2User Manual
IYPGWQ9$(90FUW.39PDI
+– ’20. Tweeter(9PDI,-89 -89
TLORYML:@ A<– ’21. -89451C-RED 2 User Manual_20190109u%]– a)H31 "A(6)2#1800
uFUW: 500
u&: 500
u2&: 400
u&: 400

– b)H31 TMTuFPGA7!: 240uIYPGWQ: 260'/JCEZL0FUWFIRST LIGHT
C−RED2 (InGaAs)
640x512 pix
15um pitch600FPS
RON < 30e \SXND] -40℃

First Light Imaging SAS | Europarc Sainte Victoire – Bât. 6 | Route de Valbrillant | Le Canet |13590 MEYREUIL | FRANCE | +33
First Light Imaging SAS au Capital de 85 000 euros | 533 716 817 RCS Aix-en-Provence | TVA : FR78 533 716 815

SEICA: B4u>9D935CB1uTMTCB+#: FPGA, IQLHOM, !7KRJ→SEIT: Second Earth Imager for TMTHPSNC%
TMTB0 ,*(&2,*)– PSI-blue: Planetary System Imager:: SEITHPSN; "– MICHI: Mid-Infrared Camera, High-disperser, & IFU– MODHIS: Multi-fiber High-resolution NIR spectometeru0 )2'B2':EWhite
Paper (WP) B-/– 7:WP
6BLOI-/→PSI-blue@<?
– 810: LOIGA8=F.$B( ()– 12: WPB6

SEICA: 1
uSEICA– " .'.
– 8696 1 .!1)– # )- ()uWoofer AO– 7=4>#: (' ()– )-?-059:<>5;=uTweeter AO– 7=4>#: SHWFS,7=40DM1$2 3/– 7=4>#: PDI,7=4 ()– &%: FPGA+ (*)7

SEICA:,))&

u6494 +$(2.0x1.6x1.6)– $1 "/0+→#'!
– 5:<-.

u

SEICA%"37<(1.4x1.4x0.5)

←

$

– 

 "37<


→

←

"

 // %%

(2l/)=&WHB-1414TS)(*$PC/2;8→

6494

8

SEICA: 1uSEICA
– " .'.
– 8696 1 .!1)– # )- ()uWoofer AO– 7=4>#: (' ()– )-?-059:<>5;=

uTweeter AO– 7=4>#: SHWFS,7=40DM1$2 3/– 7=4>#: PDI,7=4 ()– &%: FPGA+ (*)9