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Cycle 19 Preparations STUC 6 April 2011


4/6/2011



Cycle 19 Preparations


1



· · · ·

Cycle 19 Proposal Statistics
Cycle 19 Panel and TAC Preparations
Orbit Allocation and Distribution
Review Process of Regular, Treasury and Large Proposals
· XMM/HST Joint Program




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Cycle 19
Total Proposals GO SNAP Archival Research Regular Theory Total

(Cycle 18)
1007 (1051) 798 (872) 65 (51) Small 17 39 57

Proposal Statistics

Cycle 20 338 (622) Cycle 21 284 (541)

Cycle 19 18,676 (23096) 6,072 (4861) Medium 50 27 77

Legacy 10 0 10 144 (127)

ESA ESA GO ESA Snaps ESA AR

200 (197) 178 (189) 19 (8) 3 (0) ESA Orbits 462 (1276) 534 (325) 0 (0) 3,950 (4516) 1,708 (569) orbits targets

GO Large GO Treasury Pure Parallel

33 (41) 11 (12) 4 (5)

4,361 (4823) 1,582 (1761) 925 (915)

4 (11) 4 (3) 0 (0)

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Proposals by Cycle

1400 1298 1200 1000
# Submitted

1078 1025 863 1053 914 906 1046 949 747 727 733 821

1050 1007 960

800 600 400 200 0 1 2 3 4 5 6 7 8

556 427 396

502

9

10 11 12 13 14 15 16 16' 17 18 19 Cycle

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Orbits by Cycle

25000 21734 20000 17690
Requested Time

24667 19674 17257 16236 14005 10732 8169 6303 13543 14173 20771 17200

23096

18676 15000 14272 14668 15876

10000

8289 6473

5000

0 1 2 3 4 5 6 7 7N 8 9 10 11 12 13 14 15 16 16' 17 18 19 Cycle

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Taiwan

Proposals by Country (without USA)


Austria Switzerland Mexico Ireland Russia Czech Republic Belgium Korea

Japan Israel Sweden Denmark Chile Canada

USA is 761

Spain Australia Netherlands Italy France Germany United Kingdom

4/6/2011

70 60 50 40 30 20 10 0
# of Submissions

Cycle 19 Preparations


China

6



Science Categories by Proposal

ISM in External Extra-Solar Planets Galaxies Unresolved Stellar 4% Solar System 6% Populations and 4% Galaxy Structure 12% Star Formation 5% Resolved Stellar Populations 14% Cool Stars 5% ISM and Circumstellar Matter 7% Hot Stars 11% AGN/Quasars 11%

Quasar Absorption Lines And IGM 6% Cosmology 15%

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Science Categories by Orbits

Extra-Solar Planets 6% ISM in External Galaxies 4% Solar System 2% Unresolved Stellar Star Formation Populations and Galaxy 4% Structure 14% Resolved Stellar Populations 15%

AGN/Quasars 9%

Cool Stars 3% ISM and Circumstellar Matter 5% Hot Stars 7% Cosmology 23%

Quasar Absorption Lines And IGM 8%

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Instrument Details

Configuration Mode Prime % Coordinated Parallel % Total Instrument Prime + Instrument Coordinated Pure Prime Parallel Parallel Usage Usage Usage Snap Usage

!"#$#%" !"#$12" !"#$12" !"#$12" "D#$2EF "D#$GEF "D#$GEF 2H# 2H# G&", G&"7 G&"5 G&"5 #J&#$""L #J&#$""L #J&#$2EF #J&#$2EF #J&#$GEF #J&#$GEF 12"5$&9 12"5$&9 12"5$EF&# 12"5$EF&#

&'()*+) &'()*+) 9(':;2*<=>? #:>@=?AB@A: #:>@=?AB@A: &'()*+) #:>@=?AB@A: ID# J9!G# &'()*+) &'()*+) &'()*+) #:>@=?AB@A: &'()*+) #:>@=?AB@A: &'()*+) #:>@=?AB@A: &'()*+) #:>@=?AB@A: &'()*+) #:>@=?AB@A: &'()*+) #:>@=?AB@A:

C C C

C C C C C C

,-,. ,0-3. /-8. /-,. ,5-0. /-,. 7-7. ,-7. /-7. /-4. /-3. /-K. /-,. ,-/. 4-/. /-6. 5-8. /-/. 7-/. ,8-0. 5-,. 76-5. /-7. ,//.

/-/. 45-6. /-/. 5-6. /-/. /-/. /-/. /-/. /-/. /-,. /-3. /-6. /-/. /-/. /-/. /-/. /-/. /-/. /-/. 4-4. /-,. 53-4. /-/. ,//-/.

/-0. 78-,. /-3. /-0. ,/-6. /-,. ,-3. /-0. /-,. /-6. /-3. /-3. /-,. /-K. 5-8. /-5. 7-0. /-/. ,-4. ,4-3. 7-6. 7K-6. /-7. ,//-/.

7,-3.

5/-4.

,3-7. ,-6.

,7-,. ,-/.

,-0.

,-K.

,7-5.

0-7.

63-3.

64-4.

,//-/.

,//-/.

/-/. ,7-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. /-/. 68-/. ,3-/. 76-/. /-/. ,//-/.

/-/. ,8-0. ,-,. /-/. 8-3. /-/. /-/. /-/. ,-3. ,. /-/. /-/. /-/. /-0. 7-4. /-/. 6-/. /-/. /-/. 75-8. 7-/. 56-8. /-0. 00-0.

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Other Proposal Categories

· 8 Calibration proposals (3 AR & 5 GO)
· 29 Targets of Opportunity
· 16 Disruptive and 13 Non-Disruptive (< or >2 weeks)

Archival Research
Regular
Theory
Total
Small
17
39
57





Medium
50
27
77


Legacy
10
0
10


Observatory
Chandra
NOAO
Spitzer


Props
13
7
8


Requested Time
666.5
15.05
122.1


Units
Ksecs
Nights
Hours


HST Orbits
345
174
567


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HST Joint Program ­ Previous Cycles

Cycle
9
10
11
12
13
14
15
16
17
18

4/6/2011


HST
Orbits
90
51
43
77
60
25
59
62
99
84


Chandra
ksec
328
345
170
115
85
130
60
89
110
170


HST
Orbits


Spitzer
Hours


NOAO
Nights


18
74
1
24


19.1
31.8
203.1


2


5
12
6

11


Cycle 19 Preparations



C19 Panel Preparations

· Regular GO programs: 14 panels
· PSF 1/2: local and distant solar systems, exoplanets, star formation
· Stars 1/2/3: cool+hot stars, late stages, low-mass stars
· StPops 1/2: resolved stellar populations, ISM
· Galaxies 1/2/3: stellar content of galaxies, ISM in galaxies, dynamics, galaxy evolution
· AGN 1/2: AGN, QSO, IGM, QSO absorption lines
· COS 1/2: cosmology, lensing, GRB, galaxy clusters

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Break-down of proposals by panel

PANEL AGN1 AGN2 COS1 COS2 GAL1 GAL2 GAL3 PSF1 PSF2 STARS1 STARS2 STARS3 STPOPS1 STPOPS2 TAC TOTAL 62 71 64 67 65 58 57 65 67 66 68 70 88 80 59 1007 GO 33 54 47 50 49 46 47 55 54 59 56 63 72 65 48 798 AR 19 11 13 14 10 9 8 7 8 3 6 5 11 10 10 144 SNAP 10 6 4 3 6 3 2 3 5 4 6 2 5 5 1 65 ORBITS 825 1112 1036 1086 1043 927 1030 773 736 669 742 821 1184 1072 5620 18676 GOS>=40 5 7 6 4 2 6 6 1 1 2 3 2 2 2 0 49 ORBS>=40 292 387 332 215 94 314 1325 96 45 154 144 89 109 100 0 3696 TARGETS 1008 706 296 507 593 174 180 191 578 339 387 85 394 337 350 6125

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Cycle 19 Panel Preparations (cont.)


· TAC Chair: James Graham (Toronto)
· Website: http://www.stsci.edu/institute/org/spd/panel/ cycle19-panel.html?printable=1
· Panelists obtained proposals via download from website
· Preliminary grades due 5/11/2011


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Orbit Allocation and Distribution


· Total number of orbits available for allocation: 2600
· This is the same number as in C18
· Smaller than in C17 (3300) because of MCTPs and C18 proposal tail


4/16/2011


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Orbit Allocation and Distribution (cont.)


· Available for TAC (Large, Treasury): 500 orbits
· Available for panels (regular GO): 2100 orbits
· This results in factors of ~8 and 11 orbit oversubscriptions in the panels and the TAC, respectively
· Each panel will have a baseline allocation according to the submitted proposals and the orbits requested in the panel

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Review Process of Regular, Treasury
and Large Proposals

· Large: > 99 orbits
· Treasury: solves multiple scientific problems with a single, coherent dataset. Usually, but not always Large
· Large and Treasury proposals will be reviewed by the TAC, with input from the panels. Same process as in previous cycle.
· Regular (< 100 orbits) proposals will be reviewed by the panels

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Orbit Bins by Proposal

350 301 300

250 215
# of Proposals

200

150

128

100 63 50 19 0 12 5 5 0 2 31 3
150 200

1
200 250

1
250 300

1
> 300

1 - 10 11 - 20 21 - 30 31 - 40 41 - 50 51 - 60 61 - 70 71 - 80 81 - 90 91 - 99 100 150

Bins

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Review Process of Regular, Treasury
and Large Proposals (continued)

· All proposals should have a similar chance of acceptance, independent of proposal size
· In C19 we will again provide a proposal-size dependent subsidy to each panel.
· The subsidy will come out of the total allocation of 2100 orbits for the panels.
· The progression of the subsidy will be similar to the one used in earlier cycles.

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Cycle 16 Subsidy

60 Cy 16 Subs i dy Cy 16 Cos t t o Panel 50

40

30

20

10

0 1 7 13 19 25 31 37 43 49 55 61 67 73 79 85 91 97

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Cycle 16 Subsidy

Orbits 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 Cost to Panel 1 2 3 4 5 6 7 8 9 10 11 12 13 14 14 15 16 17 17 18 18 19 19 20 20 21 21 22 22 22 23 23 23 24 24 Orbits 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 Cost to Panel 24 25 25 25 26 26 26 27 27 27 28 28 28 29 29 29 29 30 30 30 30 31 31 31 31 32 32 33 33 34 34 35 35 36 36 Orbits 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 Cost to Panel 37 37 38 38 39 39 40 40 41 41 41 42 42 43 43 44 44 45 45 46 47 48 48 49 50 51 52 53 54

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XMM/HST Joint Program

· X-ray Multi-mirror Mission - Newton

· · · · · · · European Photon Imaging Camera (EPIC): 0.15-15 keV, 30 sq. armin FOV, 6 arcsec. Resolution
Reflection Grating Spectrometer (RGS): R=150-800, 0.33-2.5 keV
Optical/UV Monitor (OM): 17 sq. arcmin FOV, 170-650 nm
~30-35% of successful proposals have US PIs
Successful US PIs can apply for funding via the ADAO program
400 ksec/400 ksec time swap
CXC funding for the Chandra component


· Joint NASA/ESA mission


· XMM supports joint XMM/Chandra programs


· XMM User committee has enquired whether there is interest in instituting a joint XMM/HST program

· · 400 ksec XMM / TBD (60?) orbits
Note that HST/Spitzer joint program is currently under-subscribed

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