Pattern Point Spacing recomputed
----- Submission 1 (Tue May 16 13:34:01 GMT 2006) -----
Phase II Proposal 10902 (SSC_p2) successfully submitted.
----- Submission 2 (Wed May 17 09:49:27 GMT 2006) -----
Phase II Proposal 10902 (SSC_p2) successfully submitted.
----- Submission 3 (Wed May 17 16:36:09 GMT 2006) -----
Phase II Proposal 10902 (SSC_p2) successfully submitted.
----- Attempting Submission 4 (Fri Apr 20 15:46:00 GMT 2007) -----
Phase II Proposal 10902 (SSC_p2_ACS) successfully submitted.
----- Attempting Submission 5 (Mon Apr 23 10:47:47 GMT 2007) -----
Phase II Proposal 10902 (SSC_p2_ACS) successfully submitted.
----- Attempting Submission 6 (Fri Apr 27 11:51:27 GMT 2007) -----
Assigned ID: 235
----- Submission 1 (Fri Jan 27 15:27:00 GMT 2006) -----
The Nearest Luminous Blue Compact Galaxies: A Window on Galaxy Formation
As we move to intermediate and high redshifts, Luminous Blue Compact Galaxies (LBCGs) become increasingly common. The nearest LBCGs, with their violent starbursts and rich populations of super star clusters (SSCs) and globular clusters (GCs), thus provide ideal laboratories for studying galaxy evolution. Many LBCGs appear to be involved in mergers between dwarf galaxies, triggering their starbursts. The starburst regions in LBCGs consist of numerous young star clusters, whose populations are both easily measurable with HST and easily modelled. Studying cluster populations provides a powerful probe of the starburst and merger history which is possible neither for closer objects (of which there are too few) or for those at high redshift (which are too far away). We have previously studied the closest LBCG with WFPC2 and found hundreds of bright compact SSCs and GCs. In particular, we found a population of intermediate-age (~2 Gyr) GCs, indicating a past event of massive cluster formation. We now propose a multi-wavelength study of the three other LBCGs with the highest known number of SSCs. The extinction is small in these galaxies and age estimates robust. The age distribution of GCs and SSCs will be used to study the past evolution of the galaxies. For each LBCG, we will map its cluster formation history, unveiling its merger and starburst history, and thereby shed light on some of the processes involved in galaxy evolution at high redshift.
VISIT 1 -- 2 ORBITS
------------------
Target: Haro11
Orbit 1 : NIC3 : F160W :
1 single exposure using STEP32 and manual POS-TARG offsets
3 exposures using STEP64 and NIC-SPIRAL-DITH and manual POS-TARG offsets
Orbit 2 : NIC3 : F160W :
1 single exposure using STEP32 and manual POS-TARG offsets
3 exposures using STEP64 and NIC-SPIRAL-DITH and manual POS-TARG offsets
VISIT 2 -- 4 ORBITS
------------------
Target: ESO 350-13
Orbit 1 : NIC3 : F160W :
1 single exposure using STEP32
3 exposures using STEP64 and NIC-SPIRAL-DITH
Orbit 2 : NIC3 : F160W :
1 single exposure using STEP32
3 exposures using STEP64 and NIC-SPIRAL-DITH and manual POS-TARG offsets
Orbit 3 : ACS/SBC : F140LP : 4 exposures using ACS-SBC-DITHER-BOX and manual POS-TARG offsets
Orbit 4 : WFPC2 :
F336W : 2 exposures using manual POS-TARG offsets
F439W : 2 exposures using manual POS-TARG offsets
VISIT 3 -- 4 ORBITS
------------------
Target: MKR930
Orbit 1 : ACS/SBC : F140LP : 4 exposures using ACS-SBC-DITHER-BOX and manual POS-TARG offsets
Orbit 2 : WFPC2 :
F336W : 2 exposures using manual POS-TARG offsets
F439W : 2 exposures using manual POS-TARG offsets
Orbit 3 : NIC3 : F160W :
1 single exposure using STEP32
3 exposures using STEP64 and NIC-SPIRAL-DITH
Orbit 4 : NIC3 : F160W :
1 single exposure using STEP32
3 exposures using STEP64 and NIC-SPIRAL-DITH and manual POS-TARG offsets
VISIT 4 -- 4 ORBITS
------------------
Target: Haro11
Orbit 1 : WFPC2 : F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 2 : WFPC2 :
F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
F814W : 1 single exposure using manual POS-TARG offsets
Orbit 3 : WFPC2 : F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 4 : WFPC2 :
F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
1 single exposure using manual POS-TARG offsets
VISIT 5 -- 4 ORBITS
------------------
Target: ESO385-13
Orbit 1 : WFPC2 : F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 2 : WFPC2 :
F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
F814W : 1 single exposure using manual POS-TARG offsets
Orbit 3 : WFPC2 : F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 4 : WFPC2 :
F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
F450W : 2 exposures using manual POS-TARG offsets
VISIT 6 -- 4 ORBITS
------------------
Target: MKR930
Orbit 1 : WFPC2 : F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 2 : WFPC2 :
F606W : 1 splitted exposure in two subexp and manual POS-TARG offsets
F814W : 1 single exposure using manual POS-TARG offsets
Orbit 3 : WFPC2 : F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
Orbit 4 : WFPC2 :
F814W : 1 splitted exposure in two subexp and manual POS-TARG offsets
F450W : 2 exposures using manual POS-TARG offsets
UNRESOLVED STELLAR POPULATIONS
12
false
0.0
false
false
false
false
false
false
SUPPORTED
GALAXY
STARBURST
S0DN000005
J2000
00 36 52.0000
-33 33 19.00
J2000
GALAXY
STARBURST
SASD000600
J2000
19 45 0.0000
-54 15 4.00
J2000
GALAXY
STARBURST
N0CK000215
J2000
23 31 58.0000
+28 56 50.00
J2000
ACS/WFC
Imaging
No
No
F555W
ACS/WFC
Imaging
No
No
F814W
ACS/HRC
Imaging
No
No
F220W
ACS/HRC
Imaging
No
No
F330W
ACS/HRC
Imaging
No
No
F550M
ACS/WFC
Imaging
No
No
F555W
ACS/WFC
Imaging
No
No
F814W
ACS/HRC
Imaging
No
No
F220W
ACS/HRC
Imaging
No
No
F330W
ACS/HRC
Imaging
No
No
F550M
ACS/WFC
Imaging
No
No
F555W
ACS/WFC
Imaging
No
No
F814W
NIC3
Imaging
No
No
F160W
NIC3
Imaging
No
No
F160W
NIC3
Imaging
No
No
F160W
POS-TARG
DITHER
DITHER
2.163877
NIC-XSTRIP-DITH
false
false
3
0
POS-TARG
NIC-SPIRAL-DITH
0
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false
POS-TARG
DITHER
DITHER
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NIC-XSTRIP-DITH
false
false
3
0
POS-TARG
NIC-SPIRAL-DITH
0
2
false
POS-TARG
DITHER
0.179
LINE
0.116
false
false
63.650002
4
20.02
ACS-SBC-DITHER-BOX
3
false
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