We have added Visit 12 (2 orbits), in order to re-observe the first part of Visit 08 that failed.
(A HOPR repeat was granted.)
use FGS3 on visit 12
----- Attempting Submission 1 (Thu Jul 03 15:24:38 GMT 2008) -----
----- Attempting Submission 2 (Mon Jun 29 12:54:19 GMT 2009) -----
----- Attempting Submission 3 (Wed Jan 20 15:13:36 GMT 2010) -----
----- Attempting Submission 4 (Mon Jan 25 14:20:09 GMT 2010) -----
2 extra orbits were granted following a HOPR request
Assigned ID: 577
----- Attempting Submission 1 (Fri Mar 07 21:05:00 GMT 2008) -----
UV spectroscopy of Local Lyman Break Galaxy Analogs: New Clues to Galaxy Formation in the Early Universe
Much of our information about galaxy evolution and the interaction between galaxies and the IGM at high-z has been provided by the Lyman Break Galaxies (LBGs). However, it is difficult to investigate these faint and distant objects in detail. To address this, we have used the GALEX All-Sky Imaging Survey and the SDSS to identify for the first time a rare population of low-redshift galaxies with properties remarkably similar to the high-redshift LBGs. These local "Lyman Break Analogs" (LBAs) resemble LBGs in terms of morphology, size, UV luminosity, star formation rate, UV surface brightness, stellar mass, velocity dispersion, metallicity, and dust content. We are assembling a wide range of data on these objects with the goal of using them as local laboratories for better understanding the relevant astrophysical processes in LBGs. These data include HST imaging (95 orbits in Cy15 and 16), Spitzer photometry and spectroscopy, Chandra and XMM X-ray imaging and spectroscopy, and near-IR integral field spectroscopy (VLT, Keck, and Gemini). In this proposal we are requesting the most important missing puzzle piece: far-UV spectra with a signal-to-noise and spectral resolution significantly better than available for typical LBGs. We will use these spectra to study the LBA's galactic winds, probe the processes that regulate the escape of Ly-a and Lyman continuum radiation, determine chemical abundances for the stars and gas, and constrain the form of the high-end of the Initial Mass Function. Adding these new COS data will give us vital information about these extraordinary sites of star formation in the local universe. In so-doing it will also shed new light on the processes that led to the formation of stars, the building of galaxies, and the enrichment and heating of the IGM in the early universe.
Each target will be observed with COS/FUV/PSA in grisms G130M and G160M using TIME-TAG mode. Exposures are taken at at least one FP-POS=1 and one FP-POS=4 to get a minimum of two wavelength dithers for each spectrum, and we set FLASH=yes for better wavelength calibration.
The acquisition is done using the NUV imaging mode, either with Mirror A or Mirror B depending on the target surface brightness determined in a 9x9 pixel box. When not too time consuming, the acquisition is done by a 2x2 spiral pattern ACQ/SEARCH and centering on the brightest pixel, followed by an ACQ/IMAGE. However, for the remaining targets the acquisition is done solely by an ACQ/IMAGE, expecting that after several months into the mission the pointing accuracy will be good to 1 arcsec precision. Therefore, we have given the optional requirement that these observations should be carried out only AFTER=01-NOV-2009:00:00:00. Half of the targets have a positional accuracy to about <0.2 arcsec from HST registered with the GSC2 system. The rest have SDSS positions to about <0.5" accuracy.
The table in the 'additional comments' field below gives the FUV magnitudes and surface brightness used to estimate acquisition and buffer times.
For BUFFER-TIME, we assumed a source flat (in Fnu) with a diameter of 1 arcsec and a surface brightness within a 1.0" diameter aperture as measured from the FUV ACS images. The buffer time is the shorter value of 2/3 times the buffer time returned by the ETC and the exposure time (was always the exposure time).
To calculate the acquisition time, we used the COS ACQ ETC to estimate the time necessary to reach S/N~40 inside a 9x9 pixel box centered on the brightest part of the target. The surface brightnesses inside a 9x9pixel box fed to the ETC are listed in the table below.
(Note to self: In June 2009 we have exchanged target 083803 for 021348. However, given its faintness we may consider further changing 021348 into 113303 at a later stage, depending on the outcome of some of the targets that will be done first. 021348's first visibility window is during 30 Nov-31 Dec 2009.)
FUV magnitudes and surface brightness measured inside apertures with 2.5" and 1.0" diameters, and the maximum surface brightness inside a 9x9 pixel box centered on the brightest component of each source. Last 2 columns give the mirror used and the exposure time for each acquisition image estimated using the COS ACQ ETC.
ID REDSHIFT MAG(2.5") SB(2.5") MAG(1.0") SB(1.0") SB(9x9pixels) MIRROR ACQ. TIME
mag mag/arcsec^2 mag mag/arcsec^2 mag/arcsec^2 (seconds)
******** MAGNITUDES ARE IN AB *********
===================================================================
Haro11 0.02 16.0 17.7 16.4 16.1 14.1 B 28
080844 0.09 18.3 20.1 18.4 18.2 15.4 B 93
093813 0.10 18.0 19.7 18.3 18.0 16.0 B 162
210358 0.14 19.2 21.0 19.5 19.2 16.6 A 41
015028 0.15 19.3 21.1 19.7 19.4 17.6 A 102
005527 0.17 19.4 21.1 19.6 19.3 16.8 A 49
092600 0.18 19.0 20.7 19.2 18.9 17.4 A 85
021348 0.22 20.3 22.0 20.5 20.2 17.7 A 55
092159 0.24 19.2 20.9 19.5 19.2 16.7 A 45
ISM IN EXTERNAL GALAXIES
12
false
0.0
0.0
false
false
false
false
false
false
SUPPORTED
GALAXY
STARBURST
FUV=18.0
J2000
09 38 13.4900
+54 28 25.00
J2000
GALAXY
STARBURST
FUV=18.3
J2000
08 08 44.2600
+39 48 52.30
J2000
GALAXY
STARBURST
FUV=19.2
J2000
21 03 58.7400
-07 28 2.40
J2000
GALAXY
STARBURST
FUV=19.0
J2000
09 26 0.4000
+44 27 36.10
J2000
GALAXY
STARBURST
FUV=19.4
J2000
00 55 27.4600
-00 21 48.70
J2000
GALAXY
STARBURST
FUV=19.2
J2000
09 21 59.3800
+45 09 12.30
J2000
GALAXY
STARBURST
FUV=20.3
J2000
08 38 3.7200
+44 59 0.20
J2000
GALAXY
STARBURST
FUV=19.30
J2000
01 50 28.4000
+13 08 58.30
J2000
GALAXY
STARBURST
FUV=15.96
J2000
00 36 52.4720
+33 33 16.67
J2000
COS/FUV
Spectroscopic
No
No
G130M
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No
No
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No
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COS/FUV
Spectroscopic
No
No
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No
No
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1600
COS/FUV
Spectroscopic
No
No
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Spectroscopic
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No
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COS/FUV
Spectroscopic
No
No
G130M
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COS/FUV
Spectroscopic
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G160M
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COS/FUV
Spectroscopic
No
No
G130M
1291
COS/FUV
Spectroscopic
No
No
G160M
1600
COS/FUV
Spectroscopic
No
No
G130M
1291
COS/FUV
Spectroscopic
No
No
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:low-sky "N"
:pcs-visibility 3236
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
:visit-id "08"
:orbit-number 2
:pcs-time 195
:si-vis-utilization 3034
:al-overhead-at-end 0
:internal-dur-at-end 116
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3236
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
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:orbit-number 3
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:si-vis-utilization 3034
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
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:orbit-number 4
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:si-vis-utilization 3034
:al-overhead-at-end 0
:internal-dur-at-end 428
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3236
:pcs-gap 0
)
true
4
0
The scheduling data was generated by CASM 18.1.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 11727
:visit-id "12"
:proposal-version -1
:trans-version "20091209"
:date "20-Jan-2010 16:07:45.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 174032
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 11727
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 11727
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2897
:al-overhead-at-end 0
:internal-dur-at-end 116
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3234
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
:visit-id "12"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3004
:al-overhead-at-end 0
:internal-dur-at-end 428
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3234
:pcs-gap 0
)
false
2
0
The scheduling data was generated by CASM 17.2.
CASM was run in Phase II mode.
1261638387000
73.17135332923581
(Tic-Visit
:proposal-id 11727
:visit-id "09"
:proposal-version -1
:trans-version "20090130"
:date "29-Jun-2009 14:03:52.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 4
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 330576
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 11727
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 11727
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2915
:al-overhead-at-end 0
:internal-dur-at-end 116
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3251
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
:visit-id "09"
:orbit-number 2
:pcs-time 195
:si-vis-utilization 3054
:al-overhead-at-end 0
:internal-dur-at-end 116
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3251
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
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:orbit-number 3
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:si-vis-utilization 3054
:al-overhead-at-end 0
:internal-dur-at-end 116
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3251
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11727
:visit-id "09"
:orbit-number 4
:pcs-time 195
:si-vis-utilization 3054
:al-overhead-at-end 0
:internal-dur-at-end 428
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3251
:pcs-gap 0
)
true
4
0