0
Assigned ID: 66
----- Attempting Submission 1 (Tue Apr 08 08:51:09 GMT 2014) -----
HST Phase I Proposal 66 (elars_cos_mh1.apt) successfully submitted.
----- Attempting Submission 2 (Fri Apr 11 23:34:30 GMT 2014) -----
HST Phase I Proposal 66 (elars_cos_mh1.apt) successfully submitted.
----- Attempting Submission 3 (Fri Apr 11 23:55:59 GMT 2014) -----
HST Phase I Proposal 66 (elars_cos_mh1.apt) successfully submitted.
----- Attempting Submission 4 (Sat Apr 12 00:00:59 GMT 2014) -----
HST Phase I Proposal 66 (elars_cos_mh1.apt) successfully submitted.
----- Attempting Submission 5 (Sat Apr 12 00:09:24 GMT 2014) -----
* 150202: Completed phase II pointing and photometry for target 4/visit 4. On Hold released. Phase II for 13654 should now be complete.
* 150108 v2: Adding flux and observation information for visit 25, which I had forgotten
* 150108: Releasing On Hold status for visits 02, 03, and 12 after recent ACS and WFC3 observations. Only visit 04 remains on hold, which is scheduled for the end of January.
* 141103: I have completed phase II and am releasing On Hold status for visits 07, 08, 11, 18, 25. 4 visits are now on hold.
* 141016: I have added observation ID numbers and measured fluxes to the Comments section for each targets for which complete phase II is submitted.
* 141013: I am releasing the On Hold status for visit 22.
FUV imaging observations were done (GO 13483), which enabled me to complete the Phase II for this target.
-605391189
----- Attempting Submission 1 (Wed Jul 23 11:57:18 GMT 2014) -----
----- Attempting Submission 2 (Mon Oct 13 11:28:06 GMT 2014) -----
----- Attempting Submission 3 (Thu Oct 16 14:09:42 GMT 2014) -----
HST Phase II Proposal 13654 (spectro_elars_pii_141016.apt) successfully submitted.
----- Attempting Submission 4 (Mon Nov 03 14:51:45 GMT 2014) -----
----- Attempting Submission 5 (Thu Jan 08 16:11:03 GMT 2015) -----
----- Attempting Submission 6 (Thu Jan 08 18:25:13 GMT 2015) -----
----- Attempting Submission 7 (Mon Feb 02 09:59:14 GMT 2015) -----
Ultraviolet Spectroscopy of the Extended Lyman Alpha Reference Sample
The importance of the Lyman alpha (Lya) emission line for high-z galaxy studies cannot be overstated. Tens of thousands of galaxies have been found and confirmed through Lya, and in the next decade the samples will increase 100-fold. Yet Lya is a resonance line, and transfer effects may bias surveys in complicated and unknown ways if fundamental relations between Lya observables and physical properties are not established. This requires large samples and comprehensive multi-wavelength data sets. The Extended Lyman alpha Reference Sample is a sample of 28 star-forming galaxies, complete with 8-band HST imaging, 21 cm observations of HI gas, and a plethora of other data: it will provide the gold-standard study of Lya astrophysics in extragalactic laboratories. Currently eLARS includes no data from which to measure the Lya line profile or the covering/kinematics of the ISM - properties ranked among the most crucial for Lya transfer.
The proposed COS spectra will measure ~8 ISM absorption lines, Ly-alpha itself, and an array of stellar features. From this we will:
1. determine the covering and kinematics of the neutral and ionized ISM - the material through which Lya transfers
2. resolve the Lya emission/absorption and model the properties of the HI medium
3. quantify of mechanical feedback from massive stars and supernovae
4. enhance the accuracy and ensure maximal return from ACS Lya imaging
With large-scale galaxy surveys now beginning, eLARS spectroscopy will provide a vital interpretive dataset for the coming decades when no UV platforms are available. It adheres perfectly to the philosophy of the UV initiative.
This programme will observe 27 nearby star-forming galaxies with the COS.
25 of the visits are single-orbit visits in the CVZ; 2 visits consist of two normal (i.e. not CV) orbits each.
PSA and MIRROR A are used throughout.
All visits use ACQ/IMAGE for target acquisition, and then do four exposures of spectroscopy in the G130M grating with CENWAVE=1327. This is the optimal setting to see the absorption lines and Ly-alpha emission in which we are interested. Each of the four spectroscopic exposures is done at incremented FP-POS positions to best remove fixed pattern noise.
To design the COS observations, all photometry is done in ACS/SBC/F140LP and WFC3/UVIS/F336W images. We find the desired pointing -- the brightest UV point source -- and do photometry in two apertures. We then interpolate in log-flux (i.e. measuring the beta slope) to 2200 Angstroms, the wavelength of the NUV imager.
Photometry (F140LP and F336W) is done in two circular apertures:
- one of 0.1 arcsec. This is used to design the ACQ/IMAGE observation, where the real point-sources are important
- the second aperture has radius 1.25 arcsec, the radius of the PSA, and it is this ETC run that is used for the spectroscopic visits where it's the whole flux in the aperture that counts.
Exposure times for acquisition vary a lot, between 6 and 370 seconds; targets have similar total luminosities, but quite different morphologies and therefore surface brightnesses. This has really been optimized using the ACS+WFC3 imaging.
Four visits are currently on hold, pending data acquisition from the imaging leg of the survey, GO 13483. When these observations are conducted we will immediately obtain the images from MAST, process them, and make the same measurements as described above. Then we will update the PII and release the hold. Current scheduling windows are provided in the individual On Hold comments boxes for each target.
ISM IN EXTERNAL GALAXIES
Default
false
true
false
false
false
SUPPORTED
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 11110 J9ZP14010
F336W 13483 ICDB88010
COS/NUV full = 8.6408e-16 cgs/AA
COS/NUV ACQ = 2.8424e-16 cgs/AA
ELARS02
J2000
J2000
log(LFUV/Lsun) = 10.056
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB01020
F336W 13483 ICDB58010
COS/NUV full = 6.3514e-16 cgs/AA
COS/NUV ACQ = 1.1643e-16 cgs/AA
ELARS03
J2000
J2000
log(LFUV/Lsun) = 10.208
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB02020
F336W 13483 ICDB78010
COS/NUV full = 1.6549e-15 cgs/AA
COS/NUV ACQ = 1.9334e-16 cgs/AA
ELARS04
J2000
J2000
log(LFUV/Lsun) = 10.069
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB03020
F336W 13483 ICDB60010
COS/NUV full = 1.0353e-15 cgs/AA
COS/NUV ACQ = 5.9699e-16 cgs/AA
ELARS05
J2000
J2000
log(LFUV/Lsun) = 9.963
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB04020
F336W 13483 ICDB61010
COS/NUV full = 2.3637e-16 cgs/AA
COS/NUV ACQ = 5.8243e-17 cgs/AA
ELARS06
J2000
J2000
log(LFUV/Lsun) = 9.657
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB05020
F336W 13483 ICDB62010
COS/NUV full = 6.2077e-16 cgs/AA
COS/NUV ACQ = 1.7235e-16 cgs/AA
ELARS07
J2000
J2000
log(LFUV/Lsun) = 9.572
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB06020
F336W 13483 ICDB63010
COS/NUV full = 5.091e-16 cgs/AA
COS/NUV ACQ = 1.4866e-16 cgs/AA
ELARS08
J2000
J2000
log(LFUV/Lsun) = 9.546
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB07020
F336W 13483 ICDB64010
COS/NUV full = 1.3304e-15 cgs/AA
COS/NUV ACQ = 1.6273e-16 cgs/AA
ELARS09
J2000
J2000
log(LFUV/Lsun) = 9.542
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB08020
F336W 13483 ICDB65010
COS/NUV full = 2.524e-16 cgs/AA
COS/NUV ACQ = 3.4114e-17 cgs/AA
ELARS10
J2000
J2000
log(LFUV/Lsun) = 9.532
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB09020
F336W 13483 ICDB66010
COS/NUV full = 6.5463e-16 cgs/AA
COS/NUV ACQ = 8.2701e-17 cgs/AA
ELARS11
J2000
J2000
log(LFUV/Lsun) = 9.511
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB10020
F336W 13483 ICDB67010
COS/NUV full = 3.0154e-16 cgs/AA
COS/NUV ACQ = 2.2438e-17 cgs/AA
ELARS12
J2000
J2000
log(LFUV/Lsun) = 9.472
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB11020
F336W 13483 ICDB68010
COS/NUV full = 1.9369e-15 cgs/AA
COS/NUV ACQ = 1.469e-15 cgs/AA
ELARS13
J2000
J2000
log(LFUV/Lsun) = 9.448
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB12020
F336W 13483 ICDB69010
COS/NUV full = 5.1559e-16 cgs/AA
COS/NUV ACQ = 6.5124e-17 cgs/AA
ELARS14
J2000
J2000
log(LFUV/Lsun) = 9.345
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB13020
F336W 13483 ICDB70010
COS/NUV full = 3.3331e-16 cgs/AA
COS/NUV ACQ = 6.2011e-17 cgs/AA
ELARS15
J2000
J2000
log(LFUV/Lsun) = 9.365
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB14020
F336W 13483 ICDB71010
COS/NUV full = 1.8941e-16 cgs/AA
COS/NUV ACQ = 3.3181e-17 cgs/AA
ELARS16
J2000
J2000
log(LFUV/Lsun) = 9.310
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB15020
F336W 13483 ICDB72010
COS/NUV full = 1.6431e-16 cgs/AA
COS/NUV ACQ = 2.3122e-17 cgs/AA
ELARS17
J2000
J2000
log(LFUV/Lsun) = 9.221
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB16020
F336W 13483 ICDB73010
COS/NUV full = 1.5992e-16 cgs/AA
COS/NUV ACQ = 3.121e-17 cgs/AA
ELARS18
J2000
J2000
log(LFUV/Lsun) = 9.010
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB17020
F336W 13483 ICDB74010
COS/NUV full = 2.8279e-16 cgs/AA
COS/NUV ACQ = 6.3276e-17 cgs/AA
ELARS19
J2000
J2000
log(LFUV/Lsun) = 9.009
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB18020
F336W 13483 ICDB75010
COS/NUV full = 3.4226e-16 cgs/AA
COS/NUV ACQ = 5.1168e-17 cgs/AA
ELARS20
J2000
J2000
log(LFUV/Lsun) = 9.040
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB19020
F336W 13483 ICDB79010
COS/NUV full = 1.39e-16 cgs/AA
COS/NUV ACQ = 3.3407e-17 cgs/AA
ELARS21
J2000
J2000
log(LFUV/Lsun) = 8.982
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB20020
F336W 13483 ICDB80010
COS/NUV full = 1.1501e-15 cgs/AA
COS/NUV ACQ = 2.2816e-16 cgs/AA
ELARS22
J2000
J2000
log(LFUV/Lsun) = 10.065
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB21020
F336W 13483 ICDB89010
COS/NUV full = 2.2688e-16 cgs/AA
COS/NUV ACQ = 6.5088e-17 cgs/AA
ELARS23
J2000
J2000
log(LFUV/Lsun) = 10.047
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB22020
F336W 13483 ICDB81010
COS/NUV full = 1.1138e-15 cgs/AA
COS/NUV ACQ = 1.5245e-16 cgs/AA
ELARS24
J2000
J2000
log(LFUV/Lsun) = 9.966
GALAXY
STARBURST
ELARS25
J2000
J2000
log(LFUV/Lsun) = 9.802
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB25020
F336W 13483 ICDB86010
COS/NUV full = 1.9918e-16 cgs/AA
COS/NUV ACQ = 6.613e-17 cgs/AA
ELARS26
J2000
J2000
log(LFUV/Lsun) = 9.706
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB25020
F336W 13483 ICDB86010
COS/NUV full = 1.2626e-16 cgs/AA
COS/NUV ACQ = 2.4746e-17 cgs/AA
ELARS27
J2000
J2000
log(LFUV/Lsun) = 9.706
GALAXY
STARBURST
HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB26020
F336W 13483 ICDB87010
COS/NUV full = 4.2163e-16 cgs/AA
COS/NUV ACQ = 1.057e-16 cgs/AA
ELARS28
J2000
J2000
log(LFUV/Lsun) = 9.683
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
COS/FUV
Spectroscopic
No
No
G130M
1327
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HST Imaging Datasets for Photometry
...........
F140LP 13483 JCDB23020
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