0 Assigned ID: 1391 ----- Attempting Submission 1 (Fri Mar 01 03:57:08 GMT 2013) ----- HST Phase I Proposal 1391 (APT_lyb.pdf.apt.2013_03_01_03_19.aptbackup.apt) successfully submitted. ----- Attempting Submission 2 (Fri Mar 01 22:36:23 GMT 2013) ----- I inspected the images obtained in visit 2, located an offset star, measured its brightness, and located the NUV center of IRAS 00262+4251. This information defines the blind offset required by Visit 6, which has now been entered in APT. Please review and release Visit 6 for scheduling if you approve. -755240834 ----- Attempting Submission 1 (Fri Jun 14 21:21:11 GMT 2013) ----- ----- Attempting Submission 2 (Fri Aug 02 19:21:44 GMT 2013) ----- ----- Attempting Submission 3 (Sat Jan 11 00:17:47 GMT 2014) ----- ----- Attempting Submission 4 (Fri Jan 17 19:06:16 GMT 2014) ----- COS Gas Flows: Challenging the Optical Perspective Observations of the hydrogen Lya profile in galaxy spectra uniquely distinguish outflowing and inflowing gas. Recent COS observations of ultraluminous starbursts show the telltale signature of infalling neutral hydrogen. A radiative transfer calculation that models the profiles of Lyman series lines predicts broad scattering wings on the hydrogen Balmer lines, but the origin of the scattered Balmer emission is only unique when the Lyb profile is also fit. We show a strong kinematic similarity between the broad wings of the Lya and Ha line profiles in ULIRG spectra raising the suggestion that the sign of the gas flows producing the broad Ha wings may have been previously misinterpreted. We propose very blue G130M spectroscopy with COS to obtain the Lyb line profiles for four starburst galaxies with the aim of establishing the correct interpretation of the broad Balmer line wings in starburst spectra. Radiative transfer modeling has focused primarily on reproducing the Lya line shape. Calculating the Lya and Ha line profiles simultaneously in principle eliminates degenercies in model parameters. However, the addition of spectroscopy covering Lyb can significantly improve the constraints obtained from radiative transfer modeling; but because of the lack of data, no one has done this thus far. The Hubble Utraviolet Initiative should ensure that these data exist. This program will obtain pre-imaging of 2 ULIRGs. Blind offsets between the UV brightest knot in the ULIRG and a nearby star will be calculated from these images and used to acquire the UV knot in the COS PSA. COS G130M spectra will be obtained for each ULIRG. The other two ULIRGs have known offsets and can be acquired with existing information. The new COS spectra will provide bluer coverage than did previous observations. ISM IN EXTERNAL GALAXIES Default false true false false false SUPPORTED GALAXY EMISSION LINE NEBULA INTERACTING GALAXY STARBURST ULTRALUMINOUS IR GAL WIND J2000 J2000 R=16.0 mNUV = 18.729, mFUV=19.216 GALAXY EMISSION LINE NEBULA INTERACTING GALAXY STARBURST ULTRALUMINOUS IR GAL WIND J2000 J2000 R=15.9 mNUV=18.46 mFUV = 19.09 GALAXY EMISSION LINE NEBULA INTERACTING GALAXY STAR FORMING REGION ULTRALUMINOUS IR GAL WIND J2000 J2000 R=16.5 mNUV = 18.391, mFUV = 18.929 GALAXY EMISSION LINE NEBULA INTERACTING GALAXY STAR FORMING REGION ULTRALUMINOUS IR GAL WIND J2000 J2000 R=16.5 mNUV=18.158 mFUV=18.465 STAR UNDESIGNATED J2000 m_NUV=18.56 STAR UNDESIGNATED J2000 m(NUV) = 19.52 STAR UNDESIGNATED J2000 TBD GALAXY ULTRALUMINOUS IR GAL J2000 GALAXY ULTRALUMINOUS IR GAL J2000 COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1055 COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1055 COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1055 COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1055 WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F625W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F625W ACS/SBC Imaging No No F125LP ACS/SBC Imaging No No F125LP POS-TARG DITHER 0.472 LINE false false 2 44.4 ACS-SBC-DITHER-LINE 1 false POS-TARG DITHER 0.145 LINE false false 2 46.84 WFC3-UVIS-DITHER-LINE 2 false /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit370016533459410999.xml Timing link suitability includes constraints ([05 After 01 by 60.0 to 365.0 days]) The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. 1388216062000 72.62791404553619 (Tic-Visit :proposal-id 13407 :visit-id "01" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:58:00.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 903280 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13407 :visit-id "01" :obset-id "A1" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2999 :al-overhead-at-end 124 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3333 :pcs-gap 0 ) true 1 0 /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit4353849012384384909.xml The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. 1389492239000 322.322411419444 (Tic-Visit :proposal-id 13407 :visit-id "02" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:58:02.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 903280 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13407 :visit-id "02" :obset-id "A2" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3097 :al-overhead-at-end 124 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3430 :pcs-gap 0 ) true 1 0 /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit4953173643408964849.xml The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. 1386197175000 287.6165551353042 (Tic-Visit :proposal-id 13407 :visit-id "03" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:58:03.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 313168 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3044 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3377 :pcs-gap 0 ) true 1 0 /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit6230262405651744960.xml Timing link suitability includes constraints ([06 After 04 by 60.0 to 365.0 days]) The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 13407 :visit-id "04" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:58:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 330560 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2920 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3267 :pcs-gap 0 ) true 1 0 /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit7506411894823634037.xml Timing link suitability includes constraints ([05 After 01 by 60.0 to 365.0 days]) The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 13407 :visit-id "05" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:58:09.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 330560 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2986 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3333 :pcs-gap 0 ) true 1 0 We will use the images of this field (Visit 1) to select an offset star and enter its coordinates as Target 6. We will also identify the brightest UV knot and tweak the coordinates of Target 1 for Visit 5. Magnitude of offset star measured from from visit 1 F225W image. /private/var/folders/9w/9wdkX7XwFCyuih3XTBbeME+++TI/-Tmp-/OPVisit2229804314707696029.xml Timing link suitability includes constraints ([06 After 04 by 60.0 to 365.0 days]) The scheduling data was generated by CASM 21.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 13407 :visit-id "06" :proposal-version -1 :trans-version "20130502" :date "17-Jan-2014 10:56:53.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 330560 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13407 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13407 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3082 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3430 :pcs-gap 0 ) true 1 0 We will use the images of this field (Visit 2) to select an offset star and enter its coordinates as Target 7. We will also identify the brightest UV knot and tweak the coordinates of Target 4 for Visit 6. Magnitude of offset star is not known until Visit 2 is analyzed.