Hi, the STIS data on May 5, 2012 was used in the COS ETC to compuete the exposure time for the COS visits 22 and 23. The exposure time with MIRROR B is 314 seconds. I used 350 as the supernova is fading. The COS ETC run is COS.ta.401074 please delete visit 21. please use visits 22 and 23 we should have a very interesting COS spectrum. Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused Submission failed communicating with the submission server: java.rmi.ConnectException: Connection refused to host: 130.167.201.116; nested exception is: java.net.ConnectException: Connection refused ----- Attempting Submission 1 (Wed May 09 14:34:36 GMT 2012) ----- UV Studies of a Core Collapse Supernova The UV spectrum of a core collapse SN encodes unique information about nucleosynthesis, the star's mass loss history, shock physics, and dust formation. This proposal aims at a detailed study of one bright core collapse SN, discoved as a result of the many ongoing surveys, either a Type IIP, IIn or Ib or Ic supernova. We will address the role of circumstellar interaction and mass loss through CNO lines in the UV, the nature of dust formation from UV line profiles, and we will use the UV continuum as a diagnostic of non-thermal emission from the shock. The overall goal is to achieve a better understanding of these objects by combining ground-based observations with complementary HST data. In cycle 17 and cycle 18 we obtained excellent data for SN 2010al and SN 2010jl that live up to our expectations. In the past, we have used HST to obtain critical UV spectra from the explosion to the nebular phase with good results for a limited number of objects. The advent of COS provides new capability for UV observations which we would like to exploit. When nature provides a bright candidate, HST should be ready to respond. first visit will be just STIS/CCD second visit STISCCD+COS, 20-40 days after first visit thrid visit STIS/CCD+COS, 60=80 days after first visit HOT STARS 12 false 0.0 0.0 false false false false SUPPORTED EXT-STAR SUPERNOVA SUPERNOVA TYPE II J2000 J2000 EXT-STAR SUPERNOVA J2000 STIS/CCD Spectroscopic No No G230LB 2375 STIS/CCD Spectroscopic No No G430L 4300 COS/FUV Spectroscopic No No G130M 1300 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1300 COS/FUV Spectroscopic No No G160M 1600 STIS/CCD Spectroscopic No No G230LB 2375 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /Users/aroman/Desktop/OP-cache/12540-v01.xml ToO Acquisition time is correct for sn2011dh @ mag 14.0 1308879481000 118.53951394171418 (Tic-Visit :proposal-id 12540 :visit-id "01" :proposal-version -1 :trans-version "20120312" :date "09-May-2012 10:24:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 331664 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12540 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12540 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 72 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3144 :al-overhead-at-end 0 :internal-dur-at-end 620 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) true 2 0 Acq for supernova v=14.0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /Users/aroman/Desktop/OP-cache/12540-v02.xml Visit 2 will provide the UV spectrum of sn2011dh. Then we can measure the flux in the UV to caclulate the proper exposures times for the acqusition in visit 3. 1333051190000 197.7035196739712 (Tic-Visit :proposal-id 12540 :visit-id "02" :proposal-version -1 :trans-version "20120312" :date "09-May-2012 10:31:36.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 266432 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12540 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12540 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3036 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3128 :al-overhead-at-end 85 :internal-dur-at-end 394 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) true 2 0 Acq for supernova v=18.0 STIS.sp.357436 93J-nuv STIS.sp.357438 98S-nuv STIS.sp.357436 93J-nuv STIS.sp.357438 98S-nuv Timing link suitability includes constraints ([22 After 20 by 20.0 to 60.0 days] [23 After 20 by 20.0 to 60.0 days]) The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /Users/aroman/Desktop/OP-cache/12540-v20.xml Visit 20 will provide the UV spectrum of sn2010jl. on Jan 25, 2012 the brightness of the supernova was B 16.8 The supernova is declining @ 0.012 mags/day 1336079205000 115.62570661087102 (Tic-Visit :proposal-id 12540 :visit-id "20" :proposal-version -1 :trans-version "20120312" :date "09-May-2012 10:25:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 229632 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12540 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12540 :visit-id "20" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2863 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "20" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2978 :al-overhead-at-end 85 :internal-dur-at-end 394 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) true 2 0 an exposure time of 1 second will work find for B mag of 17.5 we expect the brightness to be about 17.5 on March 1, 2012 decling at 0.012 mags/day Timing link suitability includes constraints ([Sequence (22 23) within 3.0 days] [22 After 20 by 20.0 to 60.0 days]) The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /Users/aroman/Desktop/OP-cache/12540-v22.xml The STS observation on May 5, 2012 is shown here: COS.ta.401074 MIRROR B = 314 seconds, I put 350 as the supernova is slowly fading please try to schedule visits 22 and 23 in the same SMS. a couple days different is not critical. (Tic-Visit :proposal-id 12540 :visit-id "22" :proposal-version -1 :trans-version "20120312" :date "09-May-2012 10:25:03.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 365504 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12540 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12540 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2772 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "22" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2938 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "22" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3014 :al-overhead-at-end 0 :internal-dur-at-end 366 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) true 3 0 we will haev to update the acq time after getting the data in visit 20 new light curve shows an estimated mag of B = 16.8 for May 15, 2012 MIRROR B with 132 seconds yields a s/n = 40 We observed sn2010jl with COS on 2011-01-23. by far the brightest feature in the spectrum is the sky Lyman- alpha. the spectrum can be viewed here. https://www.cfa.harvard.edu/~pchallis/sn2010jl_cos.ps a STIS image of the SN + host is here.. there is nothing nearby that is bright. https://www.cfa.harvard.edu/~pchallis/sn2010jl_pic.jpg https://www.cfa.harvard.edu/~pchallis/sn2010jl_pic.jpg Timing link suitability includes constraints ([Sequence (22 23) within 3.0 days] [23 After 20 by 20.0 to 60.0 days]) The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /Users/aroman/Desktop/OP-cache/12540-v23.xml The STS observation on May 5, 2012 is shown here: COS.ta.401074 MIRROR B = 314 seconds, I put 350 as the supernova is slowly fading please try to schedule visits 22 and 23 in the same SMS. a couple days different is not critical. (Tic-Visit :proposal-id 12540 :visit-id "23" :proposal-version -1 :trans-version "20120312" :date "09-May-2012 10:25:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 365504 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12540 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12540 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2806 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "23" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2938 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12540 :visit-id "23" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3014 :al-overhead-at-end 0 :internal-dur-at-end 366 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) true 3 0 we will haev to update the acq time after getting the data in visit 20 new light curve shows an estimated mag of B = 16.8 for May 15, 2012 MIRROR B with 132 seconds yields a s/n = 40 We observed sn2010jl with COS on 2011-01-23. by far the brightest feature in the spectrum is the sky Lyman- alpha. the spectrum can be viewed here. https://www.cfa.harvard.edu/~pchallis/sn2010jl_cos.ps a STIS image of the SN + host is here.. there is nothing nearby that is bright. https://www.cfa.harvard.edu/~pchallis/sn2010jl_pic.jpg https://www.cfa.harvard.edu/~pchallis/sn2010jl_pic.jpg