NOW with full list of CoIs 604948414 Assigned ID: 616 ----- Attempting Submission 1 (Fri Apr 07 16:19:50 GMT 2017) ----- HST Phase I Proposal 616 (Sz102_2017.apt) successfully submitted. Receipt: # 616-1 ----- Attempting Submission 2 (Fri Apr 07 16:23:44 GMT 2017) ----- HST Phase I Proposal 616 (Sz102_2017.apt) successfully submitted. Receipt: # 616-2 ----- Attempting Submission 3 (Fri Apr 07 18:20:57 GMT 2017) ----- ----- Attempting Submission 4 (Sat Apr 08 05:12:50 GMT 2017) ----- ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN With 1-orbit visits only. All visits grouped to be executed within 30 days. All WAVECALs after science exposures. Exposure times set to maximum allowed, but may need to be reduced based on previous attempts to schedule these exposures. 1781311660 ----- Attempting Submission 1 (Wed Jul 19 20:06:42 GMT 2017) ----- HST Phase II Proposal 15210 (vers2.apt) successfully submitted. Receipt: # 15210-1 ----- Attempting Submission 2 (Thu Jul 20 16:29:21 GMT 2017) ----- ----- Attempting Submission 3 (Thu May 16 15:14:56 GMT 2019) ----- HST Phase II Proposal 15210 (re_visit.apt) successfully submitted. Receipt: # 15210-3 ----- Attempting Submission 4 (Thu May 16 16:08:01 GMT 2019) ----- ----- Attempting Submission 5 (Fri Jan 24 10:53:53 GMT 2020) ----- ----- Attempting Submission 6 (Fri Jan 24 17:02:11 GMT 2020) ----- ----- Attempting Submission 7 (Fri May 08 13:17:32 GMT 2020) ----- All errors relate to already executed visits 01, 02 (that have failed). The extremes of protostellar jets: Resolving the hot jet of Sz 102 Jets and outflows from young stellar objects are a fundamental ingredient of star formation. Studies of these jets focused mainly on low temperature plasma tracers (T~1e4 K). However, there is increasing evidence for a new jet component at much higher temperatures unpredicted by theory. In particular, the jet of the classical T Tauri star DG Tau shows stationary X-ray emission (T>1e6 K plasma) close to the driving source that is mirrored in intermediate temperature C IV emission (T~1e5 K plasma). Several other sources show jet emission from highly ionized species resembling various aspects of the well studied DG Tau system. Different models were developed that explain individual systems, but do not provide a comprehensive picture that can be generally applied. We propose STIS long-slit spectroscopy to characterize the spatial distribution and kinematics of the intermediate temperature jet of Sz 102. The Sz 102 jet shines even brighter in 1e5 K plasma tracers than the famous DG Tau jet. The proposed observations allow us to study similarities and differences between Sz 102 and DG Tau as well as to test various models that predict different spatial morphologies. The proposed observations allow us to check if the intermediate/high temperature jet plasma is caused by a general process that has been overlooked in previous studies tracing only the low temperature part of these jets. The aim of this program is to resolve the jet (HH 228) spatially as well as in velocity space, and we will use HST STIS long-slit observations with the slit oriented along the jet. The position angle of the jet is known from previous observations to be 98 deg (E of N), which implies an ORIENT constraint, i.e., ORIENT=143+-1 deg or ORIENT=323+-1 deg. We will use four different settings in two visits: Visit 1 (FUV): a) Two orbits with the G140M grating (central wavelength 1540 AA) targeting the C IV doublet in the FUV Visit 2 (optical): b) One orbit with the G430M grating (central wavelength 4961 AA) targeting [O III] at lambda = 5007 AA c) One orbit with the G430L grating targeting [Ne III] at lambda = 3869 AA (only spatial information) d) One orbit with the G750M (central wavelength 6581 AA) targeting the classical optical diagnostic jet lines In total, we will use five orbits split into two visits (two for the FUV part, three for the optical part) so that FUV and optical observations are not mixed. We ensure that both visits are executed within about one month through a "GROUP WITHIN" statement. In addition, we use the dither pattern STIS-ALONG-SLIT to improve the removal of hot pixel. We expect that two guide stars will be available from inspection of previous programs on this target, so that no re-acquisitions are needed between the orbits. All exposure times are based on the available HST data, which exist for all setting used in this program from various previous programs. Detector safety: The STIS MAMA exposure will not violate the brightness limits of the detector as the expected local count-rate (<0.1counts/pix/s) is far below the limit and the source extension is too small (<1 arcsec) to increase the global count-rate to values near the limit (see also the ETC run provided for this exposure that is based on a previously observed COS spectrum). Stellar Physics 6 false false true false false false 0.0 0.0 false SUPPORTED STAR CIRCUMSTELLAR MATTER JET PRE-MAIN SEQUENCE STAR PROTOPLANETARY DISK T TAURI STAR NO This object was generated by the targetselector and retrieved from the SIMBAD database. Based on the Visit Planer information, we manually adjusted the coordinates for the anticipated observing date in April 2018. This correction is small and the coordinates are well within 0.06 arcsec from those successfully used by PropID 14177, and only 0.57 arcsec from the "standard" 2000 position, which Simbad provides. Further target information in https://www.aanda.org/articles/aa/pdf/2017/04/aa29929-16.pdf SZ-102 J2000 J2000 the total C IV flux is 8e-14 erg/s/cm^2 measured from a previous COS observation STIS/CCD Spectroscopic No No G430M 4961 STIS/CCD Spectroscopic No No G750M 6581 STIS/CCD Spectroscopic No No G430L 4300 STIS/CCD Spectroscopic No No G430M 3936 STIS/FUV-MAMA Spectroscopic No No G140M 1540 POS-TARG DITHER 0.7 We expect spatial structures of about 0.5 arcsec size so that a shift of 0.7 arcsec provides some margin. LINE false false 3 90.0 STIS-ALONG-SLIT 1 false POS-TARG DITHER 0.7 We expect spatial structures of about 0.5 arcsec size so that a shift of 0.7 arcsec provides some margin. LINE false false 3 270 LINE 2 false Timing link suitability includes constraints ([Group (01 02) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. This visit is dedicated to the FUV C IV observations. The ORIENT value is given by the PA of the jet (=98 deg, East of North). This gives ORIENT = 143 or 323 and we allow a tolerance of +- 1 deg. 1557348990000 325.18737999999996 (Tic-Visit :proposal-id 15210 :visit-id "01" :proposal-version -1 :trans-version "20181130" :date "16-May-2019 17:14:43.0" :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 800544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2867 :al-overhead-at-end 0 :internal-dur-at-end 178 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15210 :visit-id "01" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 647 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 2 0 Stellar magnitudes from Simbad. Also, the exposure time is compatible with extrapolations based on other successful STIS ACQs of classical T Tauri stars. GO wavecal with the same central wavelength and slit width as the science exposure. Input spectrum for ETC is from the COS spectrum of this source, and most likely includes the entire FUV emission from the source (data from PropID 11616, specifically lb6b59rkq, lb6b59rmq, and lb6b59roq). GO wavecal with the same central wavelength and slit width as the science exposure. Timing link suitability includes constraints ([Group (51 52 54 56 57) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. This visit is dedicated to the FUV C IV observations. The ORIENT value is given by the PA of the jet (=98 deg, East of North). This gives ORIENT = 143 or 323 and we allow a tolerance of +- 1 deg. 1590102380000 326.0 (Tic-Visit :proposal-id 15210 :visit-id "51" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:07:48.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 365728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "51" :obset-id "51" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "51" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2807 :al-overhead-at-end 0 :internal-dur-at-end 647 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) false 1 0 Stellar magnitudes from Simbad. Also, the exposure time is compatible with extrapolations based on other successful STIS ACQs of classical T Tauri stars. Input spectrum for ETC is from the COS spectrum of this source, and most likely includes the entire FUV emission from the source (data from PropID 11616, specifically lb6b59rkq, lb6b59rmq, and lb6b59roq). GO wavecal with the same central wavelength and slit width as the science exposure. Timing link suitability includes constraints ([Group (51 52 54 56 57) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. This visit is dedicated to the FUV C IV observations. The ORIENT value is given by the PA of the jet (=98 deg, East of North). This gives ORIENT = 143 or 323 and we allow a tolerance of +- 1 deg. 1590108098000 326.0 (Tic-Visit :proposal-id 15210 :visit-id "54" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 14:33:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 365728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "54" :obset-id "54" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "54" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2807 :al-overhead-at-end 0 :internal-dur-at-end 647 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) false 1 0 Stellar magnitudes from Simbad. Also, the exposure time is compatible with extrapolations based on other successful STIS ACQs of classical T Tauri stars. Input spectrum for ETC is from the COS spectrum of this source, and most likely includes the entire FUV emission from the source (data from PropID 11616, specifically lb6b59rkq, lb6b59rmq, and lb6b59roq). GO wavecal with the same central wavelength and slit width as the science exposure. Timing link suitability includes constraints ([Group (01 02) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 1557080772000 325.18737999999996 (Tic-Visit :proposal-id 15210 :visit-id "02" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:01:07.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 276464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "02" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2927 :al-overhead-at-end 75 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15210 :visit-id "02" :orbit-number 2 :pcs-time 302 :si-vis-utilization 3038 :al-overhead-at-end 75 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15210 :visit-id "02" :orbit-number 3 :pcs-time 302 :si-vis-utilization 3038 :al-overhead-at-end 75 :internal-dur-at-end 360 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 3 3 Same as for visit 1 (the FUV part) Timing link suitability includes constraints ([Group (51 52 54 56 57) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 1590182509000 326.0 (Tic-Visit :proposal-id 15210 :visit-id "52" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:08:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 74032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "52" :obset-id "52" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "52" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2805 :al-overhead-at-end 75 :internal-dur-at-end 380 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) false 1 0 Same as for visit 1 (the FUV part) Timing link suitability includes constraints ([Group (51 52 54 56 57) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 1590188234000 326.0 (Tic-Visit :proposal-id 15210 :visit-id "56" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:08:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 74032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "56" :obset-id "56" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "56" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2806 :al-overhead-at-end 75 :internal-dur-at-end 380 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 1 0 Same as for visit 1 (the FUV part) (Tic-Visit :proposal-id 15210 :visit-id "56" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:08:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 74032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "56" :obset-id "56" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "56" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2806 :al-overhead-at-end 75 :internal-dur-at-end 380 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) false 1 0 Same as for visit 1 (the FUV part) Timing link suitability includes constraints ([Group (51 52 54 56 57) Within 30.0 days]) The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 1590193959000 326.0 (Tic-Visit :proposal-id 15210 :visit-id "57" :proposal-version -1 :trans-version "20191203" :date "08-May-2020 15:08:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 74032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15210 :visit-id "57" :obset-id "57" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15210 :visit-id "57" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2803 :al-overhead-at-end 75 :internal-dur-at-end 380 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) false 1 0 Same as for visit 1 (the FUV part)