Technical Support: Svea Hernandez
OUTLINE
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 2
I. INTRODUCTION
“The Contact ScienCst (CS) is an Instrument ScienCst (IS) belonging to the
STScI team who supports calibraCon and use of the instrument(s) in the assigned programs.”
The CS provides advice on observing strategies:
1-‐ to meet the scienCfic objecCves of the program,
2-‐ to answer quesCons about instrument performance and
3-‐ to maintain the health and safety of the detectors subject to damage by over-‐illuminaCon: COS and STIS/MAMA
Our responsibility ends when the programs have completed!
Ref: hbp://www.stsci.edu/hst/proposing/docs/proposingOverview
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 3
I. INTRODUCTION
1-‐ Excellent support of HST science and users is the fundamental reason for the existence of the InsCtute and our scienCfic staff
2-‐ Support of GO program development and implementaCon as a primary point of contact between STScI and the astronomical community
3-‐ IS bring essenCal scienCfic and instrument experCse to this process, which complements that of the PCs/RIAs in scheduling and other technical issues
(helpdesk service)
Thus it is incumbent upon us to do our best from our perspecCves to ensure opCmum effecCveness and quality of HST observing programs and data.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 4
II. Phase II Support
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 5
II. Phase II Support
Refs: hbp://www.stsci.edu/hst/proposing/docs/proposingOverview & COS Instrument Handbook-‐ Chapter 10
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 6
II. Phase II Support
The advice we give is only as good as the informa5on we receive!
1-‐ Get familiar with the Phase I proposals once sent to you. Remember they are confidenCal.
2-‐ If contacted, do not hesitate to ask the PIs for details about sources, fields, crowding, etc…-‐> important to determine feasibility and best TA mode
3-‐ CS interact directly with PIs; IS do not but can if they so wish.
4-‐ Keep all exchanges in wriCng and copy all exchanges to the new history repository (e.g.: hst12000@stsci.edu
)
5-‐ If phone exchange is inevitable (deadline crunch Cme typically):
-‐> send email to the PI summarizing decisions made
-‐> copy summary to history file and
-‐> ask PI for email confirmaCon of agreement
(should avoid future “blame game” situaCons)
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 7
II. Phase II Support
The BOT is only used to clear field stars. The ETC has to be used for science targets!
1-‐ Proposers need to run the BOT for all fields and all configuraCons (TA +
SCIENCE) and they need to check the results! Null result does not mean SAFE !
2-‐ Remind PIs to enter ETC IDs in APT form. The “warning” should not be ignored so that reviews can be expedited.
3-‐ Remind them to provide all supporCng material at the Cme of submission
4-‐ If field star unknown or unsafe, addiConal informaCon has to be provided by the PI and ETC should be used for clearance.
5-‐ PI has to idenCfy and share remaining issues at the Cme of submission.
The detailed BOT procedures are in COS IHB: chapter 10: hbp://www.stsci.edu/hst/cos/documents/handbooks/current/ch10.Bright_obj7.html
6-‐ Review AVAILABLE MODE requests and forward issues/recommendaCons to CS Lead for approval before phase II deadline .
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 8
II. Phase II Support
1-‐ Cycle 20 Phase II instrucCons-‐ P2PI.pdf: hbp://www.stsci.edu/hst/proposing/docs/p2pi.html
2-‐ COS and STIS STANS for latest technical updates: hbp://www.stsci.edu/hst/cos/documents/newslebers/
3-‐ Instrument Handbooks:
COS: hbp://www.stsci.edu/hst/cos/documents/handbooks/current/cos_cover.html
STIS: hbp://www.stsci.edu/hst/sCs/documents/handbooks/currentIHB/cover.html
4-‐ APT/BOT demos and movies.
APT general page: hbp://www.stsci.edu/hst/proposing/apt/using_apt
STIS: hbp://apst.stsci.edu/apt/external/help/documentaCon/Running-‐BOT.html
COS: hbp://apst.stsci.edu/apt/external/help/documentaCon/Running-‐COS-‐BOT.html
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 9
II. Phase II Support
5-‐ APT/Aladin & Phase II Interface demos and movies: hbp://apst.stsci.edu/apt/external/help/roadmap2.html
hbp://apst.stsci.edu/apt/external/help/documentaCon/Aladin-‐PII.html
hbp://apst.stsci.edu/apt/external/help/documentaCon/Aladin-‐PosTarg.html
hbp://apst.stsci.edu/apt/external/help/documentaCon/Aladin-‐Pabern.html
6-‐ Galex Interface: to check field coverage and crowding: hbp://galex.stsci.edu/GalexView/#
NB: The Galex fields are directly accessible via the APT/Aladin interface
7-‐ GSC V2.3 is used. hbp://gsss.stsci.edu/Catalogs/GSC/GSC2/GSCIIProperCes.htm
A few facts (see Lasker et al. 2008):
Astrometry: Complete to V=19.5 mag, F=20.5 and J= 21.5 ; Ref frame ICRF; typical error: 0.3” (worst case is 0.35-‐0.75” at edges of plates).
Photometry: Errors 0.2-‐0.25 mag. For stars brighter than V=9 mag in GSCII, Tycho-‐2 mag is used.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 10
II. Phase II Support
1-‐ Phase II deadline is nominally followed by one month for PC verificaCons/reviews and one month for CS/IS reviews -‐> Early start for available proposals is recommended. All CS/IS reviews without ongoing issues are expected to be completed by September 30th of each year to support the new cycle scheduling
(subject to any other team priority direcCves).
2-‐ BOP Reviews are to be done expediCously but not hasCly : all doubts are to be cleared before program can be allowed to execute. AddiConal informaCon has to be
provided by GOs. CS is sole judge of safety! If contenCons arise, contact the CS Lead who will resolve them.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 11
II. Phase II Support
3-‐ The CS Lead resolves all VerificaCon (TAC compliance, duplicaCons) and Change issues, for policy uniformity. These are sent to the Lead only. If you inadvertently
receive any directly, forward them to the CS Lead and Deputy.
4-‐ Moving target (MT) and Target of Opportunity (ToOs) programs cannot be
completed unCl acCvated, but instrument specificaCons should be checked early to catch any issues.
12
II. Phase II Support
1-‐ The program reviews status is maintained on our COS/STIS User Support Page hbp://www.stsci.edu/hst/insCtute/org/ins/cos_sCs/projects/UserSupport/Prop_review/cycle20/
2-‐ Lists of Urgent/verified proposals are distributed via emails under the
“Weekly Report” banner and are circulated by CS Lead/deputy weekly. Please abide by the “Review before” date. When delays occur, inform CS Lead/Deputy of
underlying reasons.
3-‐ Track your review Cme: update to nearest hour each Cme a proposal is worked on
and send final results to CS Lead. Do this conCnuously as reviews progress.
4-‐ Transmit to CS Lead notable cases of errors corrected and improvements recommended that may be useful for other CS/IS.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 13
III. CS Reviews: Tools
1-‐ The SPAR Engine:
2-‐ BOT/Aladin interfaces: called from HST Astronomers’ Proposal Tool (APT)
Current Version: 20.1
-‐> update if needed!
3-‐ Galex/GSC2/MCPS databases: to check field stars coverage: Need to be used if the BOT/Galex tool generates a warning about field empty or crowded hbp://galex.stsci.edu/GalexView/#
hbp://ngala.as.arizona.edu/dennis/mcsurvey.html
(MC survey)
4-‐ ETC to verify health and safety of science targets
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 14
III. CS Reviews: Tools
th
a-‐ login: same as AD; Password: same as AD b-‐ Enter proposal version number in template b-‐ Review template flags & check lists. c-‐ where appropriate answer YES/NO quesCons d-‐ where appropriate explain how your reach you conclusions in text boxes e-‐ submit completed template via SPAR f-‐ save unready reviews if resoluCon is lengthy to support status tracking.
NB: combined COS+STIS proposals require separate COS and STIS templates;
Do immediate reviews of MT and ToOs, insofar as possible.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 15
III. CS Reviews: Tools
1-‐ upload the proposal to review in APT (retrieve from STScI)
2-‐ Select visit or single exposure to be reviewed
3-‐ click “BOT icon” on top menu bar in APT
4-‐ Select GSC2, click “Update display” and check all results in the summary table
5-‐ Select Galex, click “Update display” and check all results in the summary table.
When relevant, acCvate “Proper MoCon” feature and Repeat steps 4-‐ and 5-‐
6-‐ Click “ LOAD DSS” icon. The exposure(s) will appear as different planes in the order they are listed in the APT spreadsheet.
7-‐ Macro-‐apertures and stars are displayed when selecCng exposure planes
8-‐ Select region in display to see details of enclosed star(s); these listed in table at bobom of Aladin window; Place cursor on star and table entry flashes (and vice versa)
9-‐ Click “Orient Ranges” in APT top menu to display specificaCons and U3 arrow. Grab
arrow or corner to rotate. “Reset Orients” returns to original sexngs.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 16
III. CS Reviews: Tools
-‐ BOT screens all fields with AIS (all-‐sky) survey coverage.
-‐ BOT assumes all Galex sources are unreddened O5V stars.
If targets do not violate local/global count rates they are declared “safe”
-‐ BOT does not check for Galex coverage of the field to be cleared!!
Need to check for coverage separately (using Galexview/Aladin, for instance).
-‐ If no Galex coverage, no sources will be returned in summary table. Note that the result is the same when there are no sources but field is covered!
-‐ Galex provides an upper limit to individual source flux because of low spaCal resoluCon (4’’). If it clears, fine. If not, the source(s) may sCll be safe but required higher resoluCon data. HST images can be loaded in Aladin. No calculaCons will be done but blended sources can be resolved.
-‐ Magnitudes between FUV=14.332-‐12.6 and NUV=14.875-‐10.2 are subject to saturaCon. Non-‐linearity correcCons are now applied by the BOT. Targets brighter than those limits are not to be cleared with Galex.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 17
-‐ Contains 2 filters F and J to derive 1 color to 21-‐22 mag over full sky.
-‐ BOT calculates V and B-‐V from J and F under conservaCve assumpCons (all main sequence stars with no reddening). Since one color does not determine SpT and E
B-‐V , all stars with B-‐V <+0.1 are treated/classified as O5V stars. All stars bluer than a given magnitude (spectral element dependent) are assumed O5V
-‐ One or both filters have significantly brighter limits on some fields (GalacCc Center and
Magellanic Clouds)
-‐ ResoluCon is inadequate in some fields; young regions in nearby Galaxy, extended regions. As a result, “unknown” and “unsafe” objects will require abenCon
-‐ GSC2 omits stars within a substanCal radius of very bright stars because of PSF arCfacts.
Star within saturated bright stellar or nebular images may be absent, requiring alternaCve sources
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 18
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III. CS Reviews: Tasks
1-‐ Make sure to review the instrument parameters in the Phase II proposal , which goes to the telescope and not those in proposal free text (APT “exposure Name” emails) that may be wrong.
2-‐ Please answer all quesCons in the BOT review secCon of the template. MulCple targets/visits may be included in the same one, but each must be addressed separately . You may paste detailed flux or calculaCon inputs from the proposal or GO email but you must also do your own ETC calcula5ons for all targets and unsafe/ unknown field objects!
3-‐ For mulCple targets with same configuraCon, look for the worst cases (brightest + bluest) to logically clear others with one ETC calculaCons. The field must me cleared for each target though.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 20
III. CS Reviews: Tasks
4-‐ Recheck FUV and NUV fields for SCIENCE exposures against screening limits using APT/BOT/Aladin interface (see above). For COS: global rates refer to the enCre detector (segment/stripe). FOR MAMA: local rate check bins data to 8x8 pix.
MulCple objects in this area will be checked as single.
5-‐ Check GO-‐supplied target parameters as thoroughly as permibed, most criCcally if count rate is within factor 2 of our screening limits. If the object parameters are judged to be uncertain, or you have any other doubts, consult with the BOP Lead. AutomaCc secondary BOP review at certain count rate levels is no longer pracCced.
6-‐ Any unresolved issue at Cme of Phase II submission must be documented by GOs.
GOs must provide whatever data and format we request to resolve issues. IUE data must be low-‐resoluCon large aperture. Annotated images must be accompanied with corresponding photometric tables (HST, IUE, 2MASS, etc…)
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 21
III. CS Reviews: Tasks
7-‐ ETC Spectral Energy DistribuCons: Use original Kurucz models for BOT earlier than Sun (earliest O5) not Castelli & Kurucz, not Bruzual. Use solar template for normal G2 but need actual data for later types in FUV because no models include chromospheric emission lines.
8-‐ Stars with only V magnitude must be treated as unreddened O5 stars .
Adding a single color they may be treated as reddened O5’s. With 2 colors SpT and reddening can be determined. A reddened O5 has more flux than and unreddened star of the same color. Do not use BOT values which are approximate. Check against our screening limits.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 22
III. CS Reviews: Tasks
9-‐ Check BUFFER TIMES which depend on source count rate
-‐> general rule is: BT(APT) = 2/3 x BT(ETC) if BT(ETC)< Texp
= Texp if BT(ETC) > Texp
= 110s if BT(ETC) < Texp
For details: hbp://www.stsci.edu/hst/cos/documents/handbooks/current/ch05.COS_Spectroscopy05.html
10-‐ POS TARG, paberns, Mosaics increase the macro-‐aperture to screen.
ORIENTS reduced the area of concern. Note that the aperture orientaCon is updated to the scheduled value in APT/Aladin
11-‐ Moving target fields must be cleared when windows are determined. Targets of opportunity when acCvated (very rapid turnaround disallowed for BOP detectors)
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 23
III. CS Reviews: Tasks
12-‐ Coordinated parallels should have unique ORIENT. The specified parallel field is now properly screened and displayed by APT/BOT. Parallel STIS/MAMA imaging /grism
and all SBC are now excluded.
13-‐ Proper moCon to the midpoint of the cycle is now implemented (Cy19) as a selectable opCon in APT/BOT. There are 3 epochs involved, the correct field will be screened by BOT but the target locaCon relaCve to the field will be incorrect.
See: hbp://www.stsci.edu/hst/proposing/apt/old19_new_cycle_p2 item 9.
Note that POS TARG is disabled when proper moCon is acCvated.
14-‐ For procedures and requirements for observaCons of unpredictably variable objects such as CVs, see ACS ISR 2006-‐04. Such targets require real Cme confirmaCon of quiescence within 24h before BOP observaCons either ground or onboard.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 24
III. CS Reviews: Tasks
15-‐ Singe GS also increases the macro-‐aperture but won’t usually become known unCl
scheduling, so required further review later. The COS 7” or STIS 5” buffers must be increased to 50” in this case. (STIS ISR 2000-‐1). Review procedure is : create a LINE pabern with 5 points and spacing of 10” at 0 deg orientaCon in the POS TARG coordinate frame. Make the exposure in quesCon use that pabern and run BOT. As always be sure NOT to save any proposal changes . Single GS is disallowed for SNAPS.
16-‐ If the GO wishes to change their specificaCons azer the STScI BOP reviews are complete, they must submit a scienCfic jusCficaCon and new BOP reviews for consideraCon.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 25
III. CS Reviews: Tasks
1-‐ All ACQ exposures must be screened. Be careful to determine which configuraCon
produces the largest field.
2-‐ Nominal macro-‐aperture is 43” diameter circle, including both the PSA and BOA
(13.2” apart) with 7” buffers, but more criCcal area depends on which aperture is
acCve. BOT calculates corresponding throughput for each aperture and reports objects
in overlap region twice (BOA reports can be ignored).
3-‐ PSA buffer increases to 15” for very bright field objects that would produce: global rates greater than 1x10 5 cts/s/segment in FUV, 2x10 5 cts/s/stripe in NUV local rates greater than 3.3 cts/s/pix in FUV and 250 cts/s/pix in NUV.
Not implemented in BOT, but should be rare.
4-‐ Screening limits are in IHB Table 10.1 hbp://www.stsci.edu/hst/cos/documents/handbooks/current/ch10.Bright_obj3.html#408103
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 26
III. CS Reviews: Tasks
1-‐ ACQ use CCD and are not subject to BOP Review
2-‐ STIS macro-‐apertures vary widely from small echelle slits to direct imaging an slitless
spectroscopy. BOT checks the field to appropriate radius from target configuraCon and adds 5” buffer. All apertures are correctly displayed and screened by BOT. Note
STIS MAMA FOV is not displayed.
3-‐ The buffer increases to 13.5” for very bright field objects that would produce: global rate greater than 1.5x10
6 cts/s local rate greater than 500 cts/s/pix
Not implemented in BOT, but should be rare.
4-‐ NDQ filters have special problems described in IHB Fig 13.82
5-‐ Screening limits are in IHB Tables 7.8, 13.44 and 14.3
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 27
III. CS Reviews: Tasks
1-‐ Change/Add aperture, filter, graCng, wavelength, sexng, detector. DuplicaCon check is required (PC). ConfiguraCon changes may be approved by the CS Lead if no duplicaCons but Science instrument changes require TTRB approval.
CS never alters the Phase II proposal: make recommenda5ons to PI only
2-‐ Add POS-‐TARG and ORIENTS to avoid uncertain fields. Any unsafe or quesConable
target must be at least 7” (COS) or 5”( STIS) away from detector edge at all allowed
rolls. Beware of POS-‐TARG back toward STIS/FUV-‐MAMA repeller wire or too close to
detector edge.
3-‐ Change target if needed. Refer to Lead for approval or TTRB referral if scienCfic
objecCves may be altered. DuplicaCon checks need be done by PC again.
4-‐ Take preliminary observaCons with safe configuraCon. Must come out of allocated
Cme unless TTRB grants Cme increase (unlikely if not requested in phase I)
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 28
Final Remarks
-‐ Health and safety rules!
-‐ All and every doubts are to be cleared before allowing observaCons
-‐Work With GOs cooperaCvely on soluCons and alternaCves, but do not accept pressure!
-‐ Do not hesitate to bring problem cases to the abenCon of the User Support Lead/BOP Lead for resoluCon.
6/5/12 COS/STIS CS training -‐ P. Sonnentrucker 29