NICMOS STScI Analysis Newsletter 22 May 2000 CONTENTS: - NICMOS NEWS + New NICMOS Exposure Time Calculator + Synthetic Darks for NIC1 - RELEASE OF THE VISUAL TARGET TUNER - RECENT PREPRINTS - APPENDIX: NICMOS CONTACTS ============================================================================ NICMOS NEWS ----------- New NICMOS Exposure Time Calculator ----------------------------------- Anand Sivaramakrishnan During cryocooler operation of NICMOS (cycle 10), the detectors in the camera will operate at significantly higher temperatures than during the previous cycles when the detector was cooled with solid nitrogen. This difference in operating temperature affects dark current adversely, but improves the quantum efficiency (QE) of the NICMOS detectors. A new exposure time calculator (ETC) which incorporates the detector behavior observed during the 'end of life' warm-up of NICMOS is now available. This ETC has a reworked thermal model for the HST OTA and NICMOS optics. It also incorporates effects of cold pupil decentering and its concomitant slight increase in thermal background in the longest wavelength NICMOS bandpasses. The dominant sources of thermal background in these filters are still the primary and secondary mirrors. The ETC uses the STSDAS.SYNPHOT.COUNTRATE task as its throughput machine, and throughput and quantum efficiency files from the Institute's Calibration Data Base System (CDBS). The ETC will soon be available at http://www.stsci.edu/instruments/nicmos/NICMOS_tools/nicmos_tools.html The NICMOS ISR 00-001 describes the ETC in more detail. Synthetic Darks for NIC1 ------------------------ Brian Monroe The NICMOS Synthetic Dark web tool http://www.stsci.edu/instruments/nicmos/NICMOS_tools/syndark.html now supports multiaccum darks for camera 1. The magnitude of the shading error is not as big as in camera 2, so visible improvements might not be as obvious. However, pixel-to-pixel noise has been greatly reduced, so it is still worth recalibrating. ============================================================================= Release of the Visual Target Tuner ---------------------------------- Steve Lubow With the June Call for Proposals, STScI will release a prototype software tool called the Visual Target Tuner (VTT). The VTT was originally developed as a proof of concept by a collaborating team from NASA Goddard and STScI (aaaprod.gsfc.nasa.gov/SEA). This tool displays HST apertures superimposed on sky images. The VTT provides capabilities to import sky images, display primary and parallel apertures, rotate apertures, centroid objects, specify excluded points and regions, experiment with various orientations, and display catalog overlays and object information. The tool can be useful for either Phase 1 or Phase 2 of HST proposal preparation, although its main use is likely to be for Phase 2. In Phase 1, the tool can be used to answer questions such as: How many fields will I need to mosaic my extended target? Which of my potential targets "fits best" in the aperture? Is there anything interesting I can pick up with a coordinated parallel in another aperture? Do any of my potential targets have nearby bright objects that could spoil the observation? Is there an orientation which would avoid the bright object? (Note: this VTT release does not incorporate moving target capabilities.) The VTT is supported for use on the Solaris and Windows operating systems. Further information about this tool will be available on the "Proposing to Use HST" web page (www.stsci.edu/observing/proposing.html) If you think you would benefit from a tool like this in either Phase 1 or Phase 2 we encourage you to download and try the software. The feedback we receive this summer will play a role in determining our priorities for the Phase 2 release in December. ============================================================================= RECENT PREPRINTS ---------------- We draw your attention to these papers, based on NICMOS data, that will appear in the next few months. This list includes all preprints received by the STScI Library not yet published in the journals. Please remember to include our Library in your preprint distribution list. DICKINSON, M. "Galaxy Evolution at 0 < z < 2 from the NICMOS HDF-North," XIXth Moriond Astrophysics Meeting. DICKINSON, M. "The First Galaxies: Structure and Stellar Populations" Phil. Trans. Royal Soc. A LUHMAN, K.L.; RIEKE, G.H.; YOUNG, E.T.; COTERA, A.S.; CHEN, H.; RIEKE, M.J.; SCHNEIDER, G.; THOMPSON, R.I. "The Initial Mass Function of Low-Mass Stars and Brown Dwarfs in Young Clusters" ApJ accepted CHARY, R.; BECKLIN, E.E.; EVANS, A.S.; NEUGEBAUER, G.; SCOVILLE, N.Z.; MATTHEWS, K.; RESSLER, M.E. "High Resolution Infrared Imaging of the Compact Nuclear Source in NGC 4258" ApJ 3-10-00 DAYAL, A.; LATTER, W.B.; BIEGING, J.; MEAKIN, C.; KELLY, D.M.; HORA, J.L.; TIELENS, A.G.G.M. "HST/NICMOS Observations of the Planetary Nebula NGC 7027" Asymmetrical Planetary Nebulae II HORA, J.L.; LATTER, W.B.; DAYAL, A.; BIEGING, J.; KELLY, D.M.; TIELENS, A.G.G.M.; TRAMMELL, S.R. "HST/NICMOS Imaging of the Planetary Nebula Hubble 12" Asymmetrical Planetary Nebulae II LATTER, W.B.; DAYAL, A.; BIEGING, J.H.; KELLY, D.M.; HORA, J.L.; TIELENS, A.G.G.M. "HST/NICMOS Imaging of the Planetary Nebulae BD+30 degrees 3639" Asymmetrical Planetary Nebulae II LATTER, W.B.; DAYAL, A.; BIEGING, J.H.; MEAKIN, C.; HORA, J.L.; KELLY, D.M.; TIELENS, A.G.G.M. "Revealing the Photodissociation Region: Hubble Space Telescope/NICMOS Imaging of NGC 7027" ApJ accepted QUILLEN, A.C.; BOWER, G.A.; STRITZINGER, M. "A NICMOS Survey of Early-Type Galaxy Centers: the Relation Between Core Properties, Gas and Dust Content and Environment" ApJS accepted QUILLEN, A.C.; SHAKED, S.; ALONSO-HERRERO, A.; MCDONALD, C.; LEE, A.; RIEKE, M.J.; RIEKE, G.H. "The Variability of Seyfert 1.8 and 1.9 Galaxies at 1.6 Microns" ApJ 532: L17-L20, 2000 http://www.journals.uchicago.edu/cgi-bin/resolve?ApJv553pL17 BIEGING, J.H.; MEAKIN, C.A.; KELLY, D.M.; DAYAL, A.; LATTER, W.B.; HORA, J.L.; TIELENS, A.G.G.M. "HST/NICMOS Near-IR Imaging of the Proto-Planetary Nebula OH 231.8+4.2" Asymmetrical Planetary Nebulae 2: ZEPF, S.; LIU, M.C.; MARLEAU, F.R.; SACKETT, P.D.; GRAHAM, J.R. "The Stellar Content of the Halo NGC 5907 from Deep HST NICMOS Imaging" AJ accepted ============================================================================ APPENDIX: NICMOS Contacts ------------------------- Analysis, STSDAS or any other HST-related questions can be addressed to help@stsci.edu. ============================================================================ To subscribe or unsubscribe send a message to majordomo@stsci.edu with the Subject: line blank and the following in the body: [un]subscribe nicmos_news ============================================================================ Comments, questions, suggestions, etc. can be e-mailed to help@stsci.edu. ============================================================================ The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. ============================================================================