... NICMOS Proposing Example - 5 . ... Phase I Proposing . ... Real_Time_Justification: Calibration_Justification: Additional_ Comments : Fixed_Targets Target_Number: 1 Target_Name : HDF Alternate_Names: Hubble Deep Field Description: GALAXY,PROTOGALAXY Position: RA=12H 36M 49.40S +/- 0.02S,DEC=62D 10' 58.0 ...

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• GHRS Instrument Handbook
• NICMOS Proposing Example - 7
• NICMOS Proposing Example - 1

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...

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• A Test for Weak Cosmic Ray Events on CCD Exposures
• Zero-Points of FOS Wavelength Scales

Star formation is often best manifested by bright H II regions.These are regions of hydrogen which have been ionized by ultraviolet photons which are emitted from massive stars (typically stars more than 20 times the mass of the Sun). ... A narrowband filter image centered on this wavelength will then readily reveal these H II regions and hence the current sites of star formation in a galaxy, The luminous blobs that can be seen here are all H II regions . ... NGC 3558 Visual . NGC 3558 Infrared . ...

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• Astro-2 and the UIT Experiment
• CCD Astronomy Magazine Article Page 5
• Galaxy Gallery Page II

... Original: 1984x1488 (612k) . Medium: 800x600 (76k) . Thumbnail: 200x150 (16k) . Flash: Flash fired . Exposure time: 1/30s . Focal length: 6.4mm . Aperture: f/2.8 . ... Original: 1984x1488 (680k) . Medium: 800x600 (116k) . Thumbnail: 200x150 (18k) . Flash: Flash did not fire . ... Original: 1984x1488 (659k) . ... Exposure time: 1/60s . ... Focal length: 6.9mm . ... Focal length: 17.1mm . ... Focal length: 25.7mm . ... Focal length: 33.8mm . ... Focal length: 24.6mm . ...

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NCA response to NCRIS Page 1 of 2 9 December 2006 NCA response to Exposure Draft of NCRIS Strategic Roadmap The National infrastructure Roadmap. It informed the Committee for Astronomy (NCA) welcomes the support for the astronomy identified by the NCRIS committee in the Exposure Draft of the Strategic is pleased to note the extent to which the Astronomy Decadal Plan has NCRIS committee in their deliberations. ... Section 7) as one of three high-priority `Landmark' facilities1. ...

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• Info for image: DSC01229.JPG (9/29)
• Info for image: dsc00228.jpg (8/9)
• Info for image: dsc00224.jpg (4/9)

... hkgtigen (hkgtigen-1.14.2) [xmmsas_20060628_1801-7.0.0] . ... This does not exclude the possibility to apply this GTI data set to single-exposure event lists. ... For doing this, please construct the GTI sets for all desired instruments (e.g. gti_om.ds , gti_emos1.ds , gti_sc.ds ) and combine them in the selection expression that drives the filtering process in task evselect : evselect table=ev.ds expression="TIME in gti(gti_emos1.ds) && \ TIME in gti(gti_om.ds) && TIME in gti(gti_sc.ds)" .. ...

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• Exposure Record

by I.M. Chertok, V.V. Fomichev, A.A. Gnezdilov, R.V. Gorgutsa, V.V. Grechnev, A.K. Markeev, R.W. Nightingale, and D.E. Sobolev . Fig. 2. Inverted TRACE images at 195 illustrating development of the EUV post-eruption arcade with the well-organized loop, two-ribbon, and spine structures. Note that the exposures have been rescaled to the same peak intensity to show the evolution of the bright elements. The field of view is 220.5 by 182 Mm. Back to paper .

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05/10/2007 1:01 PM . ... Original: 1936x1296 (418k) . ... Thumbnail: 200x134 (68k) . Flash: Flash fired, auto mode, return light detected . Exposure time: 10/2000s . Focal length: 18.0mm . Aperture: f/8 . ... Original: 1936x1296 (314k) . ... Thumbnail: 200x134 (69k) . Flash: Flash did not fire . Exposure time: 10/1600s . ... Original: 1936x1296 (388k) . ... Flash: Flash did not fire, auto mode . ... Focal length: 7.9mm . ... Focal length: 13.7mm . ... Focal length: 6.3mm . ...

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APO has implemented a prototype guide camera for the 0.5-m Telescope. ... Guiding will continue unless a guide star is lost (clouds, high background from moon or twilight, or the telescope is slewed to another field). ... ACP maintains the guiding for the same field and will not re-acquire a guide star unless the field moves (example excessive tracking jumps) or ACP needs to re-center the object. ... The prototype guider is in shared-risk mode. ...

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• Old Calibration Data
• TUI:Instruments:Expose Window
• Suggested Exposure Times For Calibration Spectra

IBIS - The Interferometric BIdimensional Spectrometer . The I nterferometric BI dimensional S pectrometer (IBIS) is a next generation bidimensional spectrometry instrument based on a dual Fabry-Perot interferometric system. ... This will allow it to address a variety of observational programs in solar physics. ... Cavallini, F., Berrilli, F., Cantarano, S., Egidi, A. and Baffa, C.: 1999, IBIS: A New Instrument for Solar Bidimensional Spectroscopy , JOSO Annual Report 1999 , 29 , p. 99 . ...

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• Arcetri Star-Formation Group Publications
• CHIANTI atomic database
• Fasti Talk Slide 5

Next: List of Tables Up: No Title Previous: Contents . A dark current CCD exposure with cosmic ray events which are removed with non--linear filters. A) original, (B) 5*5 median filter, (C) 5*1 median filter, and (D) 5*1 recursive filter. Removal of cosmic ray events on a CCD spectral exposure with different techniques: (A) original, (B) median filter, (C) recursive filter and (D) stack comparison. ... Images RINGS and OFFRINGS. ... This image is obtained by the command visual/cube . ...

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• Input Data and Preprocessing
• Association of Calibration Exposures
• An example of selection criteria

... An exposure map is provided for each ROSAT field (e.g., rp110590_mex.imh). The simplest method of applying an exposure correction is to divide the data by the exposure map yielding a count rate image. The image must first be blocked to the same size as the exposure map, e.g., for ROSAT PSPC. xi> imcalc input file (`-' for STDIN) or imcalc commands () : - # interactive mode IMC > ctrate.imh = ``xdata$rp110590.qp[bl=30]'' / ``xdata$rp110590_mex.imh'' IMC > quit . ...

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• Chandra Images for G000.1-00.1
• Chandra Images for SNR G292.0+1.8
• Chandra Images for G111.7-02.1

... This 10 min exposure shows star trails clearlтАж . Sidebar Left . ... Title: This 10 min exposure shows star trails clearly defining the south celestial pole just left of centre. Description: The Large and Small Magellanic Clouds are on the left and the Milky Way from Crux through Centaurus are on the right. ... This 10 min exposure shows star trails clearly defining the south celestial pole just left of centre. ...

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• Proposed Facility
• C/2011 W3 (Lovejoy)

... Retired ETCs . Historic ETC versions: select.. P93 phase 1 (Sep.2013) P93 phase 2 (Dec.2013) P94 phase 1 (Mar.2014) P94 phase 2 (Jun.2014) P95 phase 1 (Sep.2014) P95 phase 2 (Dec.2014) P96 phase 1 (Mar.2015) P96 phase 2 (Jun.2015) P97 phase 1 (Sep.2015) P97 phase 2 (Dec.2015) . SkyCalc Sky Model Calculator . ... MUSE ETC: New seeing/IQ PSF model . ... VISIR imaging ETC: Updated sensitivity model . ... GIRAFFE, VIMOS IFU,MOS and EFOSC2 spectroscopy: . ... Paranal UT1 . ... E-ELT . ...

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• Homepages of Christian A. Hummel
• HAWK-I Exposure Time Calculator
• ESO - Why do the flats in my data have different exposure times and how do I

... A 212 Hour Exposure of Orion . ... It is a direction in space that is rich with impressive nebulas. ... The bright orange star just above the frame center is Betelgeuse , while the bright blue star on the lower right is Rigel . ... About those famous three stars that cross the belt of Orion the Hunter -- in this busy frame they can be hard to locate, but a discerning eye will find them just below and to the right of the image center. ... Publications with keywords: Orion - deep field . ...

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• A Lunar Eclipse in Three Exposures
• Астронет > A Lunar Eclipse in Three Exposures
• Астронет > A 212 Hour Exposure of Orion

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2015 November 23 . A 212-Hour Exposure of Orion . ... It is a direction in space that is rich with impressive nebulas. ... After 212 hours of camera time and an additional year of processing, the featured 1400-exposure collage spanning over 40 times the angular diameter of the Moon emerged. ... About APOD | ...

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• APOD: 2000 January 25 - A Lunar Eclipse in Three Exposures
• APOD: May 30, 1997 - A Cosmic Snowball
• APOD: 2006 September 1 - Gemini South Star Trails

. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 23/08 Ryoanji Temple and around . Up . << Prev . In the forest, on the hill near the temple. Too dark. wrong exposure. Next >> . Created with the tool album script from Marginal Hacks by David on Tue Jun 23 14:46:19 2015 .

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• Image: Wrong exposure.
• Image: Kyoto tonight. Distorted due to large exposure without mounting.

Next: Results & Discussion Up: Coronal Hole Diagnostics out Previous: Introduction . ... The dates of the observations discussed here, their locations, pointing, slit sizes and exposure times are given in BTDW. ... Line fits are given by the dotted line. ... An estimation of the errors in the derived parameters was obtained using the GA-derived parameters as an input for a ``classical'' IDL-CURVEFIT procedure (Peter, 1999; Peter & Judge, 1999). ...

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• Armagh Observatory
• SCL Sfit Commands
• Climatology

Proposal Identi cation No.: R1154 Date Received: 1998-May-29 10:33:43 Technical Page Proposal Type: Regular General Category: Planetary Radar Observation Category: Solar System Total Time Requested: 32 Hours Proposal Title: S-Band Bistatic Radar Observations of Titan in 1998 ABSTRACT: We are proposing new observations to measure Titan's radar cross section at a wavelength of 12.6 cm. ... Maybe Part of the observing run. ...

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• How to Propose
• Proposed E-ALFA Organizational Structure