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The Hubble Space Telescope data

Automation of Hubble Space Telescope Mission Operations

Automation of Hubble Space Telescope Mission Operations

... This required the automation of routine mission operations induding telemetry and forward link acquisition, data dumping and solid-state recorder management, stored comman[r] ...

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Hubble Space Telescope Primer for Cycle 24

Hubble Space Telescope Primer for Cycle 24

... Users should note, however, that for these modes, the focus values have been set to optimize the resolution over a limited part of their wavelength range (see Figure 4.1). The resolution values quoted here are based on ...

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Searching for High-redshift Galaxies in Hubble Space Telescope Deep Data

Searching for High-redshift Galaxies in Hubble Space Telescope Deep Data

... advanced data reduction to get an improved version of the deepest image of the Universe currently available, the so called eXtreme Deep Field ...ACS data, including the minor ones such as the herring- bone ...

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SPIKE: Intelligent Scheduling of Hubble Space Telescope Observations

SPIKE: Intelligent Scheduling of Hubble Space Telescope Observations

... approach is that once the prototype is used operationally, it becomes increasingly difficult to make large changes to it. (In an ideal rapid prototyping situation, a prototype can be dis- carded after evaluation). Once ...

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Phase-resolved Hubble Space Telescope ultraviolet spectroscopy

Phase-resolved Hubble Space Telescope ultraviolet spectroscopy

... A caveat to this discussion arises if there is magnetic coupling between the stars. Recent work examining the relation between the orbital and spin periods in the intermediate polar EX Hya (King & Wynn 1998) shows that a ...

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A Hubble Space Telescope transit light curve for GJ 436b

A Hubble Space Telescope transit light curve for GJ 436b

... visit data sets separately to determine the corresponding individual transit ...visit data sets that are sensitive to the transit time us- ing a Levenberg-Marquardt ...30 data points with replace- ...

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A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae

A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae

... AC K N OW L E D G E M E N T S CRA acknowledges receipt of a studentship from the Midlands Physics Alliance. AJL thanks STFC for support under grant ID ST/I001719/1, and the Leverhulme Trust for support via a Philip ...

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A Hubble Space Telescope survey of the host galaxies of superluminous supernovae

A Hubble Space Telescope survey of the host galaxies of superluminous supernovae

... Herschel Telescope (WHT) and the Very Large Telescope ...UV data set, images are subject to greater charge transfer efficiency (CTE) losses, which arise due to inef- ficient transfer of charge ...

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Answers for the Student Worksheet for the Hubble Space Telescope Scavenger Hunt

Answers for the Student Worksheet for the Hubble Space Telescope Scavenger Hunt

... Hubbleʼs constant Telescope's crisp view along with 2003 data from NASA's Wilkinson Microwave Anisotropy Probe to refine the value of the universe's expansion rate to three percent. What does this new value imply ...

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A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search*

A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search*

... large Hubble Space Telescope project to observe a significant ( ∼ 34,000) ensemble of main-sequence stars in the globular cluster 47 Tucanae with a goal of defining the frequency of inner orbit, gas ...

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Hubble space telescope parallaxes of AM CVn stars and astrophysical consequences

Hubble space telescope parallaxes of AM CVn stars and astrophysical consequences

... AND DATA REDUCTION Ten sets of astrometric data were acquired with the Fine Guidance Sensors on board HST for each of our five science ...complete data aggregate spans ...The data were reduced ...

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A multi-wavelength, Hubble space telescope study of two globular clusters

A multi-wavelength, Hubble space telescope study of two globular clusters

... The ACS has a large field of view, at 202 ′′ ×202 ′′ , and a plate scale of 0. ′′ 05/pixel, while the WFC3 has a slightly smaller field of view of 162 ′′ ×162 ′′ , but a finer plate scale of 0. ′′ 04/pixel (see Appendix ...

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THE DISCOVERY OF CEPHEIDS AND A NEW DISTANCE TO NGC 2841 USING THE HUBBLE SPACE TELESCOPE

THE DISCOVERY OF CEPHEIDS AND A NEW DISTANCE TO NGC 2841 USING THE HUBBLE SPACE TELESCOPE

... the data to re- ject anomalous photometric measurements, most of them associated with cosmic-ray hits, and the light curve was analyzed ...individual data points were rejected in this ...

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A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope

A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope

... 12 http://archive.stsci.edu 13 http://irsa.ipac.caltech.edu/data/COSMOS/images/ acs_mosaic_2.0/tiles/ of the 8 exposures from the commanded pointing position. Generally, the relative pointing accuracy of HST is ...

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Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

... Abstract We present the first comparison of Jupiter’s auroral morphology with an extended, con- tinuous and complete set of near-Jupiter interplanetary data, revealing the response of Jupiter’s auroras to the ...

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Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

... 3. Results The data discussed in section 2 are plotted in Figure 1, while selected representative HST images are shown in Figure 2. We first note from Figure 1a that the viewing geometry-corrected UV powers ...

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Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies

Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies

... Because the dark burst sample size is modest, and Chandra determined positions typically have larger positional uncertainties, we consider the effect of including additional optically or NIR detected dark GRBs in the ...

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A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

... None were found. In between sky lines, our spectra are sensitive to emission line fl uxes of ∼ 2 – 4 × 10 − 17 erg s − 1 cm 2 ( 5 σ) . These observations therefore already provided some evidence against Figure 8. 1D ...

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Evidence for Type Ia Supernova Diversity from Ultraviolet Observations with the Hubble Space Telescope

Evidence for Type Ia Supernova Diversity from Ultraviolet Observations with the Hubble Space Telescope

... We note that the F UV /F opt value of SN 2006X peaks at t ≈ 10 days before the B-band maximum, about 5 days earlier than for SN 2005cf and the templates. This feature is similarly observed in the fast-decliner SN 2005ke, ...

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A REMARKABLY LUMINOUS GALAXY AT Z = 11.1 MEASURED WITH HUBBLE SPACE TELESCOPE GRISM SPECTROSCOPY

A REMARKABLY LUMINOUS GALAXY AT Z = 11.1 MEASURED WITH HUBBLE SPACE TELESCOPE GRISM SPECTROSCOPY

... present Hubble WFC3/IR slitless grism spectra of a remarkably bright z & 10 galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging ...grism data, combined with the pho- tometric ...

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