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GRACES 2015 Science Verification

Submitted by Anonymous on February 25, 2022
  • Read more about GRACES 2015 Science Verification

The following data was obtained during the Science Verification runs in 2015. Please feel free to download and use, as long as you mention the instrument and the software Opera which was used for the reduction.

CAUTION: Most of the spectra were obtained in the early phase of GRACES. The headers may not always be conform to the current standard.

Spectrophotometric standards

Target File of view Sample spectrum Data
Feige
  R.A.=12:37:23.55
  Dec.=25:04:00.3

GMOS-S still not available

Submitted by Anonymous on February 24, 2022
  • Read more about GMOS-S still not available

Besides the CCD2 problem reported on February 10th (which still persists), a detector translation assembly (DTA) fault occurred on Tuesday and the mechanism is stil not working. As a consequence, GMOS is still not available un the queue.

GS Telescope shutdown on February 21st due to P2WFS repairs

Submitted by frantaky on February 15, 2022
  • Read more about GS Telescope shutdown on February 21st due to P2WFS repairs

It has been found after extensive troubleshooting that the Peripheral Wave Front Sensor 2 (P2WFS) has a mechanical issue and is out of order. To address this issue the P2WFS will have to be replaced in the telescope by a dummy unit while it is being repaired. We are planning for this intervention starting Monday February 21st and the removal and installation of the dummy unit will take two days and thus the telescope will not be available from the Night February 21st to 22nd.

GMOS-S unavailable

Submitted by ggimeno on February 10, 2022
  • Read more about GMOS-S unavailable

GMOS-S is unavailable due to the re-appearance of the CTE problem on CCD1, plus high noise structure on CCD2. Troubleshooting started on Monday and is currently ongoing.

GMOS-S unavailable

Submitted by Anonymous on February 10, 2022
  • Read more about GMOS-S unavailable

GMOS-S is unavailable due to the re-appearance of the CTE problem on CCD1, plus high noise structure on CCD2. Troubleshooting started on Monday and is currently ongoing.

GPI 2.0

Submitted by Anonymous on February 3, 2022
  • Read more about GPI 2.0

Latest News

October 2024

  • TC integration efforts by the NRC-HAA team commenced.

May 2024

  • The new GPI 2.0 pyramid wavefront sensor was installed on the GPI 2.0 AO bench

June 2023 

  • Old adaptive optic was removed by UCSD team at UND facilities.

May 2022

NIFS Temporarily Unavailable at Gemini North

Submitted by sleggett on January 24, 2022
  • Read more about NIFS Temporarily Unavailable at Gemini North

NIFS is temporarily unavailable at Gemini North. The cold head is being exchanged because the instrument was not holding temperature. We expect the instrument to be available again during the week of January 31.

Gemini North Observatory Operations Update

Submitted by sleggett on January 24, 2022
  • Read more about Gemini North Observatory Operations Update

The Gemini North secondary mirror xy positioner was successfully datumed on Friday, 21 January 2022. Fine tuning of the mirror alignment is awaiting good natural seeing, in the meantime the elevation restriction on targets has been removed.

Gemini North Observatory Restricted Operations

Submitted by sleggett on January 6, 2022
  • Read more about Gemini North Observatory Restricted Operations

The secondary mirror of Gemini North Observatory has had a non-functional xy positioner since Tuesday January 4, 2022. Troubleshooting actively continues, however the fault remains unresolved. On the night of Friday January 7, 2022, we started taking data for programs that can handle poor seeing, with targets that reach an elevation greater than 55 degrees. The lack of the xy positioner introduces coma into the images, which is worse at lower elevations. At the higher elevations the coma tail extends about 2 arcseconds, with an average delivered IQ of about IQ85.

New Gemini Observatory Agreement Signed

Submitted by xzhang on January 4, 2022
  • Read more about New Gemini Observatory Agreement Signed

Multinational agreement extends operations of the international Gemini Observatory through 2027.

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International Gemini Observatory

The International Gemini Observatory  provides the astronomical communities in six participant countries with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. In addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the Canadian National Research Council (NRC), the Chilean Agencia Nacional de Investigación y Desarrollo (ANID), the Brazilian Ministério da Ciência, Tecnologia e Inovação, the Argentinean Ministerio de Ciencia, Tecnología e Innovación, and the Korea Astronomy and Space Institute (KASI). The observatory is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.     


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