The Observatorio Astrofísico de Javalambre (OAJ) has announced the call for proposals for observing in the first semester of 2025 with T80Cam, the scientific, panoramic camera installed at JAST80. The call corresponds to the Open Time that OAJ offers regularly to the astronomical community as national Unique Scientific and Technical Infrastructure (ICTS).
Linking Javalambre and SKA Observatories in Cosmos exploration
2023-11-28 11:00
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CEFCA scientists discover a supernova named JVAR21a
2022-04-21 14:00
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CEFCA announces worldwide open access to the Early Data Release (EDR) of the Javalambre Photometric Local Universe Survey. This EDR consists of 18 J-PLUS pointings at different locations of the sky, observed in the twelve J-PLUS photometric optical bands, overall amounting to 36deg2. We provide access to the J-PLUS catalogues with photometric data in all the twelve bands for more than 400.000 astronomical objects, together with the actual FITS images and proper masks to avoid bright stars and other undesired areas.
The J-PAS Pathfinder camera of the Javalambre Survey Telescope (JST250) received its first light on the night of 20th February, obtaining succesfully an image of the open cluster NGC1960. After the commissioning of the instrument, the Unique Scientific and Technical Infrastructure (ICTS, in their Spanish initials) Observatorio Astrofísico de Javalambre is working at full capacity, operating routinely the two main telescopes with first-level scientific instrumentation.
A collaboration agreement between the Euclid Consortium of the European Space Agency (ESA)-led space mission Euclid- and the Centro de Estudios de Física del Cosmos de Aragón (CEFCA; Teruel) has been signed for the provision of ground based scientific data with the Observatorio Astrofísico de Javalambre to complement the observations of the Euclid space telescope.
The aluminizing vacuum chamber and the cleaning unit for the maintenance of JST250 and JAST80 telescope's mirrors arrived yesterday at the Observatorio Astrofísico de Javalambre (OAJ). The chamber has been designed by CEFCA and Vacuum Technology Associates Inc, DYNAVAC (Boston, United States), responsible for its manufacture.
Optical fine tuning of the system during Final Acceptance tests provides images of 0.15” FWHM using “lucky imaging” techniques
CEFCA has proceeded with the final acceptance of the JST250 telescope installed at the Observatorio Astrofísico de Javalambre after carrying out additional tests with the verification camera in order to test proper operation of the telescope.
The OAJ already keeps the actuator system of JPCam in its clean room. After its arrival in mid January, the engineering team has carried out the integration of the system at the observatory in order to start with the verification and fine-tune processes, first in the clean room and, finally, in the JST250 telescope.
After an intense period of fine tuning and optimization tasks developed by the OAJ/CEFCA Team, systematic observations with T80Cam@JAST80 have started. The telescope–camera system is in optimal performance, reaching normally seeing-limited images. So far, a best gaussian FWHM of 0.63”(+/-0.09”) over the 2deg2 focal plane of T80Cam has been recorded.
Achieved images of 0.33” PSF with “lucky imaging” techniques
Last September 2015, the JST250 telescope at the Observatorio Astrofísico de Javalambre passed successfully the Provisional Acceptance test review. This milestone represents a big step forward for the completion of the project, only pending the Final Acceptance tests that shall be completed in the next weeks.
During the last months has been carried out the installation process of the main storage and processing systems for the UPAD/T250. The infrastructure has been provided and installed by the companies Bull España S.A. and Fujitsu Technologies Solutions S.A. These systems increase the already existing capabilities of the UPAD/T80 in order to deal with the huge amount of data produced by JPCam once the camera is installed at JST250 telescope.
With the successful achievement of this important milestone, e2v has demonstrated that the focal plane is well within the very strict JPCam requirements. The JPCam engineering focal plane has been successfully integrated at e2v (Chelmsford, UK). JPCam, the main scientific instrument of the JST250 telescope, is a 1.2 Gpixel camera designed to perform the J-PAS survey.
T80Cam, the scientific camera of the JAST80 telescope of the Observatorio Astrofísico de Javalambre (CEFCA's observatory), has taken its first image of the Javalambre night sky. This achievement is known as First Light, as this is the first time that light coming from an astronomical object is registered by the T80Cam detector.
J-PLUS filters have been received and accepted at CEFCA headquarters (Teruel).
The filters have been manufactured by SCHOTT (Yverdon-les-Bains, Switzerland). These have been specifically developed for the J-PLUS survey and have required more than two years of research and development effort both from SCHOTT and CEFCA.
In September 25th, at 22:57h Local Time, the Javalambre Survey Telescope (JST250) achieved engineering first light. This is a very important milestone in the project since it is the first time that photons from the Universe, in this case coming from the Polaris star, have gone through the complete optical system of the telescope as it was designed.
JST / T250 telescope of the Observatorio Astrofísico de Javalambre (OAJ) was completely integrated on September 2, 2014. The integration of the telescope with the final optical elements was made after a previous test phase in which the mechanical and control parts of the telescope were verified with dummies instead of the real optical elements.
Last week, CEFCA engineers moved to the Belgian company AMOS headquarters to discuss the final details of the final version of the control software of the telescope JST / T250. After the meetings, in which members of AMOS and of OSL company have participated, CEFCA engineers have given approval for the finalization of the software, which will be delivered to CEFCA in a few weeks.
Last February, the factory integration phase of the JAST80 telescope of the Observatorio Astrofísico de Javalambre (CEFCA) was completed. The telescope is assembled at Bamberg (Germany) where it is currently being tested with dummy optics. Preliminary tests show that the telescope can move with a velocity of up to 40 degrees per second, which makes T80 one of the worldwide fastest telescopes.
In early December, and after an international process of peer review, Brazil’s Observatório Nacional, a partner institution in the Javalambre Physics of the Accelerated Universe Astrophysical Survey collaboration (J-PAS), and British company E2V signed a contract to provide the cryogenic camera system for the JST250 telescope of the Observatorio Astrofísico de Javalambre.
Towards the end of October, AMOS, the Belgian company responsible for the construction of the telescopes for the Observatorio Astrofísico de Javalambre (OAJ), started the manufacturing of the main mechanical parts of the JST250. The construction of the telescope, to be installed at the OAJ by mid 2012, is currently on schedule and its main structure is expected to be erected at the Belgian plant by January.
The brazilian partners of the Javalambre Physics of the Accelerated Universe Astrophysical Survey (J-PAS) collaboration, will put an identical replica of the OAJ JAST80 telescope of the Observatorio Astrofísico de Javalambre (CEFCA's observatory) in the Cerro Tololo Inter-American Observatory (CTIO), in Chile.
The Final Design Review of the JST250, the main telescope which will be instaled at the Observatorio Astrofísico de Javalambre, has been held at the new headquarters of the CEFCA during March 3rd and 4th. thickness of 250 mm. The inner hole, necessary for the light beam reaching the Cassegrain focus after being reflected in the secondary mirror, has a diameter of nearly 1010 mm.
In December 15th, CEFCA personnel visited AMOS headquarters in Liege (Belgium) to attend the Design Review meeting of the Javalambre JAST80 telescope. During this visit they had the opportunity to see in situ, at AMOS shops, the progress in the grinding and polishing processes of the two primary mirrors of the OAJ telescopes.
The M1 blank has been manufactured by the german company SCHOTT AG. It is made of ZERODUR, a glass ceramic with nearly null thermal expansion, commonly used for telescope mirrors and other engineering projects which require of using high accuracy not deformable surfaces. It weights 2366 kg and has an outer diameter of 2640 mm.