paucam.pic.es

PAUCam

Welcome to the PAUCam instrument website. PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg. FoV with 18 Hamamatsu photonics 4k x 2k, 15 um pixel CCDs. FOV 1 deg x 1 deg. Pixel Scale 0.265". 18 Hamamatsu Fully-Depleted 4K x 2K CCD detectors. Detectors gain: 0.6 - 0.7. Detectors dark current (@173K): 1 e. Detectors full well: 210000 e. Bias signal: 30k ADU. ADC range: 18 bits. Readout noise: 9 e. Readout time: 20 s.

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PAUCam | paucam.pic.es Reviews

<META> DESCRIPTION

Welcome to the PAUCam instrument website. PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg. FoV with 18 Hamamatsu photonics 4k x 2k, 15 um pixel CCDs. FOV 1 deg x 1 deg. Pixel Scale 0.265. 18 Hamamatsu Fully-Depleted 4K x 2K CCD detectors. Detectors gain: 0.6 - 0.7. Detectors dark current (@173K): 1 e. Detectors full well: 210000 e. Bias signal: 30k ADU. ADC range: 18 bits. Readout noise: 9 e. Readout time: 20 s.

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1 the instrument

2 filters

3 detectors

4 optics performance

5 press release

6 technical specifications summary

7 pix/h

8 coupons

9 reviews

10 scam

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PAUCam | paucam.pic.es Reviews

https://paucam.pic.es

Welcome to the PAUCam instrument website. PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg. FoV with 18 Hamamatsu photonics 4k x 2k, 15 um pixel CCDs. FOV 1 deg x 1 deg. Pixel Scale 0.265". 18 Hamamatsu Fully-Depleted 4K x 2K CCD detectors. Detectors gain: 0.6 - 0.7. Detectors dark current (@173K): 1 e. Detectors full well: 210000 e. Bias signal: 30k ADU. ADC range: 18 bits. Readout noise: 9 e. Readout time: 20 s.

INTERNAL PAGES

paucam.pic.es

1

PAUCam

http://paucam.pic.es/detectors.html

The focal plane is composed by a mosaic of 18 detectors. They are distributed and numbered as follows, as seen in the sky:. The orientation with respect to the WHT North and East is assuming a sky position angle of 0 deg. Detectors 12 and 17 might be dedicated for auto guiding. Quantum efficiency test performed in the optical bench in Barcelona automatically changing the monochromator wavelength, the grating turret, the pass-band filter and measuring simultaneously the signal of the reference photo-diode.

2

PAUCam

http://paucam.pic.es/index.html

Welcome to the PAUCam instrument website. PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg. FoV with 18 Hamamatsu photonics 4k x 2k, 15 um pixel CCDs. FOV 1 deg x 1 deg. Pixel Scale 0.265". 18 Hamamatsu Fully-Depleted 4K x 2K CCD detectors. Detectors gain: 0.6 - 0.7. Detectors dark current (@173K): 1 e. Detectors full well: 210000 e. Bias signal: 30k ADU. ADC range: 18 bits. Readout noise: 9 e. Readout time: 20 s.

3

PAUCam

http://paucam.pic.es/press_release.html

Galaxy M51, known as the Whirlpool galaxy, situated at about 23 million light years from Earth. (Image acquired June 6th, 2015). Galaxia M51, conocida como la galaxia del remolino, situada a unos 23 millones de años luz de la Tierra. (imagen captada el 6 de junio de 2015). Planetary nebula M27, known as the Dumbbell Nebula, situated in our own galaxy, the Milky Way, at a distance of about 1000 light years from Earth. (Image acquired June 3rd, 2015). Los 18 sensores CCD de PAUcam dan como resultado un amp...

4

PAUCam

http://paucam.pic.es/filters.html

Filter system and throughputs. The PAU Camera is equipped with a system of 40 narrow-band (13nm wide in steps of 10 nm) filters spanning the wavelength range from 450nm to 850nm, and with 6 wide-band filters (u, g, r, i, z, Y). Below we display the total system throughput including atmosphere, telescope, filter and detector:. You can download the total througput response for all 40 narrow bands and the 6 broad bands here. FT u (tray id 5). FT g (tray id 4). FT r (tray id 3). FT i (tray id 2).

5

PAUCam

http://paucam.pic.es/etc.html

2015 PAU CAMERA at the WHT.

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ice.cat

Tot a punt per estudiar l�energia fosca de l�Univers amb PAUCam | Not�cies - ICE - INSTITUT DE CI�NCIES DE L'ESPAI

http://www.ice.cat/view_new.php?NID=247

INSTITUT DE CINCIES DE L'ESPAI. Astropartcules i Objectes Compactes. Estrelles, Planetes and Meteorits. Fsica i Cosmologia Teorica. Astrofsica Nuclear i d'Altes Energies. Observaci de la Terra. Estudiants de Secundria i Grau. Info per a Extrangers. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Setmana de la Cincia. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Tot a punt per estudiar lenergia fosca de lUnivers amb PAUCam. El passat 3 de juny, PAUCam. Podr&agr...

hg.ice.csic.es

Tot a punt per estudiar l�energia fosca de l�Univers amb PAUCam | Not�cies - ICE - INSTITUT DE CI�NCIES DE L'ESPAI

http://hg.ice.csic.es/view_new.php?NID=247

INSTITUT DE CINCIES DE L'ESPAI. Astropartcules i Objectes Compactes. Estrelles, Planetes and Meteorits. Fsica i Cosmologia Teorica. Astrofsica Nuclear i d'Altes Energies. Observaci de la Terra. Estudiants de Secundria i Grau. Info per a Extrangers. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Setmana de la Cincia. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Tot a punt per estudiar lenergia fosca de lUnivers amb PAUCam. El passat 3 de juny, PAUCam. Podr&agr...

ieec.uab.es

Tot a punt per estudiar l�energia fosca de l�Univers amb PAUCam | Not�cies - ICE - INSTITUT DE CI�NCIES DE L'ESPAI

http://ieec.uab.es/view_new.php?NID=247

INSTITUT DE CINCIES DE L'ESPAI. Astropartcules i Objectes Compactes. Estrelles, Planetes and Meteorits. Fsica i Cosmologia Teorica. Astrofsica Nuclear i d'Altes Energies. Observaci de la Terra. Estudiants de Secundria i Grau. Info per a Extrangers. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Setmana de la Cincia. Info per a Agncies de Noticies. Departament de Comunicaci Cientfica. Tot a punt per estudiar lenergia fosca de lUnivers amb PAUCam. El passat 3 de juny, PAUCam. Podr&agr...

pic.es

PIC

http://www.pic.es/newsDetalle.gsp?id=26

Map and driving directions. PIC Tier-1 Blog @twitter. First light for the PAU camera, designed to study the dark energy in the Universe. The complexity of the PAU camera and the requirement for it to be installed on the primary focal point of the William Herschel telescope has required the development of a revolutionary carbon fiber structure, whose advanced engineering has been done in Spain. PAUcam is the only camera of its size in the world with a carbon fiber structure. Expectations and next steps.

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PAUCam

Welcome to the PAUCam instrument website. PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg. FoV with 18 Hamamatsu photonics 4k x 2k, 15 um pixel CCDs. FOV 1 deg x 1 deg. Pixel Scale 0.265". 18 Hamamatsu Fully-Depleted 4K x 2K CCD detectors. Detectors gain: 0.6 - 0.7. Detectors dark current (@173K): 1 e. Detectors full well: 210000 e. Bias signal: 30k ADU. ADC range: 18 bits. Readout noise: 9 e. Readout time: 20 s.

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