North Eclíptico Pole Time Dominio Campo

North Eclíptico Pole Time Dominio Campo

Una franja de cielo que mide el 2% del área cubierta por la luna llena fue fotografiada con la cámara de infrarrojo cercano de Webb (NIRCAM) en ocho filtros y con la cámara avanzada de Hubble para encuestas (AC) y la cámara 3 de campo ancho (WFC3) en tres filtros que juntos abarcan el rango de longitud de ola 0.25-5 micras. Esta imagen representa una parte del campo de perlas completa, que será aproximadamente cuatro veces más grande. Miles de galaxias en un rango enorme en la distancia y el tiempo se ven con exquisito detalle, muchas por primera vez. La luz de las galaxias más distantes ha viajado casi 13.5 mil millones de años para llegar a nosotros. Debido a que esta imagen es una combinación de múltiples exposiciones, algunas estrellas muestran picos de difracción adicionales. Esta imagen de color representativo se creó utilizando filtros Hubble F275W (Purple), F435W (azul) y F606W (azul); y filtros Webb F090W (CYAN), F115W (verde), F150W (verde), F200W (verde), F277W (amarillo), F356W (amarillo), F410m (naranja) y F444W (rojo).

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ESA, CSA, Rolf A. Jansen (ASU), Jake Summers (ASU), Rosalia O'Brien (ASU), Rogier Windhorst (ASU), Aaron Robotham (UWA), Anton M. Koekemoer (STSCI), Christopher Willmer (Universidad de Arizona), JWST Pearls Team

IGELO

Rolf A. Jansen (ASU), Alyssa Pagan (Stsci)

About The Object
Object Name North Ecliptic Pole (NEP), PEARLS
Object Description Deep Survey
R.A. Position 17:22:47.90
Dec. Position +65:49:21.54
Constellation Draco
About The Data
Data Description This image was created with Webb data from proposal: (R. A. Windhorst) and Hubble data from proposals: , , and (R. A. Jansen)         
Instrument Hubble> ACS/WFC, WFC3/UVIS Webb> NIRCam
Exposure Dates 26 Aug 2022, 14 Sept 2022 (Webb)
Filters Hubble> F275W, F435W, F606W Webb> F090W, F115W, F150W, F200W, F277W, F356W, F410M, F444W
About The Image
Color Info These images are a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam instrument and the Hubble Space Telescope using the ACS/WFC and UVIS/WFC3 instruments. Several filters were used to sample specific wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Purple: F275W, Indigo: F435W, Blue: F606W, Light-Blue: F090W, Cyan: F115W, Green: F150W, Yellow/Green: F200W, Yellow: F277W, Light-Orange: F356W, Orange: F410M, Red: F444W
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  • Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.