Characterizing the evolvingK-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
نویسندگان
چکیده
منابع مشابه
The Uv Luminosity Function and Luminosity Density from 506 Hudf , Hudf - Ps , and Goods I -
1 Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs #9803. 2 Observations have been carried out using the Very Large Telescope at the European Southern Observatory (ESO) Paranal Observatory under program ID: LP1...
متن کاملGalaxies at Z ∼ 6 : the Uv Luminosity Function and Luminosity Density from 506 Hudf , Hudf - Ps , and Goods I -
1 Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs #9803. 2 Observations have been carried out using the Very Large Telescope at the European Southern Observatory (ESO) Paranal Observatory under program ID: LP1...
متن کاملThe K - Band Galaxy Luminosity Function 12
We measured the K-band luminosity function using a complete sample of 4192 morphologically-typed 2MASS galaxies with Ks = 20 mag/arcsec 2 isophotal magnitudes 7 < K 20 < 11:25 mag spread over 2:12 str. Early-type (T ?0:5) and late-type (T > ?0:5) galaxies have similarly shaped luminosity functions, for H 0 = 100h km s ?1 Mpc ?1 , such that the late-type galaxies slightly dominate the K-band lum...
متن کاملThe K-band Galaxy Luminosity Function
We measured the K-band luminosity function using a complete sample of 4192 morphologically-typed 2MASS galaxies with µ Ks = 20 mag/arcsec 2 isophotal magnitudes 7 < K 20 < 11.25 mag spread over 2.12 str. Early-type (T ≤ −0.5) and late-type (T > −0.5) galaxies have similarly shaped luminosity functions,
متن کاملThe Galaxy Luminosity Function at Z≃1 in the Hudf: Probing the Dwarf Population
We present a catalog of spectro-photometric redshifts for 1308 galaxies from the GRism ACS Program for Extragalactic Science (GRAPES) observations with the Hubble Space Telescope. These low-resolution spectra between 6000 Å and 9500 Å are supplemented with U , J , H , and Ks from various facilities, resulting in redshifts computed with ∼40 spectral bins per galaxy. For 81 galaxies between 0.5< ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2016
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stw2728