Results 131 to 140 of about 60,149 (264)

The Baryonic Tully–Fisher Relation. II. Stellar Mass Models

open access: yesThe Astronomical Journal
We present new color–ϒ _* (mass-to-light ratio) models to convert Wide-field Infrared Survey Explorer W1 fluxes into stellar masses. We outline a range of possible star formation histories and chemical evolution scenarios to explore the confidence limits
Francis Duey   +3 more
doaj   +1 more source

JWST's eyes on an alien world. [PDF]

open access: yesInnovation (Camb), 2023
Zhang X.
europepmc   +1 more source

Lessons learned in extended-extended Spitzer Space Telescope operations [PDF]

open access: gold, 2018
Lisa J. Storrie‐Lombardi   +8 more
openalex   +1 more source

OA to data from the Spitzer space telescope

open access: yes, 2006
Joe Chavez, Spitzer science archive interface, International Society for Optical Engineering, June 30, 2006.
openaire   +1 more source

Spitzer Space TelescopeObservations of Magnetic Cataclysmic Variables: Possibilities for the Presence of Dust in Polars [PDF]

open access: bronze, 2007
Carolyn Brinkworth   +8 more
openalex   +1 more source

Bright z ∼ 9 Galaxies in Parallel: The Bright End of the Rest-frame UV Luminosity Function from HST Parallel Programs

open access: yesThe Astrophysical Journal
The abundance of bright galaxies at z > 8 can provide key constraints on models of galaxy formation and evolution, as the predicted abundance varies greatly when different physical prescriptions for gas cooling and star formation are implemented.
Micaela B. Bagley   +9 more
doaj   +1 more source

Detecting Clusters of Galaxies at High Redshift with the Spitzer Space Telescope [PDF]

open access: green, 2005
Gillian Wilson   +3 more
openalex   +1 more source

Diversity of Cold Worlds: A Near-complete Spectral Energy Distribution for 2MASS J04151954−0935066 Using JWST

open access: yesThe Astrophysical Journal
We present a near-complete spectral energy distribution (SED) for an extrasolar world: the T8 brown dwarf 2MASS J04151954−0935066. Spanning from optical to mid-infrared (0.7–20.4 μ m) wavelengths, the SED for this substellar atmosphere is constructed ...
Sherelyn Alejandro Merchan   +27 more
doaj   +1 more source

Outflows from the youngest stars are mostly molecular. [PDF]

open access: yesNature, 2023
Ray TP   +22 more
europepmc   +1 more source

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