Results 131 to 140 of about 32,530 (259)

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

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

Mid‐Infrared Spectra of Classical AGNs Observed with theSpitzer Space Telescope [PDF]

open access: bronze, 2005
D. W. Weedman   +8 more
openalex   +1 more source

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

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

Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia Predictions

open access: yesThe Astrophysical Journal
In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of ∼950 microlensing events observed by the Spitzer Space Telescope between 2014 and 2019.
Krzysztof A. Rybicki   +76 more
doaj   +1 more source

A new era in solar system astronomy with JWST. [PDF]

open access: yesNat Commun, 2023
Villanueva GL, Milam SN.
europepmc   +1 more source

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

Spitzer Space TelescopeIRAC and MIPS Observations of the Interacting Galaxies IC 2163 and NGC 2207: Clumpy Emission [PDF]

open access: green, 2006
D. M. Elmegreen   +6 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

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