Euclid preparation-XVIII. The NISP photometric system
M Schirmer, K Jahnke, G Seidel, H Aussel… - Astronomy & …, 2022 - aanda.org
Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95–2.02
µm range, to a 5 σ point-source median depth of 24.4 AB mag. This unique photometric
dataset will find wide use beyond Euclid's core science. In this paper, we present accurate
computations of the Euclid YE, JE, and HE passbands used by the Near-Infrared
Spectrometer and Photometer (NISP), and the associated photometric system. We pay
particular attention to passband variations in the field of view, accounting for, among other …
µm range, to a 5 σ point-source median depth of 24.4 AB mag. This unique photometric
dataset will find wide use beyond Euclid's core science. In this paper, we present accurate
computations of the Euclid YE, JE, and HE passbands used by the Near-Infrared
Spectrometer and Photometer (NISP), and the associated photometric system. We pay
particular attention to passband variations in the field of view, accounting for, among other …
[PDF][PDF] Euclid preparation. XVIII. The NISP photometric system
E Collaboration, M Schirmer - A&A, 2022 - helda.helsinki.fi
Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95–2.02
µm range, to a 5 σ point-source median depth of 24.4 ABmag. This unique photometric
dataset will find wide use beyond Euclid's core science. In this paper, we present accurate
computations of the Euclid YE, JE, and HE passbands used by the Near-Infrared
Spectrometer and Photometer (NISP), and the associated photometric system. We pay
particular attention to passband variations in the field of view, accounting for, among other …
µm range, to a 5 σ point-source median depth of 24.4 ABmag. This unique photometric
dataset will find wide use beyond Euclid's core science. In this paper, we present accurate
computations of the Euclid YE, JE, and HE passbands used by the Near-Infrared
Spectrometer and Photometer (NISP), and the associated photometric system. We pay
particular attention to passband variations in the field of view, accounting for, among other …