How Accurately Can Obscured Galaxy Luminosities Be Measured Using Spectral Energy Distribution Fitting of Near- Through Far-Infrared Observations?

AuthID
P-01B-5BB
26
Author(s)
Farrah, D
·
Ejercito, K
·
Efstathiou, A
·
Leisawitz, D
·
Engholm, A
·
Shivaei, I
·
Bonato, M
·
Clements, DL
·
Petty, S
·
Pitchford, LK
·
[+1]·
[+5]·
Nixon, C
·
Pearson, C
·
Ricketti, BV
·
Rigopoulou, D
·
Robinson, L
·
Spencer, LD
·
Wang, LY
·
Sanders, DB
·
van Belle, G
Document Type
Article
Year published
2026
Published
in ASTROPHYSICAL JOURNAL, ISSN: 0004-637X
Volume: 997, Issue: 2, Pages: 150 (20)
Indexing
Publication Identifiers
Scopus: 2-s2.0-105034502295
Wos: WOS:001665708600001
Source Identifiers
ISSN: 0004-637X
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Name Order Name   Name Order Name   Name Order Name
1 Farrah, D;   2 Ejercito, K;   3 Efstathiou, A;
4 Leisawitz, D;   5 Engholm, A;   6 Shivaei, I;
7 Bonato, M;   8 Clements, DL;   9 Petty, S;
10 Pitchford, LK;   11 Varnava, C;   12 Afonso, J ;
13 Gruppioni, C;   14 Hatziminaoglou, E;   15 Hoffman, A;
16 Lacy, M;   17 Matthews, BC;   18 Nixon, C;
19 Pearson, C;   20 Ricketti, BV;   21 Rigopoulou, D;
22 Robinson, L;   23 Spencer, LD;   24 Wang, LY;
25 Sanders, DB;   26 van Belle, G;