2023PASP..135k4504A


Query : 2023PASP..135k4504A

2023PASP..135k4504A - Publ. Astron. Soc. Pac., 135, part no 11, 4504 (2023/November-0)

Methods for Averaging Spectral Line Data.

ANDERSON L.D., LIU B., BALSER D.S., BANIA T.M., HAFFNER L.M., LINVILLE D.J., LUISI M. and WENGER T.V.

Abstract (from CDS):

The ideal spectral averaging method depends on one's science goals and the available information about one's data. Including low-quality data in the average can decrease the signal-to-noise ratio (S/N), which may necessitate an optimization method or a consideration of different weighting schemes. Here, we explore a variety of spectral averaging methods. We investigate the use of three weighting schemes during averaging: weighting by the signal divided by the variance (“intensity-noise weighting”), weighting by the inverse of the variance (“noise weighting”), and uniform weighting. Whereas for intensity-noise weighting the S/N is maximized when all spectra are averaged, for noise and uniform weighting we find that averaging the 35%-45% of spectra with the highest S/N results in the highest S/N average spectrum. With this intensity cutoff, the average spectrum with noise or uniform weighting has ∼95% of the intensity of the spectrum created from intensity-noise weighting. We apply our spectral averaging methods to GBT Diffuse Ionized Gas hydrogen radio recombination line data to determine the ionic abundance ratio, y+, and discuss future applications of the methodology.

Abstract Copyright: © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved

Journal keyword(s): Computational methods - Warm ionized medium

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 W 43 SFR 18 47 32 -01 56.5           ~ 604 0

Query : 2023PASP..135k4504A

Basic data :
W 43 -- Star Forming Region
Other object types:
otypes_help
Rad (ASB,3C,...), Cl* ([KPS2012]), SFR (2013MNRAS), MoC (SRBY), SNR (SNR), PoC ([MSM95])
ICRS coord. (ep=J2000) :
18 47 32.4 -01 56 31 (Optical) [ ] E 2013A&A...558A..53K
FK4 coord. (ep=B1950 eq=1950) :
18 44 56.4 -01 59 52 [ ]
Gal coord. (ep=J2000) :
030.7593 -00.0186 [ ]
Proper motions mas/yr :
0.30 -10.12 [0.54 0.54 90] D 2013A&A...558A..53K
Radial velocity / Redshift / cz :
V(km/s) 91.2 [~] / z(~) 0.000304 [~] / cz 91.21 [~]
   D 1973ApJ...181..781F
Angular size (arcmin):
6.3 6.3 90 (Rad) D 2009ApJ...699.1092H
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 160
Display criteria :

Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

ASB 46 GAL 030.8+00.02 SNR G030.8-00.0 [HC69] 10
3C 390.2 LMH 35 SNR G030.8-00.2 [KCW94] 031.280+00.063
CTB 59 MM 35 SRBY 171 [KPS2012] MWSC 2993
GAL 030.8+00.0 NRAO 581 W 43 [MSM95] G30.79 FIR 6

References (604 between 1850 and 2026) (Total 604)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 1   

   

Observing logs
Herschel : 11    ISO : 4    XMM : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : W 43

Link by name to the catalogue in VizieR :

3C 390.2

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