2008AJ....136..197V


Query : 2008AJ....136..197V

2008AJ....136..197V - Astron. J., 136, 197-211 (2008/July-0)

HiRes deconvolution of Spitzer infrared images.

VELUSAMY T., MARSH K.A., BEICHMAN C.A., BACKUS C.R. and THOMPSON T.J.

Abstract (from CDS):

Spitzer provides unprecedented sensitivity in the infrared (IR), but the spatial resolution is limited by a relatively small aperture (0.85 m) of the primary mirror. In order to maximize the scientific return it is desirable to use processing techniques which make the optimal use of the spatial information in the observations. We have developed a deconvolution technique for Spitzer images. The algorithm, "HiRes" and its implementation has been discussed by Backus et al. in 2005. Here we present examples of Spitzer IR images from the Infrared Array Camera (IRAC) and MIPS, reprocessed using this technique. Examples of HiRes processing include a variety of objects from point sources to complex extended regions. The examples include comparison of Spitzer deconvolved images with high-resolution Keck and Hubble Space Telescope images. HiRes deconvolution improves the visualization of spatial morphology by enhancing resolution (to sub-arcsecond levels in the IRAC bands) and removing the contaminating sidelobes from bright sources. The results thereby represent a significant improvement over previously-published Spitzer images. The benefits of HiRes include (a) sub-arcsec resolution (∼0".6-0".8 for IRAC channels); (b) the ability to detect sources below the diffraction-limited confusion level; (c) the ability to separate blended sources, and thereby provide guidance to point-source extraction procedures; (d) an improved ability to show the spatial morphology of resolved sources. We suggest that it is a useful technique to identify features which are interesting enough for follow-up deeper analysis.

Abstract Copyright: ∼

Journal keyword(s): infrared: general - techniques: high angular resolution

Simbad objects: 24

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Number of rows : 24
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 SN 1572A SN* 00 25 21.5 +64 08 27           B8 1254 1
2 IRAS 03222+3034 Y*O 03 25 22.32 +30 45 13.9           ~ 164 0
3 IRAS 03225+3034 IR 03 25 36.49 +30 45 22.2           ~ 165 1
4 LDN 1448NA smm 03 25 36.49 +30 45 22.2           ~ 193 1
5 SSTc2d J032536.4+304522 Y*O 03 25 36.49 +30 45 22.2           ~ 208 1
6 IRAS 04239+2436 Y*O 04 26 56.29704 +24 43 35.3280           ~ 163 0
7 HH 111 HH 05 51 44.207 +02 48 33.87           ~ 418 0
8 NGC 2207 AG? 06 16 22.0336889136 -21 22 21.759218400   11.48 10.65 10.21 11.9 ~ 301 4
9 IC 2163 AG? 06 16 27.9671433048 -21 22 33.133211832   12.55   11.28   ~ 172 2
10 * alf CMa SB* 06 45 08.91728 -16 42 58.0171 -1.51 -1.46 -1.46 -1.46 -1.43 A0mA1Va 1610 0
11 NGC 2316 Cl* 06 59 41.7 -07 46 07           ~ 49 1
12 M 68 GlC 12 39 27.98 -26 44 38.6     7.96     ~ 1069 0
13 * rho Oph ** 16 25 35.11766 -23 26 49.8150 4.30 4.85 4.63 4.27 3.96 B2IV+B2V 670 0
14 WL 16 Y*O 16 27 02.33520 -24 37 27.2316           A0-F3 164 0
15 NAME WL 20S BD? 16 27 15.69 -24 38 45.7           ~ 15 0
16 WL 20 TT* 16 27 15.69840 -24 38 43.4364           M0 86 0
17 NAME WL 20E TT* 16 27 15.8951829912 -24 38 43.788560604           K7 78 0
18 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
19 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 1195 1
20 LDN 663 DNe 19 36 55 +07 34.4           ~ 698 0
21 IRAS 20582+7724 Y*O 20 57 12.9250225656 +77 35 43.656301932           ~ 119 0
22 LDN 1228 DNe 20 57 13 +77 35.8           ~ 131 0
23 NGC 7253 AG? 22 19 27.700 +29 23 44.85   14.4       ~ 88 0
24 * alf PsA PM* 22 57 39.04625 -29 37 20.0533 1.31 1.25 1.16 1.11 1.09 A4V 1303 3

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