2018ApJ...857...37O


Query : 2018ApJ...857...37O

2018ApJ...857...37O - Astrophys. J., 857, 37-37 (2018/April-2)

"Slow-scanning" in ground-based mid-infrared observations.

OHSAWA R., SAKO S., MIYATA T., KAMIZUKA T., OKADA K., MORI K., UCHIYAMA M.S., YAMAGUCHI J., FUJIYOSHI T., MORII M. and IKEDA S.

Abstract (from CDS):

Chopping observations with a tip-tilt secondary mirror have conventionally been used in ground-based mid-infrared observations. However, it is not practical for next generation large telescopes to have a large tip-tilt mirror that moves at a frequency larger than a few hertz. We propose an alternative observing method, a "slow-scanning" observation. Images are continuously captured as movie data, while the field of view is slowly moved. The signal from an astronomical object is extracted from the movie data by a low-rank and sparse matrix decomposition. The performance of the "slow-scanning" observation was tested in an experimental observation with Subaru/COMICS. The quality of a resultant image in the "slow-scanning" observation was as good as in a conventional chopping observation with COMICS, at least for a bright point-source object. The observational efficiency in the "slow-scanning" observation was better than that in the chopping observation. The results suggest that the "slow-scanning" observation can be a competitive method for the Subaru telescope and be of potential interest to other ground-based facilities to avoid chopping.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): methods: data analysis - methods: observational - techniques: image processing

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 V* V479 Her LP* 17 21 26.1754415232 +18 33 19.980912240   12.81 11.80     M5/6 10 0

Query : 2018ApJ...857...37O

Basic data :
V* V479 Her -- Long-Period Variable
Other object types:
otypes_help
* (DO,FBS,...), MIR (AKARI,WISEA,...), V* (AN,V*), LP* (2009yCat), LP? (2022yCat), NIR (2MASS), IR (IRAS)
ICRS coord. (ep=J2000) :
17 21 26.1754415232 +18 33 19.980912240 (Optical) [ 0.0309 0.0342 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
17 19 14.5480867752 +18 36 13.010013083 [ 0.0309 0.0342 90 ]
Gal coord. (ep=J2000) :
040.5912439244785 +27.9038522325586 [ 0.0309 0.0342 90 ]
Proper motions mas/yr :
-8.419 -10.018 [0.041 0.045 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -41.97 [0.28] / z(spectroscopic) -0.000140 [0.000001] / cz -41.97 [0.28]
   (Opt) A 2022yCat.1355....0G
Parallaxes (mas):
0.973 [0.0483] A 2020yCat.1350....0G
Spectral type:
M5/6 D 2012MNRAS.419.3346G
Fluxes (6) :
B 12.81 [0.27] D 2000A&A...355L..27H
V 11.80 [0.16] D 2000A&A...355L..27H
G 8.890245 [0.004538] C 2020yCat.1350....0G
J 5.113 [0.228] D 2003yCat.2246....0C
H 4.083 [0.246] D 2003yCat.2246....0C
K 3.743 [0.256] D 2003yCat.2246....0C
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Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

DO 15936 GSC 01541-00273 SV* SON 3464 WISEA J172126.19+183319.7
AKARI-IRC-V1 J1721261+183320 IRAS 17192+1836 TIC 362127625 WISE J172126.17+183319.6
AN 137.1943 IRAS F17192+1836 TYC 1541-273-1 Gaia DR3 4554280658077953792
FBS 1719+186 2MASS J17212616+1833199 V* V479 Her Gaia DR2 4554280658077953792

References (10 between 1850 and 2026) (Total 10)
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

Velocities : 1    Distance : 3    Plx : 3    PM : 2    SpT : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : V* V479 Her

Link by name to the catalogue in VizieR :

DO 15936 AKARI-IRC-V1 J1721261+183320 FBS 1719+186 GSC 01541-00273 IRAS 17192+1836
IRAS F17192+1836 2MASS J17212616+1833199 TYC 1541-273-1 V* V479 Her WISEA J172126.19+183319.7
WISE J172126.17+183319.6 Gaia DR3 4554280658077953792 Gaia DR2 4554280658077953792

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