2013A&A...559A..26R

Query : 2013A&A...559A..26R

2013A&A...559A..26R - Astronomy and Astrophysics, volume 559A26-26 (2013/11-1)

MAIA, a three-channel imager for asteroseismology: instrument design.

RASKIN G., BLOEMEN S., MORREN J., PEREZ PADILLA J., PRINS S., PESSEMIER W., VANDERSTEEN J., MERGES F., OSTENSEN R., VAN WINCKEL H. and AERTS C.

Abstract (from CDS):

MAIA, an acronym for Mercator Advanced Imager for Asteroseismology, is a three-channel instrument that targets fast-cadence three-colour photometry, installed at the 1.2-m Mercator telescope at the Roque de los Muchachos at La Palma (Canary Islands, Spain). This instrument observes a 9.4x14.1-arcmin² field-of-view simultaneously in three wavelength bands on three large frame-transfer CCDs. These detectors were developed for ESA's cancelled Eddington space mission and were offered on permanent loan to the Institute of Astronomy (KULeuven, Belgium). MAIA uses its own ugr photometric system that is a crude approximation of the SDSS system. The instrument is designed to perform multi-colour observations for asteroseismology, with specific emphasis on subdwarf and white dwarf single and binary stars. We describe the design of the instrument, discuss key components, and report on its performance and first results.

Abstract Copyright: ∼

Journal keyword(s): asteroseismology - instrumentation: photometers - instrumentation: detectors - techniques: photometric - stars: variables: general

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	Balloon 90100001	HS*	23 15 21.4810390968	+29 05 01.433373360		11.90	12.30			sdB	98	0

Query : 2013A&A...559A..26R

Basic data :

Balloon 90100001 -- Hot Subdwarf

* (TYC,GSC,...), blu (2019A&A), UV (Balloon,GALEX), HS* (2006BaltA), Pu* (2012MNRAS), V* (V*), NIR (2MASS)

23 15 21.4810390968 +29 05 01.433373360 (Optical) [ 0.0246 0.0248 90 ] A 2020yCat.1350....0G

23 12 55.0201778743 +28 48 39.914968227 [ 0.0246 0.0248 90 ]

098.8681169261531 -29.2597526629990 [ 0.0246 0.0248 90 ]

10.177 -12.046 [0.032 0.030 90] A 2020yCat.1350....0G

2.5749 [0.0369] A 2020yCat.1350....0G

sdB D 1991A&A...250..370B

B 11.90 [0.08] D 2000A&A...355L..27H

V 12.30 [0.20] D 2000A&A...355L..27H

G 12.084245 [0.003242] C 2020yCat.1350....0G

J 12.570 [0.022] C 2003yCat.2246....0C

H 12.703 [0.021] C 2003yCat.2246....0C

K 12.764 [0.027] C 2003yCat.2246....0C

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`TYC 2248-1751-1`	`GSC 02248-01751`	`UCAC2 42168244`	`Gaia DR1 2846162917391360896`
`Balloon 90100001`	`2MASS J23152147+2905015`	*`V V585 Peg`**	`Gaia DR2 2846162921688127360`
`GALEX J231521.4+290502`	`TIC 90960668`	`Gaia DR3 2846162921688127360`

References (98 between 1850 and 2026) (Total 98)
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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`TYC 2248-1751-1`	`GALEX J231521.4+290502`	`GSC 02248-01751`	`2MASS J23152147+2905015`	`UCAC2 42168244`
*`V V585 Peg`**	`Gaia DR3 2846162921688127360`	`Gaia DR1 2846162917391360896`	`Gaia DR2 2846162921688127360`

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