2001A&A...369.1140H

Query : 2001A&A...369.1140H

2001A&A...369.1140H - Astronomy and Astrophysics, volume 3691140-1142 (2001/4-3)

Useful transformations between photometric systems.

HARMANEC P. and BOZIC H.

Abstract (from CDS):

In the course of detailed studies of the long-term variations of particular Be stars, we have practically verified that the non-linear transformations, needed for a reliable transformation between a standard and an instrumental photometric system can also be successfully used to the transformations between two particular standard photometric systems. To demonstrate the importance and power of non-linear transformations and to provide pieces of information useful for a broader astronomical community, we summarize the transformation formulae already published (but hidden from the general community in papers dealing with particular Be stars) and present several other useful transformations derived by us. All transformation formulae presented here are transformations from various photometric systems to Johnson's UBV system. However, the general procedures applied here would allow construction of similar transformations between other photometric systems, too.

Abstract Copyright: ∼

Journal keyword(s): methods: observational - techniques: photometric

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	* 14 Lac	EB*	22 50 21.7785565224	+41 57 12.221400240	5.49	5.961	5.910			B4III	155	0

Query : 2001A&A...369.1140H

Basic data :

* 14 Lac -- Eclipsing Binary

* (*,AG,...), ** (**,CCDM,...), V* (CSV,V*), Be* (1982IAUS), EB* (2017ARep), Em* (EM*), UV (TD1), NIR (2MASS)

22 50 21.7785565224 +41 57 12.221400240 (Optical) [ 0.0733 0.0842 90 ] A 2020yCat.1350....0G

22 48 06.1513846507 +41 41 17.636996993 [ 0.0733 0.0842 90 ]

100.0420799703150 -15.4741981943504 [ 0.0733 0.0842 90 ]

5.105 -1.666 [0.075 0.105 90] A 2020yCat.1350....0G

V(km/s) -15.80 [3.1] / z(~) -0.000053 [0.000010] / cz -15.80 [3.10] C 2006AstL...32..759G

2.0266 [0.1300] A 2020yCat.1350....0G

B4III C 1982ApJS...50...55S

0.0067 0.0 11 (Opt) D 2001AJ....122.3466M

U 5.49 [~] D 1982IAUS...98..261J

B 5.961 [0.014] D 2000A&A...355L..27H

V 5.910 [0.009] D 2000A&A...355L..27H

G 5.861477 [0.003039] C 2022yCat.1355....0G

J 5.479 [0.032] C 2003yCat.2246....0C

H 5.428 [0.027] C 2003yCat.2246....0C

K 5.321 [0.017] C 2003yCat.2246....0C

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*` 14 Lac`**	`GCRV 14345`	`ROT 3324`	*`V V360 Lac`**
` HDS 3244A`**	`GEN# +1.00216200`	`SAO 52412`	`WDS J22504+4157A`
`AG+41 2230`	`GSC 03223-03619`	`SKY# 43394`	`WEB 20094`
`ALS 16647`	`HD 216200`	`TD1 29400`	`[JE82] 1131`
`BD+41 4623`	`HIC 112778`	`TIC 154355871`	`Gaia DR2 1932855787101481216`
`CCDM J22504+4157A`	`HIP 112778`	`TYC 3223-3619-1`	`Gaia DR3 1932855787101481216`
`CSV 103103`	`HR 8690`	`UBV 19572`
*`EM CDS 1402`**	`2MASS J22502177+4157122`	`UBV M 26660`
`GC 31861`	`PPM 63477`	`uvby98 100216200`

References (155 between 1850 and 2026) (Total 155)
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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`AG+41 2230`	`ALS 16647`	`BD+41 4623`	`CCDM J22504+4157A`	`GSC 03223-03619`
`HD 216200`	`HIC 112778`	`HIP 112778`	`HR 8690`	`2MASS J22502177+4157122`
`PPM 63477`	`SAO 52412`	`TD1 29400`	`TYC 3223-3619-1`	`uvby98 100216200`
*`V V360 Lac`**	`WDS J22504+4157A`	`Gaia DR2 1932855787101481216`	`Gaia DR3 1932855787101481216`

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