Merging galaxies in isolated environments - I. Multiband photometry, classification, stellar masses, and star formation rates

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Volume 686 (June 2024)

A&A, 686 (2024) A151

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Table B.1

Relevant parameters of the filters and images used from the different surveys. ¹All-sky ²Deep, and ³Medium Imaging Surveys from GALEX.

Survey	Band	Effective	Zero point	Resolution	Sensitivity	Pixel Scale	∆ m
		wavelength	magnitude	(arcsec)		(arcsec/pixel)	$(m_{A B} = m_{V_{e g a}} + Δ m)$ $\left( {{m_{AB}} = {m_{{V_{ega}}}} + {\rm{\Delta }}m} \right)$
GALEX	FUV	1528 A	18.82	4.2	20 (AIS¹) / 22.7 (MIS²) / 24.8 (DIS³)	1.5	2.22
	NUV	2271 A	20.08	5.3	21 / 22.7 / 24.4 (ABmag)	1.5	1.69

SDSS	u	3551 A	22.5		22.0 (ABmag)	0.396	0.91
	g	4686 A	22.5		22.2 (ABmag)	0.396	−0.08
	r	6165 A	22.5	1.3	22.2 (ABmag)	0.396	0.16
	i	7481 A	22.5		21.3 (ABmag)	0.396	0.37
	z	8931 A	22.5		20.5 (ABmag)	0.396	0.54

WISE	W1	3.4 µm	20.73	6.1	0.08 mJy (16.5 Vegamag)	1.375	2.699
	W2	4.6 µm	19.56	6.4	0.11 mJy (15.5 Vegamag)	1.375	3.339
	W3	12 µm	17.60	6.5	1mJy (11.2 Vegamag)	1.375	5.174
	W4	22 µm	12.98	12.0	6 mJy (7.9 Vegamag)	1.375	6.620

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