The environmental dependence of the stellar mass function at z ~ 1 - Comparing cluster and field between the GCLASS and UltraVISTA surveys

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Volume 557 (September 2013)

A&A, 557 (2013) A15

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Table A.1

GCLASS photometric data set.

Name^a

u _lim

g _lim

r _lim

i _lim

z _lim

J _lim

K _s,lim

3.6 μm_lim

4.5 μm_lim

5.8 μm_lim

8.0 μm_lim

[mag_AB]

SpARCS-0034

23.1^b

25.3^b

24.4^b

24.3^b

23.9^c

22.5^e

22.2^e

21.4^g

21.2^g

19.7^g

19.6^g

SpARCS-0035

24.4^b

25.4^b

24.9^b

24.3^b

23.69^c

24.1^f

23.4^f

22.8^g

22.3^g

20.8^g

20.4^g

SpARCS-0036

22.9^b

25.1^b

24.4^b

23.7^b

23.59^c

22.7^e

21.5^e

21.2^g

21.1^g

19.9^g

19.6^g

SpARCS-0215

24.8^a

25.1^b

24.7^b

24.4^b

23.7^a

22.8^e

22.0^e

21.3^g

21.1^g

19.5^g

19.4^g

SpARCS-1047

25.5^a

25.7^a

25.0^a

24.7^a

23.8^a

23.1^d

22.3^d

21.6^g

21.3^g

19.7^g

SpARCS-1051

25.6^a

25.8^a

25.2^a

25.0^a

24.0^a

23.2^d

22.4^d

21.7^g

21.3^g

19.8^g

19.7^g

SpARCS-1613

25.5^a

26.0^a

25.4^a

24.7^a

24.0^a

23.1^d

22.7^d

22.7^g

22.6^g

21.2^g

20.9^g

SpARCS-1616

25.1^a

25.7^a

25.1^a

24.8^a

23.5^a

23.3^d

22.7^d

22.6^g

22.4^g

21.2^g

20.9^g

SpARCS-1634

25.6^a

26.1^a

25.6^a

25.1^a

24.4^a

23.7^d

23.1^d

23.2^g

21.6^g

21.3^g

SpARCS-1638

25.4^a

25.9^a

25.4^a

25.1^a

24.2^a

23.4^d

22.8^d

23.0^g

23.1^g

21.3^g

Notes.The instruments used for the different clusters and filters are indicated. The limiting magnitudes reported are median 5-σ flux measurement limits for point sources measured with a Gaussian weight function.

^(a)

MegaCam, Canada-France-Hawaii Telescope (CFHT).

^(b)

IMACS, Magellan Telescope.

^(c)

MOSAIC-II, Blanco Telescope, Cerro Tololo Inter-American Observatory (CTIO).

^(d)

WIRCam, Canada-France-Hawaii Telescope (CFHT).

^(e)

ISPI, Blanco Telescope, Cerro Tololo Inter-American Observatory (CTIO).

^(f)

HAWK-I, Very Large Telescope (VLT) UT4.

^(g)

IRAC, Spitzer Space Telescope.

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