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Table 4

Photometry for NX Pup and new NIR excess candidates in CG 1 and CG 2.

NX Pup CG 1 IRS 1 CG 1 IRS 2 CG 1 IRS 3 CG 2 IRS 1

Ja 590 (8.579) ... 0.0235 (19.58) 0.0435 (18.91) 0.25 (17.01)
Ha 1250 (7.825) ... 0.0749 (17.84) 0.0943 (17.59) 0.791 (15.28)
Ka 2470 (6.080) ... 0.153 (16.60) 0.158 (16.56) 1.96 (13.83)
3.4b 5184.62 (4.440) 7.75 (11.504) 0.281 (15.104) 0.453 (14.586) 6.923 (11.626)
3.6c ... 13.94 ... ... ...
4.5c ... 23.39 ... ... ...
4.6b 8593.90 (3.252) 23.05 (9.681) 0.369 (14.170) 0.579 (13.680) 12.853 (10.315)
5.8c ... 22.29 ... ... ...
8.0c ... 34.24 ... ... ...
9.0e 5197 ... ... ... ...
12b 5047.81 (1.994) 144.91 (5.849) 2.403 (10.300) 2.271 (10.361) 24.769 (7.767)
12d 6682 ... ... ... 250h
18e 4652 1029 ... ... ...
22b 4816.84 (0.599) 2236 (1.432) 8.279 (7.511) 11.261 (7.177) 58.879 (5.381)
24f ... 2092 ... ... ...
25d 7604 ... ... ... 370h
60h ... 13120 ... ... 440h
65g ... 7697 ... ... ...
70f ... 9314 ... ... ...
90g ... 9672 ... ... 656
100d ... 33 590 ... ... 8880h
140g ... 17 370 ... ... 6259
160g ... 15 570 ... ... ...

Notes. The flux unit is mJy. For JHK and WISE we also list the magnitude in parenthesis.

(a)

SOFI.

(b)

WISE.

(c)

Spitzer IRAC.

(d)

IRAS.

(e)

Akari IRC.

(f)

Spitzer MIPS.

(g)

Akari FIS.

(h)

Data for the offset IRAS source 07144-4352, flagged U (upper limit) for 12 and 25 μm, B and A for 60 and 100 μm, respectively. Used to check the SED model behaviour.

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