CALPRODUCT-NP-006: NISP-P PN Reference Photometric Catalog

Parent requirement

R-CAL-B-NS-1100
R-CAL-B-NS-1200

Scheduling

Once during PV phase, checked after 1 year.

Time-critical

No.

Objective

The purpose of these observations is to provide a reference photometric catalog to support the NISP-S spectral observations of a Planetary Nebula (PN). In particular, the NISP-P data will be used to determine the wavelength zeropoints for the NISP-S spectral dispersion solution.

Fulfilled by

CALBLOCK-PV-009: NISP Wavelength Dispersion and VIS BFE

CALBLOCK-F-010: NISP Wavelength Dispersion and VIS BFE

Targets and pointing constraints

Table 6: Compact Planetary Nebulae. The units of the Pa-\(\beta\) line fluxes are [erg/s/cm^2]. Crowding is defined as the number of sources brighter than Gaia Gmag<19 \({\rm arcmin}^{-2}\). The radius refers to EE80 from HST imaging and slitless spectroscopy. CSV file

# ID

R.A.

Dec

log(Pa-beta)

r [“]

Crowding

Comment

SMC-SMP-20

00:56:05.39

-70:19:24.7

-13.22

0.20

2.2

USE THIS ONE

SMC-SMP-2

00:32:38.81

-71:41:58.7

-13.55

0.25

1.8

ask before using

LMC-Sa-104a

04:25:32.18

-66:47:16.3

-13.53

0.13

1.9

ask before using

SMC-SMP-1

00:23:58.67

-73:38:03.8

-13.40

0.15

4.4

ask before using

He2-436

19:32:06.69

-34:12:57.8

-12.68

0.60

4.6

ask before using

G205.8-26.7

05:03:41.85

-06:10:03.0

-13.02

1.04

1.8

ask before using

DdDm-1

16:40:18.20

+38:42:19.9

-12.15

0.60

1.3

DO NOT USE; bright star

G295.3-09.3

11:17:43.16

-70:49:32.2

-12.50

0.48

12.7

DO NOT USE; crowded

SMC-SMP-25

00:59:40.51

-71:38:15.1

-14.11

0.19

12.8

DO NOT USE; crowded

SMC-SMP-8

00:43:25.30

-72:38:18.9

-13.58

0.40

17.4

DO NOT USE; crowded

LMC-SMP-53

05:21:32.93

-67:00:05.5

-13.42

0.40

19.6

DO NOT USE; crowded

G042.9-06.9

19:34:33.54

+05:41:03.0

-11.87

0.48

23.0

DO NOT USE; crowded

SMC-SMP-13

00:49:51.71

-73:44:21.3

-13.34

0.20

24.0

DO NOT USE; crowded

G334.8-07.4

17:03:02.86

-53:55:54.0

-11.86

0.44

25.2

DO NOT USE; crowded

SMC-SMP-24

00:59:16.09

-72:01:59.7

-13.43

0.38

25.9

DO NOT USE; crowded

LMC-SMP-31

05:09:20.23

-67:47:25.2

-13.24

0.15

44.6

DO NOT USE; crowded

G025.3-04.6

18:54:20.04

-08:47:32.9

-12.69

0.48

53.4

DO NOT USE; crowded

SMC-SMP-18

00:51:57.97

-73:20:31.1

-13.35

0.14

57.9

DO NOT USE; crowded

LMC-SMP-25

05:06:24.00

-69:03:19.2

-13.09

0.23

68.4

DO NOT USE; crowded

LMC-SMP-58

05:24:20.81

-70:05:01.9

-13.19

0.13

91.8

DO NOT USE; crowded

Inter-operability constraints

None

In-orbit duration

Processing input

Ground Processing Input Data:

Data Description:

Quality control parameters

DataModel: https://gitlab.euclid-sgs.uk/

Contact person

NISP-P calibration scientist