2023A&A...674A.172E


Query : 2023A&A...674A.172E

2023A&A...674A.172E - Astronomy and Astrophysics, volume 674A172 (2023/6-1)

Euclid preparation XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration.

EUCLID COLLABORATION, PATERSON K., SCHIRMER M., COPIN Y., CUILLANDRE J.-C., GILLARD W., GUTIERREZ-SOTO L.A., GUZZO L., HOEKSTRA H., KITCHING T., PALTANI S., PERCIVAL W.J., SCODEGGIO M., STANGHELLINI L., APPLETON P.N., LAUREIJS R., MELLIER Y., AGHANIM N., ALTIERI B., AMARA A., AURICCHIO N., BALDI M., BENDER R., BODENDORF C., BONINO D., BRANCHINI E., BRESCIA M., BRINCHMANN J., CAMERA S., CAPOBIANCO V., CARBONE C., CARRETERO J., CASTANDER F.J., CASTELLANO M., CAVUOTI S., CIMATTI A., CLEDASSOU R., CONGEDO G., CONSELICE C.J., CONVERSI L., CORCIONE L., COURBIN F., DA SILVA A., DEGAUDENZI H., DINIS J., DOUSPIS M., DUBATH F., DUPAC X., FERRIOL S., FRAILIS M., FRANCESCHI E., FUMANA M., GALEOTTA S., GARILLI B., GILLIS B., GIOCOLI C., GRAZIAN A., GRUPP F., HAUGAN S.V.H., HOLMES W., HORNSTRUP A., HUDELOT P., JAHNKE K., KUMMEL M., KIESSLING A., KILBINGER M., KOHLEY R., KUBIK B., KUNZ M., KURKI-SUONIO H., LIGORI S., LILJE P.B., LLORO I., MAIORANO E., MANSUTTI O., MARGGRAF O., MARKOVIC K., MARULLI F., MASSEY R., MEDINACELI E., MEI S., MENEGHETTI M., MEYLAN G., MORESCO M., MOSCARDINI L., NAKAJIMA R., NIEMI S.-M., NIGHTINGALE J.W., NUTMA T., PADILLA C., PASIAN F., PEDERSEN K., POLENTA G., PONCET M., POPA L.A., RAISON F., RENZI A., RHODES J., RICCIO G., RIX H.-W., ROMELLI E., RONCARELLI M., ROSSETTI E., SAGLIA R., SARTORIS B., SCHNEIDER P., SECROUN A., SEIDEL G., SERRANO S., SIRIGNANO C., SIRRI G., SKOTTFELT J., STANCO L., TALLADA-CRESPI P., TAYLOR A.N., TERENO I., TOLEDO-MOREO R., TORRADEFLOT F., TUTUSAUS I., VALENZIANO L., VASSALLO T., WANG Y., WELLER J., ZAMORANI G., ZOUBIAN J., ANDREON S., BARDELLI S., BOZZO E., COLODRO-CONDE C., DI FERDINANDO D., FARINA M., GRACIA-CARPIO J., KEIHANEN E., LINDHOLM V., MAINO D., MAURI N., SCOTTEZ V., TENTI M., ZUCCA E., AKRAMI Y., BACCIGALUPI C., BALLARDINI M., BIVIANO A., BORLAFF A.S., BURIGANA C., CABANAC R., CAPPI A., CARVALHO C.S., CASAS S., CASTIGNANI G., CASTRO T., CHAMBERS K.C., COORAY A.R., COUPON J., COURTOIS H.M., DAVINI S., DE LUCIA G., DESPREZ G., ESCARTIN J.A., ESCOFFIER S., FERRERO I., GABARRA L., GARCIA-BELLIDO J., GEORGE K., GIACOMINI F., GOZALIASL G., HILDEBRANDT H., HOOK I., KAJAVA J.J.E., KANSAL V., KIRKPATRICK C.C., LEGRAND L., LOUREIRO A., MAGLIOCCHETTI M., MAINETTI G., MAOLI R., MARCIN S., MARTINELLI M., MARTINET N., MARTINS C.J.A.P., MATTHEW S., MAURIN L., METCALF R.B., MONACO P., MORGANTE G., NADATHUR S., PATRIZII L., POLLACK J., PORCIANI C., POTTER D., PONTINEN M., SANCHEZ A.G., SAKR Z., SCHNEIDER A., SEFUSATTI E., SERENO M., SHULEVSKI A., STADEL J., STEINWAGNER J., VALIERI C., VALIVIITA J., VEROPALUMBO A., VIEL M. and ZINCHENKO I.A.

Abstract (from CDS):

The Euclid mission will conduct an extragalactic survey over 15 000 deg2 of the extragalactic sky. The spectroscopic channel of the Near-Infrared Spectrometer and Photometer (NISP) has a resolution of R ∼ 450 for its blue and red grisms that collectively cover the 0.93-1.89 µm range. NISP will obtain spectroscopic redshifts for 3 × 107 galaxies for the experiments on galaxy clustering, baryonic acoustic oscillations, and redshift space distortion. The wavelength calibration must be accurate within 5 Å to avoid systematics in the redshifts and downstream cosmological parameters. The NISP pre-flight dispersion laws for the grisms were obtained on the ground using a Fabry-Perot etalon. Launch vibrations, zero gravity conditions, and thermal stabilisation may alter these dispersion laws, requiring an in-flight recalibration. To this end, we use the emission lines in the spectra of compact planetary nebulae (PNe), which were selected from a PN database. To ensure completeness of the PN sample, we developed a novel technique to identify compact and strong line emitters in Gaia spectroscopic data using the Gaia spectra shape coefficients. We obtained VLT/X-shooter spectra from 0.3 to 2.5 µm for 19 PNe in excellent seeing conditions and a wide slit, mimicking Euclid's slitless spectroscopy mode but with a ten times higher spectral resolution. Additional observations of one northern PN were obtained in the 0.80-1.90 µm range with the GMOS and GNIRS instruments at the Gemini North Observatory. The collected spectra were combined into an atlas of heliocentric vacuum wavelengths with a joint statistical and systematic accuracy of 0.1 Å in the optical and 0.3 Å in the near-infrared. The wavelength atlas and the related 1D and 2D spectra are made publicly available.

Abstract Copyright: © The Authors 2023

Journal keyword(s): instrumentation: spectrographs - space vehicles: instruments - planetary nebulae: general

VizieR on-line data: <Available at CDS (J/A+A/674/A172): sources.dat pn-0-1.dat-pn-0-20.dat fits/* list.dat sp/*>

Simbad objects: 95

goto Full paper

goto View the references in ADS

Number of rows : 95
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 LHA 115-N 1 PN 00 23 58.6295947968 -73 38 03.974747928           ~ 49 0
2 LHA 115-N 2 PN 00 32 38.8692105240 -71 41 59.628264792   16.40       ~ 53 0
3 SMP SMC 4 PN 00 40 46.21 -75 16 20.8           ~ 14 0
4 LHA 115-N 5 PN 00 41 21.6981477336 -72 45 16.785012816   14.4 15.805   17.224 ~ 53 0
5 LHA 115-N 6 PN 00 41 27.7392128784 -73 47 06.468599004 16.82 16.84 15.82   16.92 ~ 60 0
6 LHA 115-N 7 PN 00 43 25.305 -72 38 18.79     16.212   17.58 ~ 34 0
7 LIN 49 PN 00 43 53.887 -72 55 14.79   16.3 17.1 16.7 16.91 ~ 21 0
8 LHA 115-N 38 PN 00 49 51.6394321128 -73 44 21.396914988   16.1 15.382   16.913 ~ 49 0
9 LHA 115-N 43 PN 00 51 07.37 -73 57 37.7   15.96 15.341   16.444 ~ 36 0
10 LHA 115-N 42 PN 00 51 27.14 -72 26 11.7   16.32 16.741   16.922 ~ 67 0
11 LHA 115-N 44 PN 00 51 56.3619687720 -71 24 44.377505784   15.98 15.2     ~ 45 0
12 LHA 115-N 47 PN 00 51 58.311 -73 20 31.87     16.158   16.17 ~ 49 0
13 LHA 115-N 54 PN 00 56 05.3840663544 -70 19 25.878681444   16.0       ~ 38 0
14 LIN 305 PN 00 56 30.750 -72 27 02.00   17.14 17.32   18.023 ~ 39 0
15 LHA 115-N 70 PN 00 59 16.1329481088 -72 01 59.841527196   16.07 16.016   16.916 ~ 48 0
16 LIN 357 PN 00 59 40.5128319264 -71 38 15.143769276   17.48 17.856   18.581 ~ 37 0
17 [MA93] 1721 Em* 01 10 29.1350494104 -72 53 38.458806936 16.36 17.25 17.54   17.41 B0-5(V) 7 0
18 LHA 115-N 87 PN 01 21 10.6470507816 -73 14 34.846684584   15.94 15.553   16.758 ~ 47 0
19 LIN 536 PN 01 24 11.8596151032 -74 02 32.149788540   17.12 17.589   17.716 ~ 36 0
20 SMP LMC 104A PN 04 25 32.1894647472 -66 47 16.278400824   17.2 17.36     ~ 15 0
21 LHA 120-N 182 PN 04 38 34.7919606072 -70 36 43.280547120 15.735 16.086 15.050   16.538 [WC4] 45 0
22 SMP LMC 2 PN 04 40 56.6962705344 -67 48 02.172617892 15.972 17.130 17.016   17.341 ~ 38 0
23 LHA 120-N 1 PN 04 42 24.0055846008 -66 13 01.662738600 15.811 16.458 15.830 15.19 16.840 ~ 28 0
24 LHA 120-S 1 pA? 04 48 08.5534908576 -67 26 06.840156408 15.633 16.722 16.505   17.001 ~ 31 0
25 LHA 120-N 78 PN 04 50 13.1540206128 -69 33 56.775850344 16.645 16.978 15.982 16.18   ~ 52 0
26 PN MaC 2-1 PN 05 03 41.8528461912 -06 10 03.027145764     14.4     ~ 46 0
27 LHA 120-N 98 EmO 05 04.4 -69 47           ~ 3 0
28 2MASS J05060944-6745277 pA? 05 06 09.447 -67 45 27.80 15.874 16.622 15.539 15.870 17.326 ~ 37 0
29 SMP LMC 25 Em* 05 06 23.9028944576 -69 03 19.174560611 15.264 15.831 14.897 16.42 16.455 ~ 44 0
30 2MASS J05073067-6908083 pA? 05 07 30.7246467408 -69 08 08.507323248 15.534 16.563 16.656 15.42 16.680 ~ 21 0
31 LHA 120-N 102 PN 05 08 03.3523991256 -68 40 16.560238548 15.580 16.298 15.406 14.86 16.653 ~ 51 0
32 SMP LMC 31 * 05 09 20.2038929256 -67 47 25.099890216 17.001 17.815 17.117 15.470 16.582 ~ 46 0
33 2MASS J05101705-6848224 pA? 05 10 17.059 -68 48 22.42 15.833 16.651 16.023 16.35 17.259 ~ 30 0
34 LHA 120-N 107 PN 05 10 39.6656702832 -68 36 04.807039644 18.464 17.490 16.179 16.33 17.210 ~ 34 0
35 SSTISAGEMC J051102.94-674759.2 pA? 05 11 02.917 -67 47 59.38 16.283 16.902 15.807 15.360 17.494 ~ 40 0
36 LHA 120-N 110 PN 05 11 23.692 -70 01 57.36 15.971 16.222 15.008 15.53 16.678 [WC4] 45 0
37 EC 05147-5727 CV* 05 15 37.5258919656 -57 24 41.016306708 15.17 16.157 16.196     ~ 5 0
38 LHA 120-N 122 PN 05 19 54.6343865856 -69 31 04.997987184 15.479 15.916 15.080 14.84 16.317 ~ 56 0
39 LHA 120-N 123 PN 05 20 09.5114241744 -69 53 39.146648388 15.380 16.445 15.106 15.57 16.095 ~ 51 0
40 LHA 120-N 125 PN 05 20 52.438 -70 09 35.49 17.954 17.555 16.334 16.210 17.202 [WC4-5] 33 0
41 2MASS J05213282-6700045 pA? 05 21 32.8516216920 -67 00 04.750705728 15.688 16.330 15.189   17.142 ~ 39 0
42 [BE74] 568 Em* 05 22 12.815 -69 43 29.01 17.471 18.236 17.759 16.640 16.604 ~ 20 0
43 2MASS J05224097-7119067 pA? 05 22 40.9847158464 -71 19 06.636355716 15.861 16.949 16.625 15.470 16.600 ~ 36 0
44 [BE74] 263 LP* 05 23 31.2614782104 -69 04 08.857743024 16.556 17.359 17.124 16.21 17.502 ~ 48 0
45 LHA 120-N 133 PN 05 24 20.7467383224 -70 05 01.601773404 15.939 16.236 15.368 15.120 16.556 [WC4/5] 88 0
46 IRAS F05258-7343 pA? 05 24 35.9730395808 -73 40 40.240094808   16.48     16.64 WC 65 0
47 LHA 120-N 201 PN 05 24 55.1017509912 -71 32 56.326765848 14.822 15.319 14.240 14.440 15.698 ~ 66 0
48 SV* HV 5824 PN 05 25 26.0089259016 -68 55 53.818836492 15.497 15.946 14.902 15.59 16.714 ~ 53 0
49 AKARI-IRC-V1 J0526064-633703 PN 05 26 06.47 -63 37 03.2     15.68     ~ 11 0
50 SMP LMC 64 pA* 05 27 35.6519960256 -69 08 56.376548880 15.897 16.651 16.408   15.563 ~ 37 0
51 LHA 120-N 53 PN 05 29 15.6693091824 -67 32 47.610463128 15.945 17.093 18.76 16.01 17.264 ~ 45 0
52 IRAS 05312-7046S pA? 05 30 33.1706999016 -70 44 37.905626220 16.348 16.781 15.661 15.830 17.112 ~ 40 0
53 IRAS 05319-7042S pA? 05 31 21.892 -70 40 45.47 15.439 15.842 14.676 14.950 16.530 ~ 47 0
54 2MASS J05332981-7152289 pA? 05 33 29.8030370760 -71 52 28.639071300 15.961 16.327 15.199 15.510 17.082 ~ 36 0
55 LHA 120-N 151 PN 05 33 46.9756693680 -68 36 44.210530548 15.753 16.181 14.927 15.41 16.631 ~ 35 0
56 2MASS J05335609-6753092 pA? 05 33 56.1009323472 -67 53 08.838034296 15.851 16.423 15.508 15.98 16.799 ~ 50 0
57 SMP LMC 77 pA? 05 34 06.262 -69 26 18.25 15.78 16.68 16.235 15.44 16.947 ~ 32 0
58 LHA 120-N 210 EmO 05 34 08.6150910000 -74 20 06.736997868   15.64   15.70 16.87 ~ 24 0
59 SMP LMC 78 PN 05 34 21.186 -68 58 25.30 15.75 15.982 14.90 15.260 16.690 ~ 54 0
60 SMP LMC 80 PN 05 34 38.840 -70 19 56.70 16.424 17.293 16.581 16.680 17.262 ~ 28 0
61 LHA 120-N 211 PN 05 35 20.8611098856 -73 55 30.252448668   16.48     16.99 ~ 28 0
62 2MASS J05365292-7153381 pA? 05 36 52.9771253448 -71 53 38.604485220 15.999 16.611 15.729 15.970 17.066 ~ 35 0
63 LHA 120-N 69 PN 05 40 30.8107868952 -66 17 37.261370940 15.834 16.533 15.711   16.382 [WC8] 55 0
64 2MASS J05423663-7009320 pA? 05 42 36.6517103040 -70 09 32.136387696 16.127 16.158 14.984 14.710 16.796 ~ 42 0
65 MACHO 15.10552.951 Sy* 05 45 19.5266166456 -71 16 06.821141160 16.855 17.413 17.055 15.69 16.957 ~ 44 0
66 LHA 120-S 170 PN 05 54 09.5273462112 -73 02 34.163735712   17.270     13.78 ~ 25 0
67 LM 1-60 PN? 05 59.4 -72 37           ~ 2 0
68 LMC-MA 15 * 06 13 40.6 -64 00 46           ~ 9 0
69 LM 1-64 PN 06 21 04.7093063976 -66 08 00.726299376           ~ 18 0
70 [M94b] 54 PN? 06 41 24.7 -67 01 30   15.020       ~ 4 0
71 WRAY 16-40 PN 09 18 01.3172902776 -54 39 29.165596128   14 15.00     ~ 81 0
72 WRAY 16-86 PN 11 17 43.1561941272 -70 49 32.165781780   12.3 14.00     ~ 46 0
73 IRAS 12238-4907 PN? 12 26 30.4352338799 -49 24 05.529185291           ~ 6 0
74 WRAY 16-125 PN 13 09 36.2390615830 -61 19 35.976251345   14.508 13.517 13.568   B[e] 128 0
75 SDSS J132856.72+310846.0 CV* 13 28 56.7160496376 +31 08 45.995259912   18.02 17.99     O8e 15 1
76 WRAY 16-147 Sy* 14 11 52.0604355768 -51 26 24.187122024     14.20     ~ 240 1
77 * sig Her ** 16 34 06.1824264648 +42 26 13.234150680   4.177 4.196 6.02   B9V 202 0
78 PN DdDm 1 PN 16 40 18.1517248296 +38 42 20.033859348   14.0 13.90     sd+G/K 153 0
79 CD-53 7049 PN 17 03 02.8784604504 -53 55 53.966024508   11.84 11.48     B/Ae 70 1
80 V* V2944 Oph No* 17 29 13.42 -18 46 13.8           ~ 39 0
81 PN Th 4-1 PN 17 46 20.8184146392 -20 13 48.276182748           ~ 38 0
82 PN M 2-24 PN 18 02 02.8945854456 -34 27 47.275175592   15.62 14.60 15.29   ~ 100 0
83 V* V5667 Sgr No* 18 14 25.15 -25 54 34.7           ~ 21 0
84 WRAY 16-400 PN 18 18 09.0281353992 -57 11 13.457492016   12.25 11.57     ~ 21 0
85 PN K 4-8 PN 18 54 20.0197786200 -08 47 33.234394848           ~ 38 0
86 PN MaC 1-15 PN 18 57 13.9267637952 -15 29 13.266211164   16.23 15.41 16.44 16.11 ~ 7 0
87 Hen 2-436 PN 19 32 06.7087636488 -34 12 57.520724796   13.3       [WC4] 84 0
88 Hen 2-437 PN 19 32 57.6040534728 +26 52 43.087922580           ~ 98 1
89 NGC 6807 PN 19 34 33.53 +05 41 02.5     12     ~ 144 0
90 NGC 6833 PN 19 49 46.5667474512 +48 57 40.113276876           ~ 181 0
91 EM* AS 373 Sy* 19 57 05.0166505224 +39 49 36.076143036     11.50   10.592 M6/8e 594 0
92 V* V2659 Cyg No* 20 21 42.3230603346 +31 03 29.401721058           ~ 27 0
93 V* V339 Del No* 20 23 30.6873337580 +20 46 03.765339899   17.50 16.86     ~ 225 0
94 Gaia DR3 2695124138955344128 WD? 21 42 06.8074801248 +03 03 22.262645088           ~ 3 0
95 BD+28 4211 HS* 21 51 11.0221915656 +28 51 50.367627468 8.922 10.25 10.58 10.656 10.831 sdO2VIIIHe5 837 0

To bookmark this query, right click on this link: simbad:objects in 2023A&A...674A.172E and select 'bookmark this link' or equivalent in the popup menu