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

被引：6

作者：

Paterson, K. ^{[1
]}

Schirmer, M. ^{[1
]}

Copin, Y. ^{[2
]}

Cuillandre, J. -C. ^{[3
]}

Gillard, W. ^{[4
]}

Gutierrez Soto, L. A. ^{[5
,6
]}

Guzzo, L. ^{[7
,8
,9
]}

Hoekstra, H. ^{[10
]}

Kitching, T. ^{[11
]}

Paltani, S. ^{[12
]}

Percival, W. J. ^{[13
,14
,15
]}

Scodeggio, M. ^{[16
]}

Stanghellini, L. ^{[17
]}

Appleton, P. N. ^{[18
,19
]}

Laureijs, R. ^{[20
]}

Mellier, Y. ^{[21
,22
,23
,24
]}

Aghanim, N. ^{[25
]}

Altieri, B. ^{[26
]}

Amara, A. ^{[27
]}

Auricchio, N. ^{[28
]}

Baldi, M. ^{[28
,29
,30
]}

Bender, R. ^{[31
,32
]}

Bodendorf, C. ^{[31
]}

Bonino, D. ^{[33
]}

Branchini, E. ^{[34
,35
]}

Brescia, M. ^{[36
]}

Brinchmann, J. ^{[37
]}

Camera, S. ^{[33
,38
,39
]}

Capobianco, V. ^{[33
]}

Carbone, C. ^{[16
]}

Carretero, J. ^{[40
,41
]}

Castander, F. J. ^{[42
,43
]}

Castellano, M. ^{[44
]}

Cavuoti, S. ^{[45
,46
]}

Cimatti, A. ^{[47
]}

Cledassou, R. ^{[48
,49
]}

Congedo, G. ^{[50
]}

Conselice, C. J. ^{[51
]}

Conversi, L. ^{[26
,52
]}

Corcione, L. ^{[33
]}

Courbin, F. ^{[53
]}

Da Silva, A. ^{[54
,55
]}

Degaudenzi, H. ^{[12
]}

Dinis, J. ^{[54
,55
]}

Douspis, M. ^{[25
]}

Dubath, F. ^{[12
]}

Dupac, X. ^{[26
]}

Ferriol, S. ^{[2
]}

Frailis, M. ^{[56
]}

Franceschi, E. ^{[28
]}

机构：

[1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[2] Univ Lyon, Univ Claude Bernard Lyon 1, CNRS IN2P3, IP2I Lyon,UMR 5822, F-69622 Villeurbanne, France

[3] Univ Paris Saclay, Univ Paris, CNRS, AIM,CEA, F-91191 Gif Sur Yvette, France

[4] Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France

[5] Univ Sao Paulo, Dept Astron, IAG, Rua Matao 1226, BR-05509900 Sao Paulo, Brazil

[6] Inst Astrofis La Plata CCT La Plata CONICET UNLP, B1900FWA, La Plata, Argentina

[7] Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy

[8] INAF Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy

[9] INFN Sez Milano, Via Celoria 16, I-20133 Milan, Italy

[10] Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands

[11] Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England

[12] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[13] Univ Waterloo, Ctr Astrophys, Waterloo, ON N2L 3G1, Canada

[14] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada

[15] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada

[16] INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy

[17] NSFs NOIR, Lab 950 N Cherry Ave, Tucson, AZ 85719 USA

[18] Caltech IPAC, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[19] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

[20] European Space Agcy ESTEC, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands

[21] Inst Astrophys Paris, 98Bis Blvd Arago, F-75014 Paris, France

[22] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France

[23] Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France

[24] CEA Saclay, DFR IRFU, Serv Astrophys, Bat 709, F-91191 Gif Sur Yvette, France

[25] Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France

[26] ESAC ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain

[27] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[28] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy

[29] Univ Bologna, Dipartimento Fis Astron Augusto Righi Alma Mater, Via Piero Gobetti 93-2, I-40129 Bologna, Italy

[30] INFN Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[31] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

[32] Univ Munich, Fak Phys, Scheinerstr 1, D-81679 Munich, Germany

[33] INAF Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy

[34] Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy

[35] INFN Sez Roma Tre, Via Vasca Navale 84, I-00146 Rome, Italy

[36] Univ Federico II, Dept Phys E Pancini, Via Cinthia 6, I-80126 Naples, Italy

[37] Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, PT-4150762 Porto, Portugal

[38] Univ Turin, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy

[39] INFN Sez Torino, Via P Giuria 1, I-10125 Turin, Italy

[40] IFAE, Barcelona Inst Sci & Technol, Campus UAB, Bellaterra 08193, Barcelona, Spain

[41] Port Informacio Cient, Campus UAB C Albareda S-N, Bellaterra 08193, Barcelona, Spain

[42] Inst Space Sci ICE, CSIC, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain

[43] IEEC, Carrer Gran Capita 2-4, Barcelona 08034, Spain

[44] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[45] INAF Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy

[46] INFN Sect Naples, Via Cinthia 6, I-80126 Naples, Italy

[47] Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[48] Ctr Spatial Toulouse, Ctr Natl Etud Spatiales, 18 Ave Edouard Belin, F-31401 Toulouse 9, France

[49] Inst Natl Phys Nucl & Phys Particules, 3 Rue Michel Ange, F-75794 Paris 16, France

[50] Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

来源：

ASTRONOMY & ASTROPHYSICS | 2023年 / 674卷

关键词：

instrumentation: spectrographs; space vehicles: instruments; planetary nebulae: general; UPDATED EDLEN EQUATION; REFRACTIVE-INDEX; EMISSION-LINES; X-SHOOTER; CATS EYE; EVOLUTION; CATALOG; STARS; SPECTROGRAPH; POPULATION;

D O I：

10.1051/0004-6361/202346252

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Euclid mission will conduct an extragalactic survey over 15 000 deg(2) of the extragalactic sky. The spectroscopic channel of the Near-Infrared Spectrometer and Photometer (NISP) has a resolution of R similar to 450 for its blue and red grisms that collectively cover the 0.93-1.89 mu m range. NISP will obtain spectroscopic redshifts for 3 x 10(7) galaxies for the experiments on galaxy clustering, baryonic acoustic oscillations, and redshift space distortion. The wavelength calibration must be accurate within 5 angstrom 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 mu m 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 mu m 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 angstrom in the optical and 0.3 angstrom in the near-infrared. The wavelength atlas and the related 1D and 2D spectra are made publicly available.

引用

页数：32

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