Galaxies with good spectroscopic redshifts Virtual Observatory Resource

Authors
  1. Euclid Collaboration
  2. Saglia R.
  3. De Nicola S.
  4. Fabricius M.
  5. Guglielmo V.,Snigula J.
  6. Zoller R.
  7. Bender R.
  8. Heidt J.
  9. Masters D.
  10. Stern D.,Paltani S.
  11. Amara A.
  12. Auricchio N.
  13. Baldi M.
  14. Bodendorf C.
  15. Bonino D.,Branchini E.
  16. Brescia M.
  17. Brinchmann J.
  18. Camera S.
  19. Capobianco V.,Carbone C.
  20. Carretero J.
  21. Castellano M.
  22. Cavuoti S.
  23. Cledassou R.,Congedo G.
  24. Conselice C.J.
  25. Conversi L.
  26. Copin Y.
  27. Corcione L.
  28. Courbin F.,Cropper M.
  29. Da Silva A.
  30. Degaudenzi H.
  31. Douspis M.
  32. Dubath F.,Duncan C.A.J.
  33. Dupac X.
  34. Dusini S.
  35. Farrens S.
  36. Frailis M.
  37. Franceschi E.,Galeotta S.
  38. Garilli B.
  39. Gillard W.
  40. Gillis B.
  41. Giocoli C.
  42. Grazian A.,Grupp F.
  43. Haugan S.V.H.
  44. Hoekstra H.
  45. Holmes W.
  46. Hormuth F.
  47. Hornstrup A.,Jahnke K.
  48. Kummel M.
  49. Kermiche S.
  50. Kiessling A.
  51. Kunz M.
  52. Kurki-suonio H.,Laureijs R.
  53. Ligori S.
  54. Lilje P.B.
  55. Lloro I.
  56. Maiorano E.
  57. Marggraf O.,Markovic K.
  58. Marulli F.
  59. Massey R.
  60. Mccracken H.J.
  61. Melchior M.
  62. Meylan G.,Moresco M.
  63. Moscardini L.
  64. Munari E.
  65. Niemi S.M.
  66. Padilla C.
  67. Pasian F.,Pedersen K.
  68. Percival W.J.
  69. Pettorino V.
  70. Pires S.
  71. Poncet M.
  72. Popa L.,Pozzetti L.
  73. Raison F.
  74. Renzi A.
  75. Rhodes J.
  76. Riccio G.
  77. Romelli E.,Rossetti E.
  78. Sapone D.
  79. Sartoris B.
  80. Schneider P.
  81. Secroun A.
  82. Seidel G.,Sirignano C.
  83. Sirri G.
  84. Stanco L.
  85. Tallada-Crespi P.
  86. Tavagnacco D.,Taylor A.N.
  87. Tereno I.
  88. Toledo-moreo R.
  89. Torradeflot F.
  90. Tutusaus I.,Valentijn E.A.
  91. Valenziano L.
  92. Vassallo T.
  93. Wang Y.
  94. Zacchei A.,Zamorani G.
  95. Zoubian J.
  96. Andreon S.
  97. Bardelli S.
  98. Gracia-carpio J.,Maino D.
  99. Mauri N.
  100. Tramacere A.
  101. Zucca E.
  102. Alvarez Ayllon A.
  103. Aussel H.,Baccigalupi C.
  104. Balaguera-Antolinez A.
  105. Ballardini M.
  106. Biviano A.,Bolzonella M.
  107. Bozzo E.
  108. Burigana C.
  109. Cabanac R.
  110. Cappi A.
  111. Carvalho C.S.,Casas S.
  112. Castignani G.
  113. Cooray A.
  114. Coupon J.
  115. Courtois H.M.
  116. Davini S.,Desprez G.
  117. Dole H.
  118. Escartin J.A.
  119. Escoffier S.
  120. Farina M.
  121. Fotopoulou S.,Ganga K.
  122. Garcia-bellido J.
  123. George K.
  124. Giacomini F.
  125. Gozaliasl G.,Hildebrandt H.
  126. Hook I.
  127. Ilbert O.
  128. Kansal V.
  129. Kashlinsky A.
  130. Keihanen E.,Kirkpatrick C.C.
  131. Loureiro A.
  132. Macias-Perez J.
  133. Magliocchetti M.,Mainetti G.
  134. Maoli R.
  135. Martinelli M.
  136. Martinet N.
  137. Metcalf R.B.,Morgante G.
  138. Nadathur S.
  139. Nucita A.A.
  140. Patrizii L.
  141. Popa V.
  142. Porciani C.,Potter D.
  143. Pourtsidou A.
  144. Reimberg P.
  145. Sanchez A.G.
  146. Sakr Z.
  147. Schirmer M.,Sefusatti E.
  148. Sereno M.
  149. Stadel J.
  150. Teyssier R.
  151. Valieri C.
  152. Valiviita J.,Veropalumbo A.
  153. Viel M.
    154. Published by
    CDS
Abstract

The Complete Calibration of the Color-Redshift Relation survey (C3R2) is a spectroscopic program designed to empirically calibrate the galaxy color-redshift relation to the Euclid depth (I_E_=24.5), a key ingredient for the success of Stage IV dark energy projects based on weak lensing cosmology. A spectroscopic calibration sample that is as representative as possible of the galaxies in the Euclid weak lensing sample is being collected, selecting galaxies from a self-organizing map (SOM) representation of the galaxy color space. Here, we present the results of a near-infrared H- and K-band spectroscopic campaign carried out using the LUCI instruments at the LBT. For a total of 251 galaxies, we present new highly reliable redshifts in the 1.3<=z<=1.7 and 2<=z<=2.7 ranges. The newly-determined redshifts populate 49 SOM cells that previously contained no spectroscopic measurements and almost twice the occupation numbers of an additional 153 SOM cells. A final optical ground-based observational effort is needed to calibrate the missing cells, in particular in the redshift range 1.7<=z<=2.7, which lack spectroscopic calibration. In the end, Euclid itself will deliver telluric-free near-IR spectra that can complete the calibration.

Keywords
  1. galaxies
  2. visible-astronomy
  3. redshifted
Bibliographic source Bibcode
2022A&A...664A.196E
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/664/A196
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/664/A196
Document Object Identifer DOI
doi:10.26093/cds/vizier.36640196

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/664/A196
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/664/A196
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/664/A196
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/664/A196/tableb1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/664/A196/tableb1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/664/A196/tableb1?

History

2023-02-22T12:38:34Z
Resource record created
2023-02-22T12:38:34Z
Created
2023-10-06T13:59:46Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr