About the author xi
Acknowledgements xiii
1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1
1.1 The goal of this book 1
1.2 Prerequisites in astronomy 2
1.3 Units, conventions and physical values in spectroscopy 3
1.3.1 Wavelengths . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3
1.3.2 Spectral resolution of a spectrograph . . . . . . . . . . . . . . . . . . . . . . . . 3
1.3.3 Wavelength ranges . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4
1.3.4 The ADU . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
1.3.5 1D and 2D files . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
1.3.6 Binning area . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
1.3.7 Sky background subtraction areas . . . . . . . . . . . . . . . . . . . . . . . . . . 5
1.3.8 Coordinates of a celestial object . . . . . . . . . . . . . . . . . . . . . . . . . . . 6
1.3.9 Bias, darks, flats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6
1.3.10 The F/D ratio . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
1.4 The spectrographs 7
1.4.1 Building your own spectrograph . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
1.4.2 Buying a spectrograph . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
1.4.3 The spectrographs used in this book . . . . . . . . . . . . . . . . . . . . . . . . 10
1.4.4 The Star Analyser . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
1.4.5 The Alpy 600 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11
1.4.6 The LISA . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
1.4.7 The UVEX . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
1.4.8 The LHIRES III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14
1.4.9 The eShel . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16
1.5 Spectrography software 17
1.5.1 Visual Spec . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
1.5.2 ISIS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
1.5.3 Demetra . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
1.5.4 Spec INTI . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18
2 The temperature of stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
2.1 The spectral classes 19
2.2 Selecting targets 24
2.3 Spectra production 26
2.4 Highlighting the results 28
2.5 Estimating the temperature of a star 31
2.6 Bibliography 35
3 Redshift of galaxies and quasars . . . . . . . . . . . . . . . . . . . . . 37
3.1 A brief history 37
3.2 Choice of targets 40
3.3 Making a galaxy spectrum 43
3.3.1 Non-point target . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
3.3.2 Point target . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46
3.4 The calculation methods 46
3.5 Example with NGC 7469 49
3.6 Identifying the spectral lines of the galaxy NGC 7469 50
3.7 Correcting the heliocentric velocity spectrum 51
3.8 Measuring spectral line positions 54
3.9 Major redshifts: z >1 the quasar of "Andromeda parachute" 56
3.10 The case of special galaxies 59
3.11 Find the intruder 61
3.12 Redshift measurement frame of reference 62
3.13 Bibliography 63
4 Spectro-imaging of nebulae . . . . . . . . . . . . . . . . . . . . . . . . . 65
4.1 Principles of spectro-imaging 66
4.2 Target selection 67
4.3 Practical case on M57 71
4.4 Spectral sequence processing 73
4.5 Image reconstruction 76
4.6 M57 at various wavelengths 81
4.7 Making science with planetary nebulae 82
4.8 Reddening correction applied to a spectrum 84
4.9 The Balmer decrement 86
4.10 Balmer decrement represented on an image 89
4.11 Calculating the electronic temperature 92
4.12 The electronic temperature map of a nebula 96
4.13 Calculating electron density 98
4.14 The density map of a nebula 100
4.15 Bibliography 100
5 Tracking Be stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
5.1 Observe the Be stars 105
5.1.1 Medium and high resolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 106
5.1.2 Echelle-type spectrographs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 106
5.1.3 Low resolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
5.2 Selecting targets for observation: the BeSS database 108
5.3 Submit your first spectrum to BeSS database 109
5.4 The various profiles of Be stars 112
5.5 Detecting an outburst 114
5.6 Long-term measurement and monitoring 115
5.7 Measuring the V and R peaks of a spectral line 124
5.8 Measurement of equivalent width (EW) 125
5.9 Bibliography 130
6 Spectra of novae and supernovae . . . . . . . . . . . . . . . . . . . 133
6.1 Nova or supernova? 133
6.2 Where to find information? 134
6.3 Novae 135
6.4 Observing the spectrum of a nova 138
6.4.1 Low-resolution spectra . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
6.4.2 Medium/high resolution spectra . . . . . . . . . . . . . . . . . . . . . . . . . . 140
6.5 The P Cyg profile 141
6.6 Converting a wavelength graph into a velocity graph 142
6.6.1 Using ISIS software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143
6.6.2 With a Python script . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144
6.7 A practical case study with the nova V339 Del 145
6.8 Supernovae 150
6.8.1 Type Ia supernovae . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 151
6.8.2 Other types of supernovae . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152
6.9 Supernova spectrum acquisition 154
6.10 Example with SN 2021 pit 155
6.11 Calculating the velocity of the supernova ejecta 158
6.12 Bibliography 161
7 Confirming a planetary nebula . . . . . . . . . . . . . . . . . . . . . . 163
7.1 The story of the LDu 1 planetary nebula 164
7.2 How to confirm a planetary nebula? 171
7.3 Some examples of the spectra obtained 172
7.3.1 Pre 24 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 173
7.3.2 Ra 69 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175
7.3.3 Hu 6 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177
7.3.4 DeGaPe 32 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178
7.3.5 Pa 30, a very strange object... . . . . . . . . . . . . . . . . . . . . . . . . . . . . 179
7.4 Bibliography 183
8 Measuring rotational velocities . . . . . . . . . . . . . . . . . . . . . . 187
8.0.1 Influence of the rotation axis inclination . . . . . . . . . . . . . . . . . . . . 188
8.1 The rotation of the planets 189
8.2 Practical case study with Jupiter 190
8.3 The rotation of Saturn and its rings 195
8.4 Full width at half maximum of a line (FWHM) 198
8.5 Measurement of rotational velocities based on its FWHM 202
8.6 The rotation of a Be star’s disk 203
8.7 The rotation of matter near a black hole in a galaxy 208
8.8 The rotation of the arms of the M77 galaxy 212
8.8.1 Conversion of distance in pixels / distance in parsecs . . . . . . . . . 217
8.8.2 A clue to dark matter? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 220
8.9 Bibliography 221
9 Time series in spectroscopy . . . . . . . . . . . . . . . . . . . . . . . . . 225
9.1 Dynamic 2D graphics 226
9.2 BW Vul, a short-period pulsating star 229
9.2.1 Processing a series with ISIS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 231
9.3 Study RR Lyr 234
9.4 Study the flickering of spectral lines 237
9.5 Bibliography 242
10 Spectroscopic binaries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 245
10.1 Principle of measuring spectroscopic binaries 245
10.2 A bit of history 247
10.3 Observe a spectroscopic binary star 249
10.4 Practical case study based on Mizar A 251
10.5 Order the spectra according to phase 252
10.6 The spectral evolution of Mizar A 254
10.7 Measuring the period of a spectroscopic binary: the periodogram 256
10.8 The eccentricity of an orbit 261
10.9 HIP 45080, a binary star with low eccentricity 263
10.10 HIP 26241, a highly eccentric binary star 264
10.11 3D printing of the period of a spectroscopic binary 266
10.12 Bibliography 270
11 Measuring filters, slits and more... . . . . . . . . . . . . . . . . . . . . 273
11.1 WARNING: Precautions to be taken! 274
11.2 Building your own filter test bench 275
11.3 The Lab’Ex with an Alpy 600 or a Star’Ex? 276
11.4 The light module 278
11.5 Measuring the bandwidth of a filter 279
11.6 Practical case with 3 narrowband SHO filters 281
11.7 Measuring a light source 284
11.8 The spectral signature of a liquid 286
11.9 Measuring the width of a slit 288
11.10 Bibliography 291
