Data_objects
DataClass
DataClass
Bases: BASE
Standard interface to handle data.
The user-facing object that handles the loading and data access to the spectral data, independently of the instrument. Furthermore, this must be launched as a proxyObject (insert docs here) in order to avoid problems with data syncronization and optimize the speed of the code.
To use this class in SBART RV extraction routines, we place it in shared memory, allowing all processes to easily access
it. This is done with a proxyObject <https://docs.python.org/3.8/library/multiprocessing.html>_.
SBART already provides a DataClass object that is wrapped by a proxyObject:
from ASTRAdata_objects import DataClassManager
manager = DataClassManager()
manager.start()
data_object = manager.DataClass(*args, **kwargs)
This data_object has all the functions that the DataClass object implements!
Source code in src/ASTRA/data_objects/DataClass.py
71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621 622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 680 681 682 683 684 685 686 687 688 689 690 691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 731 732 733 734 735 736 737 738 739 740 741 742 743 744 745 746 747 748 749 750 751 752 753 754 755 756 757 758 759 760 761 762 763 764 765 766 767 768 769 770 771 772 773 774 775 776 777 778 779 780 781 782 783 784 785 786 787 788 789 790 791 792 793 794 795 796 797 798 799 800 801 802 803 804 805 806 807 808 809 810 811 812 813 814 815 816 817 818 819 820 821 822 823 824 825 826 827 828 829 830 831 832 833 834 835 836 837 838 839 840 841 842 843 844 845 846 847 848 849 850 851 852 853 854 855 856 857 858 859 860 861 862 863 864 865 866 867 868 869 870 871 872 873 874 875 876 877 878 879 880 881 882 883 884 885 886 887 888 889 890 891 892 893 894 895 896 897 898 899 900 901 902 903 904 905 906 907 908 909 910 911 912 913 914 915 916 917 918 919 920 921 922 923 924 925 926 927 928 929 930 931 932 933 934 935 936 937 938 939 940 941 942 943 944 945 946 947 948 949 950 951 952 953 954 955 956 957 958 959 960 961 962 963 964 965 966 967 968 969 970 971 972 973 974 975 976 977 978 979 980 981 982 983 984 985 986 987 988 989 990 991 992 993 994 995 996 997 998 999 1000 1001 1002 1003 1004 1005 1006 1007 1008 1009 1010 1011 1012 1013 1014 1015 1016 1017 1018 1019 1020 1021 1022 1023 1024 1025 1026 1027 1028 1029 1030 1031 1032 1033 1034 1035 1036 1037 1038 1039 1040 1041 1042 1043 1044 1045 1046 1047 1048 1049 1050 1051 1052 1053 1054 1055 1056 1057 1058 1059 1060 1061 1062 1063 1064 1065 1066 1067 1068 1069 1070 1071 1072 1073 1074 1075 1076 1077 1078 1079 1080 1081 1082 1083 1084 1085 1086 1087 1088 1089 1090 1091 1092 1093 1094 1095 1096 1097 1098 1099 1100 1101 1102 1103 1104 1105 1106 1107 1108 1109 1110 1111 1112 1113 1114 1115 1116 1117 1118 1119 1120 1121 1122 1123 1124 1125 1126 1127 1128 1129 1130 1131 1132 1133 1134 1135 1136 1137 1138 1139 1140 1141 1142 1143 1144 1145 1146 1147 1148 1149 1150 1151 1152 1153 1154 1155 1156 1157 1158 1159 1160 1161 1162 1163 1164 1165 1166 1167 1168 1169 1170 1171 1172 1173 1174 1175 1176 1177 1178 1179 1180 1181 1182 1183 1184 1185 1186 1187 1188 1189 1190 1191 1192 1193 1194 1195 1196 1197 1198 1199 1200 1201 1202 1203 1204 1205 1206 1207 1208 1209 1210 1211 1212 1213 1214 1215 1216 1217 1218 1219 1220 1221 1222 | |
extra_loading_functions: Dict[str, Callable] = {'CARMENES': load_CARMENES_extra_information, 'POET': load_POET_extra_information}
class-attribute
instance-attribute
sigma_clip_RVs = sigma_clip_RVs
instance-attribute
input_file = input_files
instance-attribute
observations: List[Frame, ...] = []
instance-attribute
metaData = MetaData()
instance-attribute
frameID_map = defaultdict(list)
instance-attribute
Target = Target(self.collect_KW_observations('OBJECT', self._inst_type.sub_instruments, include_invalid=False), original_name=target_name, target_dictionary_path=target_dictionary_path)
instance-attribute
StellarModel = None
instance-attribute
construct_subInstruments_by_obID() -> None
Create new sub-Instruments with the obID of the observations
Source code in src/ASTRA/data_objects/DataClass.py
add_data_from_instrument(input_files: Iterable[UI_PATH], instrument: Type[Frame], reject_subInstruments: Iterable[str] | None = None, custom_subIns_name: str | None = None, instrument_options: dict[str, Any] | None = None) -> None
Source code in src/ASTRA/data_objects/DataClass.py
get_extra_loading_functions()
load_previous_SBART_results(RV_holder, use_merged_cube: bool = False)
Load results of SBART run, store RV and uncertainty inside corresponding Frame object.
Source code in src/ASTRA/data_objects/DataClass.py
reject_order_region_from_frame(frameID: int, order: int, region)
Source code in src/ASTRA/data_objects/DataClass.py
remove_activity_lines(lines: Indicators) -> None
Find the wavelength windows in which activity-related lines are expected to appear.
This is done for all valid observations
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
lines
|
Indicators
|
Object with the wavelength blocks "original" positions. |
required |
Source code in src/ASTRA/data_objects/DataClass.py
remove_telluric_features(Telluric_Template: TelluricModel) -> None
Source code in src/ASTRA/data_objects/DataClass.py
replace_frames_with_S2D_version(new_shape: Optional[Tuple[int, int]] = None)
In-place substitution of all frames with their S2D-compatible shapes.
Source code in src/ASTRA/data_objects/DataClass.py
ingest_StellarModel(Stellar_Model: StellarModel) -> None
Source code in src/ASTRA/data_objects/DataClass.py
reject_observations(conditions: CondModel) -> None
Apply the conditions to evaluate if the VALID frame meets the specified conditions or not.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
conditions
|
ConditionModel
|
Conditions set by the user |
required |
Source code in src/ASTRA/data_objects/DataClass.py
get_Target() -> Target
load_frame_by_ID(frameID: int) -> int
set_all_as_Zscore_frames() -> None
normalize_all() -> None
Launch the normalization for all (valid) frames.
Source code in src/ASTRA/data_objects/DataClass.py
update_uncertainties_of_frame(frameID: int, new_uncerts) -> None
Update the flux uncertainties of a given frame.
.. warning:: This will change your measured data, be careful with this!!!
Source code in src/ASTRA/data_objects/DataClass.py
normalize_all_from_subInst(subInst: str) -> None
Normalize all (valid) frames from a given subInstrument.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
subInst
|
str
|
|
required |
Source code in src/ASTRA/data_objects/DataClass.py
scale_up_all_observations(factor: float) -> None
Multiply the flux and uncertainties by a given flux level (avoid possible SNR issues).
Source code in src/ASTRA/data_objects/DataClass.py
set_stellar_RV_to_zero() -> None
Allow to override the stellar RV so that it is fixed to zero.
load_all_from_subInst(subInst: str) -> int
Load all valid frames from a given subInstrument.
Source code in src/ASTRA/data_objects/DataClass.py
close_frame_by_ID(frameID: int) -> int
min_pixel_in_order() -> int
get_subInst_from_frameID(frameID: int) -> str
get_frame_OBS_order(frameID: int, order: int, include_invalid: bool = False)
Request the data from one spectral order.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
frameID
|
int
|
FrameID of the observation |
required |
order
|
int
|
NUmber of order |
required |
include_invalid
|
bool
|
Orders can also be flagged as "invalid". If False, the frame will raise an error when requesting the data |
False
|
Source code in src/ASTRA/data_objects/DataClass.py
update_interpol_properties_of_all_frames(new_properties: Dict[str, Any])
Source code in src/ASTRA/data_objects/DataClass.py
update_interpol_properties_of_stellar_model(new_properties: Dict[str, Any])
Source code in src/ASTRA/data_objects/DataClass.py
update_frame_interpol_properties(frameID, new_properties) -> None
Allow to update the interpolation settings from the outside, so that any object can configure the interpolation as it wishes
Source code in src/ASTRA/data_objects/DataClass.py
interpolate_frame_order(frameID, order, new_wavelengths, shift_RV_by, RV_shift_mode, include_invalid=False)
Interpolate a given order to a new wavelength solution
Source code in src/ASTRA/data_objects/DataClass.py
get_frame_arrays_by_ID(frameID: int)
Access data from the entire spectral range (i.e. all orders come as a matrix)
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
frameID
|
int
|
|
required |
Source code in src/ASTRA/data_objects/DataClass.py
get_KW_from_frameID(KW: str, frameID: int, use_header: bool = False) -> Any
Get Keywrod value from a given frame
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
KW
|
str
|
ASTRA compatible keyword, as defined in the Frame class |
required |
frameID
|
int
|
Selected ID of teh frame |
required |
use_header
|
bool
|
If True, searches for the KW in the header of the fits file, by default False |
False
|
Returns:
| Type | Description |
|---|---|
Any
|
Value from the header |
Source code in src/ASTRA/data_objects/DataClass.py
get_filename_from_frameID(frameID: int, full_path: bool = False) -> str | Path
Get the filename from a frame
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
frameID
|
int
|
ID of the frame that we want to select |
required |
full_path
|
bool
|
If True, returns the full disk file, by default False |
False
|
Returns:
| Type | Description |
|---|---|
str | Path
|
Either the filename (string) of the full path (Path) |
Source code in src/ASTRA/data_objects/DataClass.py
get_status_by_frameID(frameID: int) -> Status
collect_KW_observations(KW: str, subInstruments: Union[tuple, list], include_invalid: bool = False, conditions: CondModel = None, return_frameIDs: bool = False, from_header: bool = False, pad_condition_rejected: bool = True) -> Union[list, Tuple[List[float], List[int]]]
Parse through the loaded observations and retrieve a specific KW from all of them.
There is no sort of the files. The output will follow the order of the files loaded in memory.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
return_frameIDs
|
bool
|
|
False
|
KW
|
str
|
KW from the Frame.observation_info dictionary |
required |
subInstruments
|
Union[tuple, list]
|
List of the subInstruments for which we want to retrieve the KW. If there are multiple entries, the output will follow the order of this list |
required |
include_invalid
|
bool
|
If True, also retrieve the KWs of Frames deemed to not be valid. By default False |
False
|
from_header
|
bool
|
If True, searches the fits header, rather than the internal keywords. By default, False |
False
|
Returns:
| Type | Description |
|---|---|
list
|
List of the KW |
Source code in src/ASTRA/data_objects/DataClass.py
collect_RV_information(KW: str, subInst: str, frameIDs=None, include_invalid: bool = False, units=None, as_value: bool = True) -> list
Return the RV measurements (or BERV) from the observations of a given sub-Instrument.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
KW
|
KW to request
|
previousRV, previousRV_ERR or BERV |
required |
subInst
|
str
|
Name of the sub-Instrument |
required |
frameIDs
|
None | list
|
If not None, retrive only for the frameIDs inside the list. If they are not from subInst, an exception will be raised |
None
|
include_invalid
|
bool
|
Include invalid observations, by default False |
False
|
units
|
[type]
|
units to convert the measurements, by default None |
None
|
as_value
|
bool
|
provide a value instead of "units", by default True |
True
|
Returns:
| Type | Description |
|---|---|
list
|
[description] |
Raises:
| Type | Description |
|---|---|
InvalidConfiguration
|
[description] |
Source code in src/ASTRA/data_objects/DataClass.py
get_valid_frameIDS() -> list[int]
Get list of all available frame IDs (across all subInstruments).
Returns:
| Type | Description |
|---|---|
list
|
[description] |
Source code in src/ASTRA/data_objects/DataClass.py
get_invalid_frameIDs(subinstrument: None | str = None) -> list[int]
Get a list of the invalid frameIDs (by default, all of them).
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
subinstrument
|
None | str
|
subinstrument (None | str): If not None, returrns only for this subInstrument, by default None |
None
|
Returns:
| Type | Description |
|---|---|
list[int]
|
List of invalid frameIDs |
Source code in src/ASTRA/data_objects/DataClass.py
get_frameIDs_from_subInst(subInstrument: str, include_invalid: bool = False) -> list[int]
Get all frameIDs associated with a given instrument. By default, only returns the valid ones.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
subInstrument
|
str
|
SubInstrument name |
required |
include_invalid
|
bool
|
If True, also return IDs associated with the invalid frames, by default False |
False
|
Returns:
| Type | Description |
|---|---|
list
|
List of frameIDs from the instrument |
Source code in src/ASTRA/data_objects/DataClass.py
get_frame_by_ID(frameID: int) -> Frame
Get a frame by its ID
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
frameID
|
int
|
ID of the frame |
required |
Returns:
| Type | Description |
|---|---|
Frame
|
Desired Frame |
Raises:
| Type | Description |
|---|---|
NoDataError
|
If the frameID doesn't exist |
Source code in src/ASTRA/data_objects/DataClass.py
get_subInstruments_with_valid_frames() -> list[str]
Find all subInstruments that have at least one valid observation.
Source code in src/ASTRA/data_objects/DataClass.py
get_available_subInstruments() -> list[str]
get_instrument_information() -> dict
get_stellar_template(subInst: str) -> StellarTemplate
get_stellar_model() -> StellarModel
get_metaData() -> MetaData
get_internalPaths()
trigger_data_storage() -> None
Source code in src/ASTRA/data_objects/DataClass.py
has_instrument_data(instrument: str) -> bool
show_loadedData_table() -> Table
Compute the number of observations available in each subInstrument.
Find the number of valid (with and without warnings) and the invalid ones!
Source code in src/ASTRA/data_objects/DataClass.py
plot_quantity(xx_var: str, yy_var: str, axis=None, return_fig_and_axis: bool = False, show: bool = False, condition: None | CondModel = None)
Plot any quantity from the frames against each other.
Source code in src/ASTRA/data_objects/DataClass.py
load_instrument_extra_information() -> None
See if the given instrument is one of the ones that has extra information to load.
If so, then calls the relevant function.
Source code in src/ASTRA/data_objects/DataClass.py
add_extra_loading_information(name: str, loader: Callable) -> None
classmethod
Add a new loader function to run after the Instrument loads its data.
Args: name (str): Instrument name loader (Callable): function to run afterwards
Source code in src/ASTRA/data_objects/DataClass.py
hash_path_to_int(fname: Path, algo: str = 'sha256', bits: int = 32) -> int
Deterministic integer hash of a filesystem path.
- Uses hashlib (default sha256)
- Returns an integer, truncated to bits if specified
Source code in src/ASTRA/data_objects/DataClass.py
MetaData
Collect metadata from the loaded Frames.
MetaData
Class to hold metadata information of the processed data.
The Frames, when loading data from disk will collect information to work as MetaData, which will be used to provide an option of avoiding the repeated computation of exactly the same dataset. This class provides an easy interface to hold such data, write and load it to disk, and compare equality between two MetaData objects.
The data stored inside this object is divided by subInstruments, with each having a unique set of values, that is not shared with other subInstruments. Comparisons of equality are supported at the subInstrument level.
Source code in src/ASTRA/data_objects/MetaData.py
15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 | |
information = {} if data_to_hold is None else data_to_hold
instance-attribute
subInstrument_comparison(other: MetaData, subInstrument: str) -> bool
Compare the Metadata of a given subInstrument.
Checks that must pass for equality:
- The same keys are present in the two objects
- A given key has the same value in the two objects
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
other
|
MetaData
|
Other MetaData object |
required |
subInstrument
|
str
|
SubInstrument to compare |
required |
Returns:
| Name | Type | Description |
|---|---|---|
comparison_result |
bool
|
True if the MetaData matchess |
Source code in src/ASTRA/data_objects/MetaData.py
store_json(path: Path) -> None
Store the class as a json files.
Args: path (Path):Path in which this object will be stored
Source code in src/ASTRA/data_objects/MetaData.py
add_info(key: str, info: str | tuple | list, subInstrument: str) -> None
Add a new metric to be tracked, with the values being collected over all available frames.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
key
|
str
|
Name of the metric |
required |
info
|
str | tuple | list
|
data to be stored |
required |
subInstrument
|
str
|
subInstrument to which the info belongs to |
required |
Raises:
| Type | Description |
|---|---|
TypeError
|
If the info is not a list nor an iterable |
Source code in src/ASTRA/data_objects/MetaData.py
load_from_json(path: Path) -> MetaData
classmethod
Load from a json file.
Source code in src/ASTRA/data_objects/MetaData.py
Target
Representation of the star, used to query SIMBAD.
Target
Represents an observed object.
This class provides an interface to handle data sanitization and simbad lookups for the targets that we load from the S2D files.
TODO list: - [ ] Allow for the comparison of two different targets - [ ] Improve docs and interfaces of the class
Source code in src/ASTRA/data_objects/Target.py
15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 | |
to_replace = {'NAME': '', 'star': ''}
instance-attribute
extra_KW = {'KOBE-': '', 'HD-': 'HD', ' ': ''}
instance-attribute
KOBE_alias = {}
instance-attribute
secular_acceleration: RV_measurement
property
Return the secular accelaration of the target star.
true_name: str
property
Return the name of a target that is extracted from the header of the .fits files.
This name can be overriden if the user provides a new name when instantiating this object
original_name: str
property
Name that was present in the header of the files.
This will disregard any kind of user-provided name
json_ready: Dict[str, Any]
property
Data in json-compatible fmt.
clean_targ_list(target_list: list[str]) -> list[str]
Process all names to generate clean ones.
Source code in src/ASTRA/data_objects/Target.py
validate_target_list(targets: list[str]) -> None
Raise warning if we are using different targ names.
Source code in src/ASTRA/data_objects/Target.py
searchable_name(star: str) -> str
Transform star name in one that is recognized by SIMBAD.