Column 1 string | Column 2 float64 | Column 3 float64 | Column 4 float64 |
|---|---|---|---|
data1 | 3,626.089808 | 1,150.233047 | 1,615.803566 |
data2 | 5,560.852691 | 1,232.39255 | 1,561.030564 |
data3 | 5,131.142558 | 958.527539 | 1,122.846546 |
data4 | 2,530.63483 | 410.797517 | 438.184018 |
data5 | 1,569.773342 | 219.092009 | 246.47851 |
data6 | 1,810.767597 | 356.024515 | 383.411016 |
data7 | 2,211.972252 | 273.865011 | 356.024515 |
data8 | 1,735.898062 | 301.251512 | 356.024515 |
data9 | 1,614.299353 | 301.251512 | 328.638013 |
data10 | 1,628.339699 | 356.024515 | 410.797517 |
data11 | 2,485.826174 | 246.47851 | 301.251512 |
data12 | 1,553.017288 | 273.865011 | 273.865011 |
data13 | 1,135.057225 | 246.47851 | 273.865011 |
data14 | 676.770102 | 246.47851 | 273.865011 |
data15 | 937.237173 | 328.638013 | 356.024515 |
data16 | 757.860013 | 602.503025 | 657.276027 |
VSA February 2004 released products
This dataset contains LAMBDA's February 2004 VSA spectrum, x factors,
16 window functions, and 16×16 Hessian matrix. Source identifiers, numeric
values, shapes, and row order are retained. Unlabelled source columns remain
Column 1, Column 2, and so on.
Use
python -m venv .venv && .venv/bin/pip install datasets huggingface_hub pyarrow
from datasets import load_dataset
spectrum = load_dataset("astro-legacy-archive/vsa-released-products", "VSAF", split="train[:5]")
print(spectrum.column_names, spectrum.num_rows)
Output:
['Column 1', 'Column 2', 'Column 3', 'Column 4'] 5
import json
import pyarrow.parquet as pq
from huggingface_hub import hf_hub_download
path = hf_hub_download("astro-legacy-archive/vsa-released-products", "VSAF_mat.parquet", repo_type="dataset")
print(json.loads(pq.read_schema(path).metadata[b"dense_matrix"])["array"]["shape"])
Output:
[16, 16]
Structure and decode guidance
There are 19 configurations:
VSAFhas 16 rows.Column 1contains the source keysdata1throughdata16verbatim.Column 2is the CMB band-powerT0^2 l(l+1)C_l/(2pi);Column 3andColumn 4are the magnitudes of its asymmetric lower and upper 68-percent likelihood errors. The three numeric columns are inuK^2. The source does not label its columns, so their numbered names remain unchanged.VSAF1throughVSAF16are the 16 unequal-length window-function tables. In each,Column 1is multipolelandColumn 2is the corresponding band-window value. The files state no units.VSAF_xhas 16 rows and one source column,Column 1: the offset-lognormalx_iin source band order and inuK^2.VSAF_matis a dense matrix with 16 Parquet rows. Its sole column,VSAF_mat, contains the rows of the source 16×16 HessianM_ijin log-offset variables. No unit or axis names are documented.
Every configuration embeds its complete source-backed per-column descriptions,
units, source URL, source SHA-256, and requested credit in Parquet schema
metadata. The table configurations use the statistical_product metadata key;
VSAF_mat uses dense_matrix. Read the latter with the second snippet.
LAMBDA labels VSAF.tar “Hessian Matrix”, but that tar contains the 16 window
functions. The actual 256-value Hessian is VSAF_mat.txt, represented here as
the VSAF_mat dense-matrix configuration. This release has
calib_uncertainty = 0.03. VSAF_x supplies the 16 offset-lognormal x_i
values, in band order and in the same uK^2 unit as the observed powers. The
release defines O_i=log(O_i0+x_i) and
chi^2=-2 log_like=sum_ij (O_i-log(B_i+x_i)) M_ij (O_j-log(B_j+x_j)); VSAF_mat is the Hessian M_ij used by that expression.
Sources
The product page and download page serve the following pinned sources:
| Source | Bytes | SHA-256 |
|---|---|---|
VSAF.tar |
153,600 | 19e49068d6d5163d62fe29e836587f59e11142a0e90848e209b40c820324031d |
VSA-0402.tar |
163,840 | 0742da8f65fc17cf87f187ff296743ac5a623f5575455a93ecd2bac31318e726 |
VSAF.txt |
858 | a989677da188d29ce27c60af59c85480a43b915e4c756ac355a7aa50ae5536ff |
VSAF_x.txt |
224 | 933672ba63fe642231325cda5913770a2979330f1dd17773b630a65104f2ea0c |
VSAF_mat.txt |
1,767 | e796df7ce51f08562d5f127a60c35c900ff92f432943bf024e37919d64ac92c4 |
dickinson-2004.pdf |
630,318 | 4f7bf176bb2138d1a3ef8cb51a4fefa23ec15116452798c11f50cb4975caac19 |
vsa_hessian_m_info.html |
9,979 | 57f7f775db7849ec518ca3c1ba3bc7992d525e57af141487768dc099fdb1f7b8 |
The individual window sources are:
| Source | Bytes | SHA-256 |
|---|---|---|
VSAF1.txt |
4,256 | 45e36c5e3be839994668499fcd99efff58d2fce76d9980952b14d406a4f21d97 |
VSAF2.txt |
4,395 | a37e98462fd58173d49739599970574192ffb50514430bfd6a632ff9a98a873d |
VSAF3.txt |
8,435 | 471554218362451ab6631c354f555df9cba273ffff0af878957b9b0649b167df |
VSAF4.txt |
8,367 | b28dbc653acf5eeddbdfd631ca3d6867b4f0d2fe4b5ac6390a98461f7edc7d7c |
VSAF5.txt |
8,871 | 42c81a1eaaf87cf8c032f85e460cf89094eae85603b08a5bd6b5324f0ae72d0a |
VSAF6.txt |
8,103 | 3fdf7e0ddbd4c27745b024c10b5de999e795ab50bbe6bfd0a50f0b9e633b484f |
VSAF7.txt |
8,869 | a237ff2b9fce78743777bf90ec7ee09dd96ec20fd8fe15e755de1a3efe94764b |
VSAF8.txt |
8,522 | d67419be73f1448452424adee65f7741529ffa1774a02ef9b5c157c01fa4a134 |
VSAF9.txt |
8,365 | c7db7daa19c05f7166ff4837635a885f8145560c6c425e11839a9e07fc79b262 |
VSAF10.txt |
8,314 | d4cd934e8c2f7667515be46ba1124801048e78229c33f2640bb82d4c45b0a669 |
VSAF11.txt |
9,067 | ad074feace47e4dafa5120e3f0344901d906b316be87d343fde56e7b9b8cc2a7 |
VSAF12.txt |
9,154 | 316111402639da920b5657eda340d01f94b0557144549d3e267d6f6268654cc7 |
VSAF13.txt |
9,109 | b1fb08837a404d0f9bc4061d3512afb47476d5cec81b70eeb75a2bf3ffaf4c4c |
VSAF14.txt |
10,070 | fb39b0bef4e691a9d0bc5aa56a90c7368853ec08d199deb22c8f1378c233e89f |
VSAF15.txt |
10,165 | 51ad293430d5c1b32bc2504384a0937cb0283956188af18f939049be6a4cb589 |
VSAF16.txt |
12,474 | bf413945373d273a0ea9a9e7af6bcf97b57359a9918f7f9aba86e631850f1efc |
VSAF.tar duplicates the 16 individually served window files under member
names VSAF1 through VSAF16. VSA-0402.tar duplicates all 19 logical
products under the source member names VSAF.dataset, VSAF_x.dat,
VSAF_mat.dat, and VSAF1 through VSAF16; the member bytes equal the
corresponding individual files. All identifiers and filenames remain verbatim.
No released sky-map file is served on the current product table. This is the
February 2004 3%-calibration release, not the older 7%-calibration products
described by archived collaboration pages.
Licence, credit, and citation
No named or formal data licence was found on the VSA product or download pages. HEASARC states verbatim: “HEASARC materials are all available freely for your use.”
Requested LAMBDA acknowledgement, verbatim: “We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center.”
The product overview identifies C. Dickinson et al. (2004), “High sensitivity measurements of the CMB power spectrum with the extended Very Small Array,” MNRAS 353, 732, DOI 10.1111/j.1365-2966.2004.08206.x, and R. Rebolo et al. (2004), “Cosmological parameter estimation using Very Small Array data out to l=1500,” MNRAS 353, 747. No additional product-specific acknowledgement or citation boilerplate is published.
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