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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method

As of 19 August 2026, this Paper Citation Record lists 90 of 90 outbound references and 0 inbound Pith citation observations for arXiv:1908.06120.

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pith.paper-citation-record.v1
1908.06120 v2

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Outbound references

Observation 6ea283bf-1e4b-4b14-a3dd-e269fd83507f · outbound

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method , " * write output.state after.block = add.period write newline

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method write newline

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method ]+kx tɕZBKڗuTù /yţ !ϋ tj/tQʼni|gaw Hā\ u zMo ʸSz Ӝԇ9WڑУ Ɵu ^F4 `0 w / ]t rl + am?=WޙDlܸ oBR .m;'X W ztUqj V r 7 ɨ Fcf w v zn y = _ &

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Observation ff3646ed-1649-428d-80f9-7a90eee6e429 · outbound

This paper cites R., & Cook , K.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method R., & Cook , K

Reference 4

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This paper cites S., Rizzi , L., & Tully , R.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method S., Rizzi , L., & Tully , R

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This paper cites L., Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Freedman , W

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Bono , G., Braga , V

Reference 7

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

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This paper cites 2013, LEGUS: Legacy ExtraGalactic UV Survey , HST Proposal, ,.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2013, LEGUS: Legacy ExtraGalactic UV Survey , HST Proposal, ,

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This paper cites A., Clayton , G.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Clayton , G

Reference 10

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., Beaton , R

Reference 11

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2019 b , , 879, 13

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2015, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 57, 138

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This paper cites H., Aaronson , M., & Illingworth , G.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method H., Aaronson , M., & Illingworth , G

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Observation 29731c43-edec-41e0-95c2-84a8d8387c8f · outbound

This paper cites H., Aaronson , M., & Illingworth , G.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method H., Aaronson , M., & Illingworth , G

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method E., & Bono , G

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2000 b , , 112, 1397

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method R., Kennicutt , Jr., R

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2014, CHP-II: The Carnegie Hubble Program to Measure Ho to 3\ Using Population II , HST Proposal, ,

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., & Madore , B

Reference 22

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Madore , B

Reference 23

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Madore , B

Reference 24

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch

Reference 25

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., et al

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Freedman , W

Reference 27

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Madore , B

Reference 28

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2018 b , , 866, 145

Reference 29

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., Ferrarese , L., Stetson , P

Reference 30

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., Freedman , W

Reference 31

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This paper cites The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group

Reference 32

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Rizzi , L., Tully , R

Reference 33

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The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method S., & Lee , M

Reference 34

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Observation 67e1a847-9d96-4096-9426-c809e9dca8a6 · outbound

This paper cites 2017 b , , 835, 28.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2017 b , , 835, 28

Reference 35

Resolution
parse uncertain
raw_fallback, observed 2026-08-14T13:03:13.466385Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.163970Z digest=sha256:c5ab2e1150921c93d74676a8c1f70de4f5d719b1361bbbcd0d761cecb0c20310

Observation 9d0dcc0b-3afc-44d1-9869-30af27bc3824 · outbound

This paper cites S., Hatt , D., Beaton , R.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method S., Hatt , D., Beaton , R

Reference 36

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.335242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.169378Z digest=sha256:6680fd0c4bdf408ad60a11a177173f1055c20356e548ef6610378fd128942ec4

Observation d01b31b9-112e-419c-80f2-3d5bf8ca707d · outbound

This paper cites D., Illingworth , G.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method D., Illingworth , G

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.319778Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.174009Z digest=sha256:c3f443a33778e5f1a612ce7ba60a25b98fbc484f441a55dcdd7522ce54e84cc6

Observation 62a9fba9-8534-499c-9b14-15ca748d3af4 · outbound

This paper cites C., Stetson , P.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method C., Stetson , P

Reference 38

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.304295Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.178707Z digest=sha256:6d77b3beb7587b72d3ecc4160762a7120f7aca893989fc69513ea6872e1c0222

Observation 537c1261-fa15-44f8-996b-83f4a64cc634 · outbound

This paper cites E., Hook , R.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method E., Hook , R

Reference 39

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.287644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.183461Z digest=sha256:3dff1c001e72d21550faaf419a0a3989b9e96cb145042837789c0d2106d7cce5

Observation cbf611f5-119e-4203-b03c-65df9d4029e9 · outbound

This paper cites G., Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., Freedman , W

Reference 40

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.272492Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.188906Z digest=sha256:16c780ed54d74719dd50b221782922b69f437fefe860f09cd26954f65892565e

Observation 05a3f2cd-801b-4e79-a355-44acc2fb5114 · outbound

This paper cites G., & Jang , I.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., & Jang , I

Reference 41

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.256814Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.193501Z digest=sha256:5e013edf474b9b68c513d438356cd703048f5e186f6231b44feaf26c7fe147d0

Observation 55ab0e73-97e7-4ae8-8c04-9a26e7857634 · outbound

This paper cites L., Anderson , J., & Sirianni , M.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method L., Anderson , J., & Sirianni , M

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.240378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.198226Z digest=sha256:24b5a786561cbf7cd2a7cf4605656c1769496cf3e3c37857fdcc85e197471e2f

Observation ad976732-753c-49c4-9088-1272eba98cb8 · outbound

This paper cites M., Calzetti , D., Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method M., Calzetti , D., Freedman , W

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.224379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.203011Z digest=sha256:31ea553d9a52eff0360a8c5b835a2c5a6b56d123c3bb95bf742a3612e5bc5129

Observation 4eb6672f-4fc0-404d-8307-55b39cde687d · outbound

This paper cites F., & Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., & Freedman , W

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.208311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.208889Z digest=sha256:c5fd7ba1d71289f13170c7c0b250a6a34097190fe6251b453cd5ce63ad4a147a

Observation c9ef8542-b1bb-44f3-a5dd-830f5a64bf51 · outbound

This paper cites F., & Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., & Freedman , W

Reference 45

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.191836Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.213666Z digest=sha256:ca57ea36523836e53301c8e0d49fbb58d010f97d9e33c32b76457f15f8c117c3

Observation 4996e542-15a8-4e78-a212-a9809a688d4a · outbound

This paper cites F., Mager , V., & Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., Mager , V., & Freedman , W

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.175715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.218228Z digest=sha256:df252e9f4cda4270696844ca7bd763404edf702bc55bf1fd0ff835861fd8b964

Observation a5f5213b-0ec3-4a7e-b054-e8cb73eeb88f · outbound

This paper cites F., Freedman , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., Freedman , W

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.159195Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.222923Z digest=sha256:2d47de4e203df0fe39d92a1b52a610574c5c20cae6f1d9f6aecc43d364c5f421

Observation 5b2a90cd-f3f3-46ac-8a4d-ea3f1bb3e26f · outbound

This paper cites A., Madore , B.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Madore , B

Reference 48

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.227437Z digest=sha256:82203a46c516cdf3528e765d68d760dd0d3659c44345ec2a57b789a497257118

Observation 73d94ca3-f37f-46b0-965b-008a4bbb1aaf · outbound

This paper cites 2013, , 777, 79.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2013, , 777, 79

Reference 49

Resolution
parse uncertain
raw_fallback, observed 2026-08-14T13:03:13.129078Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.231921Z digest=sha256:f59ebe56427857501f312e21b0ca2d44897a43465565ab99371a7544eedf7a76

Observation 1c9d66fc-5948-48dc-83d2-46140939b452 · outbound

This paper cites 2006, , 132, 2729.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2006, , 132, 2729

Reference 50

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:13.114581Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.236471Z digest=sha256:40464b1d842c656c136933810c7ad032ae586e6a6bd04b80d3b3b3538ea3003a

Observation ba6fcb2b-e3ea-4070-80d6-33c09c649d59 · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 51

Resolution
unresolved
raw_fallback, observed 2026-08-14T13:03:13.099622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.240970Z digest=sha256:922a6e045495693989284fe24acbbd077264df6b62b92f89eefcdc2d305a8337

Observation 5c9d9a24-63ca-43fd-a063-f99e7ab342a1 · outbound

This paper cites 2016 b , , 152, 144.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2016 b , , 152, 144

Reference 52

Resolution
parse uncertain
raw_fallback, observed 2026-08-14T13:03:13.084050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.245943Z digest=sha256:4aa5490c8332734a4f3928b175ad0517e38f3e855426e3ec30907ab3386680b8

Observation ae581d52-6a4c-4fb9-9c1a-f0e55df4f25e · outbound

This paper cites 2017, , 154, 51.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2017, , 154, 51

Reference 53

Resolution
parse uncertain
raw_fallback, observed 2026-08-14T13:03:13.067588Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.250530Z digest=sha256:7a11cd230df029c97741e10a946163627a92fcba4e2436a2aee8158aa81d1015

Observation f4907867-05e6-44d7-b55c-5e1210de46fe · outbound

This paper cites 2002, , 124, 213.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2002, , 124, 213

Reference 54

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.255182Z digest=sha256:62d84bc01e4a5240a57d028c2f944a94e0a73a3e868554086e097ee2e4ce1a12

Observation 1b8cfe7b-f03d-4bf2-ae76-e4c05facdc02 · outbound

This paper cites J., Beaton , R.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., Beaton , R

Reference 55

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.259930Z digest=sha256:0ec28d85c2ba01bee1f5d5441d88c0e45102bba4e88124e734dcfa1c01ad33df

Observation 27d86204-e8a3-4089-ba61-6e962a887d79 · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 56

Resolution
unresolved
raw_fallback, observed 2026-08-14T13:03:13.018899Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.264374Z digest=sha256:0e94ead85ab7973765319f3ceae9adcf1ffe3e327a23b8884c588511d1fb036a

Observation 70aede88-7627-4328-b702-0f616b79b54c · outbound

This paper cites A., Ferrarese , L., Stetson , P.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Ferrarese , L., Stetson , P

Reference 57

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.269036Z digest=sha256:e227ab4c1c9913efffecc3c979c285cbddbba673c7d579b1595f154b8cdaea34

Observation 0c7a29b2-544f-4b04-baaa-a103d38feb1c · outbound

This paper cites 2011 a , The Astronomer's Telegram, 3581.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2011 a , The Astronomer's Telegram, 3581

Reference 58

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.273663Z digest=sha256:c84f3cfd3cbb257a3bf34e0f8ca9d055f84c8d62290bb19c0cfb80e93a213223

Observation a40b382e-be36-4f03-8958-3ff52e275d28 · outbound

This paper cites E., Sullivan , M., Cenko , S.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method E., Sullivan , M., Cenko , S

Reference 59

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.278642Z digest=sha256:d9b7bfd7ad12ce6cc90588bf4c6bb277777603458b03653a645b3bf1ea839c65

Observation e30ef52d-9ff6-4b9e-9c1f-961e59902eaf · outbound

This paper cites 1991, Lonely hearts of the cosmos.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 1991, Lonely hearts of the cosmos

Reference 60

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 51a40506-3372-44f6-a9f1-feca709d2490 · outbound

This paper cites 2002, , 389, 19.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2002, , 389, 19

Reference 61

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.288413Z digest=sha256:862f98d9afc7f042390e45b3618f3aaa367db19a6b38f84b8e1ef5129f319c44

Observation 3ffeb4dc-87ba-45d1-8183-354c35957033 · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 62

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.293177Z digest=sha256:96e9b595f1d12246b3332c2897fed4fb837cdf1c25c9c5b17e24e5469c58ba4a

Observation 83f320f3-6ed8-4a61-a466-ab82ee045657 · outbound

This paper cites E., Madore , B.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method E., Madore , B

Reference 63

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.297911Z digest=sha256:5cb1ccde00b6260811c01597fdfbf741473b6755c496592a2c606f4a50b732c1

Observation d4837878-4f96-4681-8e0c-c17fa421d317 · outbound

This paper cites G., Casertano , S., Yuan , W., Macri , L.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., Casertano , S., Yuan , W., Macri , L

Reference 64

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.302724Z digest=sha256:bfe9848c7cb50c43c6e7f27fd4f6945c50343420bb1744ade5266a5facd4c7c5

Observation f7a46cf2-81f2-45d1-8553-bf863f52495c · outbound

This paper cites G., Macri , L., Casertano , S., et al.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., Macri , L., Casertano , S., et al

Reference 65

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.307432Z digest=sha256:15fcc2b82afb5f0f92de8d04aea1469bc77d87a2d707ab12e975b2bb20f60259

Observation b0ff6ebf-6b38-411f-87c6-b01a78efead7 · outbound

This paper cites G., Macri , L.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method G., Macri , L

Reference 66

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.312104Z digest=sha256:65ea9dfff19e8f0927fc327e72ed58dd5df731796af6bb19f9dca94b8467a9d1

Observation 93c37fb4-910f-4ac8-ab0b-0bfeb6a8d2cc · outbound

This paper cites New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.316901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.316901Z digest=sha256:fd1bacc61566dc13f9f40be05023d12cee3b4349998bc703fbbb7dfd26ab84f3

Observation 08958827-3e42-4731-a5a5-d2bb0cc85245 · outbound

This paper cites B., Makarov , D., et al.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method B., Makarov , D., et al

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.322443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.322443Z digest=sha256:568a19c98d84cd9f8caa9a8bf5500af7b3690327825cfa1316179acd8975ae6e

Observation 6a584417-d379-432a-b3dd-56d33be6d227 · outbound

This paper cites A., Reindl , B., & Sandage , A.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Reindl , B., & Sandage , A

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.327253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.327253Z digest=sha256:b03e969685f4bb1cd12bd4c4cfea95005267e89628e821a61472ac2547d7caee

Observation 327c9804-4959-437a-960d-35b7a3eef507 · outbound

This paper cites C., & Saha , A.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method C., & Saha , A

Reference 70

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.834524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 4d3e2675-cdc6-4442-aef5-8abc8fdf77d4 · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 71

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 83bdc10a-90e1-4971-b9b0-c085726597d0 · outbound

This paper cites F., & Finkbeiner , D.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., & Finkbeiner , D

Reference 72

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.341481Z digest=sha256:54bce41054bd22f72412c649e79fa15837211f87fc4c8a6872b32c3eaede1938

Observation ef5e30cf-2f90-425f-9c38-032fd2f26e20 · outbound

This paper cites J., Finkbeiner , D.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., Finkbeiner , D

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.346295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.346295Z digest=sha256:507e89b645b61584d208e33a42237b1eb699df99ec9815d1ba7e30d8d1008a68

Observation 9ee9102a-5eeb-4e45-aff2-59333b863ad7 · outbound

This paper cites 2017, , 606, A33.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2017, , 606, A33

Reference 74

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.350943Z digest=sha256:69ea70ccf40037700041703309af0b4036e80f4d6f9fdce1b19bbb0f7d531ffe

Observation 778de8e0-d65e-428d-a13a-63d292027324 · outbound

This paper cites 2014, Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe , HST Proposal, ,.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2014, Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe , HST Proposal, ,

Reference 75

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 102d4c03-0f81-4d6d-8d5b-3527e4f48e35 · outbound

This paper cites 2015, Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe , HST Proposal, ,.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 2015, Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe , HST Proposal, ,

Reference 76

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.749500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation b06724b5-17eb-4f7b-b8aa-0342a9e23f73 · outbound

This paper cites J., & Stanek , K.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., & Stanek , K

Reference 77

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.732612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.366198Z digest=sha256:b879180b380f80162d3bc7ca9870d31cfdae89aece409fa7abef9d407b21ba4e

Observation a6abde06-786f-4eb9-b491-0d81242be9ae · outbound

This paper cites Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-08-14T13:03:12.474859Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.370858Z digest=sha256:53cbc3fe01b0fe5651f5f8c0d6a60dc774fff844e076411ab852795be7da751d

Observation a1ea2276-2a62-4341-aa04-ccefeeb0cc00 · outbound

This paper cites J., Benitez , N., et al.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method J., Benitez , N., et al

Reference 79

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.716282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.375610Z digest=sha256:ab5fdda62eb3d974a1ae5ae734c5df51894cbde02c50e9c1ccc50719541d6a4c

Observation f4d7aacd-e0ba-4a62-a71f-35d9b10ccce1 · outbound

This paper cites F., Mazzarella , J.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method F., Mazzarella , J

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.380111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.380111Z digest=sha256:c92770231af1a52f6d458f55f7d3b75a6b1668281a3dee4cf418600411eb452f

Observation 083dbbf3-c570-4990-92e7-fd771d7ebe4a · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.384687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.384687Z digest=sha256:0ec8e1bde2dbbf0af015853df0b14c88cd0f2b8a02a7f3b6952cdaa1ab09297b

Observation 3df259fb-d37f-448b-834e-aabc4f0b3995 · outbound

This paper cites 1990, , 102, 932.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 1990, , 102, 932

Reference 82

Resolution
parse uncertain
no resolver link, observed 2026-08-14T13:03:12.389351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.389351Z digest=sha256:1bb3baa17e2b50f58f8d6843929b750cc7ef0d1c225949a4656be49ab78e7745

Observation 13ce8f2e-a135-4b2c-8b91-4d57cbeb4cb4 · outbound

This paper cites 1994, , 106, 250.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 1994, , 106, 250

Reference 83

Resolution
parse uncertain
raw_fallback, observed 2026-08-14T13:03:12.664575Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.394148Z digest=sha256:72ccd550d254da140eb5838ef09c26296ac91d90f7e4e9a01ac2b5cd1a261aeb

Observation 6d25e4cb-e39a-4086-bc63-5a8d4ef5be05 · outbound

This paper cites B., & Harris , W.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method B., & Harris , W

Reference 84

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.647513Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.399165Z digest=sha256:5bed0cd0551d577615e61b4934d4130a8df2a3359f07834573abb88b35dc4f6e

Observation d0505d83-d935-465e-a84c-72c2ef128ef7 · outbound

This paper cites B., Saha , A., Ferrarese , L., et al.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method B., Saha , A., Ferrarese , L., et al

Reference 85

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.629934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.403862Z digest=sha256:1df358b43aba55df265bc4cf1a4c5628fab72905dd34b24f3774da95898c8c5e

Observation a06cea40-3db7-4d84-bf3c-85926ea18322 · outbound

This paper cites A., Lebedev , V.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., Lebedev , V

Reference 86

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.613129Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.408488Z digest=sha256:845c402fd79ed10131b16e620b0b09085d0ddfda7d10e149a8a1109d995a9098

Observation 7454bc66-a800-4213-a4b8-9358c9251088 · outbound

This paper cites B., Courtois , H.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method B., Courtois , H

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.413206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.413206Z digest=sha256:c6f46474c16dd228f5e68dab58264c23c5f3327b21659ab3abbfd8377d1ecce1

Observation 7fb27581-49e2-4cee-bf53-aed105f8b4be · outbound

This paper cites an unresolved cited work.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method Unresolved cited work

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:12.418189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:03:12.418189Z digest=sha256:64d959d36ebccc5ca822fa27f5cee9e374fb49cc1a3fb27ae1ae4ea14fa0496c

Observation db58f974-785e-41f0-ba0d-0eab031c4a0a · outbound

This paper cites A., & Batra , P.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method A., & Batra , P

Reference 89

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.574200Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.422875Z digest=sha256:153628ae18dba1c1621e8433763da30cab91f27a563425a0a72e9b4f6c39cdab

Observation 5fe73e2c-4426-4035-b446-8060b33baa6f · outbound

This paper cites 1994, , 108, 1619.

The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method 1994, , 108, 1619

Reference 90

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:03:12.558042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T13:03:12.427421Z digest=sha256:9a4f9398ac1528585a0e34a4068bf71ea8c59cc9deae8f5e4f9fa9f575eb448b

Pith citing papers

No inbound Pith citation observations are available.