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files","slug":"datasets-and-data-files"},{"level":2,"title":"Python Module","slug":"python-module"}],"relativePath":"guide/index.md","lastUpdated":1710919484854}',t={},o=n(`

CLI / Terminal

Philosophy

The Arcsecond CLI is using the same principle as git. The main entry point is arcsecond followed by a command. And most of the commands have the name of API endpoints.

For instance, to obtain the information about an object, and likewise, an exoplanet:

$ arcsecond objects "HD 5980"
+$ arcsecond exoplanets "51 Peg b"
+

For objects, and exoplanets, you can open the webpage in the default browser:

$ arcsecond objects "HD 5980" --open
+$ arcsecond exoplanets "51 Peg b" --open
+

Or open the API webpage in the default browser for that object:

$ arcsecond o "HD 5980" --open api
+$ arcsecond exoplanets "51 Peg b" --open api
+

For other things, such as private observing runs and night logs, likewise:

$ arcsecond observingruns <uuid>
+$ arcsecond nightlogs <uuid>    
+

Available Endpoints

The available read-only API endpoints (and thus, subcommands) available so far are:

  • objects, exoplanets, and findingcharts (public)
  • observingsites, telescopes and instruments (public)
  • profiles (public)
  • satellites (public)
  • observingruns and nightlogs (private)
  • me (personal profile, private)

Observing Runs and Night Logs will be writable in a near future. As for Observing Sites, Telescopes and Instruments, this is under study.

The available read-write API endpoints available so far are:

  • activities (public)
  • datasets and datafiles (private)

Read-write APIs use the 4 standard CRUD methods: create, read, update, delete (while, read-only APIs have only the read method, implicitly).

See below for details.

Datasets and Data files

You can entirely manage your datasets and Data/FITS files (including upload) from this CLI / Python module.

To list your datasets (the two methods are identical, the second simply having its action name explicitly written):

$ arcsecond datasets
+$ arcsecond datasets read
+

To create a dataset:

$ arcsecond datasets create --name "this is a new dataset"
+

To delete a dataset (warning: this will also delete the associated data/FITS files!):

$ arcsecond datasets delete <dataset uuid>
+

Data files are necessarily associated with a dataset. Hence a dataset UUID must be provided. To upload a data file:

$ arcsecond datafiles <dataset uuid> create --file <path to a local data file>
+

To delete a data file, one use its "id/pk" (pk = Primary Key == ID):

$ arcsecond datafiles <dataset uuid> delete <Data file pk>
+

Python Module

Using this as a Python module goes as follow

>>> from arcsecond import ArcsecondAPI
+>>> ArcsecondAPI.login(<username>, <password>)
+>>> ArcsecondAPI(ArcsecondAPI.ENDPOINT_OBJECTS).read('HD 5980')
+
`,34),p=[o];function d(l,i,c,r,u,h){return s(),e("div",null,p)}var k=a(t,[["render",d]]);export{b as __pageData,k as default}; diff --git a/assets/guide_index.md.7232036b.lean.js b/assets/guide_index.md.7232036b.lean.js new file mode 100644 index 0000000..9e33410 --- /dev/null +++ b/assets/guide_index.md.7232036b.lean.js @@ -0,0 +1 @@ +import{_ as a,y as e,x as s,W as n}from"./plugin-vue_export-helper.05763f57.js";const b='{"title":"CLI / Terminal","description":"","frontmatter":{"sidebar":true},"headers":[{"level":2,"title":"CLI / Terminal","slug":"cli-terminal"},{"level":3,"title":"Philosophy","slug":"philosophy"},{"level":3,"title":"Available Endpoints","slug":"available-endpoints"},{"level":3,"title":"Datasets and Data files","slug":"datasets-and-data-files"},{"level":2,"title":"Python Module","slug":"python-module"}],"relativePath":"guide/index.md","lastUpdated":1710919484854}',t={},o=n("",34),p=[o];function d(l,i,c,r,u,h){return s(),e("div",null,p)}var k=a(t,[["render",d]]);export{b as __pageData,k as default}; diff --git a/assets/index.md.2ffb4990.js b/assets/index.md.2ffb4990.js new file mode 100644 index 0000000..a404d1e --- /dev/null +++ b/assets/index.md.2ffb4990.js @@ -0,0 +1 @@ +import{_ as t,y as r,x as s,D as e,B as o}from"./plugin-vue_export-helper.05763f57.js";const g='{"title":"Home","description":"","frontmatter":{"home":true,"heroImage":"https://statics.arcsecond.io/img/logo-circle.png","heroAlt":"Arcsecond Logo","heroText":"Arcsecond CLI","tagline":"The command-line utility / Python module to access the resources of Arcsecond.io.","actionText":"Install & Setup","actionLink":"/install/","features":[{"title":"Command-Line","details":"All the public and private Arcsecond.io resources (objects, exoplanets, datasets...) right into your Terminal."},{"title":"Python Module","details":"All the Arcsecond.io resources inside your Python code! 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"),e("a",{class:"header-anchor",href:"#arcsecond-io","aria-hidden":"true"},"#")],-1),c=e("p",null,[e("a",{href:"http://Arcsecond.io",target:"_blank",rel:"noopener noreferrer"},"Arcsecond.io"),o(" is a unique and comprehensive cloud platform made by astronomers for astronomers providing all the necessary resources and tools for preparing astronomical observations.")],-1),i=[a,c];function d(l,h,p,u,m,_){return s(),r("div",null,i)}var A=t(n,[["render",d]]);export{g as __pageData,A as default}; diff --git a/assets/install_index.md.3c7d9f6e.js b/assets/install_index.md.3c7d9f6e.js new file mode 100644 index 0000000..318b9e5 --- /dev/null +++ b/assets/install_index.md.3c7d9f6e.js @@ -0,0 +1,8 @@ +import{_ as e,y as o,x as a,W as s}from"./plugin-vue_export-helper.05763f57.js";const f='{"title":"Install","description":"","frontmatter":{"sidebar":true},"headers":[{"level":2,"title":"Install","slug":"install"},{"level":2,"title":"Setup","slug":"setup"},{"level":3,"title":"Register to Arcsecond.io","slug":"register-to-arcsecond-io"},{"level":3,"title":"Login to Arcsecond.io","slug":"login-to-arcsecond-io"}],"relativePath":"install/index.md","lastUpdated":1710919484854}',r={},n=s(`

Install

Simply issue the following in a Terminal:

$ pip install arcsecond
+

To upgrade an existing Arcsecond installation:

$ pip install --upgrade arcsecond
+

The help is accessible like any other command line:

$ arcsecond --help
+

or, for subcommand

$ arcsecond <command> --help
+

At that point, you can access all the public resources of Arcsecond.io.

The Arcsecond CLI usage is similar to a utility like git. That is, arcsecond is the main entry point, followed by a command. Most of the commands are simply the name of API resources.

For accessing private resources, such as datasets, night logs etc, you must log in (or register first).

Setup

Register to Arcsecond.io

You can register directly from the CLI:

$ arcsecond register
+

and provide a username and a password.

Login to Arcsecond.io

You must login first before accessing APIs.

$ arcsecond login 
+

To skip prompts:

$ arcsecond login --username <username> --password <password>
+

By registering or logging in, your private API key will be stored locally in the config file in ~/.arcsecond.ini. Do not share this key. It gives a complete access to your private resources too.

Logging in again will overwrite the current API key with the new one (assuming login is a success, of course).

If you think your key is compromised, you can regenerate one in your profile settings in https://www.arcsecond.io. You cannot regenerate an API key with the cli.

`,25),t=[n];function i(c,l,p,d,g,h){return a(),o("div",null,t)}var m=e(r,[["render",i]]);export{f as __pageData,m as default}; diff --git a/assets/install_index.md.3c7d9f6e.lean.js b/assets/install_index.md.3c7d9f6e.lean.js new file mode 100644 index 0000000..50ee87f --- /dev/null +++ b/assets/install_index.md.3c7d9f6e.lean.js @@ -0,0 +1 @@ +import{_ as e,y as o,x as a,W as s}from"./plugin-vue_export-helper.05763f57.js";const f='{"title":"Install","description":"","frontmatter":{"sidebar":true},"headers":[{"level":2,"title":"Install","slug":"install"},{"level":2,"title":"Setup","slug":"setup"},{"level":3,"title":"Register to Arcsecond.io","slug":"register-to-arcsecond-io"},{"level":3,"title":"Login to Arcsecond.io","slug":"login-to-arcsecond-io"}],"relativePath":"install/index.md","lastUpdated":1710919484854}',r={},n=s("",25),t=[n];function i(c,l,p,d,g,h){return a(),o("div",null,t)}var m=e(r,[["render",i]]);export{f as __pageData,m as default}; diff --git a/assets/observations_index.md.32abe419.js b/assets/observations_index.md.32abe419.js new file mode 100644 index 0000000..5125110 --- /dev/null +++ b/assets/observations_index.md.32abe419.js @@ -0,0 +1 @@ +import{_ as e,y as o,x as t,W as r}from"./plugin-vue_export-helper.05763f57.js";const m='{"title":"Introduction","description":"","frontmatter":{"sidebar":true},"headers":[{"level":2,"title":"Introduction","slug":"introduction"},{"level":2,"title":"Nights...","slug":"nights"}],"relativePath":"observations/index.md","lastUpdated":1710919484854}',a={},n=r('

Introduction

Astroplan is an open-source package affiliated with the famous community-powered Astropy. Astroplan aims to help astronomers plan observations, similarly to iObserve and Arcsecond.io try to achieve.

One major difference with us is that Astroplan leaves you the responsibility for all the "plumbing" or "app" code. That is, it provides all the necessary information to plan observations indeed. However, there is no infrastructure nor app code to help you go much beyond a few observations without having to write (and organise and maintain) lots of non-scientific code. If you need to create dozens of observations, for dozens of observing runs, all this code is up to you.

For astronomers loving to write their own code, it is certainly a good solution (and we know many of them in that situation). But even in this case, you are left with lots of work such as maintaining your code, testing it to avoid regressions, finding a place to store targets, target lists, organise your plots and figures and so on.

Arcsecond.io and its main Pro Tool "iObserve" are developed since many years precisely to help astronomers avoid re-inventing the wheel whatever their knowledge of code. There is one key difference of course. Using a complete tool such as iObserve has a (small) price. But we think we have come up with a very affordable model for professionals and even Ph.D. students and undergrads! See our Pricing page for more details.

We provide yearly subscriptions for iObserve on the web. These

subscriptions are entirely compatible with any (US) University administration. We already set up such subscriptions with a University Physics Department in Arizona. Email us to know more and set up yours.

Nights...

',7),i=[n];function s(d,c,l,h,p,u){return t(),o("div",null,i)}var g=e(a,[["render",s]]);export{m as __pageData,g as default}; diff --git a/assets/observations_index.md.32abe419.lean.js b/assets/observations_index.md.32abe419.lean.js new file mode 100644 index 0000000..665468b --- /dev/null +++ b/assets/observations_index.md.32abe419.lean.js @@ -0,0 +1 @@ +import{_ as e,y as o,x as t,W as r}from"./plugin-vue_export-helper.05763f57.js";const m='{"title":"Introduction","description":"","frontmatter":{"sidebar":true},"headers":[{"level":2,"title":"Introduction","slug":"introduction"},{"level":2,"title":"Nights...","slug":"nights"}],"relativePath":"observations/index.md","lastUpdated":1710919484854}',a={},n=r("",7),i=[n];function s(d,c,l,h,p,u){return t(),o("div",null,i)}var g=e(a,[["render",s]]);export{m as __pageData,g as default}; diff --git a/assets/plugin-vue_export-helper.05763f57.js b/assets/plugin-vue_export-helper.05763f57.js new file mode 100644 index 0000000..4aa16a1 --- 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420px){.container[data-v-30918238]{padding:3rem 1.5rem 3.25rem}}.text[data-v-30918238]{margin:0;text-align:center;line-height:1.4;font-size:.9rem;color:var(--c-text-light)}.home[data-v-10122c92]{padding-top:var(--header-height)}.home-content[data-v-10122c92]{max-width:960px;margin:0 auto;padding:0 1.5rem} diff --git a/guide/index.html b/guide/index.html new file mode 100644 index 0000000..8acb3fb --- /dev/null +++ b/guide/index.html @@ -0,0 +1,40 @@ + + + + + + CLI / Terminal | Arcsecond CLI + + + + + + + + + + + +
Arcsecond CLI

CLI / Terminal

Philosophy

The Arcsecond CLI is using the same principle as git. The main entry point is arcsecond followed by a command. And most of the commands have the name of API endpoints.

For instance, to obtain the information about an object, and likewise, an exoplanet:

$ arcsecond objects "HD 5980"
+$ arcsecond exoplanets "51 Peg b"
+

For objects, and exoplanets, you can open the webpage in the default browser:

$ arcsecond objects "HD 5980" --open
+$ arcsecond exoplanets "51 Peg b" --open
+

Or open the API webpage in the default browser for that object:

$ arcsecond o "HD 5980" --open api
+$ arcsecond exoplanets "51 Peg b" --open api
+

For other things, such as private observing runs and night logs, likewise:

$ arcsecond observingruns <uuid>
+$ arcsecond nightlogs <uuid>    
+

Available Endpoints

The available read-only API endpoints (and thus, subcommands) available so far are:

  • objects, exoplanets, and findingcharts (public)
  • observingsites, telescopes and instruments (public)
  • profiles (public)
  • satellites (public)
  • observingruns and nightlogs (private)
  • me (personal profile, private)

Observing Runs and Night Logs will be writable in a near future. As for Observing Sites, Telescopes and Instruments, this is under study.

The available read-write API endpoints available so far are:

  • activities (public)
  • datasets and datafiles (private)

Read-write APIs use the 4 standard CRUD methods: create, read, update, delete (while, read-only APIs have only the read method, implicitly).

See below for details.

Datasets and Data files

You can entirely manage your datasets and Data/FITS files (including upload) from this CLI / Python module.

To list your datasets (the two methods are identical, the second simply having its action name explicitly written):

$ arcsecond datasets
+$ arcsecond datasets read
+

To create a dataset:

$ arcsecond datasets create --name "this is a new dataset"
+

To delete a dataset (warning: this will also delete the associated data/FITS files!):

$ arcsecond datasets delete <dataset uuid>
+

Data files are necessarily associated with a dataset. Hence a dataset UUID must be provided. To upload a data file:

$ arcsecond datafiles <dataset uuid> create --file <path to a local data file>
+

To delete a data file, one use its "id/pk" (pk = Primary Key == ID):

$ arcsecond datafiles <dataset uuid> delete <Data file pk>
+

Python Module

Using this as a Python module goes as follow

>>> from arcsecond import ArcsecondAPI
+>>> ArcsecondAPI.login(<username>, <password>)
+>>> ArcsecondAPI(ArcsecondAPI.ENDPOINT_OBJECTS).read('HD 5980')
+
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Arcsecond CLI
Arcsecond Logo

Arcsecond CLI

The command-line utility / Python module to access the resources of Arcsecond.io.

Install & Setup

Command-Line

All the public and private Arcsecond.io resources (objects, exoplanets, datasets...) right into your Terminal.

Python Module

All the Arcsecond.io resources inside your Python code! Easily plan observations with your own custom rules.

Arcsecond.io ?

Arcsecond.io is a unique and comprehensive cloud platform made by astronomers for astronomers providing all the necessary resources and tools for preparing astronomical observations.

MIT Licensed | Copyright © 2018-present Arcsecond.io (F52 Tech).

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Arcsecond CLI

Install

Simply issue the following in a Terminal:

$ pip install arcsecond
+

To upgrade an existing Arcsecond installation:

$ pip install --upgrade arcsecond
+

The help is accessible like any other command line:

$ arcsecond --help
+

or, for subcommand

$ arcsecond <command> --help
+

At that point, you can access all the public resources of Arcsecond.io.

The Arcsecond CLI usage is similar to a utility like git. That is, arcsecond is the main entry point, followed by a command. Most of the commands are simply the name of API resources.

For accessing private resources, such as datasets, night logs etc, you must log in (or register first).

Setup

Register to Arcsecond.io

You can register directly from the CLI:

$ arcsecond register
+

and provide a username and a password.

Login to Arcsecond.io

You must login first before accessing APIs.

$ arcsecond login 
+

To skip prompts:

$ arcsecond login --username <username> --password <password>
+

By registering or logging in, your private API key will be stored locally in the config file in ~/.arcsecond.ini. Do not share this key. It gives a complete access to your private resources too.

Logging in again will overwrite the current API key with the new one (assuming login is a success, of course).

If you think your key is compromised, you can regenerate one in your profile settings in https://www.arcsecond.io. You cannot regenerate an API key with the cli.

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Arcsecond CLI

Introduction

Astroplan is an open-source package affiliated with the famous community-powered Astropy. Astroplan aims to help astronomers plan observations, similarly to iObserve and Arcsecond.io try to achieve.

One major difference with us is that Astroplan leaves you the responsibility for all the "plumbing" or "app" code. That is, it provides all the necessary information to plan observations indeed. However, there is no infrastructure nor app code to help you go much beyond a few observations without having to write (and organise and maintain) lots of non-scientific code. If you need to create dozens of observations, for dozens of observing runs, all this code is up to you.

For astronomers loving to write their own code, it is certainly a good solution (and we know many of them in that situation). But even in this case, you are left with lots of work such as maintaining your code, testing it to avoid regressions, finding a place to store targets, target lists, organise your plots and figures and so on.

Arcsecond.io and its main Pro Tool "iObserve" are developed since many years precisely to help astronomers avoid re-inventing the wheel whatever their knowledge of code. There is one key difference of course. Using a complete tool such as iObserve has a (small) price. But we think we have come up with a very affordable model for professionals and even Ph.D. students and undergrads! See our Pricing page for more details.

We provide yearly subscriptions for iObserve on the web. These

subscriptions are entirely compatible with any (US) University administration. We already set up such subscriptions with a University Physics Department in Arizona. Email us to know more and set up yours.

Nights...

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