Computer support

Gserver Service

• Gserver is a windows 2008 server located at office 1513, which provides

windows client (username: cluster passwd: cluster_pub)

http and ftp service

scanner and DVD burner

• Connenction

IP address: 202.127.29.128

windows: remote desktop

linux: redesktop

Hserver Service

• Hserver is a linux server(IP: 202.127.29.3) equipped with 4 six core AMD cpus, 48 G memory and 14T hard disk, which provides high preformance computation and htppd service.

Connection

SSH Connection

windows client (MobaXterm)

VNC server

use vncviewr [1]

xrdp (remote desktop)

• linux client: rdesktop

example  rdesktop -a 16 -g 1024x768 -r clipboard:CLIPBOARD  202.127.29.3

• windows client: remote desktop(远程桌面)

Scientific softwar

IDL 7.1

coyote library

astro_lib

g95

• wget -O - http://ftp.g95.org/g95-x86-linux.tgz | tar xvfz -
• MAC: wget -O - http://ftp.g95.org/g95-x86-osx.tgz | tar xvfz -

Intel fortran compiler 11.1

• Intel® Fortran Compiler Documentation
• numeric recipies:

F77 librecipes_f.a [2]

F90: lobrecipes_f90.a [3]

c: Doc

source: /usr/local/lib/numrecip_2.10

• Nag library (libnag20d.a)

F77 [4]

F90 [5]

• cfitsio (libcfitsio) [6]

ESo-scisoft

• See http://www.eso.org/sci/software/scisoft/
• please run `sciinit` command to initialize your scisfot enviroment

starlink

The Project produced a number of well-known applications and libraries. Of these, some of the highlights are:

GAIA

The main GUI application, which acts as a general astronomical image viewer, as well as a front end to many of the other applications.

ORAC-DR

The ORAC-DR data reduction system, developed at JAC Hawai'i, is a data processing pipeline for incoming data. It is in use for online data reduction at UKIRT and JCMT for a variety of instruments. This is not a Starlink application as such, but it is tightly integrated with the Starlink suite, and by default uses Starlink software as its application engines. See the ORAC-DR home page for further details.

KAPPA

A suite of general-purpose data-analysis and visualisation tools, usable both from the command-line and graphically. It provides general-purpose applications that have wide applicability, concentrating on image processing, data visualisation, and manipulating NDF components. It integrates with other Starlink packages. In a wider context, KAPPA offers facilities not in IRAF, for instance handling of data errors, quality masking, a graphics database, availability from the shell, as well as more n-dimensional applications, widespread use of data axes, and a different style. It integrates with instrument packages developed at UK observatories. With the automatic data conversion and the availability of KAPPA and other Starlink packages from within the IRAF command language, it's possible to pick the best of the relevant tools from both systems to get the job done.

CCDPACK

A package of programs for reducing CCD-like data. They allow you to debias, remove dark current, pre-flash, flatfield, register, resample, normalize and combine your data.

AST

A flexible and powerful library for handling World Coordinate Systems, partly based on the SLALIB library. If you are writing software for astronomy and need to use celestial coordinates (e.g. RA and Dec), spectral coordinates (e.g. wavelength, frequency, etc.), or other coordinate system information, then this library should be of interest. It provides solutions for most of the problems you will meet and allows you to write robust and flexible software. It is able to read and write WCS information in a variety of formats, including FITS-WCS. It has Fortran, C and Python bindings.

SLALIB

A library of routines intended to make accurate and reliable positional-astronomy applications easier to write. Most SLALIB routines are concerned with astronomical position and time, but a number have wider trigonometrical, numerical or general applications. As well as this GPL version, there is also a commercial version of SLALIB available from its original author.

HDS

A Hierarchical Data System -- is a portable, flexible system for storing and retrieving data, and takes over from a computer's filing system at the level of an individual file. A conventional file effectively contains an 1-dimensional sequence of data elements, whereas an HDS file can contain a more complex structure. It predates the Hierarchical Data Format by several years.

NDF

NDF is the Project's principal data format. Built upon HDS the N-dimensional Data Format -- is for storing bulk data in the form of n-dimensional arrays of numbers: mostly spectra, images, and cubes. It supports concepts such as quality, data errors, world coordinate systems, and Metadata. It is also extensible to handle user-defined information.

ADAM

The ADAM environment was a standardised software environment developed initially by the RGO, and then adopted and developed by Starlink between 1985 and 1990. It was initially designed as a telescope control system, installed at the AAT at Siding Spring, the WHT at the ING on La Palma, and at the JCMT on Mauna Kea (where it is still working in legacy systems), but its role expanded to cover graphics, data access, interprocess communication, and the full range of functionality required to support a diverse range of interoperable applications. Although it is no longer seriously used for telescope control, other layers of it live on in the current versions of the Starlink applications and libraries.

super Mongo

• A user friendly plotting programme
• See http://www.astro.princeton.edu/~rhl/sm/

Backup service

there is a daily rsync backup: rsync -av home /bak/homebak

httpd service

personal webpage service

1. make your home directory readable

   $chmod -R 755 ~

2. make a public_html directory

   $mkdir ~/public_html

3. build your personal webpage

   $cd ~/public_html

   $cat "hello, world" >> index.html

• Your webpage will be avialbe at http://cluster.shao.ac.cn/~yourusername/

• How to make my webpage password protected?

please google .htaccess and .htpasswd