DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 PERSEUS OFFSET-H 50.3251 41.6598 49.495605 41.480554 58.942633 22.403293 150.73113668 -12.9828544 270.0006 55595.9611458333 2011-02-03 23:04:03 55596.3536805556 2011-02-04 08:29:18 805048010 18.241 25 18.249 18.249 0 18.241 1 1 0 1 1 0 0 14.88 14.88 33.9039 0 PROCESSED 57600.8294560185 2016-07-31 19:54:25 55979 2012-02-22 00:00:00 55610.233287037 2011-02-18 05:35:56 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 050093 We propose to map the central region (R<20') of the Perseus cluster of galaxies. The cluster is the X-ray brightest one at z=0.02. This unique object along with good performance of the SUZAKU XIS and HXD provides the best quality, wide-band and spatially-resolved X-ray spectroscopy of the ICM. Using the data, we attempt to understand temperature structure, gas dynamics and metal distribution in the ICM. In particular, this observation should provide the most robust measurement of the ICM bulk motions. EXTRAGALACTIC DIFFUSE SOURCES 8 C TAKAYUKI TAMURA JAP 5 AO5 MAPPING OF THE CENTRAL REGION OF THE PERSEUS CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805048010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805048010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏