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 ABELL 3395 96.7698 -54.5043 96.516816 -54.472103 108.474853 -77.510268 263.27498484 -25.21804833 150.0003 54815.4865046296 2008-12-15 11:40:34 54817.3168865741 2008-12-17 07:36:19 803020010 104.3469 100 104.3469 104.3469 0 104.3469 2 2 0 2 1 0 0 81.661 81.661 158.1299 3 PROCESSED 57545.0306828704 2016-06-06 00:44:11 55210 2010-01-14 00:00:00 54840.5412268518 2009-01-09 12:59:22 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030078 We propose to observe a merging cluster Abell 3395 with Suzaku for 100 ks. Abell 3395 has two X-ray emission peaks in the ICM, and they can have a large velocity difference of 3000 km/s at maximum. From the line shift of iron K line, we detect the bulk motion of the ICM, and compare it with the velocity distribution of galaxies. The difference of velocity distributions between the ICM and galaxies reflects the difference of their cross sections during the cluster merging. EXTRAGALACTIC DIFFUSE SOURCES 8 C MADOKA KAWAHARADA JAP 3 AO3 COMPARISON BETWEEN VELOCITY DISTRIBUTIONS OF ICM AND GALAXIES IN A MERGING CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803020010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803020010'

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