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 CEN45 192.5119 -41.3865 191.819775 -41.11429 209.359018 -32.811033 302.65166747 21.4844922 104.7288 54458.1467939815 2007-12-24 03:31:23 54459.2294444444 2007-12-25 05:30:24 802008010 58.2226 53 58.2226 58.2365 0 58.2306 2 2 0 2 1 0 0 64.5171 64.5171 93.5218 2 PROCESSED 57540.9525810185 2016-06-01 22:51:43 54854 2009-01-23 00:00:00 54486.1941087963 2008-01-21 04:39:31 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020011 We propose to obtain high-quality X-ray spectra of the subcluster region in the Centaurus cluster, Cen45, aiming at the first reliable detection of a supersonic motion of the intracluster gas. Previous optical and X-ray observations suggest that Cen45 is indeed in the process of merging and has a high velocity relative to the main cluster. Utilizing the high-sensitivity Suzaku/XIS spectroscopy, the line-of-sight velocity of the X-ray emitting gas can be accurately measured from the Doppler shift of iron-K lines. With our proposed 40ks observation, we can put a strong constraint on the gas motion in the subcluster region. This will also have great impacts on our understanding of dynamical state of clusters and their evolution. EXTRAGALACTIC DIFFUSE SOURCES 8 B NAOMI OTA JAP 2 AO2 MEASURING GAS MOTIONS OF THE INFALLING SUBCLUSTER CEN45 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802008010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802008010'

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