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
|
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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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