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 | A1060_OFFSET | 159.8425 | -27.5312 | 159.252316 | -27.270314 | 173.386883 | -33.06567 | 270.15539037 | 26.80693828 | 96.4852 | 54425.0245486111 | 2007-11-21 00:35:21 | 54427.7988888889 | 2007-11-23 19:10:24 | 802028010 | 103.7993 | 100 | 103.7993 | 103.7993 | 0 | 103.7993 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.1119 | 89.1119 | 239.6797 | 2 | PROCESSED | 57540.6102662037 | 2016-06-01 14:38:47 | 54804 | 2008-12-04 00:00:00 | 54434.2515509259 | 2007-11-30 06:02:14 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020060 | We propose to observe a 30' offset region of the cluster of galaxies Abell 1060 for 100 ksec to study the temperature and abundance profiles. The central region within ~0.3 times the virial radius, or 380 kpc, has been already observed as one of the SWG targets, and the temperature decrease and differnt profiles of metal abundances are clealy observed (Sato et al. 2006). This observation will reveal the temperature and abundance profiles to half the virial radius. Comparison of the abundance profiles will tell us how metals produced by type Ia and II supernovae have been enriched in the outer cluster region. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KOSUKE SATO | JAP | 2 | AO2 | TEMPERATURE AND ABUNDANCE PROFILES IN THE OUTER REGION OF THE NON-CD CLUSTER A1060 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802028010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '802028010'
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