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 | N4438 TAIL | 186.7653 | 12.9509 | 186.13191 | 13.227515 | 180.954769 | 14.552434 | 279.81897455 | 74.71807646 | 119.2941 | 56636.4959259259 | 2013-12-10 11:54:08 | 56639.0884259259 | 2013-12-13 02:07:20 | 808045010 | 102.7738 | 100 | 102.7738 | 102.7738 | 0 | 102.7738 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 92.8342 | 92.8342 | 223.962 | 2 | PROCESSED | 57613.6203587963 | 2016-08-13 14:53:19 | 57016 | 2014-12-25 00:00:00 | 56650.8089583333 | 2013-12-24 19:24:54 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080059 | We propose a 100 ks XIS observation to the Halpha/X-ray filament connecting N4438 and M86 in the Virgo cluster. Our main objective is to probe conclusively the OVII line which is marginally detected with the XMM-Newton. If established, by employing line diagnostic and non-equilibrium ionization analysis, we will be able to determine the ionization temperature and elapsed timescale of the multi-phase ISM stripped from N4438, and give constraint on the thermal conductivity and metal enrichment of the ICM. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | LIYI GU | JAP | 8 | AO8 | A SUZAKU OBSERVATION OF ONGOING IONIZATION OF ISM IN THE VIRGO CLUSTER ICM | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808045010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '808045010'
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