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 | NGC 4636 | 190.7243 | 2.7556 | 190.086173 | 3.029415 | 188.766391 | 6.778722 | 297.77503713 | 65.54179663 | 112.2967 | 53710.1073726852 | 2005-12-06 02:34:37 | 53711.9446643518 | 2005-12-07 22:40:19 | 800018010 | 79.201 | 80 | 79.201 | 79.201 | 79.201 | 79.201 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 75.7771 | 75.7771 | 158.7278 | 2 | PROCESSED | 57532.4099421296 | 2016-05-24 09:50:19 | 54247 | 2007-05-27 00:00:00 | 54038.9551388889 | 2006-10-30 22:55:24 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001083 | We propose to observe NGC 4636 for 50~ksec in a single pointing, to determine the chemical evolution of elliptical galaxies via the determination of the spatially resolved abundance of Oxygen and other elements. Being one of the most X-ray luminous ellipticals, and having been observed by both Chandra and XMM, this is also an important target to compare the capabilities of the three observatories and interpret the results of the Suzaku XIS in light of the source spectrum provided by the XMM RGS. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | ENECTALI FIGUEROA-FELICIANO | JAP | 0 | SWG | OBSERVATION OF THE X-RAY LUMINOUS EXTENDED EARLY-TYPE GALAXY NGC 4636 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800018010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '800018010'
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