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 | NGC5548 | 214.4969 | 25.1266 | 213.929993 | 25.356783 | 201.998856 | 36.406453 | 31.93001973 | 70.4949274 | 285.8791 | 54310.1810648148 | 2007-07-29 04:20:44 | 54311.0209953704 | 2007-07-30 00:30:14 | 702042070 | 31.8099 | 30 | 31.8099 | 31.8099 | 0 | 31.8099 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 29.503 | 29.503 | 72.5279 | 1 | PROCESSED | 57539.3547569444 | 2016-05-31 08:30:51 | 54706 | 2008-08-28 00:00:00 | 54339.4245486111 | 2007-08-27 10:11:21 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021307 | We propose a 2 month Suzaku monitoring program of 7 weekly 30ksec observations of the normal type 1 AGN, NGC5548. NGC5548 is uniquely well studied at all wavelengths, and will vary by a factor of 1.5, or more, at 97% probability. Variations of the Warm Absorber will determine its location in NGC5548, disciminating between models and determining the mass loss rate in the WA wind. This will provide a baseline data point for models of 'cosmological feedback' from AGN to galaxy formation. Simultaneously, the XIS and HXD spectra will study changes or lack thereof in the reflection components (narrow Fe-K, Compton Hump), again delimiting their location and choosing among models. The summed spectrum will determine the high energy continuum break, any broad Fe-K or high ionization edge. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | MARTIN ELVIS | USA | 2 | AO2 | NGC5548 MONITORING: KEY TO AGN STRUCTURE AND COSMIC FEEDBACK | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702042070/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702042070'
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